FINITE TEMPERATURE EQUATIONS OF STATE FOR MIXED STARS
2004 ◽
Vol 13
(07)
◽
pp. 1249-1253
Keyword(s):
We investigate the properties of mixed stars formed by hadronic and quark matter in β-equilibrium described by appropriate equations of state (EOS) in the framework of relativistic mean-field theory. The calculations were performed for T=0 and for finite temperatures and also for fixed entropies with and without neutrino trapping in order to describe neutron and proto-neutron stars. The star properties are discussed. Maximum allowed masses for proto-neutron stars are much larger when neutrino trapping is imposed.
2010 ◽
Keyword(s):
Keyword(s):
2018 ◽
Vol 61
(8)
◽
1994 ◽
Vol 92
(4)
◽
pp. 803-813
◽
Keyword(s):