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42677341
10.1007/JHEP09(2016)041
Using the helicity-spinor language we explore the non-perturbative constraints that Lorentz symmetry imposes on three-point amplitudes where the asymptotic states can be massive. As it is well known, in the case of only massless states the three-point amplitude is fixed up to a coupling constant by these constraints plus some physical requirements. We find that a similar statement can be made when some of the particles have mass. We derive the generic functional form of the three-point amplitude by virtue of Lorentz symmetry, which displays several functional structures accompanied by arbitrary constants. These constants can be related to the coupling constants of the theory, but in an unambiguous fashion only in the case of one massive particle. Constraints on these constants are obtained by imposing that in the UV limit the massive amplitude matches the massless one. In particular, there is a certain Lorentz frame, which corresponds to projecting all the massive momenta along the same null momentum, where the three-point massive amplitude is fully fixed, and has a universal form.Comment: 31+10 pages, 0 figures. Relevant improvements of the results. Appendix B added. Version accepted by journa
Lorentz Constraints on Massive Three-Point Amplitudes
lorentz constraints on massive three-point amplitudes
helicity spinor explore perturbative lorentz imposes amplitudes asymptotic massive. massless requirements. statement mass. derive generic virtue lorentz displays accompanied constants. unambiguous fashion massive particle. imposing massive matches massless one. lorentz projecting massive momenta massive universal pages figures. improvements results. added. journa
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42743061
10.1007/JHEP09(2016)042
A reliable comparison of different dark matter (DM) searches requires models that satisfy certain consistency requirements like gauge invariance and perturbative unitarity. As a well-motivated example, we study two-mediator DM (2MDM). The model is based on a spontaneously broken $U(1)'$ gauge symmetry and contains a Majorana DM particle as well as two $s$-channel mediators, one vector (the $Z'$) and one scalar (the dark Higgs). We perform a global scan over the parameters of the model assuming that the DM relic density is obtained by thermal freeze-out in the early Universe and imposing a large set of constraints: direct and indirect DM searches, monojet, dijet and dilepton searches at colliders, Higgs observables, electroweak precision tests and perturbative unitarity. We conclude that thermal DM is only allowed either close to an $s$-channel resonance or if at least one mediator is lighter than the DM particle. In these cases a thermal DM abundance can be obtained although DM couplings to the Standard Model are tiny. Interestingly, we find that vector-mediated DM-nucleon scattering leads to relevant constraints despite the velocity-suppressed cross section, and that indirect detection can be important if DM annihilations into both mediators are kinematically allowed.Comment: 30 pages, 9 figures + appendice
How to save the WIMP: global analysis of a dark matter model with two s-channel mediators
how to save the wimp: global analysis of a dark matter model with two s-channel mediators
reliable searches satisfy consistency invariance perturbative unitarity. motivated mediator spontaneously broken majorana mediators scan relic freeze universe imposing indirect searches monojet dijet dilepton searches colliders observables electroweak precision perturbative unitarity. mediator lighter particle. abundance couplings tiny. interestingly nucleon suppressed indirect annihilations mediators kinematically pages appendice
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42707334
10.1007/JHEP09(2016)043
We discuss aspects of theories with superpotentials given by Arnold's $A,D,E$ singularities, particularly the novelties that arise when the fields are matrices. We focus on 4d ${\cal N}=1$ variants of susy QCD, with $U(N_c)$ or $SU(N_c)$ gauge group, $N_f$ fundamental flavors, and adjoint matter fields $X$ and $Y$ appearing in $W_{A,D,E}(X,Y)$ superpotentials. Many of our considerations also apply in other possible contexts for matrix-variable $W_{A,D,E}$. The 4d $W_{A,D,E}$ SQCD-type theories RG flow to superconformal field theories, and there are proposed duals in the literature for the $W_{A_k}$, $W_{D_k}$, and $W_{E_7}$ cases. As we review, the $W_{D_\text{even}}$ and $W_{E_7}$ duals rely on a conjectural, quantum truncation of the chiral ring. We explore these issues by considering various deformations of the $W_{A,D,E}$ superpotentials, and the resulting RG flows and IR theories. Rather than finding supporting evidence for the quantum truncation and $W_{D_\text{even}}$ and $W_{E_7}$ duals, we note some challenging evidence to the contrary.Comment: 59 pages, many figure
Deformations of $W_{A,D,E}$ SCFTs
deformations of $w_{a,d,e}$ scfts
superpotentials arnold singularities novelties arise matrices. variants susy flavors adjoint appearing superpotentials. considerations contexts sqcd superconformal duals cases. duals rely conjectural truncation chiral ring. explore deformations superpotentials flows theories. supporting truncation duals challenging pages
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42697163
10.1007/JHEP09(2016)044
We show that renormalization group(RG) flow can be viewed as a gradual wave function collapse, where a quantum state associated with the action of field theory evolves toward a final state that describes an IR fixed point. The process of collapse is described by the radial evolution in the dual holographic theory. If the theory is in the same phase as the assumed IR fixed point, the initial state is smoothly projected to the final state. If in a different phase, the initial state undergoes a phase transition which in turn gives rise to a horizon in the bulk geometry. We demonstrate the connection between critical behavior and horizon in an example, by deriving the bulk metrics that emerge in various phases of the U(N) vector model in the large N limit based on the holographic dual constructed from quantum RG. The gapped phase exhibits a geometry that smoothly ends at a finite proper distance in the radial direction. The geometric distance in the radial direction measures a complexity : the depth of RG transformation that is needed to project the generally entangled UV state to a direct product state in the IR. For gapless states, entanglement persistently spreads out to larger length scales, and the initial state can not be projected to the direct product state. The obstruction to smooth projection at charge neutral point manifests itself as the long throat in the anti-de Sitter space. The Poincare horizon at infinity marks the critical point which exhibits a divergent length scale in the spread of entanglement. For the gapless states with non-zero chemical potential, the bulk space becomes the Lifshitz geometry with the dynamical critical exponent two. The identification of horizon as critical point may provide an explanation for the universality of horizon. We also discuss the structure of the bulk tensor network that emerges from the quantum RG.Comment: 37 pages, 8 figures; v2) introduction expande
Horizon as Critical Phenomenon
horizon as critical phenomenon
renormalization viewed gradual collapse evolves toward describes point. collapse holographic theory. smoothly projected state. undergoes horizon geometry. connection horizon deriving metrics emerge holographic gapped exhibits smoothly ends proper direction. geometric entangled gapless entanglement persistently spreads projected state. obstruction projection neutral manifests throat sitter space. poincare horizon infinity marks exhibits divergent spread entanglement. gapless lifshitz exponent two. horizon explanation universality horizon. emerges pages expande
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42744692
10.1007/JHEP09(2016)045
We compute the two-loop O(as*at) corrections to the Higgs boson masses in supersymmetric extensions of the Standard Model with Dirac gaugino masses. We rely on the effective-potential technique, allow for both Dirac and Majorana mass terms for the gluinos, and compute the corrections in both the DRbar and on-shell renormalisation schemes. We give detailed results for the MDGSSM and the MRSSM, and simple approximate formulae valid in the decoupling limit for all currently-studied variants of supersymmetric models with Dirac gluinos. These results represent the first explicit two-loop calculation of Higgs boson masses in supersymmetric models beyond the MSSM and the NMSSM.Comment: 36 pages, 5 figures; v2: version published in JHE
Leading two-loop corrections to the Higgs boson masses in SUSY models with Dirac gauginos
leading two-loop corrections to the higgs boson masses in susy models with dirac gauginos
boson supersymmetric extensions dirac gaugino masses. rely dirac majorana gluinos drbar renormalisation schemes. mdgssm mrssm approximate formulae valid decoupling variants supersymmetric dirac gluinos. boson supersymmetric mssm pages
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42697664
10.1007/JHEP09(2016)046
Anomalous chiral conductivities in theories with global anomalies are independent of whether they are computed in a weakly coupled quantum (or thermal) field theory, hydrodynamics, or at infinite coupling from holography. While the presence of dynamical gauge fields and mixed, gauge-global anomalies can destroy this universality, in their absence, the non-renormalisation of anomalous Ward identities is expected to be obeyed at all intermediate coupling strengths. In holography, bulk theories with higher-derivative corrections incorporate coupling constant corrections to the boundary theory observables in an expansion around infinite coupling. In this work, we investigate the coupling constant dependence and universality of anomalous conductivities (and thus of the anomalous Ward identities) in general, four-dimensional systems that possess asymptotically anti-de Sitter holographic duals with a non-extremal black brane in five dimensions, and anomalous transport introduced into the boundary theory via the bulk Chern-Simons action. We show that in bulk theories with arbitrary gauge- and diffeomorphism-invariant higher-derivative actions, anomalous conductivities, which can incorporate an infinite series of (inverse) coupling constant corrections, remain universal. Owing to the existence of the membrane paradigm, the proof reduces to a construction of bulk effective theories at the horizon and the boundary. It only requires us to impose the condition of horizon regularity and correct boundary conditions on the fields. We also discuss ways to violate the universality by violating conditions for the validity of the membrane paradigm, in particular, by adding mass to the vector fields (a case with a mixed, gauge-global anomaly) and in bulk geometries with a naked singularity.Comment: V2: 29 pages, 1 figure, version published in JHE
Universality of anomalous conductivities in theories with higher-derivative holographic duals
universality of anomalous conductivities in theories with higher-derivative holographic duals
anomalous chiral conductivities anomalies weakly hydrodynamics infinite holography. anomalies destroy universality renormalisation anomalous ward identities obeyed strengths. holography incorporate observables infinite coupling. universality anomalous conductivities anomalous ward identities possess asymptotically sitter holographic duals extremal brane anomalous chern simons action. diffeomorphism anomalous conductivities incorporate infinite universal. owing paradigm reduces horizon boundary. impose horizon regularity fields. ways violate universality violating validity paradigm adding anomaly geometries naked pages
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42717891
10.1007/JHEP09(2016)047
We consider BPS Wilson loops in planar ABJM theory, wound multiple times around the great circle. We compute the expectation value of the 1/6-BPS and 1/2-BPS Wilson loops to three- and two-loop order in perturbation theory, respectively, dealing with the combinatorics of multiple winding via recursive relations. For the 1/6-BPS Wilson loop we perform the computation at generic framing and at framing 1 we find agreement with the localization result. For the 1/2-BPS Wilson loop we compute the expectation value at trivial framing and by comparison with the matrix model expression we extract the framing dependence of the fermion diagrams.Comment: 40 page
A note on multiply wound BPS Wilson loops in ABJM
a note on multiply wound bps wilson loops in abjm
wilson loops planar abjm wound great circle. expectation wilson loops perturbation dealing combinatorics winding recursive relations. wilson generic framing framing localization result. wilson expectation trivial framing extract framing fermion
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42746503
10.1007/JHEP09(2016)049
We present a scenario where a $Z_2$-symmetric scalar field $\phi$ first drives cosmic inflation, then reheats the Universe but remains out-of-equilibrium itself, and finally comprises the observed dark matter abundance, produced by particle decays \`{a} la freeze-in mechanism. We work model-independently without specifying the interactions of the scalar field besides its self-interaction coupling, $\lambda\phi^4$, non-minimal coupling to gravity, $\xi\phi^2R$, and coupling to another scalar field, $g\phi^2\sigma^2$. We find the scalar field $\phi$ serves both as the inflaton and a dark matter candidate if $10^{-9}\lesssim \lambda\lesssim g\lesssim 10^{-7}$ and $3 \rm{keV} \lesssim m_{\rm \phi}\lesssim 85 \rm{MeV}$ for $\xi=\mathcal{O}(1)$. Such a small value of the non-minimal coupling is also found to be of the right magnitude to produce the observed curvature perturbation amplitude within the scenario. We also discuss how the model may be distinguished from other inflationary models of the same type by the next generation CMB satellites.Comment: 14 pages, 2 figures. Typos corrected, references added. To appear in JHE
Feebly Interacting Dark Matter Particle as the Inflaton
feebly interacting dark matter particle as the inflaton
drives cosmic inflation reheats universe comprises abundance decays freeze mechanism. independently specifying besides lambda sigma serves inflaton candidate lesssim lambda lesssim lesssim lesssim lesssim mathcal curvature perturbation scenario. distinguished inflationary pages figures. typos corrected added.
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73347326
10.1007/JHEP09(2016)050
We show that the relatively small but coincident excesses observed around 2 TeV in the ATLAS Run 1 and Run 2 hadronic diboson searches --- when a cut on the number of tracks in the fat jets is not applied --- and the null results of all remaining high-mass diboson searches are compatible with the decay of a triboson resonance $R$ into $WZ$ plus an extra particle $X$. These decays can take place via new neutral ($Y^0$) or charged ($Y^\pm$) particles, namely $R \to Y^0 \, W$, with $Y^0 \to Z X$, or $R \to Y^\pm Z$, with $Y^\pm \to W X$. An obvious candidate for such intermediate particle is a neutral one $Y^0$, given a $3.9\sigma$ excess found at 650 GeV by the CMS Collaboration in searches for intermediate mass diboson resonances decaying to $ZV$, with $V=W,Z$. We discuss discovery strategies for triboson resonances with small modifications of existing hadronic searches.Comment: LaTeX 32 pages, 38 figures. v2: Figs. 6, 9 and 11 modified. v3: added VH search in hadronic final state. v4: final published versio
Traces of a triboson resonance
traces of a triboson resonance
coincident excesses atlas hadronic diboson searches tracks jets diboson searches compatible triboson extra decays neutral obvious candidate neutral sigma excess searches diboson resonances decaying discovery triboson resonances modifications hadronic latex pages figures. figs. modified. hadronic state. versio
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73352427
10.1007/JHEP09(2016)054
We reconsider gravitational corrections to vacuum decay, confirming and simplifying earlier results and extending them by allowing for a non-minimal coupling of the Higgs to gravity. We find that leading-order gravitational corrections suppress the vacuum decay rate. Furthermore, we compute minor corrections to thermal vacuum decay in the SM by adding one-loop contributions to the Higgs kinetic term, two-loop contributions to the Higgs potential and allowing for time-dependent bounces.Comment: 19 pages, 7 figure
On gravitational and thermal corrections to vacuum decay
on gravitational and thermal corrections to vacuum decay
reconsider gravitational confirming simplifying extending allowing gravity. gravitational suppress rate. minor adding allowing pages
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42742514
10.1007/JHEP09(2016)057
We present a simulation program for the production of a pair of W bosons in association with a jet, that can be used in conjunction with general-purpose shower Monte Carlo generators, according to the POWHEG method. We have further adapted and implemented the MINLO' method on top of the NLO calculation underlying our WW+jet generator. Thus, the resulting simulation achieves NLO accuracy not only for inclusive distributions in WW+jet production but also WW production, i.e. when the associated jet is not resolved, without the introduction of any unphysical merging scale. This work represents the first extension of the MINLO' method, in its original form, to the case of a genuine underlying 2->2 process, with non-trivial virtual corrections.Comment: 22 pages, 9 figure
Merging WW and WW+jet with MINLO
merging ww and ww+jet with minlo
bosons conjunction shower monte carlo generators powheg method. adapted implemented minlo generator. achieves inclusive i.e. resolved unphysical merging scale. minlo genuine trivial virtual pages
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42721157
10.1007/JHEP09(2016)058
We study entanglement in states of holographic CFTs defined by Euclidean path integrals over geometries with slowly varying metrics. In particular, our CFT spacetimes have $S^1$ fibers whose size $b$ varies along one direction ($x$) of an ${\mathbb R}^{d-1}$ base. Such examples respect an ${\mathbb R}^{d-2}$ Euclidean symmetry. Treating the $S^1$ direction as time leads to a thermofield double state on a spacetime with adiabatically varying redshift, while treating another direction as time leads to a confining ground state with slowly varying confinement scale. In both contexts the entropy of slab-shaped regions defined by $|x - x_0| \le L$ exhibits well-known phase transitions at length scales $L= L_{crit}$ characterizing the CFT entanglements. For the thermofield double, the numerical coefficients governing the effect of variations in $b(x)$ on the transition are surprisingly small and exhibit an interesting change of sign: gradients reduce $L_{crit}$ for $d \le 3$ but increase $L_{crit}$ for $d\ge4$. This means that, while for general $L > L_{crit}$ they significantly increase the mutual information of opposing slabs as one would expect, for $d\ge 4$ gradients cause a small decrease near the phase transition. In contrast, for the confining ground states gradients always decrease $L_{crit}$, with the effect becoming more pronounced in higher dimensions.Comment: 32 pages, 16 figures, typos fixed and reg. procedure refine
Adiabatic corrections to holographic entanglement in thermofield doubles and confining ground states
adiabatic corrections to holographic entanglement in thermofield doubles and confining ground states
entanglement holographic cfts euclidean integrals geometries slowly metrics. spacetimes fibers varies mathbb base. mathbb euclidean symmetry. treating thermofield spacetime adiabatically treating confining slowly confinement scale. contexts slab shaped exhibits crit characterizing entanglements. thermofield governing surprisingly exhibit gradients crit crit crit mutual opposing slabs gradients transition. confining gradients crit becoming pronounced pages typos reg. refine
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42737769
10.1007/JHEP09(2016)059
Using the AdS/CFT duality, we study the expectation value of stress tensor in $2+1$-dimensional quantum critical theories with a general dynamical scaling $z$, and explore various constrains on negative energy density for strongly coupled field theories. The holographic dual theory is the theory of gravity in 3+1-dimensional Lifshitz backgrounds. We adopt a consistent approach to obtain the boundary stress tensor from bulk construction, which satisfies the trace Ward identity associated with Lifshitz scaling symmetry. In particular, the boundary stress tensor, constructed from the gravitational wave deformed Lifshitz geometry, is found up to second order in gravitational wave perturbations. {The result} is compared to its counterpart in free {scalar} field theory at the same order in an expansion of small squeezing parameters. This allows us to relate the boundary values of gravitational waves to the squeezing parameters of squeezed vacuum states. We find that, in both cases with $z=1$, the stress tensor satisfies the averaged null energy condition, and is consistent with the quantum interest conjecture. Moreover, the negative lower bound on null-contracted stress tensor, which is averaged over time-like trajectories along nearly null directions, is obtained. We find a weaker constraint on the magnitude and duration of negative null energy density in strongly coupled field theory as compared with the constraint in free relativistic field theory. The implications are discussed.Comment: This is the version(v2) published in JHE
A Holographic Description of Negative Energy States
a holographic description of negative energy states
duality expectation explore constrains theories. holographic lifshitz backgrounds. adopt satisfies trace ward lifshitz symmetry. gravitational deformed lifshitz gravitational perturbations. counterpart squeezing parameters. relate gravitational squeezing squeezed states. satisfies averaged conjecture. contracted averaged trajectories nearly directions obtained. weaker relativistic theory.
