Solar Neutrino Physics Explained in 60 Seconds
Solar neutrino physics studies neutrinos produced by nuclear fusion in the Sun's core, where hydrogen fuses into helium, releasing energy and neutrinos. These neutrinos are nearly massless, neutral particles that rarely interact with matter, allowing them to escape the Sun and reach Earth almost undisturbed.
Scientists detect solar neutrinos to understand the Sun's energy generation and test fundamental physics. Early experiments, like the Homestake experiment, detected fewer neutrinos than predicted—a mystery called the "solar neutrino problem." It was resolved when we discovered neutrino oscillation, where neutrinos change types (flavors) as they travel, implying they have mass.
Solar neutrino studies confirm our models of stellar fusion, provide insights into particle physics, and deepen our understanding of the universe.
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