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Thermal Evolution of Isolated Neutron Stars. II

Dany Page
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Abstract

After a brief summary of neutron star cooling theory I present results which emphasize the importance of baryon pairing in the neutron star core. I show how the thermal evolution may be totally controlled by pairing for models which include only nucleons and models containing also hyperons. Finally, I consider the thermal evolution of ultramagnetized neutron stars whose existence has been inferred from the soft gamma repeaters.

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Dany Page. 1998-02-13. Thermal Evolution of Isolated Neutron Stars. II. https://arxiv.org/abs/astro-ph/9802171

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