We show that with the muon neutrino mass which is necessary for explaining the solar neutrino problem through MSW mechanism, m(nu mu) similar to 2 x 10(-3) eV and m(nu tau) similar to (m(t)/m(c))(2)m(nu mu), we expect different spectra for nu(e) and nu(e) ($) over bar ($) over bar coming from supernovae.
MSW PROCESS IN SUPERNOVAE / Buccella, F; Esposito, S; Gualdi, C; Santorelli, P. - In: MODERN PHYSICS LETTERS A. - ISSN 0217-7323. - 10:3(1995), pp. 179-181. [10.1142/S021773239500020X]
MSW PROCESS IN SUPERNOVAE
ESPOSITO S;SANTORELLI P
1995
Abstract
We show that with the muon neutrino mass which is necessary for explaining the solar neutrino problem through MSW mechanism, m(nu mu) similar to 2 x 10(-3) eV and m(nu tau) similar to (m(t)/m(c))(2)m(nu mu), we expect different spectra for nu(e) and nu(e) ($) over bar ($) over bar coming from supernovae.File in questo prodotto:
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