Solar Neutrinos

Table 9

Expected solar neutrino rates in LENA (channel 𝜈𝑒→𝑒𝜈). The estimates are derived from the existing Borexino analyses [154, 188] as well as expectation values for the respective energy windows (EW) of observation [189–191]. The quoted fiducial masses, 𝑚_fid, in LAB are based on a Monte Carlo simulation of the external 𝛾-ray background in LENA. Table taken and adapted from [186].

Source	EW [MeV]	𝑚fid [kt]	Rate [cpd]
pp	>0.25	30	40
pep	0.8−1.4	30	2.8×10^2
70𝑥0𝑒𝑓88Be	>0.25	35	1.0×10^4
80𝑥0𝑒𝑓88B	>2.8	35	79
CNO	0.8–1.4	30	1.9×10^2