Abstract

So far, the standard attitude to solve the Friedmann equations in the simultaneous presence of radiation RR, matter MM and cosmological constant ΛΛ is to find solutions RR(t)R_R (t), RM(t)R_M (t) and RΛ(t)R_Λ (t) separately for each individual component alone, and next to join them together, thereby obtaining a piecewise solution Rpw(t)R_{\rm pw} (t). We instead find the exact and analytic solution R(t)R (t) of the same equations in flat space. Moreover, we quantify the error made when Rpw(t)R_{\rm pw} (t) is used in place of R(t)R (t).

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