2008/10/31 by Mattias Blennow, Alessandro Mirizzi, Pasquale D. Serpico +1 · 59 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #Measurements of neutrino speed #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Solar neutrino #Solar neutrino problem #Supernova #astro-ph #hep-ph
paper · pdf · doi:10.1103/physrevd.78.113004
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 78(11) (American Physical Society) · 9 pages, 4 figures, REVTeX4, minor changes, final version published in Phys. Rev. D
openalex publication_date 2008/12/10 · arxiv created 2008/12/17 · arxiv updated 2010/04/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We investigate the effects of nonstandard four-fermion neutrino-neutrino interactions on the flavor evolution of dense neutrino gases. We find that in the regions where the neutrino-neutrino refractive index leads to collective flavor oscillations, the presence of new neutrino interactions can produce flavor equilibration in both normal and inverted neutrino mass hierarchy. In realistic supernova environments, these effects are significant if the nonstandard neutrino-neutrino interaction strength is comparable to the one expected in the standard case, dominating the ordinary matter potential. However, very small nonstandard neutrino-neutrino couplings are enough to trigger the usual collective neutrino flavor transformations in the inverted neutrino mass hierarchy, even if the mixing angle vanishes exactly.