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42741981
10.1007/JHEP09(2016)060
The holographic entanglement entropy is studied numerically in (4+1)-dimensional spherically symmetric Gauss-Bonnet AdS black hole spacetime with compact boundary. On the bulk side the black hole spacetime undergoes a van der Waals-like phase transition in the extended phase space, which is reviewed with emphasis on the behavior on the temperature-entropy plane. On the boundary, we calculated the regularized HEE of a disk region of different sizes. We find strong numerical evidence for the failure of equal area law for isobaric curves on the temperature-HEE plane and for the correctness of first law of entanglement entropy, and briefly give an explanation for why the latter may serve as a reason for the former, i.e. the failure of equal area law on the temperature-HEE plane.Comment: 17 pages, 4 PDF figures. Update: journal versio
Thermodynamics and holographic entanglement entropy for spherical black holes in 5D Gauss-Bonnet gravity
thermodynamics and holographic entanglement entropy for spherical black holes in 5d gauss-bonnet gravity
holographic entanglement numerically spherically gauss bonnet spacetime boundary. spacetime undergoes waals reviewed emphasis plane. regularized sizes. isobaric correctness entanglement briefly explanation serve former i.e. pages figures. update versio
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42749342
10.1007/JHEP09(2016)061
The so called one-parameter (often called $\varkappa$) deformed $AdS$ string sigma models have attracted a lot of attention lately in the study of integrability in string theory. We construct various circular string solutions in the $(AdS_3 \times S^3)_{\varkappa}$ background and describe the characteristics of such solutions qualitatively. We study the Bohr-Sommerfeld like quantization for these string states to characterise the motion. Further we find a `long' string limit of such circular strings in the $\varkappa$-deformed $AdS_3$ and find a novel dependence of the oscillation number on the energy in the next to leading order expansion.Comment: v2: References added, typos correcte
On circular strings in $(AdS_3 \times S^3)_{\varkappa}$
on circular strings in $(ads_3 \times s^3)_{\varkappa}$
varkappa deformed sigma attracted lately integrability theory. circular varkappa qualitatively. bohr sommerfeld quantization characterise motion. circular strings varkappa deformed oscillation typos correcte
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42744724
10.1007/JHEP09(2016)063
We study the non-linearly realized spontaneously broken supersymmetry of the (anti-)D3-brane action in type IIB string theory. The worldvolume fields are one vector $A_\mu$, three complex scalars $\phi^i$ and four 4d fermions $\lambda^0$, $\lambda^i$. These transform, in addition to the more familiar N=4 linear supersymmetry, also under 16 spontaneously broken, non-linearly realized supersymmetries. We argue that the worldvolume fields can be packaged into the following constrained 4d non-linear N=1 multiplets: four chiral multiplets $S$, $Y^i$ that satisfy $S^2=SY^i=0$ and contain the worldvolume fermions $\lambda^0$ and $\lambda^i$; and four chiral multiplets $W_\alpha$, $H^i$ that satisfy $S W_\alpha=0$ and $S \bar D_{\dot \alpha} \bar H^{\bar \imath}=0$ and contain the vector $A_\mu$ and the scalars $\phi^i$. We also discuss how placing an anti-D3-brane on top of intersecting O7-planes can lead to an orthogonal multiplet $\Phi$ that satisfies $S(\Phi-\bar \Phi)=0$, which is particularly interesting for inflationary cosmology.Comment: 28 pages, v2: published version, 1 reference adde
String Theory Origin of Constrained Multiplets
string theory origin of constrained multiplets
linearly realized spontaneously broken supersymmetry brane theory. worldvolume scalars fermions lambda lambda transform familiar supersymmetry spontaneously broken linearly realized supersymmetries. argue worldvolume packaged constrained multiplets chiral multiplets satisfy worldvolume fermions lambda lambda chiral multiplets alpha satisfy alpha alpha imath scalars placing brane intersecting planes orthogonal multiplet satisfies inflationary pages adde
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42728456
10.1007/JHEP09(2016)064
Making use of integral forms and superfield techniques we propose supersymmetric extensions of the multimetric gravity Lagrangians in dimensions one, two, three and four. The supersymmetric interaction potential covariantly deforms the bosonic one, producing in particular suitable super-symmetric polynomials generated by the Berezinian. As an additional application of our formalism we construct supersymmetric multi-Maxwell theories in dimensions three and four.Comment: 37 pages, Latex2e, no figure
Multimetric Supergravities
multimetric supergravities
superfield propose supersymmetric extensions multimetric lagrangians four. supersymmetric covariantly deforms bosonic producing super polynomials berezinian. formalism supersymmetric maxwell pages latex
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42736070
10.1007/JHEP09(2016)065
We study a simple class of correlators with two heavy and two light operators both in the D1D5 CFT and in the dual AdS$_3 \times S^3 \times T^4$ description. On the CFT side we focus on the free orbifold point and discuss how these correlators decompose in terms of conformal blocks, showing that they are determined by protected quantities. On the gravity side, the heavy states are described by regular, asymptotically AdS$_3 \times S^3 \times T^4$ solutions and the correlators are obtained by studying the wave equation in these backgrounds. We find that the CFT and the gravity results agree and that, even in the large central charge limit, these correlators do not have (Euclidean) spurious singularities. We suggest that this is indeed a general feature of the heavy-light correlators in unitary CFTs, which can be relevant for understanding how information is encoded in black hole microstates.Comment: 32 pages, v2: citations added, typos corrected, v3: typos corrected, submitted to JHE
Correlators at large c without information loss
correlators at large c without information loss
correlators description. orbifold correlators decompose conformal blocks protected quantities. asymptotically correlators studying backgrounds. agree correlators euclidean spurious singularities. correlators unitary cfts encoded pages citations typos corrected typos corrected submitted
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42683078
10.1007/JHEP09(2016)066
We analyze the dynamical response functions of strongly interacting quantum critical states described by conformal field theories (CFTs). We construct a self-consistent holographic model that incorporates the relevant scalar operator driving the quantum critical phase transition. Focusing on the finite temperature dynamical conductivity $\sigma(\omega,T)$, we study its dependence on our model parameters, notably the scaling dimension of the relevant operator. It is found that the conductivity is well-approximated by a simple ansatz proposed by Katz et al [1] for a wide range of parameters. We further dissect the conductivity at large frequencies $\omega >> T$ using the operator product expansion, and show how it reveals the spectrum of our model CFT. Our results provide a physically-constrained framework to study the analytic continuation of quantum Monte Carlo data, as we illustrate using the O(2) Wilson-Fisher CFT. Finally, we comment on the variation of the conductivity as we tune away from the quantum critical point, setting the stage for a comprehensive analysis of the phase diagram near the transition.Comment: 25+18 pages; 8+2 figures; 1 table. v3: published versio
A Holographic Model for Quantum Critical Responses
a holographic model for quantum critical responses
analyze interacting conformal cfts holographic incorporates driving transition. focusing conductivity sigma omega notably operator. conductivity approximated ansatz katz parameters. dissect conductivity omega reveals cft. physically constrained analytic continuation monte carlo illustrate wilson fisher cft. comment conductivity tune away comprehensive pages table. versio
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42727263
10.1007/JHEP09(2016)067
We numerically construct large Randall-Sundrum II brane black holes in 4 and 5 dimensions from associated AdS/CFT spacetimes. Our solutions are leading order perturbations of a representative of the boundary conformal structure of the AdS spacetime sourced by the dual CFT stress tensor. The 4-dimensional solutions are static perturbations of the Euclidean Schwarzschild metric, while the 5-dimensional solutions are perturbations of the Myers-Perry metric with equal angular momenta. We compare the former with previous numerical results for Randall-Sundrum bulk black holes and find good agreement down to a horizon radius of about rH ~30l. The latter are the first numerical results pertaining to rotating Randall-Sundrum black holes. They have the same entropy, but a larger horizon area than Myers-Perry black holes of the same mass and angular momentum.Comment: 25 pages, 14 figures, v2: references adde
Perturbative Construction of Stationary Randall-Sundrum II Black Holes on a 5-Brane
perturbative construction of stationary randall-sundrum ii black holes on a 5-brane
numerically randall sundrum brane holes spacetimes. perturbations conformal spacetime sourced tensor. perturbations euclidean schwarzschild perturbations myers perry momenta. former randall sundrum holes horizon pertaining rotating randall sundrum holes. horizon myers perry holes pages adde
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78072213
10.1007/JHEP09(2016)068
In this work, we investigate modular Hamiltonians defined with respect to arbitrary spatial regions in quantum field theory states which have semi-classical gravity duals. We find prescriptions in the gravity dual for calculating the action of the modular Hamiltonian on its defining state, including its dual metric, and also on small excitations around the state. Curiously, use of the covariant holographic entanglement entropy formula leads us to the conclusion that the modular Hamiltonian, which in the quantum field theory acts only in the causal completion of the region, does not commute with bulk operators whose entire gauge-invariant description is space-like to the causal completion of the region.United States. Dept. of Energy (Contract DE-SC00012567
The gravity duals of modular Hamiltonians
the gravity duals of modular hamiltonians
modular hamiltonians duals. prescriptions calculating modular defining excitations state. curiously covariant holographic entanglement modular acts causal completion commute causal completion region.united states. dept. contract
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42747827
10.1007/JHEP09(2016)069
In this work, we study the SM-like Higgs pair productions in the framework of the general CP-violating two-Higgs-doublet model. Several constraints are imposed to the model sequentially, including the SM-like Higgs boson signal fits, the precise measurements of the electric dipole moments, the perturbative unitarity and stability bounds to the Higgs potential, and the most recent LHC searches for the heavy Higgs bosons. We show how are the CP-violating mixing angles related to the Higgs cubic self couplings in this setup. Afterwards, we estimate the cross sections of the future LHC/SppC searches for the Higgs pair productions, as well as other possible decay modes for the heavy Higgs bosons.Comment: JHEP style, 29 pages, 9 figures, matches the published versio
Higgs pair productions in the CP-violating two-Higgs-doublet model
higgs pair productions in the cp-violating two-higgs-doublet model
productions violating doublet model. imposed sequentially boson fits precise dipole moments perturbative unitarity bounds searches bosons. violating angles cubic couplings setup. afterwards sppc searches productions jhep style pages matches versio
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29567302
10.1007/JHEP09(2016)070
In the context of conformal field theories in general space-time dimension, we find all the possible singularities of the conformal blocks as functions of the scaling dimension $\Delta$ of the exchanged operator. In particular, we argue, using representation theory of parabolic Verma modules, that in odd spacetime dimension the singularities are only simple poles. We discuss how to use this information to write recursion relations that determine the conformal blocks. We first recover the recursion relation introduced in 1307.6856 for conformal blocks of external scalar operators. We then generalize this recursion relation for the conformal blocks associated to the four point function of three scalar and one vector operator. Finally we specialize to the case in which the vector operator is a conserved current.Comment: 55 pages, 12 figures; v2 Typos corrected, conclusions changed, reference adde
Recursion Relations for Conformal Blocks
recursion relations for conformal blocks
conformal singularities conformal blocks delta exchanged operator. argue parabolic verma modules spacetime singularities poles. recursion conformal blocks. recover recursion conformal blocks operators. generalize recursion conformal blocks operator. specialize conserved pages typos corrected changed adde
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42719570
10.1007/JHEP09(2016)071
We consider "new inflation" inflationary models at small fields, embedded in minimal ${\cal N}=1$ supergravity with a single chiral superfield. Imposing a period of inflation compatible with experiment severely restricts possible models, classified in perturbation theory. If moreover we impose that the field goes to large values and very small potential at the current time, like would be needed for instance for the inflaton being the volume modulus in large extra dimensional scenarios, the possible models are restricted to very contrived superpotentials.Comment: 25 pages, no figures; references and explanation adde
Small field inflation in ${\cal N}=1$ supergravity with a single chiral superfield
small field inflation in ${\cal n}=1$ supergravity with a single chiral superfield
inflation inflationary embedded supergravity chiral superfield. imposing inflation compatible severely restricts classified perturbation theory. impose goes inflaton modulus extra scenarios restricted contrived pages explanation adde
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42664706
10.1007/JHEP09(2016)073
We study the action of mirror symmetry on two-dimensional N=(2,2) effective theories obtained by compactifying Type IIA string theory on Calabi-Yau fourfolds. Our focus is on fourfold geometries with non-trivial three-form cohomology. The couplings of the massless zero-modes arising by expanding in these forms depend both on the complex structure deformations and the Kahler structure deformations of the Calabi-Yau fourfold. We argue that two holomorphic functions of the deformation moduli capture this information. These are exchanged under mirror symmetry, which allows us to derive them at the large complex structure and large volume point. We discuss the application of the resulting explicit expression to F-theory compactifications and their weak string coupling limit. In the latter orientifold settings we demonstrate compatibility with mirror symmetry of Calabi-Yau threefolds at large complex structure. As a byproduct we find an interesting relation of no-scale like conditions on Kahler potentials to the existence of chiral and twisted-chiral descriptions in two dimensions.Comment: 36 page
On Mirror Symmetry for Calabi-Yau Fourfolds with Three-Form Cohomology
on mirror symmetry for calabi-yau fourfolds with three-form cohomology
mirror compactifying calabi fourfolds. fourfold geometries trivial cohomology. couplings massless arising expanding deformations kahler deformations calabi fourfold. argue holomorphic deformation moduli capture information. exchanged mirror derive point. compactifications limit. orientifold settings compatibility mirror calabi threefolds structure. byproduct kahler potentials chiral twisted chiral descriptions
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42651313
10.1007/JHEP09(2016)075
We propose a new efficient algorithm to obtain the locally minimal generating set of the syzygies for an ideal, i.e. a generating set whose proper subsets cannot be generating sets. Syzygy is a concept widely used in the current study of scattering amplitudes. This new algorithm can deal with more syzygies effectively because a new generation of syzygies is obtained in each step and the irreducibility of this generation is also verified in the process. This efficient algorithm can also be applied in getting the syzygies for the modules. We also show a typical example to illustrate the potential application of this method in scattering amplitudes, especially the Integral-By-Part(IBP) relations of the characteristic two-loop diagrams in the Yang-Mills theory.Comment: 33 pages, 10 figure
Syzygies Probing Scattering Amplitudes
syzygies probing scattering amplitudes
propose locally generating syzygies ideal i.e. generating proper subsets generating sets. syzygy widely amplitudes. deal syzygies effectively syzygies irreducibility verified process. getting syzygies modules. illustrate amplitudes diagrams mills pages
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42749163
10.1007/JHEP09(2016)076
