Table 9: Expected solar neutrino rates in LENA (channel ). The estimates are derived from the existing Borexino analyses [154, 188] as well as expectation values for the respective energy windows (EW) of observation [189191]. The quoted fiducial masses, , in LAB are based on a Monte Carlo simulation of the external -ray background in LENA. Table taken and adapted from [186].

Source EW [MeV] [kt] Rate [cpd]

pp 0.25 30 40
pep 0.8−1.4 30
Be 0.25 35
B 2.8 35 79
CNO 0.8–1.4 30