Speaker
Thejs Brinckmann
(RWTH Aachen)
Description
In the next decade we will almost certainly measure the neutrino mass sum to high significance. Neutrino cosmology faces a revolution due to upcoming large-scale structure surveys such as Euclid and DESI. Although accurate modelling of non-linear scales will be crucial for reaching high levels of significance, we will have a wealth of data from other sources as well: future CMB experiments will not only complement large-scale structure data through observations of the primary CMB anisotropies and lensing, but will allow us to probe the large-scale distribution of matter through the Sunyaev-Zeldovich effect.
Primary author
Thejs Brinckmann
(RWTH Aachen)