We propose and study a novel extension of the Standard Model based on the B-L gauge symmetry that can account for dark matter and neutrino masses. In this model, right-handed neutrinos are absent and the gauge anomalies are canceled instead by four chiral fermions with fractional B-L charges. After the breaking of $U(1)_{B-L}$, these fermions arrange themselves into two Dirac particles, the lightest of which is automatically stable and plays the role of the dark matter. We determine the regions of the parameter space consistent with the observed dark matter density and show that they can be partially probed via direct and indirect dark matter detection or collider searches at the LHC. Neutrino masses, on the other hand, can be explained by a variant of the type-II seesaw mechanism involving one of the two scalar fields responsible for the dark matter mass.Comment: 23 pages, 10 figure
A new B-L model without right-handed neutrinos
a new b-l model without right-handed neutrinos
propose masses. handed neutrinos absent anomalies canceled chiral fermions fractional charges. breaking fermions arrange dirac lightest automatically plays matter. partially probed indirect collider searches lhc. variant seesaw involving pages
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42692673
10.1007/JHEP09(2016)077
We present global fits of an effective field theory description of real, and complex scalar dark matter candidates. We simultaneously take into account all possible dimension 6 operators consisting of dark matter bilinears and gauge invariant combinations of quark and gluon fields. We derive constraints on the free model parameters for both the real (five parameters) and complex (seven) scalar dark matter models obtained by combining Planck data on the cosmic microwave background, direct detection limits from LUX, and indirect detection limits from the Fermi Large Area Telescope. We find that for real scalars indirect dark matter searches disfavour a dark matter particle mass below 100 GeV. For the complex scalar dark matter particle current data have a limited impact due to the presence of operators that lead to p-wave annihilation, and also do not contribute to the spin-independent scattering cross- section. Although current data are not informative enough to strongly constrain the theory parameter space, we demonstrate the power of our formalism to reconstruct the theoretical parameters compatible with an actual dark matter detection, by assuming that the excess of gamma rays observed by the Fermi Large Area Telescope towards the Galactic centre is entirely due to dark matter annihilations. Please note that the excess can very well be due to astrophysical sources such as millisecond pulsars. We find that scalar dark matter interacting via effective field theory operators can in principle explain the Galactic centre excess, but that such interpretation is in strong tension with the non-detection of gamma rays from dwarf galaxies in the real scalar case. In the complex scalar case there is enough freedom to relieve the tension.Comment: 20 pages, 5 figure
Effective Field Theory of Dark Matter: a Global Analysis
effective field theory of dark matter: a global analysis
fits candidates. simultaneously consisting bilinears combinations gluon fields. derive seven combining planck cosmic microwave indirect fermi telescope. scalars indirect searches disfavour gev. annihilation section. informative constrain formalism reconstruct compatible excess gamma rays fermi telescope galactic entirely annihilations. please excess astrophysical millisecond pulsars. interacting galactic excess tension gamma rays dwarf case. freedom relieve pages
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42729997
10.1007/JHEP09(2016)078
The splitting processes of bremsstrahlung and pair production in a medium are coherent over large distances in the very high energy limit, which leads to a suppression known as the Landau-Pomeranchuk-Migdal (LPM) effect. In this paper, we continue analysis of the case when the coherence lengths of two consecutive splitting processes overlap (which is important for understanding corrections to standard treatments of the LPM effect in QCD), avoiding soft-gluon approximations. In particular, this paper analyzes the subtle problem of how to precisely separate overlapping double splitting (e.g.\ overlapping double bremsstrahlung) from the case of consecutive, independent bremsstrahlung (which is the case that would be implemented in a Monte Carlo simulation based solely on single splitting rates). As an example of the method, we consider the rate of real double gluon bremsstrahlung from an initial gluon with various simplifying assumptions (thick media; $\hat q$ approximation; large $N_c$; and neglect for the moment of processes involving 4-gluon vertices) and explicitly compute the correction $\Delta\,d\Gamma/dx\,dy$ due to overlapping formation times.Comment: 59 pages, 37 figures. The major changes from v1: new section I.A.4 added to give kinetic theory analogy to better explain the importance of the subtraction defining Delta[d(Gamma)/dx dy]; new appendix F added to compare/contrast with issues raised by Blaizot, Dominguez, Iancu, and Mehtar-Tani [22
The LPM effect in sequential bremsstrahlung 2: factorization
the lpm effect in sequential bremsstrahlung 2: factorization
splitting bremsstrahlung coherent distances suppression landau pomeranchuk migdal effect. continue coherence lengths consecutive splitting overlap treatments avoiding gluon approximations. analyzes subtle precisely overlapping splitting e.g. overlapping bremsstrahlung consecutive bremsstrahlung implemented monte carlo solely splitting gluon bremsstrahlung gluon simplifying assumptions thick neglect moment involving gluon explicitly delta gamma overlapping pages figures. i.a. analogy subtraction defining delta gamma raised blaizot dominguez iancu mehtar tani
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42736411
10.1007/JHEP09(2016)079
The LHC is now studying in detail the couplings of the Higgs boson in order to determine if there is new physics. Many recent studies have examined the available fits to Higgs couplings from the perspective of constraining two Higgs doublet models (2HDM). In this paper we extend those studies to include constraints on the one loop couplings of the Higgs to gluons and photons. These couplings are particularly sensitive to the existence of new colored particles that are hard to detect otherwise and we use them to constrain a 2HDM augmented with a color-octet scalar, a possibility motivated by minimal flavor violation. We first study theoretical constraints on this model and then compare them with LHC measurements.Comment: 23 pages, 10 figures; Matched the publication versio
Two Higgs doublet models augmented by a scalar color octet
two higgs doublet models augmented by a scalar color octet
studying couplings boson physics. fits couplings perspective constraining doublet extend couplings gluons photons. couplings colored detect constrain augmented octet motivated flavor violation. pages matched publication versio
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42700244
10.1007/JHEP09(2016)080
Natural realisations of supersymmetry require light stops ${\tilde t}_1$, making them a prime target of LHC searches for physics beyond the Standard Model. Depending on the kinematic region, the main search channels are ${\tilde t_1}\to t \tilde \chi^0_1$, ${\tilde t_1}\to W b \tilde \chi^0_1$ and ${\tilde t_1}\to c \tilde \chi^0_1$. We first examine the interplay of these decay modes with ${\tilde c_1}\to c \tilde \chi^0_1$ in a model-independent fashion, revealing the existence of large regions in parameter space which are excluded for any ${\tilde t_1}\to c \tilde \chi^0_1$ branching ratio. This effect is then illustrated for scenarios with stop-scharm mixing in the right-handed sector, where it has previously been observed that the stop mass limits can be significantly weakened for large mixing. Our analysis shows that once the LHC bounds from ${\tilde c_1}\to c \tilde \chi^0_1$ searches are taken into account, non-zero stop-scharm mixing leads only to a modest increase in the allowed regions of parameter space, with large areas excluded for arbitrary mixing angles.Comment: 19 pages, 9 figure
Stop searches in flavourful supersymmetry
stop searches in flavourful supersymmetry
realisations supersymmetry stops tilde prime searches model. kinematic tilde tilde tilde tilde tilde tilde examine interplay tilde tilde fashion revealing excluded tilde tilde branching ratio. illustrated scenarios stop scharm handed stop weakened mixing. bounds tilde tilde searches stop scharm modest excluded pages
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42704536
10.1007/JHEP09(2016)082
We have investigated the motion of timelike particles along geodesic in the background of accelerating and rotating black hole spacetime. We confirmed that the chaos exists in the geodesic motion of the particles by Poincar\'e sections, the power spectrum, the fast Lyapunov exponent indicator and the bifurcation diagram. Moreover, we probe the effects of the acceleration and rotation parameters on the chaotic behavior of a timelike geodesic particle in the black hole spacetime. Our results show that the acceleration brings richer physics for the geodesic motion of particles.Comment: 20 pages, 12 figures, Accepted by JHEP for publicatio
Chaotic motion of particles in the accelerating and rotating black holes spacetime
chaotic motion of particles in the accelerating and rotating black holes spacetime
timelike geodesic accelerating rotating spacetime. confirmed chaos geodesic poincar lyapunov exponent indicator bifurcation diagram. acceleration chaotic timelike geodesic spacetime. acceleration brings richer geodesic pages jhep publicatio
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42686021
10.1007/JHEP09(2016)083
The observable epsilon_K is sensitive to flavor violation at some of the highest scales. While its experimental uncertainty is at the half percent level, the theoretical one is in the ballpark of 15%. We explore the nontrivial dependence of the theory prediction and uncertainty on various conventions, like the phase of the kaon fields. In particular, we show how such a rephasing allows to make the short-distance contribution of the box diagram with two charm quarks, eta_cc, purely real. Our results allow to slightly reduce the total theoretical uncertainty of epsilon_K, while increasing the relative impact of the imaginary part of the long distance contribution, underlining the need to compute it reliably. We also give updated bounds on the new physics operators that contribute to epsilon_K.Comment: 18 pages, 6 tables, 1 figure. v2: version accepted for publication on JHEP. v3: typos corrected, all results unchange
A new look at the theory uncertainty of epsilon_K
a new look at the theory uncertainty of epsilon_k
observable epsilon flavor violation scales. percent ballpark explore nontrivial conventions kaon fields. rephasing charm quarks purely real. epsilon imaginary underlining reliably. updated bounds pages tables figure. publication jhep. typos corrected unchange
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42747057
10.1007/JHEP09(2016)084
We explore the potential for the discovery of a dilaton $\mathcal{O}(200-500)$ GeV in a classical scale/conformal invariant extension of the Standard Model by investigating the size of the corresponding breaking scale $\Lambda$ at the LHC, extending a previous analysis. In particular, we address the recent bounds on $\Lambda$ derived from Higgs boson searches. We investigate if such a dilaton can be produced via gluon-gluon fusion, presenting rates for its decay either into a pair of Higgs bosons or into two heavy gauge bosons, which can give rise to multi-leptonic final states. A detailed analysis via PYTHIA-FastJet has been carried out of the dominant Standard Model backgrounds, at a centre of mass energy of 14 TeV. We show that early data of $\sim 20$ fb$^{-1}$ can certainly probe the region of parameter space where such a dilaton is allowed. A conformal scale of 5 TeV is allowed by the current data, for almost all values of the dilaton mass investigated.Comment: 26 pages, 37 figures and 7 tables, corrected final version to appear on JHE
Bounds on the Conformal Scale of a Minimally Coupled Dilaton and Multi-Leptonic Signatures at the LHC
bounds on the conformal scale of a minimally coupled dilaton and multi-leptonic signatures at the lhc
explore discovery dilaton mathcal conformal investigating breaking lambda extending analysis. bounds lambda boson searches. dilaton gluon gluon fusion presenting bosons bosons leptonic states. pythia fastjet backgrounds tev. certainly dilaton allowed. conformal dilaton pages tables corrected
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42667084
10.1007/JHEP09(2016)085
The symmetries of string theory on ${\rm AdS}_3 \times {\rm S}^3 \times \mathbb{T}^4$ at the dual of the symmetric product orbifold point are described by a so-called Higher Spin Square (HSS). We show that the massive string spectrum in this background organises itself in terms of representations of this HSS, just as the matter in a conventional higher spin theory does so in terms of representations of the higher spin algebra. In particular, the entire untwisted sector of the orbifold can be viewed as the Fock space built out of the multiparticle states of a single representation of the HSS, the so-called `minimal' representation. The states in the twisted sector can be described in terms of tensor products of a novel family of representations that are somewhat larger than the minimal one.Comment: 34 pages; v2: typos fixe
String Theory as a Higher Spin Theory
string theory as a higher spin theory
symmetries mathbb orbifold massive organises representations representations algebra. untwisted orbifold viewed fock built multiparticle representation. twisted representations somewhat pages typos fixe
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73360566
10.1007/JHEP09(2016)086
We point out that a hypothesis of squarks and sleptons being Nambu-Goldstone (NG) bosons is consistent with pure gravity mediation or minimal split supersymmetry (SUSY). As a concrete example, we consider a SUSY $E_7/SU(5) \times U(1)^3$ non-linear sigma model in the framework of pure gravity mediation. The model accommodates three families of the quark and lepton chiral multiplets as (pseudo) NG multiplets of the Kahler manifold, which may enable us to understand the origin and number of the families. We point out that squarks in the first and second generations are likely to be as light as a few TeV if the observed baryon asymmetry is explained by the thermal leptogenesis; therefore, these colored particles can be discovered at the LHC Run-2 or at the high luminosity LHC.Comment: 18 pages, 7 figure
Nambu-Goldstone Boson Hypothesis for Squarks and Sleptons in Pure Gravity Mediation
nambu-goldstone boson hypothesis for squarks and sleptons in pure gravity mediation
squarks sleptons nambu goldstone bosons mediation split supersymmetry susy concrete susy sigma mediation. accommodates families lepton chiral multiplets pseudo multiplets kahler manifold enable families. squarks generations baryon asymmetry leptogenesis colored discovered luminosity pages
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42741006
10.1007/JHEP09(2016)087
Complex Langevin simulations allow numerical studies of theories that exhibit a sign problem, such as QCD, and are thereby potentially suitable to determine the QCD phase diagram from first principles. Here we study QCD in the limit of heavy quarks for a wide range of temperatures and chemical potentials. Our results include an analysis of the adaptive gauge cooling technique, which prevents large excursions into the non-compact directions of the SL($3, \mathbb{C}$) manifold. We find that such excursions may appear spontaneously and change the statistical distribution of physical observables, which leads to disagreement with known results. Results whose excursions are sufficiently small are used to map the boundary line between confined and deconfined quark phases.Comment: 18 pages, 10 figures, accepted for publication in JHE
The QCD phase diagram in the limit of heavy quarks using complex Langevin dynamics
the qcd phase diagram in the limit of heavy quarks using complex langevin dynamics
langevin exhibit thereby potentially principles. quarks potentials. adaptive cooling prevents excursions directions mathbb manifold. excursions spontaneously observables disagreement results. excursions sufficiently confined deconfined pages publication
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42740603
10.1007/JHEP09(2016)088
We propose a geometric method to study the residual symmetries in $N=2$, $d=4$ $\text{U}(1)$ Fayet-Iliopoulos (FI) gauged supergravity. It essentially involves the stabilization of the symplectic vector of gauge couplings (FI parameters) under the action of the U-duality symmetry of the ungauged theory. In particular we are interested in those transformations that act non-trivially on the solutions and produce scalar hair and dyonic black holes from a given seed. We illustrate the procedure for finding this group in general and then show how it works in some specific models. For the prepotential $F=-iX^0X^1$, we use our method to add one more parameter to the rotating Chow-Comp\`ere solution, representing scalar hair.Comment: 31 pages, uses jheppub.sty. Final version to appear on JHE
Duality invariance in Fayet-Iliopoulos gauged supergravity
duality invariance in fayet-iliopoulos gauged supergravity
propose geometric residual symmetries fayet iliopoulos gauged supergravity. essentially involves stabilization symplectic couplings duality ungauged theory. interested transformations trivially hair dyonic holes seed. illustrate models. prepotential rotating chow comp representing pages jheppub.sty.
