Difference between revisions of "UCSD-2019: Science Theme: Dark Universe"
From CMB-S4 wiki
Jump to navigationJump to search (→Agenda) |
m (→Agenda) |
||
| 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 | + | '''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 22:12, 16 October 2019
Contents
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)
