Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering
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...
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Isfahan University of Technology
2006-03-01
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doaj-9853566357cd46b6944e7b8a325d856b2020-11-24T22:23:12ZengIsfahan University of TechnologyIranian Journal of Physics Research1682-69572006-03-01611526Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acatteringM. ZeinaliM. Haghighat 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. http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-31&slc_lang=en&sid=1Photon-neotrino interactionnon commutative spacescattering cross-section |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
M. Zeinali M. Haghighat |
spellingShingle |
M. Zeinali 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 Photon-neotrino interaction non commutative space scattering cross-section |
author_facet |
M. Zeinali M. Haghighat |
author_sort |
M. Zeinali |
title |
Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering |
title_short |
Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering |
title_full |
Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering |
title_fullStr |
Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering |
title_full_unstemmed |
Cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering |
title_sort |
cross-section for & gamma e & rarr e & nu& nu& oline and & gamma& gamma& rarr& nu& nu& oline inelastic acattering |
publisher |
Isfahan University of Technology |
series |
Iranian Journal of Physics Research |
issn |
1682-6957 |
publishDate |
2006-03-01 |
description |
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. |
topic |
Photon-neotrino interaction non commutative space scattering cross-section |
url |
http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-31&slc_lang=en&sid=1 |
work_keys_str_mv |
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