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arXiv · hep-ph/0103209

From Quark Stars to Hybrid Stars

Alessandro Drago·Andrea Lavagno
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Abstract

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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Alessandro Drago, Andrea Lavagno. 2001-03-20. From Quark Stars to Hybrid Stars. https://doi.org/10.1016/s0370-2693(01)00579-2

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