Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints

By D. Page, Sanjay Reddy Instituto de Astronomia, Unam, Mexico., T. Division, L. Laboratory, Usa. 2006

184 citations recorded by the source corpus.

▪ Abstract We review theoretical developments in studies of dense matter and its phase structure of relevance to compact stars. Observational data on compact stars, which can constrain the properties of dense matter, are presented critically and interpreted.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Geophysics

View Paper: https://www.semanticscholar.org/paper/43963ef99c2ee97a13c0cc3e74477b9d97897a73

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In Astronomy and Astrophysics

1. M. Hempel
2. S. Weissenborn
3. Irina Sagert
4. J. Schaffner-Bielich
5. L. Núñez
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In Atomic and Molecular Physics, and Optics

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In Geophysics

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Citations in the corpus

• QUARK MATTER IN MASSIVE COMPACT STARS (2011, methodology): “The phase transitions are modelled by the Gibbs and Maxwell constructions (see e.g. Glendenning (1992)) corresponding to a small (Gibbs) and to a large value of the surface tension (Maxwell) (see discussion in Page & Reddy (2006)).”
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects (2007, background): “Much of the efforts to disentangle the physics of very dense matter is reflected by the various “radial” equations of state: Pr = Pr(ρ) availables (see [17,18] and references therein).”
• Mapping the phases of quantum chromodynamics with beam energy scan (2019, background): “16/fm3) is expected to exist inside the compact stars and thus affects their properties [3, 4].”
• Proto-Neutron and Neutron Stars in a Chiral SU(3) Model (2008, background): “…discussed in the past by a number of authors including the investigation of kaon condensation (Kaplan & Nelson 1986; Pons et al. 2000) and studies of the effect of hyperons in neutron stars (Glendenning &Moszkowski 1991; Glendenning 2001; Jha et al. 2006, 2008; and references in Page & Reddy 2006).”