Search results for "hep-ph"

showing 10 items of 3327 documents

Cosmic Dark Radiation and Neutrinos

2013

New measurements of the cosmic microwave background (CMB) by the Planck mission have greatly increased our knowledge about the universe. Dark radiation, a weakly interacting component of radiation, is one of the important ingredients in our cosmological model which is testable by Planck and other observational probes. At the moment, the possible existence of dark radiation is an unsolved question. For instance, the discrepancy between the value of the Hubble constant, H-0, inferred from the Planck data and local measurements of H-0 can to some extent be alleviated by enlarging the minimal ACDM model to include additional relativistic degrees of freedom. From a fundamental physics point of v…

Big BangNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Article SubjectAge of the universeDark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesBayron acoustic-Oscillationssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Analytic approach0103 physical sciencesPlanck010306 general physicsPhysicsAstrophysics - Cosmology and Extragalactic Astrophysics010308 nuclear & particles physicsHot dark matterFísicalcsh:QC1-999High Energy Physics - Phenomenology13. Climate actionDark radiationDark energysymbolslcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsAdvances in High Energy Physics
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Spectral function for overoccupied gluodynamics from real-time lattice simulations

2018

We study the spectral properties of a highly occupied non-Abelian non-equilibrium plasma appearing ubiquitously in weak coupling descriptions of QCD matter. The spectral function of this far-from-equilibrium plasma is measured by employing linear response theory in classical-statistical real-time lattice Yang-Mills simulations. We establish the existence of transversely and longitudinally polarized quasiparticles and obtain their dispersion relations, effective mass, plasmon frequency, damping rate and further structures in the spectral and statistical functions. Our new method can be interpreted as a non-perturbative generalization of hard thermal loop (HTL) effective theory. We see indica…

CLASSICAL APPROXIMATIONNuclear Theorynucl-thquark-gluon plasmahep-latFOS: Physical sciencesHEAVY-ION COLLISIONShiukkasfysiikka114 Physical sciences01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Lattice (order)0103 physical sciencesquantum chromodynamicsQCD PLASMA INSTABILITIESStatistical physicsGauge theorynonperturbative effects in field theory010306 general physicsHARD THERMAL LOOPSParticle Physics - PhenomenologyPhysicsQuantum chromodynamicsta114010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)kvarkki-gluoniplasmafinite temperature field theorylattice field theoryISOTROPIZATIONParticle Physics - Latticehep-ph16. Peace & justiceFIELD-THEORYGluonHigh Energy Physics - PhenomenologyNuclear Physics - TheoryQuark–gluon plasmaHIGH-TEMPERATUREGAUGE-THEORIESQuasiparticleSpectral functionkvanttikenttäteoriaStatistical correlationrelativistic heavy-ion collisions
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Study of heavy meson production in p-Pb collisions at $\sqrt{S}$=5.02 TeV in the general-mass variable-flavour-number scheme

2017

Nuclear physics / B 925, 415 - 430 (2017). doi:10.1016/j.nuclphysb.2017.10.016

CMSnucleusFOS: Physical sciencesinitial-state interaction530High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)CERN LHC CollALICEproduction [bottom]heavy [meson]ddc:530High Energy Physics::Experimentcross section [p p]Nuclear Experimentnumerical calculationscharmproduction [meson]1 [higher-order]
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Correlated gluonic hot spots meet symmetric cumulants data at LHC energies

2019

We present a systematic study on the influence of spatial correlations between the proton constituents, in our case gluonic hot spots, their size and their number on the symmetric cumulant SC(2, 3), at the eccentricity level, within a Monte Carlo Glauber framework [1]. When modeling the proton as composed by 3 gluonic hot spots, the most common assumption in the literature, we find that the inclusion of spatial correlations is indispensable to reproduce the negative sign of SC(2, 3) in the highest centrality bins as dictated by data. Further, the subtle interplay between the different scales of the problem is discussed. To conclude, the possibility of feeding a 2+1D viscous hydrodynamic sim…

COLLISIONSNuclear and High Energy PhysicsParticle physicsNuclear TheoryFLOWMonte Carlo methodFOS: Physical sciencesSmall systemshiukkasfysiikka114 Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)correlations0103 physical sciencesEntropy (information theory)ddc:530initial state010306 general physicsCumulantPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicselliptic flowElliptic flowhot spotsHigh Energy Physics - Phenomenologysmall systemsSubstructureGlauberNuclear Physics A
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The one loop gluon emission light cone wave function

2017

Light cone perturbation theory has become an essential tool to calculate cross sections for various small-$x$ dilute-dense processes such as deep inelastic scattering and forward proton-proton and proton-nucleus collisions. Here we set out to do one loop calculations in an explicit helicity basis in the four dimensional helicity scheme. As a first process we calculate light cone wave function for one gluon emission to one-loop order in Hamiltonian perturbation theory on the light front. We regulate ultraviolet divergences with transverse dimensional regularization and soft divergences with using a cut-off on longitudinal momentum. We show that when all the renormalization constants are comb…

