Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion Relation Approach

Ignacio Izaguirre, Georg Raffelt, and Irene Tamborra
Phys. Rev. Lett. 118, 021101 – Published 10 January 2017

Abstract

Collective pair conversion νeν¯eνxν¯x by forward scattering, where x=μ or τ, may be generic for supernova neutrino transport. Depending on the local angular intensity of the electron lepton number carried by neutrinos, the conversion rate can be “fast,” i.e., of the order of 2GF(nνenν¯e)Δmatm2/2E. We present a novel approach to understand these phenomena: a dispersion relation for the frequency and wave number (Ω,K) of disturbances in the mean field of νeνx flavor coherence. Runaway solutions occur in “dispersion gaps,” i.e., in “forbidden” intervals of Ω and/or K where propagating plane waves do not exist. We stress that the actual solutions also depend on the initial and/or boundary conditions, which need to be further investigated.

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  • Received 10 October 2016

DOI:https://doi.org/10.1103/PhysRevLett.118.021101

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Ignacio Izaguirre1, Georg Raffelt1, and Irene Tamborra2

  • 1Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, 80805 München, Germany
  • 2Niels Bohr International Academy, Niels Bohr Institute, Blegdamsvej 17, 2100 Copenhagen, Denmark

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Issue

Vol. 118, Iss. 2 — 13 January 2017

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