On the possibility of stable quark stars

Details On the possibility of stable quark stars On the possibility of stable quark stars

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213..840b&link_type=abstract

Astrophysical Journal, Part 1, vol. 213, May 1, 1977, p. 840-848.

Astronomy and Astrophysics

Astrophysics

18

Astrophysics, Equations Of State, Partons, Quarks, Stellar Models, Baryons, Density (Mass/Volume), Dynamic Stability, Gravitational Collapse, Neutron Stars, Stellar Evolution, Stellar Structure

Scientific paper

A recent zero-temperature equation of state which contains quark-partons separated from conventional baryons by a phase transition is used to investigate the stability of quark stars. The sensitivity to the input physics is also considered. The conclusions, which are found to be relatively model independent, indicate that a separately identifiable class of stable objects called quark stars does not exist.

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