Quark matter in neutron stars
arXiv:0907.0200 · doi:10.1016/j.nuclphysa.2009.09.034
Abstract
According to quantum chromodynamics, matter at ultra-high density and low temperature is a quark liquid, with a condensate of Cooper pairs of quarks near the Fermi surface ("color superconductivity"). This paper reviews the physics of color superconductivity, and discusses some of the proposed signatures by which we might detect quark matter in neutron stars.
8 pages, 3 figures; To appear in the conference proceedings for Quark Matter 2009, March 30 - April 4, Knoxville, Tennessee. v2: typo corrected, line numbers removed
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- Phase diagram of chiral quark matter: color and electrically neutral Fulde-Ferrell phase
- Thermal Relaxation and Cooling of Quark Stars with a Strangelet Crust
- Rotating Hybrid Stars with Color-Flavor-Locked Quark Matter
- The structure of hybrid neutron star in Einstein- gravity
- Interpreting superfluid spin up through the response of the container
- Astrophysics of dense quark matter in compact stars
- Muon bundles from the Universe
- Baryon number transfer could delay Quark-Hadron transition in cosmology
- Axion Gamma-Ray Signatures from Quark Matter in Neutron Stars and Gravitational Wave Comparisons
- Finding strangelets in cosmic rays from HESS J1731-347, a possible strange quark star using the Cherenkov Telescope Array Observatory