Search results for "relativistic"

showing 10 items of 308 documents

Collision centrality andτ0dependence of the emission of thermal photons from a fluctuating initial state in an ideal hydrodynamic calculation

2012

Fluctuations in the initial QCD matter density distribution are found to enhance the production of thermal photons significantly in the range $2\ensuremath{\leqslant}{p}_{T}\ensuremath{\leqslant}4$ GeV/$c$ compared to a smooth initial state averaged profile in ideal hydrodynamic calculation for $200A$ GeV Au+Au collisions at the Relativistic Heavy Ion Collider (RHIC) and $2.76A$ TeV Pb+Pb collisions at the Large Hadron Collider (LHC). The thermal emission of photons is strongly dependent on the initial temperature of the system where the presence of ``hot spots'' in the initial state translates into enhanced production of photons compared to a smooth profile. The effect of fluctuations in t…

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsRange (particle radiation)Photon010308 nuclear & particles physicsPlasma01 natural sciencesSpectral lineNuclear physics0103 physical sciencesProduction (computer science)Atomic physicsNuclear Experiment010306 general physicsRelativistic Heavy Ion ColliderQCD matterPhysical Review C
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Neutral pion production with respect to centrality and reaction plane in Au+Au collisions atsNN=200GeV

2013

The PHENIX experiment has measured the production of pi(0)s in Au + Au collisions at root S-NN = 200 GeV. The new data offer a fourfold increase in recorded luminosity, providing higher precision and a larger reach in transverse momentum, p(T), to 20 GeV/c. The production ratio of eta/pi(0) is 0.46 +/- 0.01(stat) +/- 0.05(syst), constant with p(T) and collision centrality. The observed ratio is consistent with earlier measurements, as well as with the p + p and d + Au values. pi(0) are suppressed by a factor of 5, as in earlier findings. However, with the improved statistical precision a small but significant rise of the nuclear modification factor R-AA vs p(T), with a slope of 0.0106 +/-(0…

PhysicsQuantum chromodynamicsNuclear physicsNuclear and High Energy PhysicsAdS/CFT correspondenceParticle physicsPionLuminosity (scattering theory)Path lengthConformal field theoryPartonRelativistic Heavy Ion ColliderPhysical Review C
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Measurement ofKS0andK*0inp+p,d+Au, and Cu + Cu collisions atsNN=200 GeV

2014

The PHENIX experiment at the Relativistic Heavy Ion Collider has performed a systematic study of K-S(0) and K*(0) meson production at midrapidity in p + p, d + Au, and Cu + Cu collisions at root s(NN) = 200 GeV. The K-S(0) and K*(0) mesons are reconstructed via their K-S(0) -> pi(0)(-> gamma gamma) pi(0)(-> gamma gamma) and K*(0) -> K-+/-pi(-/+) decay modes, respectively. The measured transverse-momentum spectra are used to determine the nuclear modification factor of K-S(0) and K*(0) mesons in d + Au and Cu + Cu collisions at different centralities. In the d + Au collisions, the nuclear modification factor of K-S(0) and K*(0) mesons is almost constant as a function of transverse momentum a…

PhysicsQuarkNuclear and High Energy PhysicsMesonNuclear TheoryStrangenessPhi mesonBaryonNuclear physicsDeuteriumHigh Energy Physics::ExperimentImpact parameterNuclear ExperimentRelativistic Heavy Ion ColliderPhysical Review C
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Charm and bottom baryon decays in the Bethe-Salpeter approach: Heavy to heavy semileptonic transitions

1998

Charm and bottom baryons and mesons are studied within the framework of a relativistically covariant 3D reduction of the Bethe-Salpeter equation. We carry out an analysis of semileptonic decays of heavy hadrons within this framework using explicit oscillator-type wave functions where we calculate Isgur-Wise functions, decay rates and asymmetry parameters. Within this model we also study the effect of interactions between the light quarks inside the heavy baryon and how they affect the values of the computed heavy baryon observables. We also elaborate on the role of relativistic effects in the calculation of the heavy baryon Isgur-Wise function.

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsBethe–Salpeter equationMesonmedia_common.quotation_subjectHadronNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesAsymmetryNuclear physicsBaryonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentCharm (quantum number)Relativistic quantum chemistryNuclear Experimentmedia_common
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Relativistic scattering theory of charged spinless particles

1986

In the context of a relativistic quantum mechanics we discuss the scattering of two and three charged spinless particles. The corresponding transition operators are shown to satisfy four-dimensional Lippmann-Schwinger and eight-dimensional Faddeev-type equations, respectively. A simplified model of two particles with Coulomb interaction can be solved exactly. We calculate: (i) The partial waveS-matrix from which we extract the bound state spectrum. The latter agrees with a fourth-order result of Schwinger, (ii) The full scattering amplitude which in the weakfield limit coincides with the expression derived by Fried et al. from eikonalized QED.

