Search results for "hep-th"

showing 10 items of 757 documents

Holographic duals of 6d RG flows

2018

A notable class of superconformal theories (SCFTs) in six dimensions is parameterized by an integer $N$, an ADE group $G$, and two nilpotent elements $\mu_\mathrm{L,R}$ in $G$. Nilpotent elements have a natural partial ordering, which has been conjectured to coincide with the hierarchy of renormalization-group flows among the SCFTs. In this paper we test this conjecture for $G=\mathrm{SU}(k)$, where AdS$_7$ duals exist in IIA. We work with a seven-dimensional gauged supergravity, consisting of the gravity multiplet and two $\mathrm{SU}(k)$ non-Abelian vector multiplets. We show that this theory has many supersymmetric AdS$_7$ vacua, determined by two nilpotent elements, which are naturally …

High Energy Physics - TheoryNuclear and High Energy PhysicsPure mathematicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesAdS-CFT Correspondence01 natural sciencesHigh Energy Physics::Theory0103 physical sciencesSupergravity ModelField theory (psychology)lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsMultipletPhysics010308 nuclear & particles physicsGroup (mathematics)hep-thGauged supergravityAdS-CFT Correspondence Supergravity Models Superstring VacuaFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIAdS/CFT correspondenceNilpotentHigh Energy Physics - Theory (hep-th)Domain (ring theory)lcsh:QC770-798Partially ordered setSupergravity ModelsParticle Physics - TheoryJournal of High Energy Physics
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Infrared facets of the three-gluon vertex

2021

We present novel lattice results for the form factors of the quenched three-gluon vertex of QCD, in two special kinematic configurations that depend on a single momentum scale. We consider three form factors, two associated with a classical tensor structure and one without tree-level counterpart, exhibiting markedly different infrared behaviors. Specifically, while the former display the typical suppression driven by a negative logarithmic singularity at the origin, the latter saturates at a small negative constant. These exceptional features are analyzed within the Schwinger-Dyson framework, with the aid of special relations obtained from the Slavnov-Taylor identities of the theory. The em…

High Energy Physics - TheoryNuclear and High Energy PhysicsQC1-999High Energy Physics::LatticeFOS: Physical sciencesThree-gluon vertexLattice QCD01 natural sciencesMomentumTheoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)SingularitySchwinger-Dyson equations0103 physical sciencesTensor010306 general physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsPhysicsHigh Energy Physics - Lattice (hep-lat)Lattice QCDQCDHigh Energy Physics - PhenomenologyLattice (module)High Energy Physics - Theory (hep-th)Vertex (curve)Constant (mathematics)Physics Letters B
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The geometry of N=3 AdS4 in massive IIA

2018

The geometry of the ${\cal N} = 3$, SO(4)--invariant, AdS$_4$ solution of massive type IIA supergravity that uplifts from the ${\cal N} = 3 $ vacuum of $D=4$ ${\cal N} = 8$ dyonic ISO(7) supergravity is investigated. Firstly, a $D=4$, SO(4)--invariant restricted duality hierarchy is constructed and used to uplift the entire, dynamical SO(4)--invariant sector to massive type IIA. The resulting consistent uplift formulae are used to obtain a new local expression for the ${\cal N} = 3 $ AdS$_4$ solution in massive IIA and analyse its geometry. Locally, the internal $S^6$ geometry corresponds to a warped fibration of $S^2$ and a hemisphere of $S^4$. This can be regarded as a warped generalisati…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesDuality (optimization)AdS-CFT Correspondence Flux compactifications Supergravity Models Superstring VacuaGeometryType (model theory)AdS-CFT Correspondence01 natural sciencesTwistor theoryAdS-CFT correspondencesupergravity modelsFlux compactifications0103 physical sciences010306 general physicsPhysicsSpinor010308 nuclear & particles physicsPhysicsSupergravityFibrationFísicaAdS/CFT correspondenceHigh Energy Physics - Theory (hep-th)Killing spinorsuperstring vacuaflux compactificationsSupergravity Models
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Non-supersymmetric AdS6 and the swampland

