Search results for "Numerical"

showing 10 items of 2002 documents

The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations

2018

The uniformity of the intra-cluster medium (ICM) enrichment level in the outskirts of nearby galaxy clusters suggests that chemical elements were deposited and widely spread into the intergalactic medium before the cluster formation. This observational evidence is supported by numerical findings from cosmological hydrodynamical simulations, as presented in Biffi et al. (2017), including the effect of thermal feedback from active galactic nuclei. Here, we further investigate this picture, by tracing back in time the spatial origin and metallicity evolution of the gas residing at z=0 in the outskirts of simulated galaxy clusters. In these regions, we find a large distribution of iron abundanc…

galaxies: clusters: intracluster mediumCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusMetallicityFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesVirial theoremmethods: numericalgalaxies: clusters: general; galaxies: clusters: intracluster medium; methods: numericalAbundance (ecology)0103 physical sciencesCluster (physics)clusters: general [galaxies]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysics010308 nuclear & particles physicsnumerical [methods]Astronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)clusters: intracluster medium [galaxies]galaxies: clusters: generalSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)HaloAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution

2018

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity, gas mass, X-ray temperature, and $Y_{X}$. Three sets of simulations are performed with an improved version of the smoothed particle hydrodynamics GADGET-3 code. These consider the following: non-radiative gas, star formation and stellar feedback, and the addition of feedback by active galactic nuclei (AGN). We select clusters with $M_{500} > 10^{14} M_{\odot} E(z)^{-1}$, mimicking the typical selection of Sunyaev-Zeldovich samples. This permits to have a mass range large enough to enable robust fitting of the r…

galaxies: clusters: intracluster mediumCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusNUMERICAL [METHODS]Ciencias FísicasFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsnumerical galaxies: clusters: general galaxies: clusters: intracluster medium X-rays: galaxies: clusters [methods]01 natural sciencesmethods: numericalLuminosity//purl.org/becyt/ford/1 [https]GALAXIES: CLUSTERS [X-RAYS]Smoothed-particle hydrodynamics0103 physical sciences010303 astronomy & astrophysicsScalingAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysicsmethods: numerical galaxies: clusters: general galaxies: clusters: intracluster medium X-rays: galaxies: clustersSettore FIS/05010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsObservable//purl.org/becyt/ford/1.3 [https]RedshiftAstronomíamethods: numerical; galaxies: clusters: general; galaxies: clusters: intracluster medium; X-rays: galaxies: clusters; Astrophysics - Cosmology and Nongalactic Astrophysicsgalaxies: clusters: generalSpace and Planetary ScienceX-rays: galaxies: clustersCLUSTERS: INTRACLUSTER MEDIUM [GALAXIES]CLUSTERS: GENERAL [GALAXIES]CIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Is ram-pressure stripping an efficient mechanism to remove gas in galaxies?

2017

We study how the gas in a sample of galaxies (M* > 10e9 Msun) in clusters, obtained in a cosmological simulation, is affected by the interaction with the intra-cluster medium (ICM). The dynamical state of each elemental parcel of gas is studied using the total energy. At z ~ 2, the galaxies in the simulation are evenly distributed within clusters, moving later on towards more central locations. In this process, gas from the ICM is accreted and mixed with the gas in the galactic halo. Simultaneously, the interaction with the environment removes part of the gas. A characteristic stellar mass around M* ~ 10e10 Msun appears as a threshold marking two differentiated behaviours. Below this mas…

galaxies: clusters: intracluster mediumCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCooling flowGalaxy merger01 natural sciencesmethods: numericalGalaxy groups and clustersGalaxy group0103 physical sciencesgalaxies: interactionsDisc010303 astronomy & astrophysicsGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesRam pressuregalaxies: haloesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Elliptical galaxyAstrophysics::Earth and Planetary Astrophysicsgalaxies: evolutiongalaxies: ISMAstrophysics - Cosmology and Nongalactic Astrophysics
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Charge fluctuations and electric mass in a hot meson gas

