University of Cambridge > Talks.cam > Cosmology Lunch > [Cancelled] Neutrino and Dark Radiation Properties from Cosmic Datasets

[Cancelled] Neutrino and Dark Radiation Properties from Cosmic Datasets

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Dongwon Han.

Zoom link: https://zoom.us/j/94455758898

Neutrinos and other light relic particles leave a number of imprints in the cosmic microwave background anisotropies and on maps of the large-scale structure of our Universe. These imprints can not only demonstrate 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-interactions and other forms of dark radiation from cosmic datasets. I will also discuss prospects for detecting neutrino mass and highlight how relic neutrinos force us to adopt new technology when modeling structures in the Universe today.

This talk is part of the Cosmology Lunch series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2022 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity