Neutron stars, hybrid stars and constraints on the equation of state from neutron stars and hybrid stars.

Details Neutron stars, hybrid stars and constraints on the equation of state from neutron stars and hybrid stars. Neutron stars, hybrid stars and constraints on the equation of state from neutron stars and hybrid stars.

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992zphya.342..235r&link_type=abstract

Z. Phys., A, Vol. 342, No. 2, p. 235 - 238

Mathematics

Logic

2

Scientific paper

Hybrid stars composed of a strange matter core surrounded by neutron matter are investigated. The authors apply star models based on phenomenological equations of state (EOS) from nuclear reactions including a phase transition between the hadronic phase and the quark gluon plasma. For specific equations of state hybrid stars might exist. While the nuclear part of the EOS has only a minor influence on the properties of hybrid stars, the EOS for the quark gluon phase has a crucial impact on the existence of such objects.

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