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>Solar Neutrinos and the Influences of Opacity, Thermal Instability, Additional Neutrino Sources, and a Central Black Hole on Solar Models
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Solar Neutrinos and the Influences of Opacity, Thermal Instability, Additional Neutrino Sources, and a Central Black Hole on Solar Models
Significant quantities that affect the internal structure of the sun are examined for factors that reduce the temperature near the sun's center. The four factors discussed are: opacity, central black hole, thermal instability, and additional neutrino sources.
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