Phase transition to hyperon matter in neutron stars

Recent progress in the understanding of the high density phase of neutron stars advances the view that a substantial fraction of the matter consists of hyperons. The possible impacts of a highly attractive interaction be
Recent progress in the understanding of the high density phase of neutron stars advances the view that a substantial fraction of the matter consists of hyperons. The possible impacts of a highly attractive interaction between hyperons on the properties of compact stars are investigated.We find that a hadronic equation of state with hyperons allows for a first order phase transition to hyperonic matter. The corresponding hyperon stars can have rather small radii of R 8 km.
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Metadaten
Author:Jürgen Schaffner-Bielich, Matthias Hanauske, Horst Stöcker, Walter Greiner
URN:urn:nbn:de:hebis:30-21319
Document Type:Article
Language:English
Date of Publication (online):2005/11/16
Year of first Publication:2002
Publishing Institution:Univ.-Bibliothek Frankfurt am Main
Release Date:2005/11/16
Tag:Neutronensterne ; hyperon
hyperon; neutron stars
Source:Phys.Rev.Lett.89:171101,2002 ,  2002 The American Physical Society
Institutes:Physik
Dewey Decimal Classification:530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License Logo Veröffentlichungsvertrag für Publikationen

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