Solar Neutrinos: from background to signal
APA
Yu, T. (2022). Solar Neutrinos: from background to signal. Perimeter Institute. https://pirsa.org/22030020
MLA
Yu, Tien-Tien. Solar Neutrinos: from background to signal. Perimeter Institute, Mar. 08, 2022, https://pirsa.org/22030020
BibTex
@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.