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Information Journal Paper

Title

CROSS-SECTION FOR YE →EVV (BAR) AND YY→VV (BAR) INELASTIC SCATTERING

Pages

  15-26

Abstract

 We study processes in which neutrinos can be generated as a possible source for the neutron emission form neutron stars. In the high energy limit and in the range em < E < Mw the cross sention for ge →ev`v is analytically calculated. We also calculate the cross section for gg→v`v in the noncommutative space. The obtained results in comparison with the cross section for gg→v`v and gg→gv`v in the commutative space could be quite important in the astrophysics. As a result the cross section for gg→v`v in the noncommutative spaces, in the range A = 100- 300Ge V, is comparable with its counterpart in the commutative space.
 

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    APA: Copy

    ZEYNALI, M., & HAGHIGHAT, M.. (2006). CROSS-SECTION FOR YE →EVV (BAR) AND YY→VV (BAR) INELASTIC SCATTERING. IRANIAN JOURNAL OF PHYSICS RESEARCH, 6(1), 15-26. SID. https://sid.ir/paper/1948/en

    Vancouver: Copy

    ZEYNALI M., HAGHIGHAT M.. CROSS-SECTION FOR YE →EVV (BAR) AND YY→VV (BAR) INELASTIC SCATTERING. IRANIAN JOURNAL OF PHYSICS RESEARCH[Internet]. 2006;6(1):15-26. Available from: https://sid.ir/paper/1948/en

    IEEE: Copy

    M. ZEYNALI, and M. HAGHIGHAT, “CROSS-SECTION FOR YE →EVV (BAR) AND YY→VV (BAR) INELASTIC SCATTERING,” IRANIAN JOURNAL OF PHYSICS RESEARCH, vol. 6, no. 1, pp. 15–26, 2006, [Online]. Available: https://sid.ir/paper/1948/en

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