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

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Note:

Published through SciTech Connect.
01/01/1988.
"fnal/pub-88/19-a"
"DE88006991"
Grassi, F.

Funding Information:

AC02-76CH03000

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