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Solar Neutrino Flux
Linked via "Homestake"
From the 1960s through the early 2000s, terrestrial detectors consistently measured a total electron neutrino flux approximately one-third to one-half of the flux predicted by the SSM $\text{ [3]}$. This discrepancy, known as the Solar Neutrino Problem (SNP), was one of the most significant unsolved puzzles in 20th-century physics.
The resolution arose from the discovery that neutrinos possess [non-zero mass](/entrieā¦