On Problems with Cosmography in Cosmic Dark Ages
arXiv:2009.04109 · doi:10.1016/j.physletb.2021.136366
Abstract
Quasars show considerable promise as standard candles in a high-redshift window beyond Type Ia supernovae. Recently, Risaliti, Lusso \& collaborators \cite{Risaliti:2018reu, Lusso:2019akb, Lusso:2020pdb} have succeeded in producing a high redshift Hubble diagram () that supports "a trend whereby the Hubble diagram of quasars is well reproduced by the standard flat CDM model up to , but strong deviations emerge at higher redshifts". This conclusion hinges upon a log polynomial expansion for the luminosity distance. In this note, we demonstrate that this expansion (or "improvements" thereof) typically can only be trusted up to . As a result, a breakdown in the validity of the expansion may be misinterpreted as a (phantom) deviation from flat CDM. We further illustrate the problem through mock data examples.
4 pages; v2 plots added, matches published version
References in corpus (3)
Cited by in corpus (18)
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