The calculated CEvNS rates and kinetic energy spectrums for 8B solar neutrinos are needed to evaluate the CEvNS detection of geo-neutrinos.
Similarly, calculated CEvNS rates and kinetic energy spectrums for 8B solar neutrinos and geo-neutrinos are needed to evaluate the CEvNS detection of reactor antineutrinos.
This is a companion task to PR #577.
The calculated CEvNS rates and kinetic energy spectrums for 8B solar neutrinos are needed to evaluate the CEvNS detection of geo-neutrinos.
Similarly, calculated CEvNS rates and kinetic energy spectrums for 8B solar neutrinos and geo-neutrinos are needed to evaluate the CEvNS detection of reactor antineutrinos.