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.
Perturbative method, spin-flavor precession, solar neutrinos, Majorana
"Perturbative approach to the spin-flavor precession of Majorana-type solar neutrinos,"
Turkish Journal of Physics: Vol. 38:
2, Article 4.
Available at: https://journals.tubitak.gov.tr/physics/vol38/iss2/4