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The H0 trouble: confronting non-thermal dark matter and phantom cosmology with the CMB, BAO, and Type Ia supernovae data

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Author(s):
da Costa, Simony Santos ; da Silva, Deivid R. ; de Jesus, Alvaro S. ; Pinto-Neto, Nelson ; Queiroz, Farinaldo S.
Total Authors: 5
Document type: Journal article
Source: Journal of Cosmology and Astroparticle Physics; v. N/A, n. 4, p. 22-pg., 2024-04-01.
Abstract

We have witnessed different values of the Hubble constant being found in the literature in the past years. Albeit, early measurements often result in an H-0 much smaller than those from late-time ones, producing a statistically significant discrepancy, and giving rise to the so-called Hubble tension. The trouble with the Hubble constant is often treated as a cosmological problem. However, the Hubble constant can be a laboratory to probe cosmology and particle physics models. In our work, we will investigate if the possibility of explaining the H-0 trouble using non-thermal dark matter production aided by phantom-like cosmology is consistent with the Cosmic Background Radiation (CMB) and Baryon Acoustic Oscillation (BAO) data. We performed a full Monte Carlo simulation using CMB and BAO datasets keeping the cosmological parameters Omega(b)h(2), Omega(c)h(2), 100 theta, tau(opt), and w as priors and concluded that a non-thermal dark matter production aided by phantom-like cosmology yields at most H-0 = 70.5 km s(-1) Mpc(-1) which is consistent with some late-time measurements. However, if H-0 > 72 km s(-1) Mpc(-1) as many late-time observations indicate, an alternative solution to the Hubble trouble is needed. Lastly, we limited the fraction of relativistic dark matter at the matter-radiation equality to be at most 1%. (AU)

FAPESP's process: 18/25225-9 - São Paulo Research and Analysis Center
Grantee:Sergio Ferraz Novaes
Support Opportunities: Special Projects
FAPESP's process: 23/01197-4 - Closing in on Dark Matter at the LHC
Grantee:Yoxara Sánchez Villamizar
Support Opportunities: Scholarships in Brazil - Post-Doctoral
FAPESP's process: 21/01089-1 - Cherenkov Telescope Array: construction and first discoveries
Grantee:Luiz Vitor de Souza Filho
Support Opportunities: Special Projects
FAPESP's process: 21/14335-0 - ICTP South American Institute for Fundamental Research: a regional center for Theoretical Physics
Grantee:Nathan Jacob Berkovits
Support Opportunities: Special Projects