Journal Article PUBDB-2026-00018

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Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae

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2025
APS College Park, Md.

Physical review letters 135(23), 231003 () [10.1103/jbmx-rbzt]
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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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Note: cc-by, 5 pages, 3 figures, plus Supplemental Material; version accepted for publication on PRL, added clarifications and changed title; Fig. S5 added

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
  2. DFG project G:(GEPRIS)390783311 - EXC 2094: ORIGINS: Vom Ursprung des Universums bis zu den ersten Bausteinen des Lebens (390783311) (390783311)
  3. DFG project G:(GEPRIS)283604770 - SFB 1258: Neutrinos und Dunkle Materie in der Astro- und Teilchenphysik (NDM) (283604770) (283604770)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2025
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Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae
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 Record created 2026-01-05, last modified 2026-02-09


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