From Quark Stars to Hybrid Stars

Details From Quark Stars to Hybrid Stars From Quark Stars to Hybrid Stars

2001-03-20

arxiv.org/abs/hep-ph/0103209v1

Phys.Lett. B511 (2001) 229-234

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, 4 figures, 1 table

Scientific paper

10.1016/S0370-2693(01)00579-2

We show the possible existence of compact stars having a surface composed of a mixed phase of quarks and hadrons. This scenario can be realized both for self-bound stars, satisfying the so-called Witten-Bodmer hypothesis, and for gravitationally bound stars. This class of solutions of the Tolman-Oppenheimer-Volkoff equation can be obtained in all the models we discuss, within a physically acceptable range of values of the model parameters.

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