Quark Hadron Phase Transition and Hybrid Stars

Details Quark Hadron Phase Transition and Hybrid Stars Quark Hadron Phase Transition and Hybrid Stars

1994-07-05

arxiv.org/abs/nucl-th/9407009v1

Z.Phys. A352 (1995) 457-466

Physics

Nuclear Physics

Nuclear Theory

25 pages in LaTex and 9 figures available on request, IP/BBSR/94-33

Scientific paper

We investigate the properties of hybrid stars consisting of quark matter in the core and hadron matter in outer region. The hadronic and quark matter equations of state are calculated by using nonlinear Walecka model and chiral colour dielectric (CCD) model respectively. We find that the phase transition from hadron to quark matter is possible in a narrow range of the parameters of nonlinear Walecka and CCD models. The transition is strong or weak first order depending on the parameters used. The EOS thus obtained, is used to study the properties of hybrid stars. We find that the calculated hybrid star properties are similar to those of pure neutron stars.

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