Difference between revisions of "UCSD-2019: Science Theme: Dark Universe"

From CMB-S4 wiki
Jump to navigationJump to search
Line 20: Line 20:
 
'''14:00''' - George Fuller - '' more neutrino science from high-ell '' (10+5)
 
'''14:00''' - George Fuller - '' more neutrino science from high-ell '' (10+5)
  
'''14:15''' - Vera Gluscevic - '' dark matter targets and measurement requirements '' (10+5)
+
'''14:15''' - Vera Gluscevic - '' dark matter physics with CMB-S4 '' (10+5) [[:Gluscevic-dark-matter-UCSD2019.pdf|slides]]
  
 
'''14:30''' - Michael Fedderke - '' axion dark matter from polarization angle '' (10+5)
 
'''14:30''' - Michael Fedderke - '' axion dark matter from polarization angle '' (10+5)

Revision as of 21:12, 16 October 2019

Link back to agenda

Charge

Copied from "Specific charges for non-L2 sessions":

  • Review science goals
  • Review/update/prioritize questions to be answered regarding measurement requirements
  • Identify priorities for science case development, if any

Agenda

13:30 - Dan Green - light relics targets and measurement requirements (10+5)

13:45 - Darcy Barron - potential CD1 questions for high-ell science (10+5)

14:00 - George Fuller - more neutrino science from high-ell (10+5)

14:15 - Vera Gluscevic - dark matter physics with CMB-S4 (10+5) slides

14:30 - Michael Fedderke - axion dark matter from polarization angle (10+5)

14:45 - Suvodip Mukherjee - axion detection from clusters (10+5)

15:00 - Discussion - what questions need to be answered by the new working groups (30)

Remote Attendance

Zoom link

Notes