Search results for "relativistic"

showing 10 items of 308 documents

On the deceleration of Fanaroff–Riley Class I jets: mass loading by stellar winds

2014

Jets in low-luminosity radio galaxies are known to decelerate from relativistic speeds on parsec scales to mildly or sub-relativistic speeds on kiloparsec scales. Several mechanisms have been proposed to explain this effect, including strong reconfinement shocks and the growth of instabilities (both leading to boundary-layer entrainment) and mass loading from stellar winds or molecular clouds. We have performed a series of axisymmetric simulations of the early evolution of jets in a realistic ambient medium to probe the effects of mass loading from stellar winds using the code Ratpenat. We study the evolution of Fanaroff-Riley Class I (FRI) jets, with kinetic powers L_j \sim 1.e41-1.e44 erg…

PhysicsStellar mass010308 nuclear & particles physicsRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaMolecular cloudAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinetic energy01 natural sciencesSpace and Planetary ScienceStellar mass loss0103 physical sciencesElliptical galaxyEntrainment (chronobiology)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsRelativistic speedMonthly Notices of the Royal Astronomical Society
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Grid-based Methods in Relativistic Hydrodynamics and Magnetohydrodynamics

2015

An overview of grid-based numerical methods used in relativistic hydrodynamics (RHD) and magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive review of the application of high-resolution shock-capturing methods. Results of a set of demanding test bench simulations obtained with different numerical methods are compared in an attempt to assess the present capabilities and limits of the various numerical strategies. Applications to three astrophysical phenomena are briefly discussed to motivate the need for and to demonstrate the success of RHD and RMHD simulations in their understanding. The review further provides FORTRAN programs to compute the exact solution…

PhysicsTest benchRelativistic hydrodynamics (RHD)FortranNumerical analysisReview ArticleGridlaw.inventionsymbols.namesakeRiemann problemExact solutions in general relativitylawPhysics::Space PhysicssymbolsCartesian coordinate systemStatistical physicsMagnetohydrodynamicscomputerRelativistic magnetohydrodynamics (RMHD)computer.programming_languageLiving Reviews in Computational Astrophysics
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General Relativistic Dynamics of Irrotational Dust: Cosmological Implications

1994

The non--linear dynamics of cosmological perturbations of an irrotational collisionless fluid is analyzed within General Relativity. Relativistic and Newtonian solutions are compared, stressing the different role of boundary conditions in the two theories. Cosmological implications of relativistic effects, already present at second order in perturbation theory, are studied and the dynamical role of the magnetic part of the Weyl tensor is elucidated.

PhysicsWeyl tensorGeneral relativityAstrophysics (astro-ph)Relativistic dynamicsFOS: Physical sciencesGeneral Physics and AstronomyEnergy–momentum relationAstrophysicsCenter of mass (relativistic)symbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicssymbolsRelativistic mechanicsRelativistic quantum chemistryRelativistic speed
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Superheavy element flerovium (element 114) is a volatile metal.

2014

The electron shell structure of superheavy elements, i.e., elements with atomic number Z ≥ 104, is influenced by strong relativistic effects caused by the high Z. Early atomic calculations on element 112 (copernicium, Cn) and element 114 (flerovium, Fl) having closed and quasi-closed electron shell configurations of 6d(10)7s(2) and 6d(10)7s(2)7p1/2(2), respectively, predicted them to be noble-gas-like due to very strong relativistic effects on the 7s and 7p1/2 valence orbitals. Recent fully relativistic calculations studying Cn and Fl in different environments suggest them to be less reactive compared to their lighter homologues in the groups, but still exhibiting a metallic character. Expe…

Physicsgas chemistryValence (chemistry)ta114Electron shellchemistry.chemical_elementelement 114Inorganic ChemistryFleroviumsuperheavy elementsPhysisorptionchemistryAtomic orbitalChemical physicsSubatomic PhysicsAtomic numberPhysical and Theoretical ChemistryAtomic physicsRelativistic quantum chemistryCoperniciumInorganic chemistry
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Stability of Relativistic Hydrodynamical Planar Jets: Linear and Nonlinear Evolution of Kelvin-Helmholtz Modes

2004

Some aspects about the stability of relativistic flows against Kelvin-Helmholtz (KH) perturbations are studied by means of relativistic, hydrodynamical simulations. In particular, we analyze the transition to the fully nonlinear regime and the long-term evolution of two jet models with different specific internal energies.

Physicssymbols.namesakeJet (fluid)Nonlinear systemClassical mechanicsPlanarAstrophysics::High Energy Astrophysical PhenomenaHelmholtz free energysymbolsNonlinear evolutionStability (probability)CosmologyRelativistic particle
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Computing Strong Shocks in Ultrarelativistic Flows: A Robust Alternative

1999

In recent years, shock capturing methods have started to be used in numerical simulations in Relativistic Fluid Dynamics (RFD). These techniques lead to explicit numerical codes that are able to successfully simulate the extreme conditions of the ultrarelativistic regime. After [2], an explicit, ready-to-use description of the full spectral decomposition of the Jacobian matrices of the RFD system is available, and this allows us to implement Marquina’s scheme [3] in RFD. The scheme is seen to maintain the good behavior shown in [3] with respect to certain numerical pathologies.

