Please use this identifier to cite or link to this item: http://paper.sci.ui.ac.id/jspui/handle/2808.28/42
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dc.contributor.authorSatiawati, L.-
dc.contributor.authorSulaksono, Anto-
dc.date.accessioned2016-02-22T02:20:42Z-
dc.date.available2016-02-22T02:20:42Z-
dc.date.issued2011-11-
dc.identifier.issn23391995-
dc.identifier.urihttp://paper.sci.ui.ac.id/jspui/handle/2808.28/42-
dc.description.abstractThe differential cross-section of neutrino interaction with dense and warm electron gasses has been calculated by taking into account the neutrino electromagnetic form factors. The significant effect of electromagnetic properties of neutrino can be found if the neutrino dipole moment, μ ν , is ≥ 5.10-9 μB and neutrino charge radius, Rv, is ≥ 5.10-6 MeV-1. The importance of the retarded correction, detailed balance and Pauli blocking factors is shown and analyzed. Many-body effects on the target matter which are included via random phase approximation (RPA) correlation as well as photon effective mass are also investigated.en_US
dc.language.isoen_USen_US
dc.publisherDirectorate of Research and Community and Enggagment UIen_US
dc.relation.ispartofseriesVolume 15;No. 2-
dc.sourceMakara Journal of Science Volume 15, Nomor. 2en_US
dc.source.urihttp://journal.ui.ac.id/index.php/science/article/view/1069en_US
dc.subjectneutrinoen_US
dc.subjectsupernova atmosphereen_US
dc.subjecttemperatureen_US
dc.subjectmatter effectsen_US
dc.titleEffect of Neutrino Electromagnetic from Factors on Neutrino Interaction with Finite Temperature Electron Mattersen_US
dc.typeArticleen_US
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