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Neutrino spin-flip effects in active galactic nuclei

dc.citation.epage264en_US
dc.citation.issue3en_US
dc.citation.spage251en_US
dc.citation.volume40en_US
dc.citation.woscount2
dc.contributor.authorMughal, MAen_US
dc.contributor.authorAthar, Hen_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.date.accessioned2014-12-08T15:42:20Z
dc.date.available2014-12-08T15:42:20Z
dc.date.issued2002-06-01en_US
dc.description.abstractWe study the effects of neutrino spin-flips in the magnetic field, BAGN, of an active galactic nuclei (AGN) for high-energy neutrinos (E greater than or equal to 10(6) GeV) originating from the AGN, induced by an interplay of a violation of the equivalence principle parameterized by Deltaf and the twist in B-AGN. We point out that a conversion effect may exist for Deltaf similar to 10(-34)(deltam(2)/10(-5) eV(2)) independent of the gravity mixing angle. Observational consequences for this conversion effect are discussed.en_US
dc.identifier.issn0577-9073en_US
dc.identifier.journalCHINESE JOURNAL OF PHYSICSen_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/28748
dc.identifier.wosnumberWOS:000176171700006
dc.language.isoen_USen_US
dc.titleNeutrino spin-flip effects in active galactic nucleien_US
dc.typeArticleen_US

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