Speaker
Mrs
Irene Tamborra
(Department of Physics, University of Bari & INFN, Bari)
Description
When the neutrino density is very high, as in core-collapse supernovae, neutrino-neutrino interactions are not negligible and can appreciably influence the evolution of flavor. The physics of these phenomena is briefly highlighted, and their effects are shown on observable energy spectra from a future galactic supernova. Detection of such effects could provide a handle on two unknowns: the neutrino mass hierarchy, and the 1-3 mixing angle.
Author
Mrs
Irene Tamborra
(Department of Physics, University of Bari & INFN, Bari)
Co-authors
Dr
Antonio Marrone
(Department of Physics, University of Bari & INFN, Bari)
Dr
Eligio Lisi
(INFN, Bari)
Prof.
Gianluigi Fogli
(Department of Physics, University of Bari & INFN, Bari)