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Title: Mu-tau neutrino refraction and collective three-flavor transformations in supernovae

Journal Article · · Physical Review. D, Particles Fields
; ;  [1];  [2];  [3]
  1. Institut de Fisica Corpuscular, CSIC-Universitat de Valencia, Ed. Instituts d'Investigacio, Ap. correus 22085, 46071 Valencia (Spain)
  2. Max-Planck-Institut fuer Physik, Werner-Heisenberg-Institut, Foehringer Ring 6, 80805 Muenchen (Germany)
  3. II. Institut fuer theoretische Physik, Universitaet Hamburg, Luruper Chaussee 149, 22761 Hamburg (Germany) and APC (AstroParticules et Cosmologie), 10, rue Alice Domon et Leonie Duquet, 75205 Paris Cedex 13 (France)

We study three-flavor collective neutrino transformations in the dense-neutrino region above the neutrino sphere of a supernova core. We find that two-flavor conversions driven by the atmospheric mass difference and the 13-mixing angle capture the full effect if one neglects the second-order difference between the {nu}{sub {mu}} and {nu}{sub {tau}} refractive index. Including this 'mu-tau matter term' provides a resonance at a density of {rho}{approx_equal}3x10{sup 7} g cm{sup -3} that typically causes significant modifications of the overall {nu}{sub e} and {nu}{sub e} survival probabilities. This effect is surprisingly sensitive to deviations from maximal 23-mixing, being different for each octant.

OSTI ID:
21249877
Journal Information:
Physical Review. D, Particles Fields, Vol. 77, Issue 6; Other Information: DOI: 10.1103/PhysRevD.77.065024; (c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
Country of Publication:
United States
Language:
English