From Neutron Stars to Strange Stars

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dc.creatorWeber, Fridolin
dc.date2001-12-04
dc.date.accessioned2026-07-07T02:01:40Z
dc.date.available2026-07-07T02:01:40Z
dc.descriptionThis paper discusses several most intruigung astrophysical implications connected with the possible absolute stability of strange quark matter.This is followed by a discussion of two astrophysical signals that may point at the existence of quark matter in both isolated neutron stars as well as in neutron stars in low-mass x-ray binaries (LMXBs).
dc.descriptionPaper presented at the int. conference "Compact Stars in the QCD Phase Diagram", held in Copenhagen (NORDITA - Niels Bohr Institute), August 15-18, 2001; organized by Rachid Ouyed and Francesco Sannino; (12 pages, 6 figures)
dc.identifierhttps://arxiv.org/abs/astro-ph/0112058
dc.identifierhttp://arxiv.org/abs/astro-ph/0112058
dc.identifiereConf C010815 (2002) 17-28
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3834
dc.subjectAstrophysics
dc.titleFrom Neutron Stars to Strange Stars
dc.typetext

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