dorsal/arxiv
View SchemaBaryon superfluidity and neutrino emissivity of neutron stars
| Authors | T. Takatsuka, R. Tamagaki |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0402011 |
| URL | https://arxiv.org/abs/nucl-th/0402011 |
| DOI | 10.1143/PTP.112.37 |
| Journal | Prog.Theor.Phys. 112 (2004) 37-72 |
Abstract
For neutron stars with hyperon-mixed core, neutrino emissivity is studied under the equation of state, obtained by introducing repulsive three-body force universal for all baryons so as to assure the maximum mass compatible with the observation. By paying attention to the density-dependence of critical temperatures of baryon superfluids, which reflect the nature of baryon-baryon interaction and control neutron star cooling, we show what neutrino emission processes are efficient in the regions with and without hyperon mixing and remark its implications related to neutron star cooling.
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"abstract": "For neutron stars with hyperon-mixed core, neutrino emissivity is studied\nunder the equation of state, obtained by introducing repulsive three-body force\nuniversal for all baryons so as to assure the maximum mass compatible with the\nobservation. By paying attention to the density-dependence of critical\ntemperatures of baryon superfluids, which reflect the nature of baryon-baryon\ninteraction and control neutron star cooling, we show what neutrino emission\nprocesses are efficient in the regions with and without hyperon mixing and\nremark its implications related to neutron star cooling.",
"arxiv_id": "nucl-th/0402011",
"authors": [
"T. Takatsuka",
"R. Tamagaki"
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"nucl-th"
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"doi": "10.1143/PTP.112.37",
"journal_ref": "Prog.Theor.Phys. 112 (2004) 37-72",
"title": "Baryon superfluidity and neutrino emissivity of neutron stars",
"url": "https://arxiv.org/abs/nucl-th/0402011"
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