Search results for "Particles"

showing 10 items of 8085 documents

Yangian Symmetry for Fishnet Feynman Graphs

2017

Various classes of fishnet Feynman graphs are shown to feature a Yangian symmetry over the conformal algebra. We explicitly discuss scalar graphs in three, four and six spacetime dimensions as well as the inclusion of fermions in four dimensions. The Yangian symmetry results in novel differential equations for these families of largely unsolved Feynman integrals. Notably, the considered fishnet graphs in three and four dimensions dominate the correlation functions and scattering amplitudes in specific double scaling limits of planar, gamma-twisted N=4 super Yang-Mills or ABJM theory. Consequently, the study of fishnet graphs allows us to get deep insights into the integrability of the plana…

High Energy Physics - Theorydimension: 4Feynman graphScalar (mathematics)[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesConformal mapintegrability01 natural sciencesalgebra: conformal[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]symbols.namesake0103 physical sciencesFeynman diagramcorrelation function010306 general physicsABJM modelMathematical PhysicsMathematical physicsPhysicsfield theory: conformalSpacetimeAdS/CFT correspondence010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Mathematical analysisscattering amplitudescalingdifferential equationsMathematical Physics (math-ph)FermionScattering amplitudespace-time: dimension: 6AdS/CFT correspondenceHigh Energy Physics - Theory (hep-th)symmetry: Yangiansupersymmetry: 4symbols[ PHYS.MPHY ] Physics [physics]/Mathematical Physics [math-ph]Yangian
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Method to compute the stress-energy tensor for a quantized scalar field when a black hole forms from the collapse of a null shell

2020

A method is given to compute the stress-energy tensor for a massless minimally coupled scalar field in a spacetime where a black hole forms from the collapse of a spherically symmetric null shell in four dimensions. Part of the method involves matching the modes for the in vacuum state to a complete set of modes in Schwarzschild spacetime. The other part involves subtracting from the unrenormalized expression for the stress-energy tensor when the field is in the in vacuum state, the corresponding expression when the field is in the Unruh state and adding to this the renormalized stress-energy tensor for the field in the Unruh state. The method is shown to work in the two-dimensional case wh…

High Energy Physics - Theorydimension: 4space-time: SchwarzschildField (physics)Vacuum stateFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)coupling: scalarcoupling: minimal01 natural sciencesGeneral Relativity and Quantum Cosmologyrenormalizationvacuum stateGeneral Relativity and Quantum Cosmologyblack hole: formation0103 physical sciencesStress–energy tensorsymmetry: rotationTensordimension: 2010306 general physicsMathematical physicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsshell modelfield theory: scalarfield theory in curved spacegravitation: collapseBlack holeFormal aspects of field theoryUnruh effectHigh Energy Physics - Theory (hep-th)tensor: energy-momentum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]quantizationSchwarzschild radiusScalar fieldPhysical Review D
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Momentum anisotropy effects for quarkonium in a weakly coupled quark-gluon plasma below the melting temperature

2017

In the early stages of heavy-ion collisions, the hot QCD matter expands more longitudinally than transversely. This imbalance causes the system to become rapidly colder in the longitudinal direction and a local momentum anisotropy appears. In this paper, we study the heavy-quarkonium spectrum in the presence of a small plasma anisotropy. We work in the framework of pNRQCD at finite temperature. We inspect arrangements of non-relativistic and thermal scales complementary to those considered in the literature. In particular, we consider temperatures larger and Debye masses smaller than the binding energy, which is a temperature range relevant for presently running LHC experiments. In this set…

High Energy Physics - Theoryheavy ion: scatteringNuclear Theoryhiukkasfysiikka01 natural sciences7. Clean energy[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]High Energy Physics - Phenomenology (hep-ph)quarkonium: heavyquarkonium: mass spectrum[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)AnisotropyNuclear Experiment[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]quark gluon: plasmaQCD matterDebyeQuantum chromodynamicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]quarkonium: momentumQuarkoniumHigh Energy Physics - PhenomenologyQuantum electrodynamicssymbolsquarkonium[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesanisotropy[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]plasma: anisotropyNuclear Theory (nucl-th)Momentumsymbols.namesake0103 physical sciencesplasma: expansionparticle physicsquantum chromodynamics: perturbation theory010306 general physicsquantum chromodynamics: matterquantum chromodynamics: nonrelativisticta114effect: anisotropy010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPlasmamomentum: anisotropyquarkonium: dissociationHigh Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Quark–gluon plasma[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physical Review D
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Dark matter, dark photon and superfluid He-4 from effective field theory

2020

We consider a model of sub-GeV dark matter whose interaction with the Standard Model is mediated by a new vector boson (the dark photon) which couples kinetically to the photon. We describe the possibility of constraining such a model using a superfluid He-4 detector, by means of an effective theory for the description of the superfluid phonon. We find that such a detector could provide bounds that are competitive with other direct detection experiments only for ultralight vector mediator, in agreement with previous studies. As a byproduct we also present, for the first time, the low-energy effective field theory for the interaction between photons and phonons.

