http://arxiv.org/abs/1807.07070
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.
V. Cirigliano, M. Paris and S. Shalgar
Fri, 20 Jul 18
22/63
Comments: 13 pages, 5 figures
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