skip to content

Mathematical Research at the University of Cambridge

 

"The cosmic neutrino background is like the cosmic microwave back-
ground, but less photon-y and more neutrino-ey. The CNB is also less
talked about than the CMB, mostly because it’s nearly impossible to
detect directly. But if it could be detected, it would be interesting in
several ways that are discussed."

Further information

Time:

26Jan
Jan 26th 2026
13:00 to 14:00

Venue:

CMS, Pav. B, CTC Common Room (B1.19) [Potter Room]

Speaker:

Douglas Scott (University of British Columbia)

Series:

Cosmology Lunch