Neutrino emission from solar models with a metal-depleted core

Details Neutrino emission from solar models with a metal-depleted core Neutrino emission from solar models with a metal-depleted core

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326..392s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 1, 1988, p. 392-394.

Astronomy and Astrophysics

Astrophysics

7

Abundance, Metallicity, Solar Neutrinos, Stellar Cores, Stellar Models

Scientific paper

The authors have calculated the capture rates for the solar neutrino chlorine experiment with models in which heavy elements were removed from the core with a mass fraction 0 < qc < 0.32. The reduced central opacity leads to the reduction of the central temperature, and hence to a large reduction of the flux of neutrinos detectable with the chlorine experiment, even when the metal-depleted core has a mass fraction of only 0.05 to 0.1. No physical reason for the reduction of heavy element content in the core can be provided.

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