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.

DOI

10.3906/fiz-1401-13

Keywords

Perturbative method, spin-flavor precession, solar neutrinos, Majorana

First Page

187

Last Page

192

Recommended Citation

YILMAZ, D (2014). Perturbative approach to the spin-flavor precession of Majorana-type solar neutrinos. Turkish Journal of Physics 38 (2): 187-192. https://doi.org/10.3906/fiz-1401-13

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