Phases of dense matter in neutron stars

Preprint

15 February 1999

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.nucl-th/9902033

Abstract

Recent equations of state for dense nuclear matter are discussed with possible phase transitions arising in neutron stars such as pion, kaon and hyperon kondensation, 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.

Keywords

PHASE TRANSITIONS
RECENT EQUATIONS
NEUTRON STARS
STARS RECENT
QUARK MATTER
DENSE MATTER
RADII

All Related Versions

Version 1, 1999-02-15, ArXiv
Version 1, 1999-10-12, ArXiv (Unconfirmed version)
Version 2, 1999-10-15, ArXiv (Unconfirmed version)
Published version: Physics Reports, 328 (5-6), 237.

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