2006

Net-Charge fluctuations in a hadron gas are studied using an effective hadronic interaction. The emphasis of this work is to investigate the corrections of hadronic interactions to the charge fluctuations of a non-interacting resonance gas. Several methods, such as loop, density and virial expansions are employed. The calculations are also extended to SU(3) and some resummation schemes are considered. Although the various corrections are sizable individually, they cancel to a large extent. As a consequence we find that charge fluctuations are rather well described by the free resonance gas.

gas [meson]Nuclear and High Energy PhysicsNuclear TheoryMesonresonance [gas]HadronFOS: Physical sciencesElectric chargeResonance (particle physics)fluctuation [charge]susceptibilityVirial theoremNuclear Theory (nucl-th)Nuclear physicsmass [rho(770)]electric [mass]unitarityddc:530Resummationnumerical calculationsinteraction [pi pi]Physicshigher-order [correction]effective Lagrangianvirial [expansion]High Energy Physics::PhenomenologySU(3) [symmetry]Charge (physics)relativistic [expansion]quantum [statistics]Quantum electrodynamicsQuark–gluon plasmaPhysical Review C
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Temari Balls, Spheres, SphereHarmonic: From Japanese Folkcraft to Music

2022

Temari balls are traditional Japanese toys and artworks. The variety of their geometries and tessellations can be investigated formally and computationally with the means of combinatorics. As a further step, we also propose a musical application of the core idea of Temari balls. In fact, inspired by the classical idea of music of spheres and by the CubeHarmonic, a musical application of the Rubik’s cube, we present the concept of a new musical instrument, the SphereHarmonic. The mathematical (and musical) description of Temari balls lies in the wide background of interactions between art and combinatorics. Concerning the methods, we present the tools of permutations and tessellations we ado…

geometry music sphere Temari ballsSettore ING-INF/05 - Sistemi Di Elaborazione Delle InformazioniComputational MathematicsNumerical AnalysisComputational Theory and MathematicsSettore INF/01 - Informaticageometry; Temari balls; music; sphereSettore MAT/03 - GeometriaTheoretical Computer Science
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Directionlets: Anisotropic Multidirectional representation with separable filtering

2006

In spite of the success of the standard wavelet transform (WT) in image processing in recent years, the efficiency of its representation is limited by the spatial isotropy of its basis functions built in the horizontal and vertical directions. One-dimensional (1-D) discontinuities in images (edges and contours) that are very important elements in visual perception, intersect too many wavelet basis functions and lead to a nonsparse representation. To efficiently capture these anisotropic geometrical structures characterized by many more than the horizontal and vertical directions, a more complex multidirectional (M-DIR) and anisotropic transform is required. We present a new lattice-based pe…

geometrysparse image representationMultiresolution analysisInformation Storage and RetrievalGeometryBasis functionDirectional vanishing momentsseparable filteringwaveletsWaveletmultiresolutionImage Interpretation Computer-AssistedComputer GraphicsCurveletComputer SimulationmultidirectionMathematicsStochastic ProcessesModels StatisticalMathematical analysisWavelet transformfilter banksNumerical Analysis Computer-AssistedSignal Processing Computer-AssistedImage EnhancementFilter bankComputer Graphics and Computer-Aided DesignContourletFilter designAnisotropyArtifactsdirectionletsAlgorithmsFiltrationSoftware
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Up-wind difference approximation and singularity formation for a slow erosion model

2020

We consider a model for a granular flow in the slow erosion limit introduced in [31]. We propose an up-wind numerical scheme for this problem and show that the approximate solutions generated by the scheme converge to the unique entropy solution. Numerical examples are also presented showing the reliability of the scheme. We study also the finite time singularity formation for the model with the singularity tracking method, and we characterize the singularities as shocks in the solution.

