Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1998-03-26
Phys.Rev. D58 (1998) 113001
Physics
High Energy Physics
High Energy Physics - Phenomenology
43 pages, 8 figures, RevTeX; to appear in Phys. Rev. D, accepted version
Scientific paper
10.1103/PhysRevD.58.113001
Energy-dependent solar neutrino flux reduction caused by the Mikheyev-Smirnov-Wolfenstein (MSW) effect is applied to the Exact Parity Model. Several scenarios are possible, depending on the region of parameter space chosen. The interplay between intergenerational MSW transitions and vacuum ``intragenerational'' ordinary-mirror neutrino oscillations is discussed. Expectations for the ratio of charged to neutral current event rates at the Sudbury Neutrino Observatory (SNO) are estimated. The implications of the various scenarios for the Boron neutrino energy spectrum and BOREXINO are briefly discussed. The consequences of MSW-induced solar neutrino depletion within the Exact Parity Model differ in interesting ways from the standard $\nu_e - \nu_{\mu, \tau}$ and $\nu_e - \nu_s$ cases. The physical causes of these differences are determined.
Volkas Raymond R.
Wong Yvonne Y. Y.
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