Supernova neutrino energy spectra and the MSW effect View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

1997-12

AUTHORS

F. Buccella, S. Esposito, C. Gualdi, G. Miele

ABSTRACT

The distortions in the thermal energy spectra for neutrinos produced in a supernova when a resonant oscillation, MSW effect, occurs are determined. In order to show this effect for some relevant and representative examples of unified gauge models, we have chosen SO(10), and SU(5)SUSY, SO(10)SUSY with a particular scheme for fermion masses (DHR model). The analysis has been performed for two choices of neutrinos parameters, predicted by the above models, and capable to explain the solar neutrino problem. In both cases one observes a strong distortion in the electron neutrino energy spectrum. This effect, computed for a wide range of SO(10)SUSY models has produced the same results of the previous supersymmetric ones. More... »

PAGES

633-639

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s002880050354

DOI

http://dx.doi.org/10.1007/s002880050354

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1030168545


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