Investigation of possible structures of hybrid neutron stars

Details Investigation of possible structures of hybrid neutron stars Investigation of possible structures of hybrid neutron stars

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1296..362p&link_type=abstract

XI HADRON PHYSICS. AIP Conference Proceedings, Volume 1296, pp. 362-365 (2010).

Physics

Neutron Stars, Quarks, Supernovae, Fermion Systems, Hadrons, Neutron Star Core, Quark Deconfinement, Quark-Gluon Plasma Production, And Phase Transitions, Explosive Burning In Accreting Binary Systems, Degenerate Fermi Gases, Forces In Hadronic Systems And Effective Interactions

Scientific paper

This work investigates the structure of hybrid stars built in two different ways. The first one considers the existence of a mixed phase at intermediate stellar densities. The second implies the inexistence of this mixed phase. In this case, the hadron phase and the quark phase are in direct contact. We use the non-linear Walecka model (NLWM) to describe the hadron phase and the Nambu-Jona-Lasinio model (NJL) for the quark phase.

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