Phase transition and properties of compact star

Details Phase transition and properties of compact star Phase transition and properties of compact star

2006-11-13

arxiv.org/abs/nucl-th/0611039v1

Phys.Rev.C75:035808,2007

Physics

Nuclear Physics

Nuclear Theory

11 pages with 7 figures

Scientific paper

10.1103/PhysRevC.75.035808

We investigate the phase transition to a deconfined phase and the consequences in the formation of neutron stars. We use the recently proposed effective field theory motivated relativistic mean field theory for hadron and the MIT Bag model and color-flavor locked (CFL) phase for the quark matter in order to get the appropriate equation of state. The properties of star are then calculated. The differences between unpaired and CFL quark matter are discussed.

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