Quasi-sterile neutrinos from dark sectors
Daniele Alves - Los Alamos National Laboratory
Yu, T. (2022). Solar Neutrinos: from background to signal. Perimeter Institute. https://pirsa.org/22030020
Yu, Tien-Tien. Solar Neutrinos: from background to signal. Perimeter Institute, Mar. 08, 2022, https://pirsa.org/22030020
@misc{ pirsa_PIRSA:22030020,
doi = {10.48660/22030020},
url = {https://pirsa.org/22030020},
author = {Yu, Tien-Tien},
keywords = {Particle Physics},
language = {en},
title = {Solar Neutrinos: from background to signal},
publisher = {Perimeter Institute},
year = {2022},
month = {mar},
note = {PIRSA:22030020 see, \url{https://pirsa.org}}
}
Solar neutrinos are an inevitable background to any dark matter direct detection experiment as they closely mimic the signature of dark matter. In this talk, I will discuss the effects of solar neutrinos on the reach of dark matter-electron scattering experiments, with a focus on semiconductor and xenon-based detectors. In addition, I will present the prospects of measuring and understanding the various solar neutrino components using the same detectors, as well as the effects of non-standard neutrino interactions, thus turning solar neutrinos from a background to an interesting signal in their own right.