PhysicsScattering amplitudeScatteringQuantum mechanicsQuantum electrodynamicsGeneral Physics and AstronomyScattering lengthRelativistic quantum mechanicsScattering theoryMott scatteringLippmann–Schwinger equationS-matrixCzechoslovak Journal of Physics
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Measurement of ϕ -meson production at forward rapidity in p+p collisions at s=510  GeV and its energy dependence from s=200  GeV to 7 TeV

2018

The PHENIX experiment at the Relativistic Heavy Ion Collider has measured the differential cross section of φ(1020)-meson production at forward rapidity in p+p collisions at s=510 GeV via the dimuon decay channel. The partial cross section in the rapidity and pT ranges 1.2

PhysicsScattering cross-sectionMeson production010308 nuclear & particles physicsNuclear TheoryStrangeness01 natural sciencesNuclear physics0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsRelativistic Heavy Ion ColliderPhysical Review D
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Influence of Internal Energy on the Stability of Relativistic Flows

2003

A set of simulations concerning the influence of internal energy on the stability of relativistic jets is presented. Results show that perturbations saturate when the amplitude of the velocity perturbation approaches the speed of light limit. Also, contrary to what predicted by linear stability theory, jets with higher specific internal energy appear to be more stable.

PhysicsShear layerClassical mechanicsAmplitudeInternal energyAstrophysical jetLinear stability theoryLinear stability analysisAstrophysics::High Energy Astrophysical PhenomenaPerturbation (astronomy)MechanicsAstrophysicsRelativistic particle
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Probing the Internal Structure of Magnetized, Relativistic Jets with Numerical Simulations

2016

From an observational point of view, unveiling the physical processes behind the nature of the jets emanating from radio-loud AGN demands the resolution of the structure across the jet with the highest angular resolutions. Relying on a magneto-fluid dynamical description, numerical simulations can help to characterize the internal structure of jets (transversal structure, magnetic field structure, internal shocks, etc.). In the first part of the paper, we shall discuss equilibrium models of magnetized, relativistic, infinite, axisymmetric jets with rotation propagating through a homogeneous, static, unmagnetized ambient medium. Then, these transversal equilibrium profiles will be used to bu…

PhysicsShock waveJet (fluid)Internal energyMagnetic energyMHDlcsh:Astronomy010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeAstronomy and Astrophysicsshock wavesgalaxies: jets01 natural sciencesmethods: numericalComputational physicsMagnetic fieldlcsh:QB1-991galaxies: active; galaxies: jets; methods: numerical; MHD; shock wavesRelativistic beamingClassical mechanicsAstrophysical jet0103 physical sciencesMagnetohydrodynamics010303 astronomy & astrophysicsGalaxies
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VLBI-selected sample of Compact Symmetric Object candidates and frequency-dependent position of hotspots

2011

The Compact Symmetric Objects (CSOs) are small (<1 kiloparsec) and powerful extragalactic radio sources showing emission on both sides of an active galactic nucleus and no signs of strong relativistic beaming. They may be young radio sources, progenitors of large FRII radio galaxies. We aim to study the statistical properties of CSOs by constructing and investigating a new large sample of CSO candidates on the basis of dual-frequency, parsec-scale morphology. For the candidate selection we utilized VLBI data for 4170 extragalactic objects obtained simultaneously at 2.3 and 8.6 GHz (S and X band) within the VLBA Calibrator Survey 1-6 and the Research and Development - VLBA projects. Prope…

PhysicsSpectral indexActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesRadio galaxyX bandFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesSpectral lineRelativistic beamingSpace and Planetary ScienceBrightness temperature0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysics0105 earth and related environmental sciencesAstrophysics - Cosmology and Nongalactic Astrophysics
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High-resolution observations of SN 2001gd in NGC 5033

2005

We report on 8.4 GHz VLBI observations of SN2001gd in the spiral galaxy NGC5033 made on 26 June 2002 and 8 April 2003. Our data nominally suggests a relatively strong deceleration for the expansion of SN2001gd, but we cannot dismiss the possibility of a free supernova expansion. From our VLBI observations on 8 April 2003, we inferred a minimum total energy in relativistic particles and magnetic fields in the supernova shell of E_min =(0.3-14) 10^{47} ergs, and a corresponding equipartition average magnetic field of B_min = (50--350) mG. We also present multiwavelength VLA measurements of SN2001gd, which are well fit by an optically thin, synchrotron spectrum, partially absorbed by thermal p…

PhysicsSpiral galaxyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRelativistic particleMagnetic fieldLuminositySupernovaSpace and Planetary ScienceVery-long-baseline interferometryAstrophysics::Galaxy Astrophysics
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