granular flowsNumerical AnalysisEntropy solutionsup-wind schemeApplied MathematicsMathematical analysisEngquist–Osher schemeEntropy solutions up-wind scheme Engquist–Osher scheme spectral analysis complex singularities granular flowsspectral analysiscomplex singularitiesComputational MathematicsSingularityEntropy solutions / up-wind scheme / Engquist–Osher scheme / spectral analysis / complex singularities / granular flowsModeling and SimulationSpectral analysisGravitational singularityFinite timeSettore MAT/07 - Fisica MatematicaAnalysisMathematics
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First measurement of the Sivers asymmetry for gluons using SIDIS data

2017

The Sivers function describes the correlation between the transverse spin of a nucleon and the transverse motion of its partons. It was extracted from measurements of the azimuthal asymmetry of hadrons produced in semi-inclusive deep inelastic scattering of leptons off transversely polarised nucleon targets, and it turned out to be non-zero for quarks. In this letter the evaluation of the Sivers asymmetry for gluons in the same process is presented. The analysis method is based on a Monte Carlo simulation that includes three hard processes: photon-gluon fusion, QCD Compton scattering and leading-order virtual-photon absorption process. The Sivers asymmetries of the three processes are simul…

hadron: angular distributionmuon+: polarized beamNuclear TheoryPartonmuon+ deuteron: deep inelastic scatteringhadron: transverse momentumtransverse momentum dependence01 natural sciencesCOMPASSHigh Energy Physics - ExperimentSubatomär fysikSivers functionHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)photon gluon: fusionSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]partonNuclear Experimentmedia_commonQuantum chromodynamicsPhysicsgluon: distribution functiondeep inelastic scattering: semi-inclusive reactionhigher-order: 0polarized target: transversehep-phDeep inelastic scattering; Gluon; PDF; Sivers; TMD; Nuclear and High Energy Physicslcsh:QC1-999High Energy Physics - PhenomenologySivereffect: CollinsNucleonCompton scatteringnumerical calculations: Monte Carlospin: asymmetryParticle Physics - ExperimentDeep inelastic scatteringQuarkParticle physicsNuclear and High Energy Physicsdata analysis methoddeuteron: polarized targethadron: asymmetryangular distribution: asymmetryneural networkmedia_common.quotation_subjectpolarization: longitudinalFOS: Physical sciencesAsymmetryPDFGluonNuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesquantum chromodynamicsSivers010306 general physicsParticle Physics - Phenomenology010308 nuclear & particles physicshep-ex160 GeV/cHigh Energy Physics::PhenomenologyTMDnucleon: spin: transverseCERN SPSDeep inelastic scatteringGluonmuon+ p: deep inelastic scatteringcorrelation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentabsorptionlcsh:PhysicsLeptonexperimental results
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Flow dominance and factorization of transverse momentum correlations in Pb-Pb collisions at the LHC

2017

Physical review letters 118(16), 162302 (2017). doi:10.1103/PhysRevLett.118.162302

heavy ion: scattering:Kjerne- og elementærpartikkelfysikk: 431 [VDP]transverse momentum [correlation function]correlation [momentum]550Pb-PbPb-Pb collisionsGeneral Physics and Astronomyhiukkasfysiikkanucl-exPP01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEDEPENDENCEddc:550Nuclear Experiment (nucl-ex)ROOT-S(NN)=2.76 TEVNuclear ExperimentPERSPECTIVENuclear ExperimentPhysics and Astronomy (all); ALICE; LHCPhysicscorrelation function: transverse momentumPhysicsflow ; transverse ; momentum ; Pb-Pbtransverse momentum: correlationtwo-particleHanbury-Brown-Twiss effect:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]PRIRODNE ZNANOSTI. Fizika.transverseTransverse planeCorrelation function (statistical mechanics)CERN LHC Coll:Nuclear and elementary particle physics: 431 [VDP]flowPseudorapidityLHCParticle Physics - ExperimentdeconfinementParticle physicscollectiveVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431FOS: Physical sciencesmomentumtriangulationPhysics and Astronomy(all)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciencesBethe ansatzMomentumNuclear physicsCENTRALITYPhysics and Astronomy (all)statistical analysisFactorizationscattering [heavy ion]Relativistic heavy-ion collisions0103 physical sciencesALICE / ALICE2760 GeV-cmsNuclear Physics - ExperimentRapiditystructurenumerical calculations010306 general physicsNuclear Physicstwo-particle transverse momentum differential correlation functionAnsatzleadDEPENDENCE PERSPECTIVE CENTRALITY PP.ta114VDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431hep-ex010308 nuclear & particles physics:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]momentum: correlationBethe ansatzROOT-S(NN)=2.76 TEV; DEPENDENCE; PERSPECTIVE; PPNATURAL SCIENCES. Physics.rapiditypile-uptransverse momentum: factorizationfactorization [transverse momentum]correlation [transverse momentum]experimental results
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Review of Particle Physics

