Neutrino Flavor Evolution Near a Supernova's Core

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J. Pantaleone This is my paper · ORCID

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keywords corecorrectedcrossingdiscussionevolutionexpandedflavormistake

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(The discussion is expanded, and a mistake in the crossing probability is corrected.)

Forward citations

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae
hep-ph 2026-07 conditional novelty 6.0 of 10

Nearby neutrino flavor conversion in a supernova can boost νp-process yields of p-nuclides like 92Mo and 92Nb by up to two orders of magnitude, matching solar abundances when conversion starts within ~10 km of the pro...