Gapless Superfluidity and Neutron Star Cooling
The presence of currents in the interior of cold neutron stars can lead to a state in which nucleons remain superfluid while the quasiparticle energy spectrum has no gap. We show within the self-consistent time-dependent nuclear energy density functional theory that the nucleon specific heat is then...
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| Hlavní autoři: | , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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MDPI AG
2023-02-01
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| Edice: | Physical Sciences Forum |
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| On-line přístup: | https://www.mdpi.com/2673-9984/7/1/9 |
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