Solar g-modes cause undetectable time-varying neutrino flux fluctuations but a non-negligible net mean flux increase proportional to mode amplitude squared that may vary over the 11-year solar activity cycle.
Because of the reaction threshold, flux intensities, and the energy dependence of the cross section, the reaction predominantly occurs by solar 8B neutrons (Bahcall et al
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Solar Neutrino Flux Fluctuations Caused by Solar Gravity Modes
Solar g-modes cause undetectable time-varying neutrino flux fluctuations but a non-negligible net mean flux increase proportional to mode amplitude squared that may vary over the 11-year solar activity cycle.