Abstract
Abstract The redshift of the cosmic microwave background (CMB) radiation in the R h = ct cosmology (Melia & Shevchuk 2012) is inferred from nearly model-independent measurements of the angular baryon acoustic oscillations and the first acoustic peak location of the CMB power spectrum, based on the assumption that the two phenomena occur at the same comoving scale in the R h = ct model (Melia & López-Corredoira 2017). The derived redshift, z * ≈ 23, which corresponds to the radiation temperature T * ≈ 65 K, is inconsistent with the standard interpretation of the CMB as the relic radiation of the Big Bang.
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