Gulden Othman
(University Of North Carolina)
13/02/2020, 08:45
Jan D. Behrens
13/02/2020, 09:15
Chelsea Bartram
(Boston University)
13/02/2020, 11:00
Mr
Deepak Tiwari
(PICO, Université de Montréal)
13/02/2020, 11:30
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)
13/02/2020, 18:15