Stellar matter in the Quark-Meson-Coupling Model with neutrino trapping
Nuclear Theory
2009-11-10 v2
Abstract
The properties of hybrid stars formed by hadronic and quark matter in -equilibrium are described by appropriate equations of state (EoS) in the framework of the quark meson coupling (QMC) model. In the present work we include the possibility of trapped neutrinos in the equation of state and obtain the properties of the related hybrid stars. We use the quark meson coupling model for the hadron matter and two possibilities for the quark matter phase, namely, the unpaired quark phase and the color-flavor locked phase. The differences are discussed and a comparison with other relativistic EoS is done.
Keywords
Cite
@article{arxiv.nucl-th/0312112,
title = {Stellar matter in the Quark-Meson-Coupling Model with neutrino trapping},
author = {P. K. Panda and D. P. Menezes and C. Providência},
journal= {arXiv preprint arXiv:nucl-th/0312112},
year = {2009}
}
Comments
Reference added, accepted in PRC