期刊
PHYSICS LETTERS B
卷 511, 期 2-4, 页码 229-234出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/S0370-2693(01)00579-2
关键词
neutron stars; quark matter; phase transition
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. (C) 2001 Elsevier Science B.V. All rights reserved.
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