Ultra-Dense Neutron Star Matter, Strange Quark Stars, and the Nuclear Equation of State

Details Ultra-Dense Neutron Star Matter, Strange Quark Stars, and the Nuclear Equation of State Ultra-Dense Neutron Star Matter, Strange Quark Stars, and the Nuclear Equation of State

2006-06-05

arxiv.org/abs/astro-ph/0606093v1

Int.J.Mod.Phys.E16:1165-1180,2007

Astronomy and Astrophysics

Astrophysics

15 pages, 9 figures; paper presented at the International Symposium on Heavy Ion Physics 2006, April 3 to April 6, 2006, Frank

Scientific paper

10.1142/S0218301307006599

With central densities way above the density of atomic nuclei, neutron stars contain matter in one of the densest forms found in the universe. Depending of the density reached in the cores of neutron stars, they may contain stable phases of exotic matter found nowhere else in space. This article gives a brief overview of the phases of ultra-dense matter predicted to exist deep inside neutron stars and discusses the equation of state associated with such matter.

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