Orateur
Masaya Hasegawa
(KEK)
Description
The frontier of cosmic microwave background (CMB) studies is to measure the CMB polarization. It provides a unique and powerful way to explore cosmic inflation, neutrino masses, and other possible light relics such as Axions.
In this talk, I will present an overview and status of two CMB polarization projects in the Atacama Desert, Chile; Simons Array and Simons Observatory.
Auteur principal
Masaya Hasegawa
(KEK)
