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Investigation of matter enhanced neutrino oscillations relevant to the solar neutrino problem
dc.contributor.authorLosecco, J. M.en_US
dc.contributor.authorBionta, Richard M.en_US
dc.contributor.authorBlewitt, G.en_US
dc.contributor.authorBratton, C. B.en_US
dc.contributor.authorCasper, David W.en_US
dc.contributor.authorClaus, R.en_US
dc.contributor.authorCortez, B. G.en_US
dc.contributor.authorErrede, S.en_US
dc.contributor.authorFoster, G. W.en_US
dc.contributor.authorGajewski, W.en_US
dc.date.accessioned2006-04-07T19:58:04Z
dc.date.available2006-04-07T19:58:04Z
dc.date.issued1987-01-29en_US
dc.identifier.citationLosecco, J. M., Bionta, R. M., Blewitt, G., Bratton, C. B., Casper, D., Claus, R., Cortez, B., Errede, S., Foster, G., Gajewski, W. (1987/01/29)."Investigation of matter enhanced neutrino oscillations relevant to the solar neutrino problem." Physics Letters B 184(2-3): 305-308. <http://hdl.handle.net/2027.42/26834>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVN-47GJ7RH-SG/2/b6f8cae2bd1c3f9f374f1289e3c1795aen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/26834
dc.description.abstractWe study the effect of matter enhanced neutrino oscillations on atmospheric neutrinos. A recently proposed solution to the solar neutrino problem with [Delta]m2 = 1.1 x 10-4 eV2 suggests enhanced effects in the range 200 MeV-500MeV. We find no evidence of this effect for v[mu]ve mixing. Limits are set on the magnitude of the mixing angle. Our limit is sin [theta] v&lt; 0.14 at 90% confidence level. The limit is dominated by statistical errors and may be improved.en_US
dc.format.extent306398 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleInvestigation of matter enhanced neutrino oscillations relevant to the solar neutrino problemen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelMathematicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherUniversity of Notre Dame, Notre Dame, IN 46556, USAen_US
dc.contributor.affiliationotherCalifornia Institute of Technology, Pasadena, CA 91125, USAen_US
dc.contributor.affiliationotherCleveland State University, Cleveland, OH 44115, USAen_US
dc.contributor.affiliationotherCalifornia Institute of Technology, Pasadena, CA 91125, USAen_US
dc.contributor.affiliationotherUniversity of California, Irvine, CA 92717, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/26834/1/0000394.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0370-2693(87)90587-9en_US
dc.identifier.sourcePhysics Letters Ben_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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