Neutrino Emission, Population II Stars and Big-Band Cosmology

Details Neutrino Emission, Population II Stars and Big-Band Cosmology Neutrino Emission, Population II Stars and Big-Band Cosmology

Aug 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..12..325c&link_type=abstract

Astrophysics and Space Science, Volume 12, Issue 2, pp.325-328

Astronomy and Astrophysics

Astrophysics

Scientific paper

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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