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Maximum mass of neutron stars

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dc.contributor.authorSchulze, H.-J.cat
dc.contributor.authorPolls Martí, Arturcat
dc.contributor.authorRamos Gómez, Àngelscat
dc.contributor.authorVidaña Haro, Isaaccat
dc.date.accessioned2010-01-29T10:30:48Z
dc.date.available2010-01-29T10:30:48Z
dc.date.issued2006cat
dc.description.abstractWe determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realistic nucleon-nucleon, nucleon-hyperon, and hyperon-hyperon interactions. Our results indicate rather low maximum masses below 1.4 solar masses. This feature is insensitive to the nucleonic part of the EOS due to a strong compensation mechanism caused by the appearance of hyperons and represents thus strong evidence for the presence of nonbaryonic "quark" matter in the interior of heavy stars.eng
dc.format.extent4 p.cat
dc.format.mimetypeapplication/pdfeng
dc.identifier.idgrec540740cat
dc.identifier.issn0556-2813cat
dc.identifier.urihttps://hdl.handle.net/2445/11019
dc.language.isoengeng
dc.publisherThe American Physical Societycat
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.73.058801cat
dc.relation.ispartofPhysical Review C, 2006, vol. 73, núm. 5, p. 058801-1-058801-4cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevC.73.058801
dc.rights(c) The American Physical Society, 2006
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationAstrofísica nuclearcat
dc.subject.classificationReaccions nuclearscat
dc.subject.otherNuclear astrophysicseng
dc.subject.otherNuclear reactionseng
dc.titleMaximum mass of neutron starseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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