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1. Solar Neutrino Flux

   Linked via "Solar Neutrino Problem"

   The $^8\text{B}$ decay is particularly important as it yields the highest-energy neutrinos detectable on Earth, which were central to early flux discrepancies.
   The theoretical integrated flux $\Phi_{\nu}^{\text{theory}}$ is highly sensitive to the precise temperature profile of the solar core, often modeled using the Standard Solar Model (SSM). Deviations from the SSM predictions led to the famous [Solar Neutrino Problem](/entri…

2. Solar Neutrino Flux

   Linked via "Solar Neutrino Problem (SNP)"

   The Solar Neutrino Problem and Flavor Oscillation
   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 [neutrino…