High Energy Physics - Theorylight dark matterNuclear and High Energy PhysicsPhotonDark matterFOS: Physical scienceshelium01 natural sciencesDark photonVector bosonStandard ModelSuperfluidityeffective theoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theory010306 general physicsphononLight dark matterPhysics010308 nuclear & particles physicslcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsdark photondark photon; effective theory; helium; light dark matter; phononlcsh:Physics
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Correlation patterns from massive phonons in 1+1 dimensional acoustic black holes: A toy model

2018

Transverse excitations in analogue black holes induce a mass like term in the longitudinal mode equation. With a simple toy model we show that correlation functions display a rather rich structure characterized by groups of parallel peaks. For the most part the structure is completely different from that found in the massless case.

High Energy Physics - TheorylongitudinalPhononOne-dimensional spacetoy modelFOS: Physical sciencesalternative theories of gravityGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLongitudinal modeGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencesexcited stateMassive phonons Hawking radiationcorrelation functionstructure010306 general physicsdimension: 2PhysicsToy model010308 nuclear & particles physicsMassless particleCorrelation function (statistical mechanics)Transverse planetransverseblack hole: acousticHigh Energy Physics - Theory (hep-th)General relativityQuantum Gases (cond-mat.quant-gas)correlation[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]phonon: massiveCondensed Matter - Quantum GasesHawking radiation
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Pseudospectrum and Black Hole Quasinormal Mode Instability

2020

We study the stability of quasinormal modes (QNM) in asymptotically flat black hole spacetimes by means of a pseudospectrum analysis. The construction of the Schwarzschild QNM pseudospectrum reveals the following: (i) the stability of the slowest-decaying QNM under perturbations respecting the asymptotic structure, reassessing the instability of the fundamental QNM discussed by Nollert [H. P. Nollert, About the Significance of Quasinormal Modes of Black Holes, Phys. Rev. D 53, 4397 (1996)] as an "infrared" effect; (ii) the instability of all overtones under small-scale ("ultraviolet") perturbations of sufficiently high frequency, which migrate towards universal QNM branches along pseudospec…

High Energy Physics - TheoryperturbationcompactificationQC1-999[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityStability (probability)General Relativity and Quantum Cosmologyoperator: spectrumGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciencesQuasinormal modestructurenumerical calculations010306 general physicsMathematical PhysicsPseudospectrumPhysicsCompactification (physics)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsPhysicsOperator (physics)black hole: stabilityMathematical Physics (math-ph)Schwarzschildquasinormal mode: spectrumBlack holeHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]spectralSchwarzschild radiusPhysical Review X
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Born–Infeld inspired modifications of gravity

2017

General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own limit of validity. In particular, the breakdown of unitarity near the Planck scale strongly suggests that General Relativity needs to be modified at high energies and quantum gravity effects are expected to be important. This is related to the existence of spacetime singularities when the solutions of General Relativity are extrapolated to regimes where curvatures are large. In this sense, Born-Infeld inspired modifications of gravity have shown an extraordin…

High Energy Physics - Theorystar: compactcosmological model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]space-time: black holeGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Gravitationquantum gravity: effectBorn–Infeld gravityPhysicsenergy: highBlack holes[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationCosmologyregularizationcurvaturewormhole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational singularitySingularitiesAstrophysics - Cosmology and Nongalactic AstrophysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityEarly universegeneral relativity: solutionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Theoretical physicsGeneral Relativity and Quantum Cosmologyspace-time: singularity0103 physical sciencesunitaritystructureWormholeinflation010306 general physicsCompact objectsSpacetime010308 nuclear & particles physicsscale: PlanckBlack holeBorn-Infeld modelHigh Energy Physics - Theory (hep-th)gravitationQuantum gravity[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Oh, wait, O8 de Sitter may be unstable!

2021

We analyze the stability of four-dimensional de Sitter vacua constructed by compactifying massive Type IIA supergravity in the presence of two O8 sources [1]. When embedded in String Theory the first source has a clear interpretation as an O8$_-$ plane, but the second one could correspond to either an O8$_+$ plane or to an O8$_-$ plane with 16 D8-branes on top. We find that this latter solution has a tachyonic instability, corresponding to the D8-branes moving away from the O8$_-$ plane. We comment on the possible ways of distinguishing between these sources.