2021

We discuss infinite families of non-supersymmetric AdS$_6$ solutions in Type IIB string theory. They are siblings of supersymmetric solutions which are associated with $(p,q)$ 5-brane webs and holographically dual to 5d SCFTs engineered by those brane webs. The non-supersymmetric backgrounds carry identical 5-brane charges and are connected to the supersymmetric ones by RG flows. We study the stability of the non-supersymmetric solutions, identifying perturbative and non-perturbative decay channels for all the backgrounds explicitly available. We also identify likely decay mechanisms for solutions that have not been constructed explicitly but may be expected to exist based on brane web cons…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesQC770-798domain wallAdS-CFT Correspondencestring model: Type IIB01 natural sciencesGauge-gravity correspondenceHigh Energy Physics::TheoryNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciences010306 general physicsAdS-CFT Correspondence Gauge-gravity correspondence Superstring Vacua Supersymmetry BreakingSupersymmetry Breaking[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsbubbleComputer Science::Information RetrievalAdS-CFT Correspondence; Gauge-gravity correspondence; Superstring Vacua; Supersymmetry Breakingduality: holographystabilitydecay: nonperturbativeHigh Energy Physics - Theory (hep-th)renormalization group: flowD-brane: 5spin: 2Journal of High Energy Physics
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On AdS7 stability

2019

AdS$_7$ supersymmetric solutions in type IIA have been classified, and they are infinitely many. Moreover, every such solution has a non-supersymmetric sister. In this paper, we study the perturbative and non-perturbative stability of these non-supersymmetric solutions, focusing on cases without orientifolds. Perturbatively, we first look at the KK spectrum of spin-2 excitations. This does not exhibit instabilities, but it does show that there is no separation of scales for either the BPS and the non-BPS case, thus proving for supersymmetric AdS$_7$ a well-known recent conjecture. We then use 7d gauged supergravity and a brane polarization computation to access part of the spectrum of KK sc…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi Matematicistability: nonperturbativeComputationSuperstring VacuaType (model theory)AdS-CFT Correspondence01 natural sciencesInstabilityStability (probability)orientifoldmembrane modelTheoretical physicsHigh Energy Physics::Theory0103 physical sciencesexcited stateanti-de Sitterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysicsSupersymmetry BreakingpolarizationConjecture010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thbubbleSpectrum (functional analysis)Gauged supergravityHigh Energy Physics::PhenomenologyFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIBPSlcsh:QC770-798supergravityBranesupersymmetryAdS-CFT Correspondence Superstring Vacua Supersymmetry BreakingParticle Physics - TheoryJournal of High Energy Physics
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Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics

2016

Using recently proposed method of discrete Hirota dynamics for integrable (1+1)D quantum field theories on a finite space circle of length L, we derive and test numerically a finite system of nonlinear integral equations for the exact spectrum of energies of SU(N)xSU(N) principal chiral field model as functions of m L, where m is the mass scale. We propose a determinant solution of the underlying Y-system, or Hirota equation, in terms of determinants (Wronskians) of NxN matrices parameterized by N-1 functions of the spectral parameter, with the known analytical properties at finite L. Although the method works in principle for any state, the explicit equations are written for states in the …

High Energy Physics - TheoryNuclear and High Energy PhysicsSigma modelField (physics)FOS: Physical sciences2 dimensionsrepresentation-theory01 natural sciencesexcited-state energiesnonlinear integral-equationsQuantum mechanics0103 physical sciencesBound statelcsh:Nuclear and particle physics. Atomic energy. Radioactivityvolume dependenceQuantum field theory010306 general physicsS-matrixMathematical physicsPhysics[PHYS]Physics [physics][ PHYS ] Physics [physics]010308 nuclear & particles physicsWronskiano(n) sigma-modeln phase-transitionState (functional analysis)goldstone bosonsAdS/CFT correspondenceHigh Energy Physics - Theory (hep-th)lcsh:QC770-798tba equations
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QUANTUM EFFECTS IN ACOUSTIC BLACK HOLES: THE BACKREACTION.

