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Coherent Development of Neutrino Flavor in the Supernova Environment

2006/08/31 by Huaiyu Duan, George M. Fuller, J. Carlson +1 · 1 citation
Physics and Astronomy · #astro-ph #hep-ph

paper · pdf · doi:10.1103/physrevlett.97.241101

published as Phys.Rev.Lett.97:241101,2006 · 4 pages, 3 figures

arxiv created 2006/12/13 · arxiv updated 2009/12/01

Abstract

We calculate coherent neutrino and antineutrino flavor transformation in the supernova environment, for the first time including a self-consistent treatment of forward scattering-induced coupling and entanglement of intersecting neutrino/antineutrino trajectories. For the atmospheric neutrino mass-squared difference we find that in the normal (inverted) mass hierarchy the more tangentially-propagating (radially-propagating) neutrinos and antineutrinos can initiate collective, simultaneous medium-enhanced flavor conversion of these particles across broad ranges of energy and propagation direction. Accompanying alterations in neutrino/antineutrino energy spectra and/or fluxes could affect supernova nucleosynthesis and the expected neutrino signal.

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