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

Fiorillo DFG, Janka HT, Raffelt GG

DOI: 10.1103/jbmx-rbzt
Published: 2025 Dec 5
Container: Physical review letters
Publisher: Not recorded
Open access: unknown

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Cite this work

BibTeX

@article{allodium:10.1103/jbmx-rbzt,
  title = {Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae.},
  author = {Fiorillo DFG and Janka HT and Raffelt GG},
  year = {2025},
  journal = {Physical review letters},
  doi = {10.1103/jbmx-rbzt},
  url = {https://doi.org/10.1103/jbmx-rbzt}
}

RIS

TY  - JOUR
TI  - Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae.
AU  - Fiorillo DFG
AU  - Janka HT
AU  - Raffelt GG
PY  - 2025
JO  - Physical review letters
DO  - 10.1103/jbmx-rbzt
UR  - https://doi.org/10.1103/jbmx-rbzt
ER  -

APA

DFG, F., HT, J., & GG, R. (2025). Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae.. Physical review letters. https://doi.org/10.1103/jbmx-rbzt

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pubmed · retrieved 2026-09-25T11:46:38.507Z