Solar Neutrinos

Table 6

Best estimates for the pep and CNO solar neutrino interaction rates. For the results in the last two columns both statistical and systematic uncertainties are considered. Total fluxes have been obtained assuming MSW-LMA and using the scattering cross-sections from [146, 148, 149] and a scintillator 𝑒⁻ density of (3.307±0.003)⋅10²⁹ton⁻¹. The last column gives the ratio between our measurement and the high-Z (GS98) SSM [64]. Table taken from [74].

𝜈	Interaction rate	Solar-𝜈 flux	Data/SSM
	[counts/(day · 100 ton)]	[10^8cm^−2s^−1]	ratio
pep	3.1±0.6stat±0.3syst	1.6±0.3	1.1±0.2
CNO	<7.9 (<7.1statonly)	<7.7	<1.5