Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2003-12-25
Phys.Rev. C69 (2004) 058801
Physics
Nuclear Physics
Nuclear Theory
Reference added, accepted in PRC
Scientific paper
10.1103/PhysRevC.69.058801
The properties of hybrid stars formed by hadronic and quark matter in $\beta$-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.
Menezes Débora P.
Panda Prafulla Kumar
Providencia Constança
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