The Cosmic Timeline Implied by the JWST Reionization Crisis

Abstract

JWST's discovery of well-formed galaxies and supermassive black holes only a few hundred Myr after the big bang, and the identification of polycyclic aromatic hydrocarbons (PAHs) at $z=6.71$, seriously challenge the timeline predicted by Lambda CDM. Moreover, the implied bright UV-irradiation of the early Universe suggests a reionization history much too short to comply with the observed evolution of the hydrogen ionization fraction, $x_ HII (z)$. A recent analysis of reionization after JWST by Munoz:2024 has concluded that the Lambda CDM timeline simply cannot accommodate the combined JWST- Planck observations even if exotic fixes are introduced to modify the standard reionization model. In this paper, we argue that this so-called `photon budget crisis' is more likely due to flaws in the cosmological model itself. We aim to re-analyze the data in the context of established astrophysics with $R_ h =ct$ as the background cosmology, an approach that has already been shown to mitigate the tension created by the too-early appearance of galaxies, quasars and PAHs. We employ the standard reionization model using the JWST-measured UV luminosity function in the early Universe and the timeline and physical conditions in both Lambda CDM and $R_ h =ct$. The former has already been fully probed and discussed by Munoz:2024 and we here merely redo the calculation to ensure consistency with their pioneering work. We then contrast the predicted reionization histories in these two scenarios and compare them with the data. We confirm that the reionization history predicted by Lambda CDM is in significant tension with the observations, and demonstrate that the latter are instead in excellent agreement with the $R_ h =ct$ timeline. Together, the four anomalies uncovered by JWST, including the newly discovered reionization `crisis' discussed in this paper, provide strong evidence against the timeline predicted by Lambda CDM and in favor of the evolutionary history in $R_ h =ct$.