Neutrino and antineutrino elastic scattering and photoneutrino reactions

dc.contributor.authorAydın, Zeki Zekeriya
dc.contributor.departmentFen Fakültesitr_TR
dc.date.accessioned2020-02-17T11:59:48Z
dc.date.available2020-02-17T11:59:48Z
dc.date.issued1983
dc.description.abstractThe processes ν ν → ν ν , ν ¯ ν → ν ¯ ν , ν ¯ ν → 2 γ , and ν γ → ν γ , which are of astrophysical interest, are calculated both in the electroweak model and in the magnetic model when the neutrino has a small magnetic moment κ . Received 31 January 1983
dc.description.indexScopus
dc.description.indexScopus
dc.description.indexWos
dc.identifier.endpage2874tr_TR
dc.identifier.issn/e-issn1550-2368
dc.identifier.issn/e-issn1550-7998
dc.identifier.issue11tr_TR
dc.identifier.startpage2872tr_TR
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.28.2872tr_TR
dc.identifier.urihttp://hdl.handle.net/20.500.12575/69612
dc.identifier.volume28tr_TR
dc.language.isoentr_TR
dc.relation.isversionof10.1103/PhysRevD.28.2872tr_TR
dc.relation.journalPhysical Review D - Particles, Fields, Gravitation and Cosmologytr_TR
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıtr_TR
dc.rightsCC0 1.0 Universal*
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/*
dc.titleNeutrino and antineutrino elastic scattering and photoneutrino reactionstr_TR
dc.typeArticletr_TR

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