Journal
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
Volume 328, Issue 5-6, Pages 237-327Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/S0370-1573(99)00110-6
Keywords
neutron star properties; phase transitions; equation of state for dense neutron star matter
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Recent equations of state for dense nuclear matter are discussed with possible phase transitions arising in neutron stars such as pion, kaon and hyperon condensation, superfluidity and quark matter. Specifically, we treat the nuclear to quark matter phase transition, the possible mixed phase and its structure. A number of numerical calculations of rotating neutron stars with and without phase transitions are given and compared to observed masses, radii, temperatures and glitches. (C) 2000 Elsevier Science B.V. All rights reserved.
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