The stability of quark matter

Details The stability of quark matter The stability of quark matter

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phlb..116..137o&link_type=abstract

Physics Letters B, Volume 116, Issue 2-3, p. 137-140.

Physics

10

Scientific paper

The possibility of quark matter existing in the interior of neutron stars is examined under a wide variety of conditions. The existence of a ``quark star'' relies only on its stability against gravitational collapse after the transition to quark matter occurs. It is found that for all choices of temperature and density, a star can not remain stable with a quark interior. In the context of model given, a maximum temperature of 30 MeV and a corresponding maximum mass of 2.8 M⊗ is derived for neutron stars.
I would like to thank W. Press and S. Teukolsky for valuable discussions.

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