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- W4387502309 endingPage "030" @default.
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- W4387502309 abstract "Abstract Young neutron stars cool via the emission of neutrinos from their core. A precise understanding of all the different processes producing neutrinos in the hot and degenerate matter is essential for assessing the cooling rate of such stars. The main Standard Model processes contributing to this effect are ν bremsstrahlung, mURCA among others. In this paper, we investigate another Standard Model process initiated by the Wess-Zumino-Witten term, leading to the emission of neutrino pairs via Nγ → Nνν̅ . We find that for proto-neutron stars, such processes with degenerate neutrons can be comparable and even dominate over the typical and well-known cooling mechanisms." @default.
- W4387502309 created "2023-10-11" @default.
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- W4387502309 date "2023-10-01" @default.
- W4387502309 modified "2023-10-12" @default.
- W4387502309 title "Anomaly induced cooling of neutron stars: a Standard Model contribution" @default.
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- W4387502309 doi "https://doi.org/10.1088/1475-7516/2023/10/030" @default.
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