Large Extra Dimensions, Sterile neutrinos and Solar Neutrino Data

Details Large Extra Dimensions, Sterile neutrinos and Solar Neutrino Data Large Extra Dimensions, Sterile neutrinos and Solar Neutrino Data

2000-10-31

arxiv.org/abs/hep-ph/0010353v2

Phys.Rev.Lett.87:041601,2001

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 2 figures

Scientific paper

10.1103/PhysRevLett.87.041601

Solar, atmospheric and LSND neutrino oscillation results require a light sterile neutrino, $\nu_B$, which can exist in the bulk of extra dimensions. Solar $\nu_e$, confined to the brane, can oscillate in the vacuum to the zero mode of $\nu_B$ and via successive MSW transitions to Kaluza-Klein states of $\nu_B$. 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.

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