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Self-Refraction of Supernova Neutrinos: Mixed Spectra and Three-Flavor Instabilities

2010/01/31 by Alexander Friedland · 2 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #Flavor #Instability #Neutrino #Neutrino Physics Research #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum mechanics #Spectral line #Supernova #Type II supernova #astro-ph.SR #hep-ph

paper · pdf · doi:10.1103/physrevlett.104.191102

published as Phys.Rev.Lett.104:191102,2010 · 7 pages, 5 figures; updated to match the PRL version

arxiv created 2010/05/11 · openalex publication_date 2010/05/11 · arxiv updated 2010/05/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Neutrinos in a core-collapse supernova undergo coherent flavor transformations in their own background. We explore this phenomenon during the cooling stage of the explosion. Our three-flavor calculations reveal qualitatively new effects compared to a two-flavor analysis. These effects are especially clearly seen for the inverted mass hierarchy: we find a different pattern of spectral "swaps" in the neutrino spectrum and a novel "mixed" spectrum for the antineutrinos. A brief discussion of the relevant physics is presented, including the instability of the two-flavor evolution trajectory, the three-flavor pattern of spectral "swaps," and partial nonadiabaticity of the evolution.

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