Exotic Solutions to the Solar Neutrino Anomaly

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3196

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DC Field	Value	Language
dc.creator	Guzzo M. M.	-
dc.date	2001	-
dc.date.accessioned	2013-05-30T00:53:12Z	-
dc.date.available	2013-05-30T00:53:12Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000200017	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=2&spage=263	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/3196	-
dc.description	We analyze the status of the exotic solutions to the solar neutrino problem, i.e., those solutions based on new phenomena which are not the usual neutrino oscillations induced by masses and mixing. These solutions are based on different assumptions: a) resonant spin-flavor precession induced by non-vanishing neutrino magnetic moment, b) the existence of non-standard flavor-changing and non-universal neutrino interactions and c) the violation of the equivalence principle. We investigate the quality of the fit provided by each one of these solutions not only to the total rate measured by all solar neutrino experiments but also to the day-night and seasonal variations of the event rate, as well as the recoil electron energy spectrum measured by the SuperKamiokande collaboration.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Exotic Solutions to the Solar Neutrino Anomaly	-
Appears in Collections:	Physics and Astronomy

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