Role of dense matter in collective supernova neutrino transformations

A. Esteban-Pretel, A. Mirizzi, S. Pastor, R. Tomàs, G. G. Raffelt, P. D. Serpico, and G. Sigl
Phys. Rev. D 78, 085012 – Published 16 October 2008

Abstract

For neutrinos streaming from a supernova core, dense matter suppresses self-induced flavor transformations if the electron density ne significantly exceeds the neutrino density nν in the conversion region. If ne is comparable to nν, one finds multiangle decoherence, whereas the standard self-induced transformation behavior requires that in the transformation region nν is safely above ne. This condition need not be satisfied in the early phase after the supernova core bounce. Our new multiangle effect is a subtle consequence of neutrinos traveling on different trajectories when streaming from a source that is not pointlike.

  • Figure
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  • Received 16 July 2008

DOI:https://doi.org/10.1103/PhysRevD.78.085012

©2008 American Physical Society

Authors & Affiliations

A. Esteban-Pretel1, A. Mirizzi2,3, S. Pastor1, R. Tomàs4, G. G. Raffelt2, P. D. Serpico5, and G. Sigl4,6

  • 1Institut de Física Corpuscular (CSIC-Universitat de València), Edifici Instituts d’Investigació, Apartado 22085, 46071 València, Spain
  • 2Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, 80805 München, Germany
  • 3Istituto Nazionale di Fisica Nucleare, Roma, Italy
  • 4II. Institut für Theoretische Physik, Universität Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • 5Center for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500, USA
  • 6APC (AstroParticules et Cosmologie), UMR 7164 (CNRS, Université Paris 7, CEA, Observatoire de Paris), 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France

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Issue

Vol. 78, Iss. 8 — 15 October 2008

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