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Nucleation of quark matter bubbles in neutron stars

Michael L. Olesen·Jes Madsen
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Abstract

The thermal nucleation of quark matter bubbles inside neutron stars is examined for various temperatures which the star may realistically encounter during its lifetime. It is found that for a bag constant less than a critical value, a very large part of the star will be converted into the quark phase within a fraction of a second. Depending on the equation of state for neutron star matter and strange quark matter, all or some of the outer parts of the star may subsequently be converted by a slower burning or a detonation.

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BibTeXRIS

Michael L. Olesen, Jes Madsen. 1994-01-03. Nucleation of quark matter bubbles in neutron stars. https://doi.org/10.1103/physrevd.49.2698

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