Phases of dense matter in neutron stars
arXiv:nucl-th/9902033 · doi:10.1016/S0370-1573(99)00110-6
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.
114 pages, 42 figs, report commisioned for Physics Reports
Cited by in corpus (210)
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- Approximate Universal Relations for Neutron Stars and Quark Stars
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- The neutron star in the Relativistic Mean-Field Theory
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- Effective interactions in medium heavy nuclei
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- Computational Nuclear Physics and Post Hartree-Fock Methods
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- Free Energy of Anisotropic Strangeon Stars
- Exploring pathways to forming twin stars
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- Constraining the Surface Curvature of an Anisotropic Neutron Star
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- Hybrid Stars with Hyperons and Strange Quark Matter
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- Impact of Anisotropy on Neutron Star Structure and Curvature
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- Formation of large chunk of nuclear matter in heavy-ion collisions