Large Extra Dimensions, Sterile neutrinos and Solar Neutrino Data

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dc.creatorCaldwell, D. O.
dc.creatorMohapatra, R. N.
dc.creatorYellin, S. J.
dc.date2000-10-31
dc.date2001-06-04
dc.date.accessioned2026-07-07T11:09:04Z
dc.date.available2026-07-07T11:09:04Z
dc.descriptionSolar, atmospheric and LSND neutrino oscillation results require a light sterile neutrino, $ν_B$, which can exist in the bulk of extra dimensions. Solar $ν_e$, confined to the brane, can oscillate in the vacuum to the zero mode of $ν_B$ and via successive MSW transitions to Kaluza-Klein states of $ν_B$. This new way to fit solar data is provided by both low and intermediate string scale models. From average rates seen in the three types of solar experiments, the Super-Kamiokande spectrum is predicted with 73% probability, but dips characteristic of the 0.06 mm extra dimension should be seen in the SNO spectrum.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0010353
dc.identifierhttp://arxiv.org/abs/hep-ph/0010353
dc.identifierPhys.Rev.Lett.87:041601,2001
dc.identifierdoi:10.1103/PhysRevLett.87.041601
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190344
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLarge Extra Dimensions, Sterile neutrinos and Solar Neutrino Data
dc.typetext

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