Physics::Fluid DynamicsPhysicssymbols.namesakeShock capturing methodJacobian matrix and determinantsymbolsStatistical physicsRelativistic fluidMatrix decomposition
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Use of a running coupling in the NLO calculation of forward hadron production

2018

We address and solve a puzzle raised by a recent calculation [1] of the cross-section for particle production in proton-nucleus collisions to next-to-leading order: the numerical results show an un- reasonably large dependence upon the choice of a prescription for the QCD running coupling, which spoils the predictive power of the calculation. Specifically, the results obtained with a prescription formulated in the transverse coordinate space differ by one to two orders of magnitude from those obtained with a prescription in momentum space. We show that this discrepancy is an artefact of the interplay between the asymptotic freedom of QCD and the Fourier transform from coordinate space to mo…

Position and momentum spaceQCD EVOLUTION01 natural sciencesAsymptotic freedomquantum chromodynamics: correctionhard scatteringHigh Energy Physics - Phenomenology (hep-ph)coupling constant: energy dependencestrong interaction: coupling constantEQUATIONkvanttifysiikkaComputingMilieux_MISCELLANEOUSPhysicsQuantum chromodynamicsQUARKhigher-order: 1nuclear physicssddc:12.39.StHigh Energy Physics - Phenomenology12.38.Bxsymbolsydinfysiikkahadron: forward productionFOS: Physical sciences114 Physical sciencesRENORMALIZATION-GROUP12.38.Cysymbols.namesakeCross section (physics)Theoretical physicsquantum chromodynamics0103 physical sciencessirontarelativistic heavy-ion collisionCoordinate spacenumerical calculations010306 general physicsp nucleus: scatteringcorrection: higher-orderCouplingta114010308 nuclear & particles physics25.75.-qCOLOR GLASS CONDENSATENONLINEAR GLUON EVOLUTIONRenormalization groupFourier transformasymptotic freedom[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physical Review D
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Consistent treatment of relativistic corrections in deuteron photodisintegration in a one-pion-exchange model

1992

Using a one-pion-exchange model for the nucleon-nucleon interaction the relativistic corrections to potential and to the electromagnetic operators are derived in a power expansion of (p/M). All corrections up to the order (p/M)3 are consistently included. Numerical results are shown for differential cross section and polarization observables for deuteron photodisintegration. A sizeable influence of relativistic effects on some observables is found even at low energies. A comparison of our operators with the expressions of other authors is given.

Power seriesNuclear physicsPhysicsPionPhotodisintegrationNuclear TheoryObservableElementary particleNuclear ExperimentPolarization (waves)Relativistic quantum chemistryWave functionAtomic and Molecular Physics and OpticsFew-Body Systems
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Elliptic flow in nuclear collisions at ultrarelativistic energies available at the CERN Large Hadron Collider

2009

We use perfect-fluid hydrodynamical model to predict the elliptic flow coefficients in $\mathrm{Pb}+\mathrm{Pb}$ collisions at the Large Hadron Collider (LHC). The initial state for the hydrodynamical calculation for central $A+A$ collisions is obtained from the perturbative QCD $+$ saturation model. The centrality dependence of the initial state is modeled by the optical Glauber model. We show that the baseline results obtained from the framework are in good agreement with the data from the Relativistic Heavy Ion Collider and show predictions for the ${p}_{T}$ spectra and elliptic flow of pions in $\mathrm{Pb}+\mathrm{Pb}$ collisions at the LHC. Also mass and multiplicity effects are discu…

Quantum chromodynamicsNuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsPionLarge Hadron ColliderElliptic flowPerturbative QCDNuclear ExperimentRelativistic Heavy Ion ColliderGlauberSpectral linePhysical Review C
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Measurement of charged pion double spin asymmetries at midrapidity in longitudinally polarized p+p collisions at s=510  GeV

2020

The PHENIX experiment at the Relativistic Heavy Ion Collider has measured the longitudinal double spin asymmetries, $A_{LL}$, for charged pions at midrapidity ($|\eta|<0.35$) in longitudinally polarized $p+p$ collisions at $\sqrt{s}=510$ GeV. These measurements are sensitive to the gluon spin contribution to the total spin of the proton in the parton momentum fraction $x$ range between 0.04 and 0.09. One can infer the sign of the gluon polarization from the ordering of pion asymmetries with charge alone. The asymmetries are found to be consistent with global quantum-chromodynamics fits of deep-inelastic scattering and data at $\sqrt{s}=200$ GeV, which show a nonzero positive contribution of…

Quantum chromodynamicsPhysics010308 nuclear & particles physicsScatteringHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyNuclear TheoryPartonDeep inelastic scattering7. Clean energy01 natural sciencesGluonNuclear physicsPion0103 physical sciencesProton spin crisisHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsRelativistic Heavy Ion ColliderPhysical Review D
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