Summary
The emission of neutrino-pairs by a stellar plasma is calculated. Our expressions for longitudinal and transverse emissivities differ from the corresponding expressions of Adams, Ruderman and Woo by factors of 3/8 and 1/4, respectively.
Riassunto
Si calcola l'emissione di coppie di neutrini da un plasma stellare. Le nostre expressioni per le emissività longitudinale e trasversale differiscono dalle corrispondenti espressioni di Adams, Ruderman e Woo per fattori di 3/8 e 1/4 rispettivamente.
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References
J. B. Adams, M. A. Ruderman andC. H. Woo:Phys. Rev.,129, 1383 (1963). Hereafter referred to as ARW.
V. N. Tsytovich:Žurn. Ėksper. Teor. Fiz.,45, 1183 (1963);Sov. Phys. JETP (English translation),18, 816 (1964).
V. N. Tsytovich:Žurn. Ėksper. Teor. Fiz.,40, 1775 (1961);Sov. Phys. JETP (English translation),13, 1249 (1961).
C. L. Inman andM. A. Ruderman:Astrophys. Journ.,140, 1025 (1964).
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Supported in part by the U.S. Air Force Office of Scientific Research under Contract AF 19(628) 4019.
Traduzione a cura della Redazione.
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Zaidi, M.H. Emission of neutrino-pairs from a stellar plasma. Nuovo Cimento A (1965-1970) 40, 502–505 (1965). https://doi.org/10.1007/BF02721039
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DOI: https://doi.org/10.1007/BF02721039