-
14:00
Team 1a: Direct detection below neutrino floor
-
Adam Davis
(University of Cincinnati (US))
-
14:18
Team 1b: Direct detection below neutrino floor
-
Alden Fan
(UCLA)
Dan Jardin
(Southern Methodist University)
Jayden Newstead
(Arizona State University)
-
14:36
Team 3: Devise prediction using Dark Sky simulation
-
Andrew Scacco
(UC Davis)
Devon Powell
(Stanford)
-
14:54
Team 5: DM signal vs astrophysical sources
-
Anna Kwa
(UC Irvine)
Helen Poon
(Max Planck Institut fur Kernphysik)
Mathieu Boudaud
(LAPTh)
-
15:12
Team 8: How to detect invisible Higgs decays
-
Asher Berlin
(University of Chicago)
-
15:30
Team 10: LHC missing Et excess => DM signal ?
-
Cristian Ignacio Pena Herrera
(California Institute of Technology (US))
Sebastian Liem
(NIKHEF (NL))
-
15:48
Team 11: Direct detection down to 100 MeV
-
Geertje Heuermann
(KIT)
Nadine Foerster
(KIT)
-
16:24
Team 13: Maximum mass of DM particle
-
Elwin Martin
(UCLA)
William Jay
(University of Colorado)
-
16:42
Team 16: How to tell if axion is 20% of DM signal ?
-
Daniel Egana
(Rutgers University)
Dustin Lorshbough
(Univ of Texas, Austin)
Ignacio Izaguirre
(MPP)
-
17:00
Team 17: Observations to distinguish CDM from other models
-
Stephen Portillo
(Harvard University)
-
17:18
Team 19: How to distinguish decaying and stable DM ?
-
Lene Bryngemark
(Lund University (SE))
Rebecca Carney
(University of Edinburgh (GB))
Siim Tolk
(NIKHEF (NL))
-
17:36
Team 20: Constrain density slope in the Milkyway
-
Anjali Tripathi
(Harvard University)
Hamish Silverwood
(University of Amsterdam)
Weishi Li
(Ohio State U)
Zachary Slepian
(H)
