Massless neutrinos and the stellar stopping power via the V-A and Weinberg interactions

Physics – General Physics

Scientific paper

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Antineutrinos, Elementary Particle Interactions, Neutrinos, Solar Neutrinos, Stellar Radiation, Stopping Power, Weak Energy Interactions, Cosmology, Energy Dissipation, Particle Mass, Q Factors

Scientific paper

A formula for the stopping power of matter for neutrinos and antineutrinos, interacting with electrons via the weak interaction in the context of both the conventional V-A theory and the Weinberg theory is derived in the high-Q approximation and applied to study the solar-neutrino anomaly. The neutrinos' energy loss caused inside the sun is found to be completely insignificant compared to their original energy, and hence they escape into space with undiminished energy. The energy of stellar neutrinos remains essentially undiminished as they traverse the universe, and they should be distributed uniformly throughout it.

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