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arXiv · 1206.5011

Pairing and the Cooling of Neutron Stars

Dany Page
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Abstract

In this review, I present a brief summary of the impact of nucleon pairing at supra-nuclear densities on the cooling of neutron stars. I also describe how the recent observation of the cooling of the neutron star in the supernova remnant Cassiopeia A may provide us with the first direct evidence for the occurrence of such pairing. It also implies a size of the neutron 3P-F2 energy gap of the order of 0.1 MeV.

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Dany Page. 2012-06-21. Pairing and the Cooling of Neutron Stars. https://doi.org/10.1142/9789814412490_0024

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