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| Journal Article | PUBDB-2026-00018 |
; ;
2025
APS
College Park, Md.
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Please use a persistent id in citations: doi:10.1103/jbmx-rbzt doi:10.3204/PUBDB-2026-00018
Report No.: arXiv:2507.22985
Abstract: Collective neutrino flavor conversions in core-collapse supernovae begin with instabilities, initially triggered when the dominant νe outflow concurs with a small antineutrino flux of opposite lepton number, with $\bar{ν}_e$ dominating over $\bar{ν}_μ$. When these “flipped” neutrinos emerge in the energy-integrated angular distribution (angular crossing), they initiate a fast instability. However, before such conditions arise, spectral crossings typically appear within 20 ms of collapse, i.e., local spectral excesses of $\bar{ν}_e$ over $\bar{ν}_μ$ along some direction. Therefore, postprocessing supernova simulations cannot consistently capture later fast instabilities because the early slow ones have already altered the conditions.
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Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae
College Park, Md. : APS (2025)
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