Damping of neutrino flavour conversions in a 'noisy' supernova shock-wave

Details Damping of neutrino flavour conversions in a 'noisy' supernova shock-wave Damping of neutrino flavour conversions in a 'noisy' supernova shock-wave

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phst..127...80f&link_type=abstract

Physica Scripta, Volume 127, Issue , pp. 80-81 (2006).

Physics

Scientific paper

In recent literature, it has been realized that supernova (SN) shock-wave propagation after the core-bounce can leave a peculiar imprint on the observable SN neutrino signal at Earth. We show that small-scale stochastic density fluctuations in SN matter might modify this scenario, potentially suppressing the signature associated with the shock wave on the neutrino spectra.

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