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42707200
10.1007/JHEP09(2016)090
We investigate quantum phase transitions in a 2+1 dimensional gauge theory at finite chemical potential $\chi$ and magnetic field $B$. The gravity dual is based on 4D $\mathcal{N}=2$ Fayet-Iliopoulos gauged supergravity and the solutions we consider---that are constructed analytically---are extremal, dyonic, asymptotically $AdS_4$ black-branes with a nontrivial radial profile for the scalar field. We discover a line of second order fixed points at $B=B_c(\chi)$ between the dyonic black brane and an extremal "thermal gas" solution with a singularity of good-type, according to the acceptability criteria of Gubser [1]. The dual field theory is the ABJM theory [2] deformed by a triple trace operator $\Phi^3$ and placed at finite charge and magnetic field. This line of fixed points might be useful in studying the various strongly interacting quantum critical phenomena such as the ones proposed to underlie the cuprate superconductors. We also find curious similarities between the behaviour of the VeV $\langle \Phi \rangle$ under B and that of the quark condensate in 2+1 dimensional NJL models.Comment: 33 pages, 7 figure
A magnetically induced quantum phase transition in holography
a magnetically induced quantum phase transition in holography
mathcal fayet iliopoulos gauged supergravity analytically extremal dyonic asymptotically branes nontrivial field. discover dyonic brane extremal singularity acceptability gubser abjm deformed triple trace placed field. studying interacting phenomena underlie cuprate superconductors. curious similarities langle rangle condensate pages
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42715273
10.1007/JHEP09(2016)091
We present the calculation of the master integrals needed for the two-loop QCDxEW corrections to $ q + \bar{q} \to l^- + l^+$ and $ q + \bar{q}' \to l^- + \overline{\nu} \, , $ for massless external particles. We treat W and Z bosons as degenerate in mass. We identify three types of diagrams, according to the presence of massive internal lines: the no-mass type, the one-mass type, and the two-mass type, where all massive propagators, when occurring, contain the same mass value. We find a basis of 49 master integrals and evaluate them with the method of the differential equations. The Magnus exponential is employed to choose a set of master integrals that obeys a canonical system of differential equations. Boundary conditions are found either by matching the solutions onto simpler integrals in special kinematic configurations, or by requiring the regularity of the solution at pseudo-thresholds. The canonical master integrals are finally given as Taylor series around d=4 space-time dimensions, up to order four, with coefficients given in terms of iterated integrals, respectively up to weight four.Comment: 1+45 pages, 6 figures, 1 table, 5 ancillary file
Two-Loop Master Integrals for the mixed EW-QCD virtual corrections to Drell-Yan scattering
two-loop master integrals for the mixed ew-qcd virtual corrections to drell-yan scattering
master integrals qcdxew overline massless particles. treat bosons degenerate mass. diagrams massive massive propagators occurring value. master integrals equations. magnus exponential master integrals obeys canonical equations. matching simpler integrals kinematic configurations requiring regularity pseudo thresholds. canonical master integrals taylor iterated integrals pages ancillary file
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42697960
10.1007/JHEP09(2016)092
We construct effective field theories for gapped quantum Hall systems coupled to background geometries with local Galilean invariance i.e. Bargmann spacetimes. Along with an electromagnetic field, these backgrounds include the effects of curved Galilean spacetimes, including torsion and a gravitational field, allowing us to study charge, energy, stress and mass currents within a unified framework. A shift symmetry specific to single constituent theories constraints the effective action to couple to an effective background gauge field and spin connection that is solved for by a self-consistent equation, providing a manifestly covariant extension of Hoyos and Son's improvement terms to arbitrary order in $m$.Comment: v2: updated version published in JHEP; v1: 25 pages + Appendi
Covariant effective action for a Galilean invariant quantum Hall system
covariant effective action for a galilean invariant quantum hall system
gapped hall geometries galilean invariance i.e. bargmann spacetimes. electromagnetic backgrounds curved galilean spacetimes torsion gravitational allowing currents unified framework. constituent couple connection solved manifestly covariant hoyos .comment updated jhep pages appendi
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42702017
10.1007/JHEP09(2016)093
Large mass splittings between new scalars in two-Higgs-doublet models (2HDM) open a key avenue to search for these new states via exotic heavy Higgs decays. We discuss in detail the different search channels for these new scalars at the LHC in the presence of a sizable mass splitting, i.e. a hierarchical 2HDM scenario, taking into account the theoretical and experimental constraints. We provide benchmark planes to exploit the complementarity among these searches, analyzing their potential to probe the hierarchical 2HDM parameter space during LHC Run 2
Anatomy of Exotic Higgs Decays in 2HDM
anatomy of exotic higgs decays in 2hdm
splittings scalars doublet avenue exotic decays. scalars sizable splitting i.e. hierarchical constraints. benchmark planes exploit complementarity searches analyzing hierarchical
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73347338
10.1007/JHEP09(2016)094
We prove that the scattering equation formalism for Yang-Mills amplitudes can be used to make manifest the theory's color-kinematics duality. This is achieved through a concrete reduction algorithm which renders this duality manifest term-by-term. The reduction follows from the recently derived set of identities for amplitudes expressed in the scattering equation formalism that are analogous to monodromy relations in string theory. A byproduct of our algorithm is a generalization of the identities among gravity and Yang-Mills amplitudes.Comment: 20 pages, 20 figure
Manifesting Color-Kinematics Duality in the Scattering Equation Formalism
manifesting color-kinematics duality in the scattering equation formalism
formalism mills amplitudes manifest kinematics duality. concrete renders duality manifest term. identities amplitudes formalism analogous monodromy theory. byproduct generalization identities mills pages
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42752596
10.1007/JHEP09(2016)095
We discuss in detail level/rank duality in three-dimensional Chern-Simons theories and various related dualities in three-dimensional Chern-Simons-matter theories. We couple the dual Lagrangians to appropriate background fields (including gauge fields, spin$_c$ connections and the metric). The non-trivial maps between the currents and the line operators in the dual theories is accounted for by mixing of these fields. In order for the duality to be valid we must add finite counterterms depending on these background fields. This analysis allows us to resolve a number of puzzles with these dualities, to provide derivations of some of them, and to find new consistency conditions and relations between them. In addition, we find new level/rank dualities of topological Chern-Simons theories and new dualities of Chern-Simons-matter theories, including new boson/boson and fermion/fermion dualities.Comment: 36 pages, clarifications about the fixed point with several flavor
Level/rank Duality and Chern-Simons-Matter Theories
level/rank duality and chern-simons-matter theories
duality chern simons dualities chern simons theories. couple lagrangians connections trivial currents accounted fields. duality valid counterterms fields. resolve puzzles dualities derivations consistency them. dualities topological chern simons dualities chern simons boson boson fermion fermion pages clarifications flavor
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42657143
10.1007/JHEP09(2016)096
Dark matter may be coupled to dark radiation: light degrees of freedom that mediate forces between dark sector particles. Cosmological constraints favor dark radiation that is colder than Standard Model radiation. In models with fixed couplings between dark matter and the Standard Model, these constraints can be difficult to satisfy if thermal equilibrium is assumed in the early universe. We construct a model of asymmetric reheating of the visible and dark sectors from late decays of a long-lived particle (for instance, a modulus). We show, as a proof-of-principle, that such a model can populate a sufficiently cold dark sector while also generating baryon and dark matter asymmetries through the out of equilibrium decay. We frame much of our discussion in terms of the scenario of dissipative dark matter, as in the Double-Disk Dark Matter scenario. However, our results may also be of interest for other scenarios like the Twin Higgs model that are in danger of overproducing dark radiation due to nonnegligible dark-visible couplings.Comment: v2: accepted by JHEP; added discussion of baryon violation constraints, some correction
Nonthermal production of dark radiation and dark matter
nonthermal production of dark radiation and dark matter
freedom mediate forces particles. cosmological favor colder radiation. couplings satisfy universe. asymmetric reheating visible sectors decays lived modulus populate sufficiently cold generating baryon asymmetries decay. dissipative scenario. scenarios twin danger overproducing nonnegligible visible jhep baryon violation
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73352937
10.1007/JHEP09(2016)098
We perform several tests on a recent proposal by Shifman and Stepanyantz for an exact expression for the current correlation functions in supersymmetric gauge theories. We clarify the meaning of the relation in superconformal theories. In particular we show that it automatically follows from known relations between the current correlation functions and anomalies. It therefore also automatically matches between different dual realizations of the same superconformal theory. We use holographic examples as well as calculations in free theories to show that the proposed relation fails in theories with mass terms.Comment: 13 page
Supersymmetric Adler Functions and Holography
supersymmetric adler functions and holography
proposal shifman stepanyantz supersymmetric theories. clarify meaning superconformal theories. automatically anomalies. automatically matches realizations superconformal theory. holographic fails
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42694691
10.1007/JHEP09(2016)099
The analytic continuation from the Euclidean domain to real space of the one-particle irreducible quantum effective action is discussed in the context of generalized local equilibrium states. Discontinuous terms associated with dissipative behavior are parametrized in terms of a conveniently defined sign operator. A generalized variational principle is then formulated, which allows to obtain causal and real dissipative equations of motion from the analytically continued quantum effective action. Differential equations derived from the implications of general covariance determine the space-time evolution of the temperature and fluid velocity fields and allow for a discussion of entropy production including a local form of the second law of thermodynamics.Comment: 34 pages, improved discussion of dissipative terms in energy momentum tensor, references adde
Variational principle for theories with dissipation from analytic continuation
variational principle for theories with dissipation from analytic continuation
analytic continuation euclidean irreducible states. discontinuous dissipative parametrized conveniently operator. variational formulated causal dissipative analytically continued action. covariance pages dissipative adde
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42750842
10.1007/JHEP09(2016)100
We prove that non-extremal black holes in four-dimensional general relativity exhibit an infinite-dimensional symmetry in their near horizon region. By prescribing a physically sensible set of boundary conditions at the horizon, we derive the algebra of asymptotic Killing vectors, which is shown to be infinite-dimensional and includes, in particular, two sets of supertranslations and two mutually commuting copies of the Virasoro algebra. We define the surface charges associated to the asymptotic diffeomorphisms that preserve the boundary conditions and discuss the subtleties of this definition, such as the integrability conditions and the correct definition of the Dirac brackets. When evaluated on the stationary solutions, the only non-vanishing charges are the zero-modes. One of them reproduces the Bekenstein-Hawking entropy of Kerr black holes. We also study the extremal limit, recovering the NHEK geometry. In this singular case, where the algebra of charges and the integrability conditions get modified, we find that the computation of the zero-modes correctly reproduces the black hole entropy. Furthermore, we analyze the case of three spacetime dimensions, in which the integrability conditions notably simplify and the field equations can be solved analytically to produce a family of exact solutions that realize the boundary conditions explicitly. We examine other features, such as the form of the algebra in the extremal limit and the relation to other works in the literature.Comment: 24 pages, minor correction
Extended Symmetries at the Black Hole Horizon
extended symmetries at the black hole horizon
extremal holes relativity exhibit infinite horizon region. prescribing physically sensible horizon derive asymptotic killing infinite supertranslations mutually commuting copies virasoro algebra. charges asymptotic diffeomorphisms preserve subtleties integrability dirac brackets. stationary vanishing charges modes. reproduces bekenstein hawking kerr holes. extremal recovering nhek geometry. singular charges integrability correctly reproduces entropy. analyze spacetime integrability notably simplify solved analytically realize explicitly. examine extremal pages minor
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42689267
10.1007/JHEP09(2016)101
We re-examine a closed-string model defined by altering the boundary conditions for one handedness of two-dimensional propagators in otherwise-standard string theory. We evaluate the amplitudes using Kawai-Lewellen-Tye factorization into open-string amplitudes. The only modification to standard string theory is effectively that the spacetime Minkowski metric changes overall sign in one open-string factor. This cancels all but a finite number of states: As found in earlier approaches, with enough supersymmetry (e.g., type II) the tree amplitudes reproduce those of the massless truncation of ordinary string theory. However, we now find for the other cases that additional fields, formerly thought to be auxiliary, describe new spin-2 states at the two adjacent mass levels (tachyonic and tardyonic). The tachyon is always a ghost, but can be avoided in the heterotic case.Comment: v2: minor corrections; discussion section modified; more references adde
Factorization of Chiral String Amplitudes
factorization of chiral string amplitudes
examine altering handedness propagators theory. amplitudes kawai lewellen factorization amplitudes. modification effectively spacetime minkowski factor. cancels supersymmetry e.g. amplitudes reproduce massless truncation ordinary theory. formerly thought auxiliary adjacent tachyonic tardyonic tachyon ghost avoided heterotic minor adde
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42673972
10.1007/JHEP09(2016)102
We consider the problem of defining localized subsystems in gauge theory and gravity. Such systems are associated to spacelike hypersurfaces with boundaries and provide the natural setting for studying entanglement entropy of regions of space. We present a general formalism to associate a gauge-invariant classical phase space to a spatial slice with boundary by introducing new degrees of freedom on the boundary. In Yang-Mills theory the new degrees of freedom are a choice of gauge on the boundary, transformations of which are generated by the normal component of the nonabelian electric field. In general relativity the new degrees of freedom are the location of a codimension-2 surface and a choice of conformal normal frame. These degrees of freedom transform under a group of surface symmetries, consisting of diffeomorphisms of the codimension-2 boundary, and position-dependent linear deformations of its normal plane. We find the observables which generate these symmetries, consisting of the conformal normal metric and curvature of the normal connection. We discuss the implications for the problem of defining entanglement entropy in quantum gravity. Our work suggests that the Bekenstein-Hawking entropy may arise from the different ways of gluing together two partial Cauchy surfaces at a cross-section of the horizon.Comment: 46 pages. v2: Error corrected in appendix B, results unchange
Local subsystems in gauge theory and gravity
local subsystems in gauge theory and gravity
defining localized subsystems gravity. spacelike hypersurfaces boundaries studying entanglement space. formalism associate slice introducing freedom boundary. mills freedom transformations nonabelian field. relativity freedom codimension conformal frame. freedom transform symmetries consisting diffeomorphisms codimension deformations plane. observables symmetries consisting conformal curvature connection. defining entanglement gravity. bekenstein hawking arise ways gluing cauchy pages. corrected unchange
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42752441
10.1007/JHEP09(2016)103
Melnikov's method is an analytical way to show the existence of classical chaos generated by a Smale horseshoe. It is a powerful technique, though its applicability is somewhat limited. In this paper, we present a solution of type IIB supergravity to which Melnikov's method is applicable. This is a brane-wave type deformation of the AdS$_5\times$S$^5$ background. By employing two reduction ans\"atze, we study two types of coupled pendulum-oscillator systems. Then the Melnikov function is computed for each of the systems by following the standard way of Holmes and Marsden and the existence of chaos is shown analytically.Comment: 37 pages, 5 figure
Melnikov's method in String Theory
melnikov's method in string theory
melnikov chaos smale horseshoe. powerful applicability somewhat limited. supergravity melnikov applicable. brane deformation background. employing atze pendulum oscillator systems. melnikov holmes marsden chaos pages
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42725786
10.1007/JHEP09(2016)104
We consider a class of topological defects in $(1,1)$-dimensions with a deformed $\phi^4$ kink structure whose stability analysis leads to a Schr\"odinger-like equation with a zero-mode and at least one vibrational (shape) mode. We are interested in the dynamics of kink-antikink collisions, focusing on the structure of two-bounce windows. For small deformation and for one or two vibrational modes, the observed two-bounce windows are explained by the standard mechanism of a resonant effect between the first vibrational and the translational modes. With the increasing of the deformation, the effect of the appearance of more than one vibrational mode is the gradual disappearance of the initial two-bounce windows. The total suppression of two-bounce windows even with the presence of a vibrational mode offers a counterexample from what expected from the standard mechanism. For even larger deformation, some two-bounce windows reappear, but with a non-standard structure.Comment: 13 pages, 6 figure
Suppression of two-bounce windows in kink-antikink collisions
suppression of two-bounce windows in kink-antikink collisions
topological defects deformed kink schr odinger vibrational mode. interested kink antikink collisions focusing bounce windows. deformation vibrational bounce windows resonant vibrational translational modes. deformation appearance vibrational gradual disappearance bounce windows. suppression bounce windows vibrational offers counterexample mechanism. deformation bounce windows reappear pages
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42702949
10.1007/JHEP09(2016)105
We present exact large N calculus of four point function in general Chern-Simons bosonic and fermionic vector models. Applying the LSZ formula to the four point function we determine two body scattering amplitudes in these theories taking a special care for a non-analytic term to achieve unitarity in the singlet channel. We show that the S-matrix enjoys the bosonization duality, unusual crossing relation and non-relativistic reduction to Aharonov-Bohm scattering. We also argue that the S-matrix develops a pole in a certain range of coupling constants, which disappears in the range where the theory reduces to Chern-Simons theory interacting with free fermions.Comment: 1+28 pages, 5 figures, v2: minor correction
Scattering Amplitude and Bosonization Duality in General Chern-Simons Vector Models
scattering amplitude and bosonization duality in general chern-simons vector models
calculus chern simons bosonic fermionic models. amplitudes analytic unitarity singlet channel. enjoys bosonization duality unusual crossing relativistic aharonov bohm scattering. argue develops pole disappears reduces chern simons interacting pages minor
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73350977
10.1007/JHEP09(2016)106
We present for the first time a ghost-free higher-derivative chiral model with a propagating auxiliary F-term field (highest component of the chiral multiplet). We obtain this model by removing a ghost in a higher derivative chiral model, with Higgsing it in terms of an auxiliary vector superfield. Depending on the sign of the quadratic derivative term of the chiral superfield, the model contains two ghost free branches of the parameter regions. We find that supersymmetry is spontaneously broken in one branch while it is preserved in the other branch. As a consequence of dynamical F-term field, a conserved U(1) charge corresponding to the number density of $F$ appears, which can be regarded as a generalization of the R-symmetry.Comment: 15 pages, v2:references adde
Ghostbusters in higher derivative supersymmetric theories: who is afraid of propagating auxiliary fields?
