Precision cosmology made more precise
Abstract
So far, the standard attitude to solve the Friedmann equations in the simultaneous presence of radiation R, matter M and cosmological constant is to find solutions RR (t), RM (t) and R (t) separately for each individual component alone, and next to join them together, thereby obtaining a piecewise solution R pw (t). We instead find the exact and analytic solution R (t) of the same equations in flat space. Moreover, we quantify the error made when R pw (t) is used in place of R (t).
0