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. Dear user; Recently we have changed our software to Sinaweb. If you had already registered with the old site, you may use the same USERNAME but you need to change your password. To do so at the first use, please choose, 2019; 6(1): 15-26.
