Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ara..conf...55j&link_type=abstract
ASTRONOMY AND RELATIVISTIC ASTROPHYSICS New Phenomena and New States of Matter in the Universe. Proceedings of the Third Worksho
Astronomy and Astrophysics
Astrophysics
Quark-Gluon Plasma, Phase Transition, Neutron Stars
Scientific paper
This work is a study of nuclear matter at high densities considering the hadronic and quark phases at zero temperature. We describe the hadron-meson phase using a phenomenological Lagrangian which exhibits a parametrization, through mathematical constants, of the intensity of the meson-nucleon coupling. We have included into the formalism the chemical equilibrium equations, lepton degrees of freedom, the fundamental octet of baryons and the charge neutrality condition. In the quark matter study, we have considered the classic MIT bag model with a constant bag pressure. Phase transition is determined by the Gibbs criteria. The influence of the model couplings in the determination of the phase transition density is discussed. We have also calculated maximum mass and radius for hybrid stars.
Bodmann Bardo E. J.
Fernandez Francisco
Jacobsen R. B.
Vasconcellos Cesar A. Z.
No associations
LandOfFree
Quark-Gluon Plasma in Neutron Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Quark-Gluon Plasma in Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quark-Gluon Plasma in Neutron Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1803970