English

Precision cosmology made more precise

Cosmology and Nongalactic Astrophysics 2021-02-03 v1

Abstract

So far, the standard attitude to solve the Friedmann equations in the simultaneous presence of radiation RR, matter MM and cosmological constant Λ{\Lambda} is to find solutions RR(t)R_R (t), RM(t)R_M (t) and RΛ(t)R_{\Lambda} (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).

Keywords

Cite

@article{arxiv.2102.01637,
  title  = {Precision cosmology made more precise},
  author = {Giorgio Galanti and Marco Roncadelli},
  journal= {arXiv preprint arXiv:2102.01637},
  year   = {2021}
}

Comments

9 pages, 3 figures

R2 v1 2026-06-23T22:46:25.491Z