COLLISIONSParticle physicsNuclear TheoryRENORMALIZATIONQUANTUM ELECTRODYNAMICSGeneral Physics and AstronomyFOS: Physical sciencesloop calculations114 Physical sciences01 natural scienceslight cone perturbation theoryRenormalizationNuclear Theory (nucl-th)Dimensional regularizationHigh Energy Physics - Phenomenology (hep-ph)INFINITE-MOMENTUMLight cone0103 physical sciencesSCATTERINGHelicity basis010306 general physicsNuclear ExperimentQuantum chromodynamicsPhysicsCoupling constantgluon emissionta114010308 nuclear & particles physicsCOLOR GLASS CONDENSATEDeep inelastic scatteringFRONT QCDHelicityEVOLUTIONHigh Energy Physics - PhenomenologyCHROMODYNAMICSQuantum electrodynamicsgluon saturation
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Abelian realization of phenomenological two-zero neutrino textures

2014

In an attempt at explaining the observed neutrino mass-squared differences and leptonic mixing, lepton mass matrices with zero textures have been widely studied. In the weak basis where the charged lepton mass matrix is diagonal, various neutrino mass matrices with two zeros have been shown to be consistent with the current experimental data. Using the canonical and Smith normal form methods, we construct the minimal Abelian symmetry realizations of these phenomenological two-zero neutrino textures. The implementation of these symmetries in the context of the seesaw mechanism for Majorana neutrino masses is also discussed.

CP ViolationPhysicsSterile neutrinoParticle physicsNuclear and High Energy Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesZerosHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Seesaw mechanismMass Matrix0103 physical sciencesCP violationlcsh:QC770-798High Energy Physics::Experimentlcsh:Nuclear and particle physics. Atomic energy. RadioactivityAbelian groupNeutrino010306 general physicsNeutrino oscillationLeptonNuclear Physics B
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Strange and charm mesons at FAIR

2010

Presented at the XXXI Mazurian Lakes Conference on Physics, Piaski, Poland, August 30–September 6, 2009.

CharmCBMNuclear TheoryNuclear TheoryScalar ResonancesFOS: Physical sciencesStrange ; Charm ; Mesons ; CBM ; FAIR ; GSI ; Finite temperature ; Spectral functions ; Scalar ResonancesStrange mesonUNESCO::FÍSICA::Física molecular::Moléculas mesónicas y muónicasGSINuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph):FÍSICA [UNESCO]Nuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentNUCLEAR-MATTERFAIREnergyMesonsFinite temperatureHigh Energy Physics::PhenomenologyUNESCO::FÍSICASpectral functionsTemperatureStrangeHigh Energy Physics - PhenomenologyCharm mesonsHigh Energy Physics::Experiment:FÍSICA::Física molecular::Moléculas mesónicas y muónicas [UNESCO]RESONANCES
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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Chiral expansion of the nucleon mass to order q^6

2006

We present the results of a complete two-loop calculation at order q^6 of the nucleon mass in manifestly Lorentz-invariant chiral perturbation theory. The renormalization is performed using the reformulated infrared renormalization, which allows for the treatment of two-loop integrals while preserving all relevant symmetries, in particular chiral symmetry.

Chiral anomalyPhysicsNuclear and High Energy PhysicsChiral perturbation theoryHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesLorentz covarianceRenormalizationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeQuantum mechanicsHomogeneous spacePerturbation theoryChiral symmetry breakingNucleonMathematical physics
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In-medium pi-pi Correlation Induced by Partial Restoration of Chiral Symmetry

2000

We show that both the linear and the non-linear chiral models give an enhancement of the pi-pi cross section near the 2pi threshold in the scalar-iso-scalar (I=J=0) channel in nuclear matter. The reduction of the chiral condensate, i.e., the partial chiral restoration in nuclear matter, is responsible for the enhancement in both cases. We extract an effective 4pi-nucleon vertex which is responsible for the enhancement but has not been considered in the non-liear models for in-medium pi-pi interaction. Relation of this vertex and a next-to-leading order terms in the heavy-baryon chiral lagrangian, L_piN^(2), is also discussed.

Chiral anomalyPhysicsNuclear and High Energy PhysicsChiral symmetryChiral perturbation theoryNuclear TheoryScatteringHigh Energy Physics::PhenomenologyFOS: Physical sciencesNuclear matterNuclear Theory (nucl-th)Formalism (philosophy of mathematics)symbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicssymbolsChiral symmetry breakingNuclear ExperimentLagrangianMathematical physics
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