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Quark matter in neutron stars

โœ Scribed by Mark G. Alford


Publisher
Elsevier Science
Year
2009
Tongue
English
Weight
282 KB
Volume
830
Category
Article
ISSN
0375-9474

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โœฆ Synopsis


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.

Nuclear Physics A 830 (2009) 385c-392c


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