2004

We investigate the backreaction equations for an acoustic black hole formed in a Laval nozzle under the assumption that the motion of the fluid is one-dimensional. The solution in the near-horizon region shows that as phonons are (thermally) radiated the sonic horizon shrinks and the temperature decreases. This contrasts with the behaviour of Schwarzschild black holes, and is similar to what happens in the evaporation of (near-extremal) Reissner-Nordstrom black holes (i.e. infinite evaporation time). Finally, by appropriate boundary conditions the solution is extended in both the asymptotic regions of the nozzle.

High Energy Physics - TheoryNuclear and High Energy PhysicsSonic black holeEvent horizonWhite holeAstrophysics::High Energy Astrophysical PhenomenaHAWKINGFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black holeGeneral Relativity and Quantum CosmologyACOUSTICPhysics::Fluid DynamicsMicro black holeGeneral Relativity and Quantum CosmologyQuantum mechanicsPhysicsBLACK HOLEBACK REACTIONFLUIDCondensed Matter - Other Condensed MatterBlack holeHigh Energy Physics - Theory (hep-th)RADIATIONSchwarzschild radiusOther Condensed Matter (cond-mat.other)Hawking radiation
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Spin Glasses on Thin Graphs

1995

In a recent paper we found strong evidence from simulations that the Isingantiferromagnet on ``thin'' random graphs - Feynman diagrams - displayed amean-field spin glass transition. The intrinsic interest of considering such random graphs is that they give mean field results without long range interactions or the drawbacks, arising from boundary problems, of the Bethe lattice. In this paper we reprise the saddle point calculations for the Ising and Potts ferromagnet, antiferromagnet and spin glass on Feynman diagrams. We use standard results from bifurcation theory that enable us to treat an arbitrary number of replicas and any quenched bond distribution. We note the agreement between the f…

High Energy Physics - TheoryNuclear and High Energy PhysicsSpin glassCondensed Matter (cond-mat)FOS: Physical sciencesCondensed Matter01 natural sciencesCondensed Matter::Disordered Systems and Neural Networks010305 fluids & plasmassymbols.namesakeHigh Energy Physics - LatticeSaddle point0103 physical sciencesAntiferromagnetismFeynman diagram010306 general physicsRandom graphPhysicsBethe latticeCondensed matter physicsHigh Energy Physics - Lattice (hep-lat)Mean field theoryHigh Energy Physics - Theory (hep-th)symbolsIsing modelCondensed Matter::Strongly Correlated Electrons
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Sterile neutrinos and B–L symmetry

2017

We revisit the relation between the neutrino masses and the spontaneous breaking of the B-L gauge symmetry. We discuss the main scenarios for Dirac and Majorana neutrinos and point out two simple mechanisms for neutrino masses. In this context the neutrino masses can be generated either at tree level or at quantum level and one predicts the existence of very light sterile neutrinos with masses below the eV scale. The predictions for lepton number violating processes such as mu to e and mu to e gamma are discussed in detail. The impact from the cosmological constraints on the effective number of relativistic degree of freedom is investigated.

High Energy Physics - TheoryNuclear and High Energy PhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Computer Science::Digital Libraries01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationGauge symmetryPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999High Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Theory (hep-th)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters B
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Relations for Einstein–Yang–Mills amplitudes from the CHY representation

2017

We show that a recently discovered relation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with one graviton and $(n-1)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons, can be derived from the CHY representation. In addition we show that there is a generalisation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with $r$ gravitons and $(n-r)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons. We present a general formula for this case.

High Energy Physics - TheoryNuclear and High Energy PhysicsTrace (linear algebra)High Energy Physics::LatticeFOS: Physical sciencesYang–Mills existence and mass gap01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryQuantum mechanics0103 physical sciencesEinstein010306 general physicsLinear combinationMathematical physicsPhysicsCondensed Matter::Quantum GasesIntroduction to gauge theoryGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGravitonlcsh:QC1-999High Energy Physics - Theory (hep-th)Supersymmetric gauge theorysymbolslcsh:PhysicsPhysics Letters B
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