Speaker
Carlo Baccigalupi
(SISSA)
Description
We review the expected impact of high precision measurements of the B-Mode of CMB anisotropies onto the tensions in the Cosmological Concordance Model. We focus on the reconstruction of the expansion history through cosmological gravitational lensing of the CMB, and discuss the existing constraints on tensions from operating CMB B-Mode probes and the expected ones for the future network of ground based and satellite missions.
Primary author
Carlo Baccigalupi
(SISSA)
