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Collective neutrino oscillations with the halo effect in single-angle approximation

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arxiv 1807.07070 v1 pith:CXRG5DQI submitted 2018-07-18 hep-ph astro-ph.HE

Vincenzo Cirigliano , Mark Paris , Shashank Shalgar This is my paper · ORCID
classification hep-phastro-ph.HE
keywords effecthaloapproximationcollectiveneutrinooscillationssingle-angleback
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We perform a self-consistent calculation of collective neutrino oscillations including the effect of back scattered neutrinos (Halo effect) in the `single-angle' approximation, within a spherically symmetric supernova model. We find that due to the Halo effect the onset of flavor transformations is pushed to smaller radii, by a few kilometers. The celebrated phenomenon of the spectral split is found to be robust under the present inclusion of the Halo effect.

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Cited by 1 Pith paper

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  1. Neutrino halo effect on collective neutrino oscillation in iron core-collapse supernova model of a 9.6 $M_{\odot}$ star

    astro-ph.HE 2019-08 conditional novelty 6.0 of 10

    For a 9.6 solar mass supernova, including scattered halo neutrinos delays the onset of collective neutrino oscillation at early times and sharpens spectral swap features, improving their detectability.

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