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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Published in | The Astrophysical journal Vol. 955; no. 1; pp. 76 - 80 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.09.2023
IOP Publishing |
Subjects | |
Online Access | Get full text |
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