Authors: DENİZ YILMAZ
Abstract: Spin-flavor precession (SFP) of Majorana-type solar neutrinos is investigated in the case of 2 generations. The evolution equation in the SFP framework is solved by using the perturbative method, in which mu B is accepted to be small. The approximate analytical formula including SFP effect is provided.
Keywords: Perturbative method, spin-flavor precession, solar neutrinos, Majorana
Full Text: PDF