ghostbusters in higher derivative supersymmetric theories: who is afraid of propagating auxiliary fields?
ghost chiral propagating auxiliary chiral multiplet removing ghost chiral higgsing auxiliary superfield. quadratic chiral superfield ghost branches regions. supersymmetry spontaneously broken branch preserved branch. conserved regarded generalization pages adde
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42747624
10.1007/JHEP09(2016)110
The presence of non-unitary neutrino mixing can affect the measurement of the three-neutrino leptonic Dirac CP phase and hamper efforts to probe CP violation due to degeneracies of the extra non-unitary CP phase with the standard CP phase. We study the effect of including non-unitarity on probing CP violation with the long-baseline experiments NO$\nu$A, T2K and DUNE. We analyze the effect of non-unitary mixing at the level of oscillation probabilities associated with the relevant baselines, and present the CP violation sensitivity for the individual experiments and their combination. Our results show that there is an improvement in the CP violation sensitivity of the combination compared to the individual experiments.Comment: 22 pages, 9 figure
Probing CP violation with T2K, NO$\nu$A and DUNE in the presence of non-unitarity
probing cp violation with t2k, no$\nu$a and dune in the presence of non-unitarity
unitary leptonic dirac hamper efforts violation degeneracies extra unitary phase. unitarity probing violation dune. analyze unitary oscillation probabilities baselines violation combination. violation pages
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42723334
10.1007/JHEP09(2016)111
We investigate the possibility of gauge coupling unification in various radiative neutrino mass models, which generate neutrino masses at one- and/or two-loop level. Renormalization group running of gauge couplings is performed analytically and numerically at one- and two-loop order, respectively. We study three different classes of neutrino mass models: (I) minimal ultraviolet completions of the dimension-7 $\Delta L=2$ operators which generate neutrino masses at one- and/or two-loop level without and with dark matter candidates, (II) models with dark matter which lead to neutrino masses at one-loop level and (III) models with particles in the adjoint representation of $\mathrm{SU}(3)$. In class (I), gauge couplings unify in a few models and adding dark matter amplifies the chances for unification. In class (II), about a quarter of the models admit gauge coupling unification. In class (III), none of the models leads to gauge coupling unification. Regarding the scale of unification, we find values between $10^{14}$ GeV and $10^{16}$ GeV for models belonging to class (I) without dark matter, whereas models in class (I) with dark matter as well as models of class (II) prefer values in the range $5 \cdot 10^{10}-5 \cdot 10^{14}$ GeV.Comment: 28 pages, 2 figures. Updated to match journal versio
Unification of Gauge Couplings in Radiative Neutrino Mass Models
unification of gauge couplings in radiative neutrino mass models
unification radiative level. renormalization running couplings analytically numerically respectively. ultraviolet completions delta candidates adjoint mathrm couplings unify adding amplifies chances unification. quarter admit unification. none unification. unification belonging prefer cdot cdot pages figures. updated match versio
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42738251
10.1007/JHEP09(2016)112
We evaluate in the framework of QCD factorization the two-loop vertex corrections to the decays $\bar{B}_{(s)}\to D_{(s)}^{(\ast)+} \, L^-$ and $\Lambda_b \to \Lambda_c^+ \, L^-$, where $L$ is a light meson from the set $\{\pi,\rho,K^{(\ast)},a_1\}$. These decays are paradigms of the QCD factorization approach since only the colour-allowed tree amplitude contributes at leading power. Hence they are sensitive to the size of power corrections once their leading-power perturbative expansion is under control. Here we compute the two-loop ${\cal O}(\alpha_s^2)$ correction to the leading-power hard scattering kernels, and give the results for the convoluted kernels almost completely analytically. Our newly computed contribution amounts to a positive shift of the magnitude of the tree amplitude by $\sim 2$\%. We then perform an extensive phenomenological analysis to NNLO in QCD factorization, using the most recent values for non-perturbative input parameters. Given the fact that the NNLO perturbative correction and updated values for form factors increase the theory prediction for branching ratios, while experimental central values have at the same time decreased, we reanalyze the role and potential size of power corrections by means of appropriately chosen ratios of decay channels.Comment: 38 pages, 5 tables, 4 figures. v2: Added explicit numbers for semi-leptonic rates that enter the factorization test, plus a few more minor adjustments. Matches version accepted by JHE
Two-body non-leptonic heavy-to-heavy decays at NNLO in QCD factorization
two-body non-leptonic heavy-to-heavy decays at nnlo in qcd factorization
factorization decays lambda lambda meson decays paradigms factorization colour contributes power. perturbative control. alpha kernels convoluted kernels analytically. newly amounts extensive phenomenological nnlo factorization perturbative parameters. nnlo perturbative updated branching reanalyze appropriately pages tables figures. leptonic enter factorization minor adjustments. matches
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73350218
10.1007/JHEP09(2016)113
This paper contains some new results on the hadronic light-by-light contribution (HLbL) to the muon $g-2$. The first part argues that we can expect large effects from disconnected diagrams in present and future calculations by lattice QCD of HLbL. The argument is based on the dominance of pseudo-scalar meson exchange. In the second part, we revisit the pion loop HLbL contribution to the muon anomalous magnetic moment. We study it in the framework of some models studied earlier, pure pion loop, full VMD and hidden local symmetry for inclusion of vector mesons. In addition we study possible ways to include the axial-vector meson. The main part of the work is a detailed study of how the different momentum regions contribute. We derive a short distance constraint on the $\gamma^*\gamma^*\to\pi\pi$ amplitude and use this as a constraint on the models used for the pion loop. As a byproduct we present the general result for integration using the Gegenbauer polynomial method.Comment: 26 page
Pion light-by-light contributions to the muon $g-2$
pion light-by-light contributions to the muon $g-2$
hadronic hlbl muon argues disconnected diagrams hlbl. argument dominance pseudo meson exchange. revisit pion hlbl muon anomalous moment. pion hidden inclusion mesons. ways axial meson. contribute. derive gamma gamma pion loop. byproduct gegenbauer
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42752491
10.1007/JHEP09(2016)115
We present a consistent renormalization scheme for the CP-conserving Two-Higgs-Doublet Model based on $\overline{MS}$ renormalization of the mixing angles and the soft-$Z_2$-symmetry-breaking scale $M_{sb}$ in the Higgs sector. This scheme requires to treat tadpoles fully consistently in all steps of the calculation in order to provide gauge-independent $S$-matrix elements. We show how bare physical parameters have to be defined and verify the gauge independence of physical quantities by explicit calculations in a general $R_{\xi}$-gauge. The procedure is straightforward and applicable to other models with extended Higgs sectors. In contrast to the proposed scheme, the $\overline{MS}$ renormalization of the mixing angles combined with popular on-shell renormalization schemes gives rise to gauge-dependent results already at the one-loop level. We present explicit results for electroweak NLO corrections to selected processes in the appropriately renormalized Two-Higgs-Doublet Model and in particular discuss their scale dependence.Comment: 52 pages, PDFLaTeX, PDF figures, JHEP version with Eq. (5.23) correcte
Gauge-independent $\overline{MS}$ renormalization in the 2HDM
gauge-independent $\overline{ms}$ renormalization in the 2hdm
renormalization conserving doublet overline renormalization angles breaking sector. treat tadpoles consistently elements. bare verify independence quantities gauge. straightforward applicable sectors. overline renormalization angles popular renormalization schemes level. electroweak appropriately renormalized doublet pages pdflatex jhep correcte
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42678982
10.1007/JHEP09(2016)116
We study the properties of 4d N=3 superconformal field theories whose rank is one, i.e. those that reduce to a single vector multiplet on their moduli space of vacua. We find that the moduli space can only be of the form C^3/Z_k for k=1,2,3,4,6, and that the supersymmetry automatically enhances to N=4 for k=1,2. In addition, we determine the central charges a and c in terms of k, and construct the associated 2d chiral algebras, which turn out to be exotic N=2 supersymmetric W-algebras.Comment: 24 page
On 4d rank-one N=3 superconformal field theories
on 4d rank-one n=3 superconformal field theories
superconformal i.e. multiplet moduli vacua. moduli supersymmetry automatically enhances charges chiral algebras exotic supersymmetric
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42738849
10.1007/JHEP09(2016)117
We consider an $O(N)$ scalar field model with quartic interaction in $d$-dimensional Euclidean de Sitter space. In order to avoid the problems of the standard perturbative calculations for light and massless fields, we generalize to the $O(N)$ theory a systematic method introduced previously for a single field, which treats the zero modes exactly and the nonzero modes perturbatively. We compute the two-point functions taking into account not only the leading infrared contribution, coming from the self-interaction of the zero modes, but also corrections due to the interaction of the ultraviolet modes. For the model defined in the corresponding Lorentzian de Sitter spacetime, we obtain the two-point functions by analytical continuation. We point out that a partial resummation of the leading secular terms (which necessarily involves nonzero modes) is required to obtain a decay at large distances for massless fields. We implement this resummation along with a systematic double expansion in an effective coupling constant $\sqrt\lambda$ and in 1/N. We explicitly perform the calculation up to the next-to-next-to-leading order in $\sqrt\lambda$ and up to next-to-leading order in 1/N. The results reduce to those known in the leading infrared approximation. We also show that they coincide with the ones obtained directly in Lorentzian de Sitter spacetime in the large N limit, provided the same renormalization scheme is used.Comment: 31 pages, 5 figures. Minor changes. Published versio
$O(N)$ model in Euclidean de Sitter space: beyond the leading infrared approximation
$o(n)$ model in euclidean de sitter space: beyond the leading infrared approximation
quartic euclidean sitter space. avoid perturbative massless generalize treats nonzero perturbatively. infrared coming ultraviolet modes. lorentzian sitter spacetime continuation. resummation secular necessarily involves nonzero distances massless fields. implement resummation sqrt lambda explicitly sqrt lambda infrared approximation. coincide lorentzian sitter spacetime renormalization pages figures. minor changes. versio
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73352007
10.1007/JHEP09(2016)118
The anomalies recently found by the LHCb collaboration in $B$-meson decays seem to point towards the existence of new physics coupled non-universally to muons and electrons. We show that a beyond-the-Standard-Model dynamics with these features naturally arises in models with a warped extra-dimension that aim to solve the electroweak Hierarchy Problem. The attractiveness of our set-up is the fact that the dynamics responsible for generating the flavor anomalies is automatically present, being provided by the massive Kaluza--Klein excitations of the electroweak gauge bosons. The flavor anomalies can be easily reproduced by assuming that the bottom and muon fields have a sizable amount of compositeness, while the electron is almost elementary. Interestingly enough, this framework correlates the flavor anomalies to a pattern of corrections in the electroweak observables and in flavor-changing processes. In particular the deviations in the bottom and muon couplings to the $Z$-boson and in $\Delta F = 2$ flavor-changing observables are predicted to be close to the present experimental bounds, and thus potentially testable in near-future experiments.Comment: 33 pages, 14 figures, 1 table. References adde
A Natural origin for the LHCb anomalies
a natural origin for the lhcb anomalies
anomalies lhcb meson decays seem universally muons electrons. naturally arises warped extra solve electroweak hierarchy problem. attractiveness generating flavor anomalies automatically massive kaluza klein excitations electroweak bosons. flavor anomalies reproduced muon sizable compositeness elementary. interestingly correlates flavor anomalies electroweak observables flavor changing processes. deviations muon couplings boson delta flavor changing observables bounds potentially testable pages table. adde
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42746804
10.1007/JHEP09(2016)119
We study possible string theory compactifications which, in the low-energy limit, describe chaotic inflation with a stabilizer field. We first analyze type IIA setups where the inflationary potential arises from a D6-brane wrapping an internal three-cycle, and where the stabilizer field is either an open-string or bulk K\"ahler modulus. We find that after integrating out the relevant closed-string moduli consistently, tachyonic directions arise during inflation which cannot be lifted. This is ultimately due to the shift symmetries of the type IIA K\"ahler potential at large compactification volume. This motivates us to search for stabilizer candidates in the complex structure sector of type IIB orientifolds, since these fields couple to D7-brane Wilson lines and their shift symmetries are generically broken away from the large complex structure limit. However, we find that in these setups the challenge is to obtain the necessary hierarchy between the inflationary and Kaluza-Klein scales.Comment: 26 pages, typos corrected and comments added. Published versio
Challenges for D-brane large-field inflation with stabilizer fields
challenges for d-brane large-field inflation with stabilizer fields
compactifications chaotic inflation stabilizer field. analyze setups inflationary arises brane wrapping stabilizer ahler modulus. integrating moduli consistently tachyonic directions arise inflation lifted. ultimately symmetries ahler compactification volume. motivates stabilizer candidates orientifolds couple brane wilson symmetries generically broken away limit. setups challenge hierarchy inflationary kaluza klein pages typos corrected comments added. versio
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42706051
10.1007/JHEP09(2016)120
We study the 6d N=(0,2) superconformal field theory, which describes multiple M5-branes, on the product space S^2 x M_4, and suggest a correspondence between a 2d N=(0,2) half-twisted gauge theory on S^2 and a topological sigma-model on the four-manifold M_4. To set up this correspondence, we determine in this paper the dimensional reduction of the 6d N=(0,2) theory on a two-sphere and derive that the four-dimensional theory is a sigma-model into the moduli space of solutions to Nahm's equations, or equivalently the moduli space of k-centered SU(2) monopoles, where k is the number of M5-branes. We proceed in three steps: we reduce the 6d abelian theory to a 5d Super-Yang-Mills theory on I x M_4, with I an interval, then non-abelianize the 5d theory and finally reduce this to 4d. In the special case, when M_4 is a Hyper-Kahler manifold, we show that the dimensional reduction gives rise to a topological sigma-model based on tri-holomorphic maps. Deriving the theory on a general M_4 requires knowledge of the metric of the target space. For k=2 the target space is the Atiyah-Hitchin manifold and we twist the theory to obtain a topological sigma-model, which has both scalar fields and self-dual two-forms.Comment: 78 pages, 2 figure
M5-branes on S^2 x M_4: Nahm's Equations and 4d Topological Sigma-models
m5-branes on s^2 x m_4: nahm's equations and 4d topological sigma-models
superconformal describes branes correspondence twisted topological sigma manifold correspondence sphere derive sigma moduli nahm equivalently moduli centered monopoles branes. proceed abelian super mills abelianize hyper kahler manifold topological sigma holomorphic maps. deriving space. atiyah hitchin manifold twist topological sigma pages
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42753656
10.1007/JHEP09(2016)121
The partition function of 2d conformal field theory is a modular invariant function. It is known that the partition function of a holomorphic CFT whose central charge is a multiple of 24 is a polynomial in the Klein function. In this paper, by using the medium temperature expansion we show that every modular invariant partition function can be mapped to a holomorphic partition function whose structure can be determined similarly. We use this map to study partition function of CFTs with half-integer left and right conformal weights. We show that the corresponding left and right central charges are necessarily multiples of 4. Furthermore, the degree of degeneracy of high-energy levels can be uniquely determined in terms of the degeneracy in the low energy states.Comment: v2: 19 pages, few footnotes and a reference added, to appear in JHE
Non-chiral 2d CFT with integer energy levels
non-chiral 2d cft with integer energy levels
partition conformal modular function. partition holomorphic klein function. modular partition mapped holomorphic partition similarly. partition cfts integer conformal weights. charges necessarily multiples degeneracy uniquely degeneracy pages footnotes
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42689303
10.1007/JHEP09(2016)122
