Hybrid stars and the equation of state

Details Hybrid stars and the equation of state Hybrid stars and the equation of state

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nuphs..24..156r&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 24, Issue 2, p. 156-159.

Physics

Nuclear Physics

3

Scientific paper

Gross properties of hybrid stars consisting of a core of strange matter surrounded by ordinary neutron matter are investigated. We discuss star models based on phenomenological equations of state from nuclear reactions including a phase transition between the hadronic phase and the quark-gluon plasma. For certain parameters, such equations of state support the existence of hybrid stars: While the nuclear equation of state has a minor influence on the gross properties of hybrid stars, the identification of such objects could provide us with a rather stringent constraint on the vacuum energy density of the quark gluon plasma.

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