We study processes in which neutrinos can be generated as a possible source for the neutrion emission form neutron stars. In the high energy limit and in the range em< E< Mw the cross sention for ye→evv is analytically calculated. We also calculate the cross section for yy→vv in the noncommutative space. The obtained results in comparison with the cross section for yy→vv and yy→ yvv in the commutative space could be quite important in the astrophysics. As a result the cross section for yy→ vv in the noncommutative spaces, in the range =100-300Gev , is comparable with its counterpart in the commutative space.
Zeinali,M and Haghighat,M . (2019). Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering. Iranian Journal of Physics Research, 6(1), 15-26.
MLA
Zeinali,M , and Haghighat,M . "Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering", Iranian Journal of Physics Research, 6, 1, 2019, 15-26.
HARVARD
Zeinali M, Haghighat M. (2019). 'Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering', Iranian Journal of Physics Research, 6(1), pp. 15-26.
CHICAGO
M Zeinali and M Haghighat, "Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering," Iranian Journal of Physics Research, 6 1 (2019): 15-26,
VANCOUVER
Zeinali M, Haghighat M. Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering. Iranian Journal of Physics Research. 2019;6(1):15-26 (In Persian).
