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SUMMARY:[Cancelled] Neutrino and Dark Radiation Properties from Cosmic Dat
 asets - Marilena LoVerde (U. Washington\, Seattle)
DTSTART:20220523T150000Z
DTEND:20220523T160000Z
UID:TALK174704@talks.cam.ac.uk
CONTACT:Dongwon Han
DESCRIPTION:Neutrinos and other light relic particles leave a number of im
 prints in the cosmic microwave background anisotropies and on maps of the 
 large-scale structure of our Universe. These imprints can not only demonst
 rate the presence of these particles and constrain their masses\, but can 
 provide insight into their nature via signatures of interactions or other 
 behavior that changes during the history of the Universe. I will describe 
 this physics\, present constraints on non-standard neutrino self-interacti
 ons and other forms of dark radiation from cosmic datasets. I will also di
 scuss prospects for detecting neutrino mass and highlight how relic neutri
 nos force us to adopt new technology when modeling structures in the Unive
 rse today.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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