Contribution to a conference proceedings/Contribution to a book | PUBDB-2017-00182 |
2011
Verlag Deutsches Elektronen-Synchrotron
Hamburg
ISBN: 978-3-935702-53-9
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2011-03/kneller
Abstract: As neutrinos propagate from the neutrinosphere through the mantle of a core-collapse supernova they will pass through regions of turbulence. The turbulence leads to stochastic neutrino flavor mixing thus leaving fingerprints in the Galactic supernova neutrino burst signal. In this talk I explore the effect of turbulence upon the neutrinos focusing upon the case of large amplitudes and demonstrate that the ensemble of S matrices that describe the neutrino evolution in this limit is Dyson's Circular Ensemble.
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Book/Proceedings/Report
Hamburg neutrinos from supernova explosions. Proceedings, Workshop, HANSE 2011
Hamburg Neutrinos From Supernova Explosions, HAνSE 2011, HamburgHamburg, Germany, 19 Jul 2011 - 23 Jul 2011
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 1-166 (2011) [10.3204/DESY-PROC-2011-03]
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