Neutron activation resolves the 71Ge M-shell X-ray line at 158.7 eVee in a CONUS+ germanium detector, reducing CEvNS signal prediction uncertainty below 4%.
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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.
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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.