Speaker
Yawen Xiao
Description
Detecting axion and dark photon dark matter in the milli-eV mass range has been considered being a significant challenge due to its frequency being too high for high-Q cavity resonators and too low for single-photon detectors to register. I will present a method that overcomes this difficulty (based on recent work arXiv:2208.06519) by using trapped electrons as high-Q resonators to detect axion and dark photon dark matter, and set a new limit on dark photon dark matter at 148 GHz (~0.6meV) that is around 75 times better than previous constraints by a 7 days proof-of-principle measurement. I will also propose some updates to this work that improve the result a lot by optimizing some of the experimental parameters and techniques.
Primary authors
Yawen Xiao
Peter Graham
Gerald Gabrielse
(Harvard University)
Harikrishnan Ramani
Roni Harnik
(Fermilab)
Xing Fan
Mr
Samuel Wong
(Stanford University)
Thomas Myers
Benedict Sukra