Negative magnetoresistivity is a special magnetotransport property associated with chiral anomaly in four dimensional chiral anomalous systems, which refers to the transport behavior that the DC longitudinal magnetoresistivity decreases with increasing magnetic field. We calculate the longitudinal magnetoconductivity in the presence of backreactions of the magnetic field to gravity in holographic zero charge and axial charge density systems with and without axial charge dissipation. In the absence of axial charge dissipation, we find that the quantum critical conductivity grows with increasing magnetic field when the backreaction strength is larger than a critical value, in contrast to the monotonically decreasing behavior of quantum critical conductivity in the probe limit. With axial charge dissipation, we find the negative magnetoresistivity behavior. The DC longitudinal magnetoconductivity scales as $B$ in the large magnetic field limit, which deviates from the exact $B^2$ scaling of the probe limit result. In both cases, the small frequency longitudinal magnetoconductivity still agrees with the formula obtained from the hydrodynamic linear response theory, even in the large magnetic field limit.Comment: 33 pages, 13 figures; v2, minor change, version to appear in JHE
Negative magnetoresistivity in holography
negative magnetoresistivity in holography
magnetoresistivity magnetotransport chiral anomaly chiral anomalous refers longitudinal magnetoresistivity field. longitudinal magnetoconductivity backreactions holographic axial axial dissipation. axial dissipation conductivity grows backreaction monotonically decreasing conductivity limit. axial dissipation magnetoresistivity behavior. longitudinal magnetoconductivity deviates result. longitudinal magnetoconductivity agrees hydrodynamic pages minor
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42668953
10.1007/JHEP09(2016)124
We study the first law of black hole thermodynamics in the presence of surrounding gravitational fields and argue that variations of these fields are naturally incorporated in the first law by defining gravitational tension or gravitational binding energy. We demonstrate that this notion can also be applied in Anti-de Sitter spacetime, in which the surrounding gravitational field is sourced by a cosmological fluid, therefore showing that spacetime volume and gravitational tension encode the same physics as spacetime pressure and black hole volume. We furthermore show that it is possible to introduce a definition of spacetime pressure and black hole volume for any spacetime with characteristic length scales which does not necessarily require a cosmological constant sourcing Einstein equations. However, we show that black hole volume is non-universal in the flat spacetime limit, questioning its significance. We illustrate these ideas by studying the resulting black hole volume of Kaluza-Klein black holes and of a toy model for a black hole binary system in five spacetime dimensions (the black saturn solution) as well as of several novel perturbative black hole solutions. These include the higher-dimensional Kerr-Newman solution in Anti-de Sitter spacetime as well as other black holes in plane wave and Lifshitz spacetimes.Comment: v3: 42pp, improved discussion in section 6, to be published in JHE
Gravitational Tension, Spacetime Pressure and Black Hole Volume
gravitational tension, spacetime pressure and black hole volume
thermodynamics surrounding gravitational argue naturally incorporated defining gravitational tension gravitational energy. notion sitter spacetime surrounding gravitational sourced cosmological spacetime gravitational tension encode spacetime volume. spacetime spacetime necessarily cosmological sourcing einstein equations. universal spacetime questioning significance. illustrate ideas studying kaluza klein holes spacetime saturn perturbative solutions. kerr newman sitter spacetime holes lifshitz
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42751296
10.1007/JHEP09(2016)125
We study instanton corrections to the vacuum expectation value (VEV) of 1/6 BPS Wilson loops in ABJM theory from the Fermi gas approach. We mainly consider Wilson loops in the fundamental representation and winding Wilson loops, but we also initiate the study of Wilson loops with two boundaries. We find that the membrane instanton corrections to the Wilson loop VEV are determined by the refined topological string in the Nekrasov-Shatashvili limit, and the pole cancellation mechanism between membrane instantons and worldsheet instantons works also in the Wilson loop VEVs as in the case of the partition functions.Comment: 40 pages, 12 figure
Instanton Corrections of 1/6 BPS Wilson Loops in ABJM Theory
instanton corrections of 1/6 bps wilson loops in abjm theory
instanton expectation wilson loops abjm fermi approach. wilson loops winding wilson loops initiate wilson loops boundaries. instanton wilson refined topological nekrasov shatashvili pole cancellation instantons worldsheet instantons wilson vevs partition pages
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73351251
10.1007/JHEP09(2016)126
We consider the simplest realization of leptogenesis with one heavy Majorana neutrino species much lighter than the other ones. In this scenario, when the temperature of the early universe is smaller than the lightest Majorana neutrino mass, we compute at first order in the Standard Model couplings and, for each coupling, at leading order in the termperature the CP asymmetry in the decays of the lightest neutrino into leptons and anti-leptons. We perform the calculation using a hierarchy of two effective field theories organized as expansions in the inverse of the heavy-neutrino masses. In the ultimate effective field theory, leading thermal corrections proportional to the Higgs self coupling and the gauge couplings are encoded in one single operator of dimension five, whereas corrections proportional to the top Yukawa coupling are encoded in four operators of dimension seven, which we compute.Comment: 34 pages, 23 figure
CP asymmetry in heavy Majorana neutrino decays at finite temperature: the hierarchical case
cp asymmetry in heavy majorana neutrino decays at finite temperature: the hierarchical case
simplest realization leptogenesis majorana lighter ones. universe lightest majorana couplings termperature asymmetry decays lightest leptons leptons. hierarchy organized expansions masses. ultimate couplings encoded yukawa encoded seven pages
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29560084
10.1007/JHEP09(2016)127
We construct a class of codimension-2 solutions in supergravity that realize T-folds with arbitrary $O(2,2,\mathbb{Z})$ monodromy and we develop a geometric point of view in which the monodromy is identified with a product of Dehn twists of an auxiliary surface $\Sigma$ fibered on a base $\mathcal{B}$. These defects, that we call T-fects, are identified by the monodromy of the mapping torus obtained by fibering $\Sigma$ over the boundary of a small disk encircling a degeneration. We determine all possible local geometries by solving the corresponding Cauchy-Riemann equations, that imply the equations of motion for a semi-flat metric ansatz. We discuss the relation with the F-theoretic approach and we consider a generalization to the T-duality group of the heterotic theory with a Wilson line.Comment: 60 pages, 12 figure
The monodromy of T-folds and T-fects
the monodromy of t-folds and t-fects
codimension supergravity realize folds mathbb monodromy geometric monodromy dehn twists auxiliary sigma fibered mathcal defects call fects monodromy torus fibering sigma encircling degeneration. geometries solving cauchy riemann imply ansatz. theoretic generalization duality heterotic wilson pages
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73347944
10.1007/JHEP09(2016)128
We compute entanglement entropy for free massive scalar fields in anti-de Sitter (AdS) space. The entangling surface is a minimal surface whose boundary is a sphere at the boundary of AdS. The entropy can be evaluated from the thermal free energy of the fields on a topological black hole by using the replica method. In odd-dimensional AdS, exact expressions of the Renyi entropy $S_n$ are obtained for arbitrary $n$. We also evaluate 1-loop corrections coming from the scalar fields to holographic entanglement entropy. Applying the results, we compute the leading difference of entanglement entropy between two holographic CFTs related by a renormalization group flow triggered by a double trace deformation. The difference is proportional to the shift of a central charge under the flow.Comment: v3: 25 pages, 2 figures, typos correcte
Entanglement entropy for free scalar fields in AdS
entanglement entropy for free scalar fields in ads
entanglement massive sitter space. entangling sphere ads. topological replica method. expressions renyi coming holographic entanglement entropy. entanglement holographic cfts renormalization triggered trace deformation. pages typos correcte
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42721208
10.1007/JHEP09(2016)130
Bulk localized excited states in an AdS spacetime can be constructed from Ishibashi states with respect to the global conformal symmetry in the dual CFT. We study boundary two point functions of primary operators in the presence of bulk localized excitations in two dimensional CFTs. From two point functions in holographic CFTs, we observe causal propagations of radiations when the mass of dual bulk scalar field is close to the BF bound. This behavior for holographic CFTs is consistent with the locality and causality in classical gravity duals. We also show that this cannot be seen in free fermion CFTs. Moreover, we find that the short distance behavior of two point functions is universal and obeys the relation which generalizes the first law of entanglement entropy.Comment: 23pages, Late
Causal Evolutions of Bulk Local Excitations from CFT
causal evolutions of bulk local excitations from cft
localized excited spacetime ishibashi conformal cft. localized excitations cfts. holographic cfts causal propagations radiations bound. holographic cfts locality causality duals. fermion cfts. universal obeys generalizes entanglement pages
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42733261
10.1007/JHEP09(2016)132
A number of phenomenologically relevant processes at hadron colliders, such as Higgs and Z boson production in association with b quarks, can be conveniently described as scattering of heavy quarks in the initial state. We present a detailed analysis of this class of processes, identifying the form of the leading initial-state collinear logarithms that allow the relation of calculations performed in different flavour schemes in a simple and reliable way. This procedure makes it possible to assess the size of the logarithmically enhanced terms and the effects of their resummation via heavy-quark parton distribution functions. As an application, we compare the production of (SM-like and heavy) scalar and vector bosons in association with b quarks at the LHC in the four- and five-flavour schemes as well as the production of a heavy Z' in association with top quarks at a future 100 TeV hadron collider in the five- and six-flavour schemes. We find that, in agreement with a previous analysis of single heavy-quark initiated processes, the size of the initial-state logarithms is mitigated by a kinematical suppression. The most important effects of the resummation are a shift of the central predictions typically of about 20% at a justified value of the scale of each considered process and a significant reduction of scale variation uncertainties.Comment: 27 pages, 12 figure
Anatomy of double heavy-quark initiated processes
anatomy of double heavy-quark initiated processes
phenomenologically hadron colliders boson quarks conveniently quarks state. identifying collinear logarithms flavour schemes reliable way. logarithmically resummation parton functions. bosons quarks flavour schemes quarks hadron collider flavour schemes. initiated logarithms mitigated kinematical suppression. resummation justified pages
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42735193
10.1007/JHEP09(2016)133
The evaluation of generic Cachazo-He-Yuan(CHY)-integrands is a big challenge and efficient computational methods are in demand for practical evaluation. In this paper, we propose a systematic decomposition algorithm by using cross-ratio identities, which provides an analytic and easy to implement method for the evaluation of any CHY-integrand. This algorithm aims to decompose a given CHY-integrand containing higher-order poles as a linear combination of CHY-integrands with only simple poles in a finite number of steps, which ultimately can be trivially evaluated by integration rules of simple poles. To make the method even more efficient for CHY-integrands with large number of particles and complicated higher-order pole structures, we combine the $\Lambda$-algorithm and the cross-ratio identities, and as a by-product it provides us a way to deal with CHY-integrands where the $\Lambda$-algorithm was not applicable in its original formulation.Comment: 37 pages, 6 figures, v2 references update
Cross-ratio Identities and Higher-order Poles of CHY-integrand
cross-ratio identities and higher-order poles of chy-integrand
generic cachazo yuan integrands challenge practical evaluation. propose decomposition identities analytic implement integrand. aims decompose integrand poles integrands poles ultimately trivially poles. integrands complicated pole combine lambda identities deal integrands lambda applicable pages update
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42720262
10.1007/JHEP09(2016)134
This paper is a new step in the project of systematic description of colored knot polynomials started in arXiv:1506.00339. In this paper, we managed to explicitly find the inclusive Racah matrix, i.e. the whole set of mixing matrices in channels R^3->Q with all possible Q, for R=[3,1]. The calculation is made possible by the use of a newly-developed efficient highest-weight method, still it remains tedious. The result allows one to evaluate and investigate [3,1]-colored polynomials for arbitrary 3-strand knots, and this confirms many previous conjectures on various factorizations, universality, and differential expansions. We consider in some detail the next-to-twist-knots three-strand family (n,-1|1,-1) and deduce its colored HOMFLY. Also confirmed and clarified is the eigenvalue hypothesis for the Racah matrices, which promises to provide a shortcut to generic formulas for arbitrary representations.Comment: 21 page
HOMFLY polynomials in representation [3,1] for 3-strand braids
homfly polynomials in representation [3,1] for 3-strand braids
colored knot polynomials started managed explicitly inclusive racah i.e. newly tedious. colored polynomials strand knots confirms conjectures factorizations universality expansions. twist knots strand deduce colored homfly. confirmed clarified eigenvalue racah promises shortcut generic formulas
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42741464
10.1007/JHEP09(2016)135
Continuing the quest for exclusive Racah matrices, which are needed for evaluation of colored arborescent-knot polynomials in Chern-Simons theory, we suggest to extract them from a new kind of a double-evolution -- that of the antiparallel double-braids, which is a simple two-parametric family of two-bridge knots, generalizing the one-parametric family of twist knots. In the case of rectangular representations $R=[r^s]$ we found an evidence that the corresponding differential expansion miraculously factorizes and can be obtained from that for the twist knots. This reduces the problem of rectangular exclusive Racah to constructing the answers for just a few twist knots. We develop a recent conjecture on the structure of differential expansion for the simplest members of this family (the trefoil and the figure-eight knot) and provide the exhaustive answer for the first unknown case of $R=[33]$. The answer includes HOMFLY of arbitrary twist and double-braid knots and Racah matrices $\bar S$ and $S$ -- what allows to calculate $[33]$-colored polynomials for arbitrary arborescent (double-fat) knots. For generic rectangular representations described in detail are only the contributions of the single- and two-floor pyramids, the way to proceed is explicitly illustrated by the examples of $R=[44]$ and $R=[55]$. This solves the difficult part of the problem, but the last tedious step towards explicit formulas for generic exclusive rectangular Racah matrices still remains to be made.Comment: 32 page
Factorization of differential expansion for antiparallel double-braid knots
factorization of differential expansion for antiparallel double-braid knots
continuing quest exclusive racah colored arborescent knot polynomials chern simons extract kind antiparallel braids parametric bridge knots generalizing parametric twist knots. rectangular representations miraculously factorizes twist knots. reduces rectangular exclusive racah constructing answers twist knots. conjecture simplest trefoil eight knot exhaustive answer unknown answer homfly twist braid knots racah colored polynomials arborescent knots. generic rectangular representations floor pyramids proceed explicitly illustrated solves tedious formulas generic exclusive rectangular racah
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73347783
10.1007/JHEP09(2016)137
We explore some aspects of three-dimensional higher-spin holography by studying scalar fluctuations in the background of higher-spin black holes. We furnish an independent derivation of the bulk-boundary propagator by purely invoking a well-known infinite dimensional matrix representation of $hs[\lambda]$ algebra related to its construction as a quotient of the universal enveloping algebra of $sl(2)$, thus evading the need in previous literature to perform an analytic continuation from some integer to $\lambda$. The propagator and the boundary two-point functions are derived for black hole solutions in $hs[\lambda]\times hs[\lambda]$ Chern-Simons theory with spin-3 and spin-4 charges up to second-order in the potentials. We match them with three- and four-point torus correlation functions of the putative dual conformal field theory which has $\mathcal{W}_\infty [\lambda]$ symmetry and is deformed by higher-spin currents.Comment: 27 pages. v3: references adde
On scalar propagators of three-dimensional higher-spin black holes
on scalar propagators of three-dimensional higher-spin black holes
explore holography studying holes. furnish derivation propagator purely invoking infinite lambda quotient universal enveloping evading analytic continuation integer lambda propagator lambda lambda chern simons charges potentials. match torus putative conformal mathcal infty lambda deformed pages. adde
