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Neutrino emission, population II stars and big-bang cosmology

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Abstract

The spectroscopic determination of the helium abundance in the oldest stars of the galaxy is supported by the theory of stellar evolution when neutrino emission is considered according to the photon-neutrino coupling theory, if it is assumed that the population II stars started their life with a low surface helium content.

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Authors and Affiliations

  1. Electronics Division, Indian Statistical Institute, Calcutta, India

    Probhas Ray Chaudhuri

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  1. Probhas Ray Chaudhuri
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Chaudhuri, P.R. Neutrino emission, population II stars and big-bang cosmology. Astrophys Space Sci 12, 325–328 (1971). https://doi.org/10.1007/BF00651422

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  • DOI: https://doi.org/10.1007/BF00651422

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