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A critical discussion on the H₀ Hubble constant tension is presented by considering both early and late-type observations. From recent precise measurements, discrepancies emerge when comparing results for some cosmological quantities obtained at different redshifts. We highlight the most relevant measurements of H₀ and propose potential ideas to solve its tension. These solutions concern the exploration of new physics beyond the CDM model or the evaluation of H₀ by other methods. In particular, we focus on the role of the look-back time.
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Salvatore Capozziello
Giuseppe Sarracino
Giulia De Somma
Universe
University of Naples Federico II
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
Astronomical Observatory of Capodimonte
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Capozziello et al. (Wed,) studied this question.
www.synapsesocial.com/papers/68e7433fb6db6435876bc0af — DOI: https://doi.org/10.3390/universe10030140