Effects of magnetohydrodynamics matter density fluctuations on the solar neutrino resonant spin-flavor precession

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3048

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DC Field	Value	Language
dc.creator	Reggiani N.	-
dc.creator	Guzzo M.M.	-
dc.creator	Colonia J.H.	-
dc.creator	Holanda P.C.	-
dc.date	2000	-
dc.date.accessioned	2013-05-30T00:17:28Z	-
dc.date.available	2013-05-30T00:17:28Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332000000300018	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2000&volume=30&issue=3&spage=594	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/3048	-
dc.description	Taking into account the stringent limits from helioseismology observations on possible matter density fluctuations described by magnetohydrodynamics theory, we find the corresponding time variations of solar neutrino survival probability due to the resonant spin-flavor precession phenomenon with amplitude of order O(10%). We discuss the physics potential of high statistics real time experiments, like as Superkamiokande, to observe the effects of such magnetohydrodynamics fluctuations on their data. We conclude that these observations could be thought as a test of the resonant spin-flavor precession solution to the solar neutrino anomaly.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Effects of magnetohydrodynamics matter density fluctuations on the solar neutrino resonant spin-flavor precession	-
Appears in Collections:	Physics and Astronomy

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