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Ultimate Energy Density of Observable Cold Baryonic Matter

, and . Physical Review Letters, 94 (11): 111101+ (March 2005)
DOI: 10.1103/physrevlett.94.111101

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Superfluid Neutrons in the Core of the Neutron Star in Cassiopeia A, , , and . (Oct 24, 2011)Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter, , , and . Physical Review Letters, 106 (8): 081101+ (February 2011)Ultimate Energy Density of Observable Cold Baryonic Matter, and . Physical Review Letters, 94 (11): 111101+ (March 2005)Minimal Cooling of Neutron Stars: A New Paradigm, , , and . (2004)cite arxiv:astro-ph/0403657 Comment: Version to appear in ApJ Supplements. Minor modifications in text and discussion of updated data with new figures.