Search results for "Q star"

showing 2 items of 2 documents

Influence of pions and hyperons on stellar black hole formation

2013

We present numerical simulations of stellar core-collapse with spherically symmetric, general relativistic hydrodynamics up to black hole formation. Using the CoCoNuT code, with a newly developed grey leakage scheme for the neutrino treatment, we investigate the effects of including pions and \Lambda-hyperons into the equation of state at high densities and temperatures on the black hole formation process. Results show non-negligible differences between the models with reference equation of state without any additional particles and models with the extended ones. For the latter, the maximum masses supported by the proto-neutron star are smaller and the collapse to a black hole occurs earlie…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics[PHYS]Physics [physics]Nuclear and High Energy PhysicsNuclear Theory010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesPrimordial black holeAstrophysics01 natural sciencesNuclear Theory (nucl-th)Black holeBinary black holeRotating black holeIntermediate-mass black hole0103 physical sciencesExtremal black holeStellar black holeQ starAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSPhys. Rev. D., 87, id.043006 (2013)
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Neutron star formation with presence of hyperons

2001

We study the influence of hyperons during the early stages of the birth of a neutron star (Kelvin-Helmholtz phase), employing neutrino opacities calculated consistently with the equation of state by considering all possible neutrino-hyperon reactions. Our results from numerical simulations of newly born neutron stars, or proto-neutron stars, show an increasingly important influence of hyperons at later times. It is remarkable the existence of metastable stars, which are stable at birth but become unstable during the evolution as the deleptonization proceeds and the hyperon concentration increases. We also present results from hydrodynamical simulations of the collapse to a black hole of met…

PhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNuclear TheoryX-ray binaryAstrophysicsCompact starAtomic and Molecular Physics and OpticsStarsNeutron starExotic starr-processHigh Energy Physics::ExperimentStellar black holeQ starNuclear ExperimentNuclear Physics B - Proceedings Supplements
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