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42731766
10.1007/JHEP09(2016)139
The replica trick defines Renyi entropies as partition functions on conically singular geometries. We discuss their gravity duals: regular bulk solutions to the Einstein equations inducing conically singular metrics at the boundary. When the conical singularity is supported on a flat or spherical surface, these solutions are rewritings of the hyperbolic black hole. For more general shapes, these solutions are new. We construct them perturbatively in a double expansion in the distance and strength of the conical singularity, and extract the vacuum polarisation due to the cone. Recent results about the structure of logarithmic divergences of Renyi entropies are reproduced ---in particular, $f_b\neq f_c$. We discuss in detail the dynamical resolution of the singularity in the bulk. This resolution is in agreement with a previous proposal, and indicates a non-minimal settling to the `splitting problem': an apparent ambiguity in the holographic entropy formula of certain theories with higher derivatives.Comment: v3: 31 pages. Typos corrected and some clarifications. Matches publishe
Gravity duals of boundary cones
gravity duals of boundary cones
replica trick defines renyi entropies partition conically singular geometries. duals einstein inducing conically singular metrics boundary. conical singularity spherical rewritings hyperbolic hole. shapes new. perturbatively conical singularity extract polarisation cone. logarithmic divergences renyi entropies reproduced singularity bulk. proposal settling splitting apparent ambiguity holographic pages. typos corrected clarifications. matches publishe
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29511404
10.1007/JHEP09(2016)140
Recent astronomical observations show that the universe may be anisotropic on large scales. The Union2 SnIa data hint that the universe has a preferred direction. If such a cosmological privileged axis indeed exists, one has to consider an anisotropic expanding Universe instead of the isotropic cosmological model. In this paper, we present a detailed analysis of the dark energy dipole in $f(R,T)=f_{1}(R)+f_{2}(T)$ Cosmological Model using three types of dipole fit (DF) method which are (I)dipole + monopole fitting for distance modulus(DMFDM), (II)dipole + monopole fitting for luminosity distance(DMFLD) and (III) general dipole fitting for luminosity distance(GDFLD). We have found the maximum anisotropic deviation direction for (DMFDM) method as $(l, b)=(315^{+25}_{-25},-23^{+14}_{-15})$, for (DMFLD) as $(l, b)=(l, b)=(315^{+35}_{-37},-23^{+18}_{-18})$, and for (GDFLD) method as $(l, b)=(317^{+32}_{-32},-23^{+18}_{-18})$ which are located very close to each other. We compare our model with the $CPL$, $\Lambda CDM$ and $\omega CDM$ models. Constraints on $(l, b)$ in $f(R, T)$ model are not much different from the cases of the $CPL$, $\Lambda CDM$ and $\omega CDM$ models. Moreover, the results are consistent with other studies.Comment: 40 page 25 fig. arXiv admin note. arXiv admin note: text overlap with arXiv:1303.0961, arXiv:1302.1866, arXiv:1411.1466, arXiv:1107.5807, arXiv:1306.3164 by other author
Searching for a Cosmological Preferred Axis in complicated class of cosmological models:Case study $f(R,T)$ model
searching for a cosmological preferred axis in complicated class of cosmological models:case study $f(r,t)$ model
astronomical universe anisotropic scales. union snia hint universe preferred direction. cosmological privileged anisotropic expanding universe isotropic cosmological model. dipole cosmological dipole dipole monopole fitting modulus dmfdm dipole monopole fitting luminosity dmfld dipole fitting luminosity gdfld anisotropic dmfdm dmfld gdfld other. lambda omega models. lambda omega models. fig. admin note. admin overlap
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73356073
10.1007/JHEP09(2016)141
In four dimensions, partially massless fields of all spins and depths possess a duality invariance akin to electric-magnetic duality. We construct metric-like gauge invariant curvature tensors for partially massless fields of all integer spins and depths, and show how the partially massless equations of motion can be recovered from first order field equations and Bianchi identities for these curvatures. This formulation displays duality in its manifestly local and covariant form, in which it acts to interchange the field equations and Bianchi identities.Comment: 46 pages, 1 figur
Manifest Duality for Partially Massless Higher Spins
manifest duality for partially massless higher spins
partially massless spins depths possess duality invariance akin duality. curvature tensors partially massless integer spins depths partially massless recovered bianchi identities curvatures. formulation displays duality manifestly covariant acts interchange bianchi pages figur
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42675274
10.1007/JHEP09(2016)142
Using black brane solutions in 5d Lifshitz-like backgrounds with arbitrary dynamical exponent $\nu$, we construct the Vaidya geometry, asymptoting to the Lifshitz-like spacetime, which represents a thin shell infalling at the speed of light. We apply the new Lifshitz-Vaidya background to study the thermalization process of the quark-gluon plasma via the thin shell approach previously successfully used in several backgrounds. We find that the thermalization depends on the chosen direction because of the spatial anisotropy. The plasma thermalizes thus faster in the transversal direction than in the longitudinal one. To probe the system described by the Lifshitz-like backgrounds, we also calculate the holographic entanglement entropy for the subsystems delineated along both transversal and longitudinal directions. We show that the entropy has some universality in the behavior for both subsystems. At the same time, we find that certain characteristics strongly depend on the critical exponent $\nu$.Comment: 39 pages, 23 figures; v3: typos corrected, references and clarifications added, version published in JHE
Analytic black branes in Lifshitz-like backgrounds and thermalization
analytic black branes in lifshitz-like backgrounds and thermalization
brane lifshitz backgrounds exponent vaidya asymptoting lifshitz spacetime infalling light. lifshitz vaidya thermalization gluon successfully backgrounds. thermalization anisotropy. thermalizes faster transversal longitudinal one. lifshitz backgrounds holographic entanglement subsystems delineated transversal longitudinal directions. universality subsystems. exponent .comment pages typos corrected clarifications
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42724897
10.1007/JHEP09(2016)143
The 2-Higgs-Doublet Model (2HDM) belongs to the simplest extensions of the Standard Model (SM) Higgs sector that are in accordance with theoretical and experimental constraints. In order to be able to properly investigate the experimental Higgs data and, in the long term to distinguish between possible models beyond the SM, precise predictions for the Higgs boson observables have to be made available on the theory side. This requires the inclusion of the higher order corrections. In this work, we investigate in detail the renormalization of the 2HDM, a pre-requisite for the computation of higher order corrections. We pay particular attention to the renormalization of the mixing angles $\alpha$ and $\beta$, which diagonalize the Higgs mass matrices and which enter all Higgs observables. The implications of various renormalization schemes in next-to-leading order corrections to the sample processes $H^\pm \to W^\pm h/H$ and $H \to ZZ$ are investigated. Based on our findings, we will present a renormalization scheme that is at the same time process independent, gauge independent and numerically stable
Gauge-independent Renormalization of the 2-Higgs-Doublet Model
gauge-independent renormalization of the 2-higgs-doublet model
doublet belongs simplest extensions accordance constraints. properly distinguish precise boson observables side. inclusion corrections. renormalization requisite corrections. renormalization angles alpha beta diagonalize enter observables. renormalization schemes investigated. renormalization numerically
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42737254
10.1007/JHEP09(2016)144
In this paper, we show that a higher derivative theory, such as New Massive Gravity, allows the existence of new entangling surfaces with non-zero extrinsic curvature. We perform the analysis for Lifshitz and Warped $AdS$ space times, revealing the role of the higher derivative contributions in the calculation of the holographic entanglement entropy. Finally, as an outcome of our holographic analysis we briefly comment on the dual boundary theory.Comment: 23 pages, 1 figure. v3: published versio
Holographic Entanglement Entropy in NMG
holographic entanglement entropy in nmg
massive entangling extrinsic curvature. lifshitz warped revealing holographic entanglement entropy. holographic briefly comment pages figure. versio
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42750541
10.1007/JHEP09(2016)145
We consider a truncation of type IIB supergravity on four-torus where in addition to the Ramond-Ramond 2-form field, the Ramond-Ramond axion (w) and the NS-NS 2-form field (B) are also retained. In the (w, B) sector we construct a linearised perturbation carrying only left moving momentum on two-charge non-extremal D1-D5 geometries of Jejjala, Madden, Ross and Titchener. The perturbation is found to be smooth everywhere and normalizable. It is constructed by matching to leading order solutions of the perturbation equations in the inner and outer regions of the geometry.Comment: 24 pages, no figures; v2: footnotes added; v3: JHEP version; v4: results unchanged, app B removed, a footnote added, supersedes published versio
Hair on non-extremal D1-D5 bound states
hair on non-extremal d1-d5 bound states
truncation supergravity torus ramond ramond ramond ramond axion retained. linearised perturbation carrying moving extremal geometries jejjala madden ross titchener. perturbation everywhere normalizable. matching perturbation outer pages footnotes jhep unchanged removed footnote supersedes versio
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42663274
10.1007/JHEP09(2016)146
The assumption of anarchic quark flavor puts serious stress on composite Higgs models: flavor bounds imply a tuning of a few per-mille (at best) in the Higgs potential. Composite twin Higgs (CTH) models significantly reduce this tension by opening up a new region of parameter space, obtained by raising the coupling among the composites close to the strong coupling limit $g_* \sim 4\pi$, thereby raising the scale of composites to around 10 TeV. This does not lead to large tuning in the Higgs potential since the leading quantum corrections are canceled by the twin partners (rather than the composites). We survey the leading flavor bounds on the CTH, which correspond to tree-level $\Delta F=2$ four-Fermi operators from Kaluza-Klein (KK) Z exchange in the kaon system and 1-loop corrections from KK fermions to the electric dipole moment of the neutron. We provide a parametric estimate for these bounds and also perform a numeric scan of the parameter space using the complete calculation for both quantities. The results confirm our expectation that CTH models accommodate anarchic flavor significantly better than regular composite Higgs (CH) models. Our conclusions apply both to the identical and fraternal twin cases.Comment: 35 pages, 9 figure
The Flavor of the Composite Twin Higgs
the flavor of the composite twin higgs
anarchic flavor puts serious composite flavor bounds imply tuning mille potential. composite twin tension opening raising composites thereby raising composites tev. tuning canceled twin partners composites flavor bounds delta fermi kaluza klein kaon fermions dipole moment neutron. parametric bounds numeric scan quantities. confirm expectation accommodate anarchic flavor composite models. fraternal twin pages
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73355724
10.1007/JHEP09(2016)147
The observation of neutrino masses, mixing and the existence of dark matter are amongst the most important signatures of physics beyond the Standard Model (SM). In this paper, we propose to extend the SM by a local $L_\mu - L_\tau$ gauge symmetry, two additional complex scalars and three right-handed neutrinos. The $L_\mu - L_\tau$ gauge symmetry is broken spontaneously when one of the scalars acquires a vacuum expectation value. The $L_\mu - L_\tau$ gauge symmetry is known to be anomaly free and can explain the beyond SM measurement of the anomalous muon $({\rm g-2})$ through additional contribution arising from the extra $Z_{\mu\tau}$ mediated diagram. Small neutrino masses are explained naturally through the Type-I seesaw mechanism, while the mixing angles are predicted to be in their observed ranges due to the broken $L_\mu-L_\tau$ symmetry. The second complex scalar is shown to be stable and becomes the dark matter candidate in our model. We show that while the $Z_{\mu\tau}$ portal is ineffective for the parameters needed to explain the anomalous muon $({\rm g-2})$ data, the correct dark matter relic abundance can easily be obtained from annihilation through the Higgs portal. Annihilation of the scalar dark matter in our model can also explain the Galactic Centre gamma ray excess observed by Fermi-LAT. We show the predictions of our model for future direct detection experiments and neutrino oscillation experiments.Comment: 33 pages, 12 figures, 3 Tables, Version accepted for publication in JHE
Neutrino Mass, Dark Matter and Anomalous Magnetic Moment of Muon in a $U(1)_{L_{\mu}-L_{\tau}}$ Model
neutrino mass, dark matter and anomalous magnetic moment of muon in a $u(1)_{l_{\mu}-l_{\tau}}$ model
amongst signatures propose extend scalars handed neutrinos. broken spontaneously scalars acquires expectation value. anomaly anomalous muon arising extra diagram. naturally seesaw angles ranges broken symmetry. candidate model. portal ineffective anomalous muon relic abundance annihilation portal. annihilation galactic gamma excess fermi lat. oscillation pages tables publication
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42739831
10.1007/JHEP09(2016)148
We consider Abelian tensor hierarchy in four-dimensional ${\cal N}=1$ supergravity in the conformal superspace formalism, where the so-called covariant approach is used to antisymmetric tensor fields. We introduce $p$-form gauge superfields as superforms in the conformal superspace. We solve the Bianchi identities under the constraints for the superforms. As a result, each of form fields is expressed by a single gauge invariant superfield. The action of superforms is shown with the invariant superfields. We also show the relation between the superspace formalism and the superconformal tensor calculus.Comment: 31 page
Abelian tensor hierarchy in 4D ${\cal N}=1$ conformal supergravity
abelian tensor hierarchy in 4d ${\cal n}=1$ conformal supergravity
abelian hierarchy supergravity conformal superspace formalism covariant antisymmetric fields. superfields superforms conformal superspace. solve bianchi identities superforms. superfield. superforms superfields. superspace formalism superconformal
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42686707
10.1007/JHEP09(2016)149
We explore a new class of natural models which ensure the one-loop divergences in the Higgs mass are cancelled. The top-partners that cancel the top loop are new gauge bosons, and the symmetry relation that ensures the cancellation arises at an infrared fixed point. Such a cancellation mechanism can, a la Little Higgs models, push the scale of new physics that completely solves the hierarchy problem up to 5-10 TeV. When embedded in a supersymmetric model, the stop and gaugino masses provide the cutoffs for the loops, and the mechanism ensures a cancellation between the stop and gaugino mass dependence of the Higgs mass parameter.Comment: 15 pages, 3 figure
Little Conformal Symmetry
little conformal symmetry
explore ensure divergences cancelled. partners cancel bosons ensures cancellation arises infrared point. cancellation push solves hierarchy tev. embedded supersymmetric stop gaugino cutoffs loops ensures cancellation stop gaugino pages
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42682291
10.1007/JHEP09(2016)150
We present a supersymmetric version of a two-field relaxion model that naturalizes tuned versions of supersymmetry. This arises from a relaxion mechanism that does not depend on QCD dynamics and where the relaxion potential barrier height is controlled by a second axion-like field. During the cosmological evolution, the relaxion rolls with a nonzero value that breaks supersymmetry and scans the soft supersymmetric mass terms. Electroweak symmetry is broken after the soft masses become of order the supersymmetric Higgs mass term and causes the relaxion to stop rolling for superpartner masses up to $\sim 10^9$ GeV. This can explain the tuning in supersymmetric models, including split-SUSY models, while preserving the QCD axion solution to the strong CP problem. Besides predicting two very weakly-coupled axion-like particles, the supersymmetric spectrum may contain an extra Goldstino, which could be a viable dark matter candidate.Comment: 33 pages, 3 figures; v2: bounds and figures correcte
Naturalizing Supersymmetry with a Two-Field Relaxion Mechanism
naturalizing supersymmetry with a two-field relaxion mechanism
supersymmetric relaxion naturalizes tuned versions supersymmetry. arises relaxion relaxion barrier axion field. cosmological relaxion rolls nonzero breaks supersymmetry scans supersymmetric terms. electroweak broken supersymmetric relaxion stop rolling superpartner gev. tuning supersymmetric split susy preserving axion problem. besides predicting weakly axion supersymmetric extra goldstino viable pages bounds correcte
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42704356
10.1007/JHEP09(2016)154
