A Retrospective on the Design and Characterization of Simons Observatory’s Detectors
SLAC, Kavli 2nd Floor Conf. Room
Zoom info: https://stanford.zoom.us/j/868697145
SLAC, Kavli 2nd Floor Conf. Room
Zoom info: https://stanford.zoom.us/j/868697145
SLAC, Kavli 2nd Floor Conf. Room
Zoom info: zoom (https://stanford.zoom.us/j/868697145)
Please email mmebrat1@stanford.edu for zoom password.
SLAC, Kavli 3rd Floor Conf. Room
SLAC, Building 053, Trinity Conf. Room
SLAC, Kavli 3rd Floor Conf. Room
SLAC, Building 048, Redwood C/D
SLAC, Kavli 3rd Floor Conf. Room
Zoom
Zoom info: https://stanford.zoom.us/j/91603226165?pwd=eDMyQTlFZ04yQzJUR0tFbGxJZXEzQT09
Passcode (033843)
Particulate dark matter is a long hypothesized solution to various astrophysical observations seemingly at odds with a completely luminous universe. Despite the success of dark matter in explaining these observations, to date physicists have been unable to conclusively observe its interactions with Standard Model matter directly.
Zoom
Zoom
Zoom https://stanford.zoom.us/j/94163224948?pwd=cks1VVg3Q3FlSU44UVYrOXFMRU5E…
Passcode (987480)
In the direct detection of dark matter with masses down to O(keV), the energies im- parted in the detector become vanishingly small. Many novel ideas have been proposed for instrumenting athermal phonon sensors on Fermi-degenerate materials [1], polar crys- tals [2–4], and CVD diamond [5], requiring detector energy thresholds of O(1−100) meV.