Hadron-quark mixed phase in hyperon stars

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dc.creatorMaruyama, Toshiki
dc.creatorChiba, Satoshi
dc.creatorSchulze, Hans-Josef
dc.creatorTatsumi, Toshitaka
dc.date2007-08-24
dc.date.accessioned2026-07-07T11:18:51Z
dc.date.available2026-07-07T11:18:51Z
dc.descriptionWe analyze the different possibilities for the hadron-quark phase transition occurring in beta-stable matter including hyperons in neutron stars. We use a Brueckner-Hartree-Fock approach including hyperons for the hadronic equation of state and a generalized MIT bag model for the quark part. We then point out in detail the differences between Maxwell and Gibbs phase transition constructions including the effects of surface tension and electromagnetic screening. We find only a small influence on the maximum neutron star mass, whereas the radius of the star and in particular its internal structure are more affected.
dc.description11 pages, 9 figures
dc.identifierhttps://arxiv.org/abs/0708.3277
dc.identifierhttp://arxiv.org/abs/0708.3277
dc.identifierPhys.Rev.D76:123015,2007
dc.identifierdoi:10.1103/PhysRevD.76.123015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193485
dc.subjectNuclear Theory
dc.titleHadron-quark mixed phase in hyperon stars
dc.typetext

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