Kavli Affiliate: Thomas Crawford | First 5 Authors: [#item_custom_name[1]], [#item_custom_name[2]], [#item_custom_name[3]], [#item_custom_name[4]], [#item_custom_name[5]] | Summary: Diffusion damping of the cosmic microwave background (CMB) power spectrum results from imperfect photon-baryon coupling in the pre-recombination plasma. At redshift $5 times 10^4 < z < 2 times 10^6$, the plasma acquires an effective chemical potential, and energy injections […]
Continue.. CMB-S4: Forecasting Constraints on $f_mathrm{NL}$ Through $μ$-distortion Anisotropy