Triplet Pairing in Neutron Matter

The presence of superfluidity in neutron star interiors can affect the cooling of neutron stars in intricate ways, enhancing certain mechanisms and suppressing others. Model calculations employing realistic nuclear potentials in Bardeen–Cooper–Schrieffer theory generally suggest the development of a...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 955; no. 1; pp. 76 - 80
Main Authors Krotscheck, Eckhard, Papakonstantinou, Panagiota, Wang, Jiawei
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.09.2023
IOP Publishing
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