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Quark core stars, quark stars and strange stars [electronic resource].

Published
Batavia, Ill. : Fermi National Accelerator Laboratory, 1988.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description
Pages: 38 : digital, PDF file
Additional Creators
Fermi National Accelerator Laboratory and United States. Department of Energy. Office of Scientific and Technical Information
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Summary
A recent one flavor quark matter equation of state is generalized to several flavors. It is shown that quarks undergo a first order phase transition. In addition, this equation of state depends on just one parameter in the two flavor case, two parameters in the three flavor case, and these parameters are constrained by phenomenology. This equation of state is then applied to the hadron-quark transition in neutron stars and the determination of quark star stability, the investigation of strange matter stability and possible strange star existence. 43 refs., 6 figs.
Report Numbers
E 1.99:fnal/pub-88/19-a
fnal/pub-88/19-a
Subject(s)
Other Subject(s)
Note
Published through SciTech Connect.
01/01/1988.
"fnal/pub-88/19-a"
"DE88006991"
Grassi, F.
Funding Information
AC02-76CH03000
View MARC record | catkey: 13828392