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dc.contributor.authorChyi, TKen_US
dc.contributor.authorHwang, CWen_US
dc.contributor.authorKao, WFen_US
dc.contributor.authorLin, GLen_US
dc.contributor.authorNg, KWen_US
dc.contributor.authorTseng, JJen_US
dc.date.accessioned2014-12-08T15:46:03Z-
dc.date.available2014-12-08T15:46:03Z-
dc.date.issued1999-11-04en_US
dc.identifier.issn0370-2693en_US
dc.identifier.urihttp://hdl.handle.net/11536/30971-
dc.description.abstractWe study the neutrino-photon processes such as gamma gamma --> <v(v)over bar>, v gamma --> v gamma, and <v(v)over bar> --> gamma gamma in a background magnetic field smaller than the critical magnetic field Bc + m(e)(2)/e. Using Schwinger's formalism, we extract leading magnetic-field contributions to the above processes. Our result is valid throughout the kinematic regime where both neutrino and photon energies are significantly smaller than m(w). We briefly discuss the astrophysical implications of our result. (C) 1999 Published by Elsevier Science B.V. All rights reserved.en_US
dc.language.isoen_USen_US
dc.titleNeutrino-photon scattering and its crossed processes in a background magnetic fielden_US
dc.typeArticleen_US
dc.identifier.journalPHYSICS LETTERS Ben_US
dc.citation.volume466en_US
dc.citation.issue2-4en_US
dc.citation.spage274en_US
dc.citation.epage280en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000083810900028-
dc.citation.woscount11-
Appears in Collections:Articles


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