Strange star equations of state revisited

Details Strange star equations of state revisited Strange star equations of state revisited

2005-06-08

arxiv.org/abs/astro-ph/0506158v1

Astronomy and Astrophysics

Astrophysics

9 pages, 5 figures, 2 tables

Scientific paper

10.1071/AS05022

Motivated by recent suggestions that strange stars can be responsible for glitches and other observational features of pulsar, we review some possible equations of state and their implications for models of neutron, hybrid and strange stars. We consider the MIT bag model and also strange matter in the color-flavored-locked phase. The central energy densities for strange stars are higher than the central densities of ordinary neutron stars. Strange stars are bound by the strong force and so can also rotate much faster than neutron stars. These results are only weakly dependent on the model used for the quark matter. If just one of the existing mass to radius ratio constraint is valid, most neutron stars equations of state are ruled out, but all the strange stars equations of state presented in this work remain consistent with the constraint.

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