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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Main Authors: M. Zeinali, M. Haghighat
Format: Article
Language:English
Published: Isfahan University of Technology 2006-03-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-31&slc_lang=en&sid=1
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spelling 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
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