Speaker
Chandra Shekhar Saraf
(Korea Astronomy and Space Science Institute)
Description
In the era of high precision Cosmic Microwave Background (CMB) anisotropy measurements, detection of primordial B-modes polarisation will be one of the goals of the current and upcoming CMB experiments. In this talk I will present the methodology of detecting B-modes from Simons Observatory-like CMB experiment. I will also discuss how including probes of large scale structure can improve the measurement of tensor-to-scalar ratio.