Equation of State of Dense Matter and Maximum Mass of Neutron Stars

Abstract

Theoretical models of the equation of state (EOS) of neutronstar matter (starting with the crust and ending at the densest region of the stellar core) are reviewed. Apart from a broad set of baryonic EOSs, strange quark matter, and even more exotic (abnormal and Q-matter) EOSs are considered. Results of calculations of Mmax for non-rotating neutron stars… (More)

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Cite this paper

@inproceedings{Haensel2003EquationOS, title={Equation of State of Dense Matter and Maximum Mass of Neutron Stars}, author={Pawel Haensel}, year={2003} }