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Theoretical developments in supernova neutrino physics : mass corrections and pairing correlators

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arxiv 1601.05018 v1 pith:GIW6MA6X submitted 2016-01-18 astro-ph.HE astro-ph.SRhep-ph

Cristina Volpe This is my paper · ORCID
classification astro-ph.HEastro-ph.SRhep-ph
keywords neutrinoanticorrectionsextendedmasspairingparticularapproximation
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We highlight the progress in our understanding of how neutrinos change their flavor in astrophysical environments, in particular effects from the neutrino self-interaction. We emphasize extended descriptions of neutrino propagation in massive stars that are beyond the current one based on the mean-field approximation. The extended equations include, in particular, corrections from (anti)neutrino-(anti)neutrino pairing correlations and from the neutrino mass. We underline open issues and challenges.

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Cited by 1 Pith paper

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  1. Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH

    astro-ph.HE 2019-09 conditional novelty 6.0 of 10

    Neutrino self-interactions inside neutrino-cooled accretion disks are argued to push flavors toward equipartition, reducing the neutrino-antineutrino annihilation energy deposition around black holes by a factor up to...

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