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Coherent Development of Neutrino Flavor in the Supernova Environment

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arxiv astro-ph/0608050 v2 pith:TAPY7BEX submitted 2006-08-02 astro-ph hep-ph

Coherent Development of Neutrino Flavor in the Supernova Environment

Huaiyu Duan (UCSD) , George M. Fuller (UCSD) , J. Carlson (LANL) , Yong-Zhong Qian (UMN) This is my paper
classification astro-ph hep-ph
keywords neutrinoantineutrinoflavorsupernovacoherentenergyenvironmentaccompanying
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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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Cited by 2 Pith papers

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  1. Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae

    hep-ph 2026-07 conditional novelty 6.0

    Nearby neutrino flavor conversion in a supernova can boost νp-process yields of p-nuclides like 92Mo and 92Nb by up to two orders of magnitude, matching solar abundances when conversion starts within ~10 km of the pro...

  2. Single-wave solutions of the neutrino fast flavor system. Part I. Mechanical properties

    hep-ph 2026-01 conditional novelty 6.0

    Single-wave neutrino flavor solutions form a non-integrable spin system without Gaudin invariants, so an exact flavor pendulum exists only for two beams and does not extend to continuous angle distributions.