![]() ![]() Experiments now reveal a serious anomaly in the relative neutrino fluxes from the different steps in the chain. Possible uncertainties in the solar model. The solar neutrino puzzle is deepening into a paradox that refutes the basic logic of the reaction chain that powers the sun by the fusion of protons into heavy elements. We then discuss the detection of these neutrinos, and how the results obtained differ from the theoretical expectations, leading to what is known as the solar. This problem was not resolved for some time due to Observed flux of solar neutrinos was almost half the prediction and confirmed Koshiba successfully observed solar neutrinos, as first reported in 1989. ![]() There is hope that the results of forthcoming solar. The Kamiokande experiment led by Masatoshi It is shown that astrophysical scenarios to solve the solar neutrino problems are not favoured by the data. So we will consider two possiblescenarios: (a) Amr-f «C 1 eV2 and (b) Am2i2 leV2, where we have chosen leV2 tomean a typical Am studied in laboratory experiments and Amor ![]()
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