How A New Type of R_h = ct Cosmological Model Outperforms the Λ-CDM Model in Numerous Categories and Resolves the Hubble Tension

Espen Gaarder Haug; Eugene Terry Tatum

doi:10.20944/preprints202410.1570.v1

Preprint Article Version 1 This version is not peer-reviewed

Version 1 : Received: 15 October 2024 / Approved: 21 October 2024 / Online: 21 October 2024 (07:10:36 CEST)

This paper provides a brief overview of how the Haug and Tatum Cosmological Model (HTC) outperforms the Λ-CDM model in numerous categories. In particular, we show why the HTC model is a strong competitor to the Λ-CDM model. For example, HTC appears to resolve the Hubble tension by making use of newly-discovered fundamental relationships between the CMB temperature, the Hubble parameter, and cosmological redshift. Moreover, HTC appears to better explain certain early universe telescopic observations than the Λ-CDM model.

R_h = ct cosmology; black hole cosmology; CMB temperature; hubble parameter; hubble tension; Λ-CDM model; cosmic age; early galaxy formation; high-precision cosmology

Physical Sciences, Astronomy and Astrophysics

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How A New Type of R_h = ct Cosmological Model Outperforms the Λ-CDM Model in Numerous Categories and Resolves the Hubble Tension

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