Propagation and Oscillation of Neutrinos with Magnetic Moment Inside the Sun

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3579

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2008-09-12T11:02:52Z	-
dc.date.available	2008-09-12T11:02:52Z	-
dc.date.issued	1990	-
dc.identifier.citation	IAU Symposium, No. 142, pp. 63 - 64	en
dc.identifier.issn	0074-1809	-
dc.identifier.uri	http://hdl.handle.net/2248/3579	-
dc.description.abstract	The VVO mechanism suggests that the existence of a neutrino magnetic moment would lead to variations of the observed solar neutrino flux with the magnetic activity of the sun. The MSW mechanism suggests neutrino oscillations in the dense plasma solar interior. Assuming a non- vanishing neutrino magnetic moment and a magnetic field gradient increasing towards the solar core as required in some dynamo models, the combined effects of the oscillations and the flipping on neutrino propagation in the solar interior is studied. The effects of charge is scattering cross- section is also considered.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..142...63S	en
dc.subject	Oscillation of Neutrinos	en
dc.subject	Magnetic activities of the Sun	en
dc.title	Propagation and Oscillation of Neutrinos with Magnetic Moment Inside the Sun	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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