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Oliver Schulz (MPI for Physics, Munich)13/02/2020, 08:30
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Gulden Othman (University Of North Carolina)13/02/2020, 08:45
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Ashley Back (Queen Mary, University of London)13/02/2020, 09:00
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Jan D. Behrens13/02/2020, 09:15
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Yonatan Kahn (University of Illinois at Urbana-Champaign)13/02/2020, 09:30
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Michael De Nuccio13/02/2020, 10:45
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Chelsea Bartram (Boston University)13/02/2020, 11:00
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Enze Zhang13/02/2020, 11:15
The SuperCDMS SNOLAB experiment is designed to be a next generation dark matter direct detection experiment, following SuperCDMS Soudan. The experiment is currently under construction. The main science goal is to improve the sensitivity for dark matter particles with masses ≤10 GeV by at least one order of magnitude in cross section over current results from the SuperCDMS Soudan experiment....
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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...
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Sean Daugherty13/02/2020, 17:45
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Marie-Cécile Piro (University of Alberta)13/02/2020, 18:00
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Ryan Thomas (University of Chicago)13/02/2020, 18:15
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Holger Müller13/02/2020, 18:30
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Hafizh Prihtiadi (Bandung Institute of Technology)
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Yi Wang
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