Gulden Othman
(University Of North Carolina)
2/13/20, 8:45 AM
Jan D. Behrens
2/13/20, 9:15 AM
Chelsea Bartram
(Boston University)
2/13/20, 11:00 AM
Mr
Deepak Tiwari
(PICO, Université de Montréal)
2/13/20, 11:30 AM
The PICO collaboration uses bubble chambers filled with superheated C3F8 as a target for dark matter detection. PICO-60, with a threshold of 2.45 keV, set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section at 3.2 × 10−41cm2 for a 25 GeV WIMP [Phys. Rev. D100 022001 (2019)]. Its successor PICO-40L employs...
Ryan Thomas
(University of Chicago)
2/13/20, 6:15 PM