High Energy Physics - Theoryvacuum state: de SitterNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi Matematicidimension: 4compactificationSuperstring VacuaFOS: Physical sciencesD-braneString theory01 natural sciencessupergravity: Type IIADe Sitter universeFlux compactifications0103 physical sciencesC++ string handlingBrane cosmologylcsh:Nuclear and particle physics. Atomic energy. RadioactivityD-brane010306 general physicsMathematical physicsPhysicsCompactification (physics)010308 nuclear & particles physicsPlane (geometry)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Supergravitytachyon: stabilitySuperstring Vacua D-branes Flux compactificationsHigh Energy Physics - Theory (hep-th)D-branesstringlcsh:QC770-798
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Measurement of CP asymmetry in D 0 → K - K + and D 0 → π - πdecays

2014

Time-integrated $CP$ asymmetries in $D^0$ decays to the final states $K^- K^+$ and $\pi^- \pi^+$ are measured using proton-proton collisions corresponding to $3\mathrm{\,fb}^{-1}$ of integrated luminosity collected at centre-of-mass energies of $7\mathrm{\,Te\kern -0.1em V}$ and $8\mathrm{\,Te\kern -0.1em V}$. The $D^0$ mesons are produced in semileptonic $b$-hadron decays, where the charge of the accompanying muon is used to determine the initial flavour of the charm meson. The difference in $CP$ asymmetries between the two final states is measured to be \begin{align} \Delta A_{CP} = A_{CP}(K^-K^+)-A_{CP}(\pi^-\pi^+) = (+0.14 \pm 0.16\mathrm{\,(stat)} \pm 0.08\mathrm{\,(syst)})\% \ . \nonu…

High Energy Physics::Lattice14.40.Lb01 natural sciencesLuminositySettore FIS/04 - Fisica Nucleare e SubnucleareFlavor physicsABSORPTIONPhysics::Chemical PhysicsNuclear ExperimentQCmedia_commonCharm physicsPhysicsHadronic decays of charmed mesonCharm physics; CP violation; Flavor physics; Hadron-Hadron ScatteringParticle physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronCharge conjugation parity time reversal and other discrete symmetrieFIS/01 - FISICA SPERIMENTALECP violation13.25.FtSCATTERING-AMPLITUDEFísica nuclearLHCParticle physicsCharm physicNuclear and High Energy PhysicsMesonmedia_common.quotation_subjectLHCb - Abteilung HofmannHadronsAsymmetryREGENERATIONTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYSEARCH0103 physical sciencesPiSCATTERINGSCATTERING-AMPLITUDE; REGENERATION; ABSORPTION; SEARCHSDG 7 - Affordable and Clean Energy010306 general physicsLarge Hadron Collider (France and Switzerland)/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyMuonHadron-Hadron Scattering010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGran Col·lisionador d'HadronsCharge (physics)LHCbFlavor physic11.30.ErHigh Energy Physics::ExperimentFísica de partículesExperiments13.85.NiCharmed mesons (|C|>0 B=0)FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
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Multi-boson block factorization of fermions

2017

The numerical computations of many quantities of theoretical and phenomenological interest are plagued by statistical errors which increase exponentially with the distance of the sources in the relevant correlators. Notable examples are baryon masses and matrix elements, the hadronic vacuum polarization and the light-by-light scattering contributions to the muon g-2, and the form factors of semileptonic B decays. Reliable and precise determinations of these quantities are very difficult if not impractical with state-of-the-art standard Monte Carlo integration schemes. I will review a recent proposal for factorizing the fermion determinant in lattice QCD that leads to a local action in the g…

High Energy Physics::Latticeaction: local01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Vacuum polarizationcorrelation functionQuantum Chromodynamics Lattice gauge theory Computational PhysicsMonte CarloBosonPhysicsform factorPhysicsHigh Energy Physics - Lattice (hep-lat)lattice field theoryPropagatorpropagator [quark]hep-phParticle Physics - Latticestatistical [error]Lattice QCDFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIHigh Energy Physics - Phenomenologyerror: statisticalquark: factorizationquark: propagatorMonte Carlo integrationQuarkParticle physicsQC1-999fermion: determinantdeterminant [fermion]FOS: Physical scienceshep-latbaryon: massHigh Energy Physics - LatticeFactorization0103 physical sciencesmagnetic moment [muon]hadronic [vacuum polarization]010306 general physicsnumerical calculationsParticle Physics - Phenomenologymuon: magnetic moment010308 nuclear & particles physicsvacuum polarization: hadronicHigh Energy Physics::Phenomenologyphoton photon: scatteringB: decaylocal [action]Fermiondecay [B]mass [baryon]scattering [photon photon]gauge field theoryHigh Energy Physics::Experimentfactorization [quark]
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