Speaker
Dr
Shashank Shalgar
(Univsersity of New Mexico)
Description
99% of the energy emitted by core collapse supernovae is in the form of
neutrinos. Highly non-linear effects, due to neutrino self-interactions, that are
present only in the dense environments such as a supernova core offers an
unique opportunity to study neutrino properties. We demonstrate a new technique for calculating probability of collective neutrino oscillations.
Primary author
Dr
Shashank Shalgar
(Univsersity of New Mexico)
Co-author
Prof.
Huaiyu Duan
(Univsersity of New Mexico)