Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002arep...46..255f&link_type=abstract
Astronomy Reports, Volume 46, Issue 3, March 2002, pp.255-258
Astronomy and Astrophysics
Astronomy
Scientific paper
Calculations using a standard solar model show that the decrease in proton-proton chain nuclear reaction rates due to collective plasma processes increases the theoretical solar neutrino flux, while the decrease in the opacity of the solar interior associated with the same processes decreases this flux. Taking into account both of these effects decreases the total neutrino flux, easing the solar neutrino problem.
Fedorova Alexandra V.
Tutukov Aleksandr V.
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