Sensitivity of a low threshold directional detector to CNO-cycle solar neutrinos
Abstract
A first measurement of neutrinos from the CNO fusion cycle in the Sun would allow a resolution to the current solar metallicity problem. Detection of these low-energy neutrinos requires a low-threshold detector, while discrimination from radioactive backgrounds in the region of interest is significantly enhanced via directional sensitivity. This combination can be achieved in a water-based liquid scintillator target, which offers enhanced energy resolution beyond a standard water Cherenkov detector. We study the sensitivity of such a detector to CNO neutrinos under various detector and background scenarios, and draw conclusions about the requirements for such a detector to successfully measure the CNO neutrino flux. A detector designed to measure CNO neutrinos could also achieve a few-percent measurement of pep neutrinos.
Keywords
Cite
@article{arxiv.1803.07109,
title = {Sensitivity of a low threshold directional detector to CNO-cycle solar neutrinos},
author = {R. Bonventre and G. D. Orebi Gann},
journal= {arXiv preprint arXiv:1803.07109},
year = {2018}
}