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. & 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., & 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
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, 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).
