On Resonances and Mixing Angles in Three Neutrino Oscillations in Matter

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/2243

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DC Field	Value	Language
dc.creator	Bellandi J.	-
dc.creator	Guzzo M.M.	-
dc.creator	Aquino V.M.	-
dc.date	1997	-
dc.date.accessioned	2013-05-29T22:02:40Z	-
dc.date.available	2013-05-29T22:02:40Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97331997000300008	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=1997&volume=27&issue=3&spage=	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/2243	-
dc.description	We find exact analytical expressions for mixing angles in matter in the context of three generation neutrino oscillations in matter to discuss the role of resonances in this phenomenon. We show that some knowledge from conventional two neutrino MSW effect, which has been extended to approximated solutions to three neutrino oscillations, has to be abandoned in this exact approach. We observe that maximal values for the mixing angles in matter are found in nonresonant regions and stationary phases do not coincide anymore with resonances in this simple extension of the MSW effect. We present a general way to identify a resonance and discuss what we can physically expect in these regions	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	On Resonances and Mixing Angles in Three Neutrino Oscillations in Matter	-
Appears in Collections:	Physics and Astronomy

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