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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


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