The Solar Solution: Tracking the Sun with Low Energy Neutrinos
Abstract
As neutrinos become a significant background for projected dark matter experiments, the community will become concerned with determining if events counted in a dark matter experiment are good dark matter candidates or low-energy neutrinos from astrophysical sources. We investigate the feasibility of using neutrino-electron scattering in a terrestrial detector medium as a means to determine the flight direction of the original, low-energy solar neutrino.Using leading-order weak interactions in the Standard Model and constrains from energy and momentum conservation, we developed a simple simulation that suggests that 68% of the time the ejected electron would be within 0.99 radians of the incident neutrino's direction. This suggests that it may be fruitful to pursue low-energy neutrino detection capability that can utilize such ejected electrons.
Cite
@article{arxiv.1605.01787,
title = {The Solar Solution: Tracking the Sun with Low Energy Neutrinos},
author = {Nicole Hartman and Stephen Sekula},
journal= {arXiv preprint arXiv:1605.01787},
year = {2016}
}