We calculate accurately the number of solar neutrino events expected as a function of solar zenith angle, with and without neutrino oscillations, for detectors at the locations of Super-Kamiokande,… (More)

We show that the effects of neutrino oscillations on B solar neutrinos are described well by the first two moments~the average and the variance ! of the energy distribution of scattered or recoil… (More)

We point out that the assumption of Lorentz noninvariance examined recently by Coleman and Glashow leads to neutrino flavor oscillations which are phenomenologically equivalent to those obtained by… (More)

We calculate the range of predicted values for 10 quantities that will be measured by the Sudbury Neutrino Observatory~SNO!. We use neutrino oscillation solutions ~vacuum and MSW; active and sterile… (More)

1Instituto de Fı ́sica Corpuscular—C.S.I.C., Departamento de Fı ́sica Teòrica, Universitat of València, 46100 Burjassot, València, Spain 2Instituto de Fı ́sica Gleb Wataghin, Universidade Estadual de… (More)

We present a global analysis of all the available solar neutrino data treating consistently the B and hep neutrino fluxes as free parameters. The analysis reveals at 99.7% C.L. eight… (More)

We present the status of FCNC solutions to the solar neutrino problem. Our analysis shows that the FCNC solutions with massless neutrinos provide a good fit to the latest solar neutrino data.… (More)

Measurements of the interaction rates of the solar neutrino lines of Be andpep can be used, independent of solar models, to test whether electron flavor is conserved, to determine survival… (More)

We analyze the current status of the solution to the solar neutrino problem based both on: a) non-standard flavor changing neutrino interactions (FCNI) and b) non-universal flavor diagonal neutrino… (More)

If the low energy cross section for He + p → He + e + νe, the ‘hep’ reaction, is ∼ > 20 times larger than the best (but uncertain) theoretical estimates, then this reaction could significantly… (More)