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dc.contributor.authorNARAYAN, Men_US
dc.contributor.authorRAJASEKARAN, Gen_US
dc.contributor.authorSANKAR, SUen_US
dc.date.accessioned2011-07-17T22:08:35Zen_US
dc.date.accessioned2011-12-26T12:50:31Zen_US
dc.date.accessioned2011-12-27T05:35:41Z-
dc.date.available2011-07-17T22:08:35Zen_US
dc.date.available2011-12-26T12:50:31Zen_US
dc.date.available2011-12-27T05:35:41Z-
dc.date.issued1998en_US
dc.identifier.citationPHYSICAL REVIEW D, 58(3), -en_US
dc.identifier.issn0556-2821en_US
dc.identifier.urihttp://dspace.library.iitb.ac.in/xmlui/handle/10054/4852en_US
dc.identifier.urihttp://hdl.handle.net/10054/4852-
dc.description.abstractWe analyze the recent result of the CHOOZ Collaboration in the context of mixing and oscillations between all the three neutrino flavors. If one assumes the hierarchy among the vacuum mass eigenvalues delta(21) much less than delta(31) Where delta(21) = mu(22) - mu(1)(2) and delta(31) = mu(3)(2) - mu(1)(2), then the CHOOZ result puts a strong constraint on the allowed values of the (13) mixing angle phi. It is also shown that, in light of the CHOOZ result, the maximum contribution of the nu(mu) <-> nu(e) oscillation channel to the atmospheric neutrino anomaly is less than 7 percent, thus demonstrating that the atmospheric neutrino anomaly is mainly due to nu(mu) <-> nu(tau) oscillations. Most importantly the CHOOZ result now excludes a large part of the three flavor parameter space which was previously allowed as solutions to the solar and atmospheric neutrino problems. [S0556-2821(98)50415-8]en_US
dc.language.isoenen_US
dc.publisherAMERICAN PHYSICAL SOCen_US
dc.subjectOscillationsen_US
dc.subjectSolaren_US
dc.titleThree flavor implications of the result of the CHOOZ Collaborationen_US
dc.typeArticleen_US
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