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The cosmic timeline implied by the highest redshift quasars

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arxiv 2412.02706 v1 pith:YANETPCT submitted 2024-11-24 astro-ph.CO astro-ph.GA

classification astro-ph.COastro-ph.GA
keywords standardodotquasarsbeenblackcosmologyemergenceformation
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abstract

The conventional picture of supermassive black-hole growth in the standard model had already been seriously challenged by the emergence of $\sim 10^9\;M_\odot$ quasars at $z\sim 7.5$, conflicting with the predicted formation of structure in the early $\Lambda$CDM Universe. But the most recent {\it JWST} discovery of a $\sim 10^8\;M_\odot$ source at $z\sim 10.1$ argues even more strongly against the possibility that these black holes were created in Pop II or III supernovae, followed by Eddington-limited accretion. Attempts at resolving this anomaly have largely focused on the formation of seeds via an exotic, direct collapse of primordial gas to an initial mass $\sim 10^5\;M_\odot$ -- a process that has never been seen anywhere in the cosmos. Our goal in this {\it Letter} is to demonstrate that the emergence of these black holes is instead fully consistent with standard astrophysics in the context of the alternative Friedmann-Lema\^itre-Robertson-Walker cosmology known as the $R_{\rm h}=ct$ universe. We show that, while the predicted evolution in the standard model is overly compressed, the creation, growth and appearance of such high-$z$ quasars fall comfortably within the evolutionary history in this cosmology, thereby adding considerable observational support to the existing body of evidence favoring it over the standard scenario.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Comparison of $R_h=ct$ and $\Lambda$CDM using DESI DR1 measurements

    astro-ph.CO 2025-06 conditional novelty 5.0 of 10

    Using DESI DR1 distance measurements, flat LambdaCDM is decisively preferred over R_h=ct, driven almost entirely by the Lyman-alpha data point at redshift 2.33.

  2. Joint constraints on $R_h=ct$ cosmology from DESI DR2 BAO, CC, and SN\textit{Ia} Pantheon$^+$ sample

    astro-ph.CO 2025-12 conditional novelty 4.0 of 10

    ΛCDM fits the joint DESI DR2 BAO + Pantheon+ + cosmic-chronometer data better than the coasting R_h=ct model, which yields an older universe and a lower fitted H0.

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