Spectro-spatial evolution of the CMB I: discretisation of the thermalisation Green’s function
Publication
This paper is the first in a series of three papers on the spectro-spatial evolution of the CMB. In this paper we present a new method to solve the Kompaneets equation for the CMB photon distribution function. The method constructs a discrete set of characteristic photon spectra, which allows numerical solvers to reduce the size of the equation set by two or three orders of magnitude while also providing better physical insight to the system. This paper motivates the discretisation and shows the new method converges to expected results for the average spectrum.
The distorted CMB photon spectrum as seen today arising from energy injection at different redshifts.