New Directions in Dark Matter Direct Detection
APA
Yu, T. (2017). New Directions in Dark Matter Direct Detection. Perimeter Institute. https://pirsa.org/17040029
MLA
Yu, Tien-Tien. New Directions in Dark Matter Direct Detection. Perimeter Institute, Apr. 04, 2017, https://pirsa.org/17040029
BibTex
@misc{ pirsa_PIRSA:17040029, doi = {10.48660/17040029}, url = {https://pirsa.org/17040029}, author = {Yu, Tien-Tien}, keywords = {Particle Physics}, language = {en}, title = {New Directions in Dark Matter Direct Detection}, publisher = {Perimeter Institute}, year = {2017}, month = {apr}, note = {PIRSA:17040029 see, \url{https://pirsa.org}} }
Sub-GeV dark matter is a theoretically motivated but largely unexplored paradigm of dark matter. In this talk, I will discuss recent work on the direct detection of sub-GeV dark matter through dark matter-electron scattering. I will present some motivated models that can be probed with these techniques as well as projections for current and near-term noble liquid, semiconductor, and scintillator experiments. Finally, I will discuss some new techniques that may allow us to more robustly discriminate between dark matter signatures and background.