2020

The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, …

high energyleptonmixing [neutrino]High Energy Physics::LatticeCosmic microwave backgrounddiffractionTechnicolorAstrophysicsOmega01 natural sciencesPhysics Particles & Fieldshiggs-boson productionBig Bang nucleosynthesiscosmological model: parameter spacetaudark energyMonte CarlofieldspentaquarkinstrumentationSettore FIS/01gauge bosonAnomalous magnetic dipole momentdeep-inelastic scatteringnew physicsPhysicsDOUBLE-BETA-DECAYElectroweak interactiondensity [dark matter]HEAVY FLAVOURQuarkoniumreview; particle; physicsSUPERSYMMETRIC STANDARD MODELsquare-root-sPhysics Nucleargrand unified theoryboson: heavystatisticsPhysical SciencesHiggs bosonaxion: massflavor: violationNeutrinoELECTROWEAK SYMMETRY-BREAKINGnumerical calculations: Monte Carlophysicson-lineS013EPHQuarkheavy [boson]particle[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Physics Multidisciplinaryanomalous magnetic-momentelectroweak radiative-correctionsdark matter: densityHiggs particlemesonneutrino masses neutrino mixing; neutrino oscillations114 Physical sciencesCHIRAL PERTURBATION-THEORYneutrino mixingStandard Modelquark0202 Atomic Molecular Nuclear Particle And Plasma PhysicsNucleosynthesisquantum chromodynamicsCP: violationDark matterddc:530particle physicsStrong Interactions010306 general physicssparticleS013DFgrand unified theoriesPRODUCTIONGauge bosonScience & Technologyneutrino oscillationsneutrino masses010308 nuclear & particles physicsC50 Other topics in experimental particle physicsParticle Data GroupAstronomy and AstrophysicsDeep inelastic scatteringto-leading-order* Automatic Keywords *heavy bosonaxiontables (particle physics)Tetraquarkproton-proton collisionsSupersymmetryhadronneutrino: mixing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyVolume (compression)HIGGS-BOSONUB-VERTICAL-BARcosmological modeldark energy densityexperimental methodsddc:539.72021Physics beyond the Standard Modelstandard modelgroup theoryGeneral Physics and Astronomytables particle physicshigh energy physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamicsPhysicsenergy: highE Rev 2016[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Settore FIS/01 - Fisica SperimentalephotonSupersymmetryNuclear & Particles Physicsparameter space [cosmological model]dark energy: densityhigh [energy]M013WXfermion-pair productionNuclear and High Energy PhysicsParticle physicsHiggs bosonreviewAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics530dark matterstatistical analysisDouble beta decay0103 physical sciencesconservation lawcold dark-matterTAU LEPTONSAstrophysics::Galaxy AstrophysicstablesDEEP-INELASTIC-SCATTERINGelectroweak interactionHigh Energy Physics::Phenomenology750 GeV diphoton excessPRODUCTION CROSS-SECTIONbaryondensity [dark energy]Physics and AstronomygravitationCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentsupersymmetryMinimal Supersymmetric Standard Model
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