Sufficient and Necessary Conditions for Collective Neutrino Instability: Fast, Slow, and Mixed
Fuente:
arXiv
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| Autores principales: | , |
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| Formato: | Preprint |
| Publicado: |
2025
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| Acceso en línea: | |
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| _version_ | 1866914323635372032 |
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| author | Dasgupta, Basudeb Mukherjee, Dwaipayan |
| author_facet | Dasgupta, Basudeb Mukherjee, Dwaipayan |
| contents | Collective neutrino oscillations exhibit instabilities that induce appreciable flavor conversion, with crucial astrophysical implications. While the importance of initial phase-space distributions is well-established, a general instability criterion for distributions dependent on both energy and emission angle has been lacking. We identify and analyze the sufficient (and necessary) conditions for a generic collective neutrino flavor instability. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_03886 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Sufficient and Necessary Conditions for Collective Neutrino Instability: Fast, Slow, and Mixed Dasgupta, Basudeb Mukherjee, Dwaipayan High Energy Physics - Phenomenology Solar and Stellar Astrophysics Collective neutrino oscillations exhibit instabilities that induce appreciable flavor conversion, with crucial astrophysical implications. While the importance of initial phase-space distributions is well-established, a general instability criterion for distributions dependent on both energy and emission angle has been lacking. We identify and analyze the sufficient (and necessary) conditions for a generic collective neutrino flavor instability. |
| title | Sufficient and Necessary Conditions for Collective Neutrino Instability: Fast, Slow, and Mixed |
| topic | High Energy Physics - Phenomenology Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2505.03886 |