Solar model differences between CLES and Cesam2k20 are traced largely to opacity table interpolation, while turbulent mixing tuned to destroy lithium leaves CNO neutrino fluxes far below Borexino measurements.
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The impact of the transport of chemicals and electronic screening on helioseismic and neutrino observations in solar models
Solar model differences between CLES and Cesam2k20 are traced largely to opacity table interpolation, while turbulent mixing tuned to destroy lithium leaves CNO neutrino fluxes far below Borexino measurements.