Name: Quark core stars, quark stars and strange stars
Creator: F. Grassi
Keywords: 0103 physical sciences, 7. Clean energy, 01 natural sciences

descriptionPublicationkeyboard_double_arrow_right Article 01 Mar 1989 English Publisher:Springer Science and Business Media LLCJournal:Zeitschrift f�r Physik C Particles and Fields, volume 44, pages 129-138 (issn: 0170-9739, eissn: 1434-6052,

Authors: F. Grassi;

doi: 10.1007/bf01548591

Quark core stars, quark stars and strange stars

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Abstract

A recent one flavor (zero temperature) 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 few parameters, one in the two flavor case, two in the three flavor case, and these parameters can be constrained by phenomenology. This equation of state is then applied to 1) the hadronquark transition in neutron stars and the determination of quark star stability, 2) the investigation of strange matter stability and possible strange star existence.

Related Organizations

National Aeronautics and Space Administration
United States
Fermilab
United States

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