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

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.