Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-01-27
PoS Confinement8:171,2008
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
4 pages, 8th Conference Quark Confinement and the Hadron Spectrum,Mainz, Germany, 1-6 September, 2008
Scientific paper
Equation of state for superdense nuclear matter is considered in the framework of relativistic mean-field theory, when the scalar-isovector -meson effective field is taken into account, as well. Assuming that the transition to the strange quark matter is a usual first-order phase transition described by Maxwells construction, the changes of the parameters of phase transition caused by the presence of -meson field are investigated. To describe a quark phase the advanced version of the MIT bag model is used, in which the interactions between quarks are taken into account in the one-gluon exchange approximation. For different values of the bag constant B, some series of the equations of the state of matter with deconfinement phase transition are constructed. Also the upper bound, Bcr, corresponding to the unstable state of the infinitizimal quark core in a neutron star is found.
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