## Quark deconfinement and implications for the radius and the limiting mass of compact stars

- Ignazio Bombaci, Irene Parenti
- 2004

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)

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