Recently, two groups have made distinct proposals for a de Sitter space that is emergent from conformal field theory (CFT). The first proposal is that, for two-dimensional holographic CFTs, the kinematic space of geodesics on a spacelike slice of the asymptotically anti-de Sitter bulk is two-dimensional de Sitter space (dS$_2$), with a metric that can be derived from the entanglement entropy of intervals in the CFT. In the second proposal, de Sitter dynamics emerges naturally from the first law of entanglement entropy for perturbations around the vacuum state of CFTs. We provide support for the equivalence of these two emergent spacetimes in the vacuum case and beyond. In particular, we study the kinematic spaces of nontrivial solutions of $3$d gravity, including the BTZ black string, BTZ black hole, and conical singularities. We argue that the resulting spaces are generically globally hyperbolic spacetimes that support dynamics given boundary conditions at future infinity. For the BTZ black string, corresponding to a thermal state of the CFT, we show that both prescriptions lead to an emergent hyperbolic patch of dS$_2$. We offer a general method for relating kinematic space and the auxiliary de Sitter space that is valid in the vacuum and thermal cases.Comment: 46 pages, 20 figures; v2: typos fixed, minor clarifications, added analysis of entanglement entropy phase transitions in Sections 2.4, 2.5 and
Equivalence of Emergent de Sitter Spaces from Conformal Field Theory
equivalence of emergent de sitter spaces from conformal field theory
proposals sitter emergent conformal proposal holographic cfts kinematic geodesics spacelike slice asymptotically sitter sitter entanglement intervals cft. proposal sitter emerges naturally entanglement perturbations cfts. equivalence emergent spacetimes beyond. kinematic nontrivial conical singularities. argue generically globally hyperbolic spacetimes infinity. prescriptions emergent hyperbolic patch offer relating kinematic auxiliary sitter valid pages typos minor clarifications entanglement
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42679153
10.1007/JHEP09(2016)155
In this letter, we provide evidence for universality in the low-energy expansion of tree-level string interactions. More precisely, in the alpha'-expansion of tree-level scattering amplitudes, we conjecture that the leading transcendental coefficient at each order in alpha' is universal for all perturbative string theories. We have checked this universality up to seven points and trace its origin to the ability to restructure the disk integrals of open bosonic string into those of the superstring. The accompanying kinematic functions have the same low-energy limit and do not introduce any transcendental numbers in their alpha'-corrections. Universality in the closed-string sector then follows from the KLT-relations.Comment: 5 pages, Mathematica notebook on the five-point open-string amplitude included in submissio
Universality in string interactions
universality in string interactions
letter universality interactions. precisely alpha amplitudes conjecture transcendental alpha universal perturbative theories. checked universality seven trace restructure integrals bosonic superstring. accompanying kinematic transcendental alpha corrections. universality pages mathematica notebook submissio
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42747266
10.1007/JHEP09(2016)156
We present a systematic procedure to obtain the one-loop low-energy effective Lagrangian resulting from integrating out the heavy fields of a given ultraviolet theory. We show that the matching coefficients are determined entirely by the hard region of the functional determinant involving the heavy fields. This represents an important simplification with respect the conventional matching approach, where the full and effective theory contributions have to be computed separately and a cancellation of the infrared divergent parts has to take place. We illustrate the method with a descriptive toy model and with an extension of the Standard Model with a heavy real scalar triplet. A comparison with other schemes that have been put forward recently is also provided.Comment: 24 pages. Uses feynMF packag
Integrating out heavy particles with functional methods: a simplified framework
integrating out heavy particles with functional methods: a simplified framework
lagrangian integrating ultraviolet theory. matching entirely determinant involving fields. simplification matching separately cancellation infrared divergent place. illustrate descriptive triplet. schemes pages. feynmf packag
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42742144
10.1007/JHEP09(2016)157
We calculate the double pole contribution to two to four fermion scattering through $W^{\pm}$ currents at tree level in the Standard Model Effective Field Theory (SMEFT). We assume all fermions to be massless, $\rm U(3)^5$ flavour and $\rm CP$ symmetry. Using this result, we update the global constraint picture on SMEFT parameters including LEPII data on these charged current processes, and also include modifications to our fit procedure motivated by a companion paper focused on $W^{\pm}$ mass extractions. The fit reported is now to 177 observables and emphasises the need for a consistent inclusion of theoretical errors, and a consistent treatment of observables. Including charged current data lifts the two-fold degeneracy previously encountered in LEP (and lower energy) data, and allows us to set simultaneous constraints on 20 of 53 Wilson coefficients in the SMEFT, consistent with our assumptions. This allows the model independent inclusion of LEP data in SMEFT studies at LHC, which are projected into the SMEFT in a consistent fashion. We show how stronger constraints can be obtained by using some combinations of Wilson coefficients, when making assumptions on the UV completion of the Standard Model, or in an inconsistent analysis. We explain why strong bounds at the per-mille or sub-per-mille level on some combinations of Wilson coefficients in the Effective Lagrangian can be artificially enhanced in fits of this form in detail. This explains some of the different claims present in the literature.Comment: 27 pages + appendix, 9 fig, Acknowledgement updated with grant number
Incorporating doubly resonant $W^\pm$ data in a global fit of SMEFT parameters to lift flat directions
incorporating doubly resonant $w^\pm$ data in a global fit of smeft parameters to lift flat directions
pole fermion currents smeft fermions massless flavour symmetry. update picture smeft lepii modifications motivated companion focused extractions. observables emphasises inclusion observables. lifts degeneracy encountered simultaneous wilson smeft assumptions. inclusion smeft projected smeft fashion. stronger combinations wilson assumptions completion inconsistent analysis. bounds mille mille combinations wilson lagrangian artificially fits detail. explains claims pages acknowledgement updated
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42748250
10.1007/JHEP09(2016)158
We consider scenarios of Higgs compositeness where the Higgs doublet arises as a pseudo-Nambu Goldstone boson. Our focus is the physical scalar ("radial") excitation associated with the global symmetry breaking vacuum, which we call the "global Higgs". For the minimal case of a $SO(5)/SO(4)$ coset, the couplings of the global Higgs to Standard Model (SM) particles are fully determined by group theoretical factors and two decay constants. The global Higgs also couples to the composite resonances of the theory, inducing an interaction with the SM gauge bosons at one-loop. We thoroughly analyze representative fermionic sectors, considering a global Higgs both in the $\bf 5$ and $\bf 14$ representations of $SO(5)$ and taking into account the renormalization group evolution of couplings in the composite sector. We derive the one-loop effective couplings and all decays of the global Higgs, showing that its decay width over mass can range from $ O (10^{-3})$ to $ O(1)$. Because of the multiplicity of the resonances, the coupling of the global Higgs to gluons is sizeable, potentially opening a new window into composite models at the LHC.Comment: 27 pages, 2 figures. v3: References and comments added. Matches JHEP versio
The Excitation of the Global Symmetry-Breaking Vacuum in Composite Higgs Models
the excitation of the global symmetry-breaking vacuum in composite higgs models
scenarios compositeness doublet arises pseudo nambu goldstone boson. breaking call coset couplings constants. couples composite resonances inducing bosons loop. thoroughly analyze fermionic sectors representations renormalization couplings composite sector. derive couplings decays multiplicity resonances gluons sizeable potentially opening window composite pages figures. comments added. matches jhep versio
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42738445
10.1007/JHEP09(2016)159
Applying the dispersion approach we compute perturbative QCD corrections to the power suppressed soft contribution of $B \to \gamma \ell \nu$ at leading twist. QCD factorization for the $B \to \gamma^{\ast}$ form factors is demonstrated explicitly for the hard-collinear transverse polarized photon at one loop, with the aid of the method of regions. While the one-loop hard function is identical to the matching coefficient of the QCD weak current $\bar u \, \gamma_{\mu \perp} \, (1- \gamma_5) \, b$ in soft-collinear effective theory, the jet function from integrating out the hard-collinear fluctuations differs from the corresponding one entering the factorization formula of $B \to \gamma \ell \nu$. Furthermore, we evaluate the sub-leading power contribution to the $B \to \gamma$ form factors from the three-particle $B$-meson distribution amplitudes (DAs) at tree level. The soft contribution to the $B \to \gamma$ form factors from the three-particle $B$-meson DAs is shown to be of the same power compared with the corresponding hard correction, in contrast to the two-particle counterparts. Numerically the next-to-leading-order QCD correction to the soft two-particle contribution in $B \to \gamma$ form factors will induce an approximately $\left (10 \sim 20 \right) \%$ shift to the tree-level contribution at $\lambda_B(\mu_0)=354 \, {\rm MeV}$. Albeit of power suppression parametrically, the soft two-particle correction can decrease the leading power predictions for the $B \to \gamma$ form factors by an amount of $\left (10 \sim 30 \right) \%$ with the same value of $\lambda_B(\mu_0)$. Employing the phenomenological model of the three-particle $B$-meson DAs inspired by a QCD sum rule analysis, the three-particle contribution to the $B \to \gamma$ form factors is predicted to be of ${\cal O} (1 \%)$, at leading order in $\alpha_s$, with the default theory inputs.Comment: 32 pages, 9 figure
Factorization and dispersion relations for radiative leptonic $B$ decay
factorization and dispersion relations for radiative leptonic $b$ decay
perturbative suppressed gamma twist. factorization gamma explicitly collinear polarized regions. matching gamma perp gamma collinear integrating collinear differs entering factorization gamma gamma meson amplitudes level. gamma meson counterparts. numerically gamma induce lambda albeit suppression parametrically gamma lambda employing phenomenological meson inspired gamma alpha default pages
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73349270
10.1007/JHEP09(2016)160
In this article we extend the effective field theory framework describing new physics effects to the case where the underlying low-energy theory is a Two-Higgs-Doublet model. We derive a complete set of independent operators up to dimension six assuming a $Z_2$-invariant CP-conserving Higgs potential. The effects on Higgs and gauge boson masses, mixing angles in the Higgs sector as well as couplings to fermions and gauge bosons are computed. At variance with the case of a single Higgs doublet, we find that pair production of SM-like Higgses, arising through dimension-six operators, is not fixed by fermion-fermion-Higgs couplings and can therefore be sizable.Comment: 19 pages, 8 table
Effective Field Theory with Two Higgs Doublets
effective field theory with two higgs doublets
extend describing doublet model. derive conserving potential. boson angles couplings fermions bosons computed. doublet higgses arising fermion fermion couplings pages
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42743783
10.1007/JHEP09(2016)161
Recently a Complexity-Action (CA) duality conjecture has been proposed, which relates the quantum complexity of a holographic boundary state to the action of a Wheeler-DeWitt (WDW) patch in the anti-de Sitter (AdS) bulk. In this paper we further investigate the duality conjecture for stationary AdS black holes and derive some exact results for the growth rate of action within the Wheeler-DeWitt (WDW) patch at late time approximation, which is supposed to be dual to the growth rate of quantum complexity of holographic state. Based on the results from the general $D$-dimensional Reissner-Nordstr\"{o}m (RN)-AdS black hole, rotating/charged Ba\~{n}ados-Teitelboim-Zanelli (BTZ) black hole, Kerr-AdS black hole and charged Gauss-Bonnet-AdS black hole, we present a universal formula for the action growth expressed in terms of some thermodynamical quantities associated with the outer and inner horizons of the AdS black holes. And we leave the conjecture unchanged that the stationary AdS black hole in Einstein gravity is the fastest computer in nature.Comment: v1, 10 pages, 2 figures, two columns; v2, 20 pages, 2 figures, JHEP style, references added; v3, 23 pages, 2 figures, discussions extended and references added, to be published in JHEP with title "Action Growth for AdS Black Holes
Complexity Growth for AdS Black Holes
complexity growth for ads black holes
duality conjecture relates holographic wheeler dewitt patch sitter bulk. duality conjecture stationary holes derive wheeler dewitt patch supposed holographic state. reissner nordstr rotating ados teitelboim zanelli kerr gauss bonnet universal thermodynamical quantities outer horizons holes. leave conjecture unchanged stationary einstein fastest pages columns pages jhep style pages discussions jhep title holes
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29547609
10.1007/JHEP09(2016)162
We consider a model in which dark matter is a composite baryon of a dark sector governed by $SU(3)$ gauge theory, with vector-like quarks also charged under $U(1)_Y$. The model provides simple answer to the dark matter stability problem: it is a result of the accidental dark baryon number conservation. And with an analogy to QCD, all physical quantities of the dark matter can be calculated by rescaling the QCD experimental results. According to the thermal freeze-out mechanism the mass of the dark matter is predicted to be $\mathcal{O}(100)$~TeV in order to achieve a correct relic abundance. Such heavy dark matter is in general hard for detection due to small dark matter number density in the universe. However, dark baryon number in our model is not necessarily strictly preserved thanks to operators suppressed by the Planck scale, and such decay operator results in a decay lifetime marginal to the current detection bound. We show our model with $\mathcal{O}(10^{27})~s$ dark matter decay life time can explain the AMS-02 anti-proton data, if it is experimentally interpreted as an access, although some theoretical uncertainty may weaken its significance. We also investigate other phenomena of this model such as the extragalactic gamma ray and neutrino signatures.Comment: 14 pages, 43 figures, published in JHE
A scenario of heavy but visible baryonic dark matter
a scenario of heavy but visible baryonic dark matter
composite baryon governed quarks answer accidental baryon conservation. analogy quantities rescaling results. freeze mathcal relic abundance. universe. baryon necessarily strictly preserved thanks suppressed planck lifetime marginal bound. mathcal proton experimentally interpreted weaken significance. phenomena extragalactic gamma pages
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73367430
10.1007/JHEP09(2016)163
In this note we first review the degenerate vacua arising from the BMS symmetries. According to the discussion in [1] one can define BMS-analogous supertranslation and superrotation for spacetime with black hole in Gaussian null coordinates. In the leading and subleading orders of near horizon approximation, the infinitely degenerate black hole solutions are derived by considering Einstein equations with or without cosmological constant, and they are related to each other by the diffeomorphism generated by horizon supertranslation. Higher order results and degenerate Rindler horizon solutions also are given in appendices.Comment: 21 pages,no figures, references added, match the version published in JHE
Horizon supertranslation and degenerate black hole solutions
horizon supertranslation and degenerate black hole solutions
degenerate vacua arising symmetries. analogous supertranslation superrotation spacetime coordinates. subleading orders horizon infinitely degenerate einstein cosmological diffeomorphism horizon supertranslation. degenerate rindler horizon pages match
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42729546
10.1007/JHEP09(2016)166
The open string metric arises kinematically in studying fluctuations of open string degrees of freedom on a D-brane. An observer, living on a probe D-brane, can send signals through the spacetime by using such fluctuations on the probe, that propagate in accordance with a metric which is conformal to the open string metric. Event horizons can emerge in the open string metric when one considers a D-brane with an electric field on its worldvolume. Here, we emphasize the role of and investigate, in details, the causal structure of the resulting open string event horizon and demonstrate, among other things, its close similarities to an usual black hole event horizon in asymptotically AdS-spaces. To that end, we analyze relevant geodesics, Penrose diagrams and various causal holographic observables for a given open string metric. For analytical control, most of our calculations are performed in an asymptotically AdS$_3$-background, however, we argue that the physics is qualitatively the same in higher dimensions. We also discuss how this open string metric arises from an underlying D-brane configuration in string theory.Comment: 42 pages, multiple figure
Emergent Horizons and Causal Structures in Holography
emergent horizons and causal structures in holography
arises kinematically studying freedom brane. observer living brane send spacetime propagate accordance conformal metric. horizons emerge considers brane worldvolume. emphasize causal horizon things similarities usual horizon asymptotically spaces. analyze geodesics penrose diagrams causal holographic observables metric. asymptotically argue qualitatively dimensions. arises brane pages
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