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Fast rotation of neutron stars and equation of state of dense matter

✍ Scribed by Paweł Haensel; Julian L. Zdunik; Michał Bejger

Publisher: Elsevier Science
Year: 2008
Tongue: English
Weight: 221 KB
Volume: 51
Category: Article
ISSN: 1387-6473
DOI: 10.1016/j.newar.2008.03.007

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The role of the equation of state in the structure of neutron stars is summarized. At densities beyond a few times the normal nuclear saturation density, the neutron-proton-electron sea can be supplemented with more exotic matter, usually involving strangeness, such as hyperons, kaon or pion condens