Dark energy in light of DESI DR1 and Hubble tension
University of Chinese Academy of Sciences · Chinese Academy of Sciences · +2 more institutions
Abstract
Recently, Dark Energy Spectroscopic Instrument (DESI) collaboration based on their first year data has reported a ≳ 3 σ evidence for an evolving dark energy (DE) against the cosmological constant (CC), so the standard ΛCDM model. However, it is necessary to assess the impact of models able to reduce the Hubble tension on the DESI preference for a dynamical equation of state, where w 0 and w a is the parameters of state equation of DE. In this paper, using DESI DR1 BAO measurements combined with Planck CMB and Pantheon Plus dataset, we perform the Monte Carlo Markov Chain (MCMC) analysis for the w 0 w a CDM model with possible pre-recombination resolutions of the Hubble tension. It is found that, although w 0 >…
Citation impact
- FWCI
- 105.90
- Percentile
- 100%
- References
- 47
Authors
2- HWHao WangCorresponding
University of Chinese Academy of Sciences
- YPYun-Song PiaoCorresponding
Chinese Academy of Sciences, International Centre for Theoretical Physics Asia-Pacific, Institute of Theoretical Physics, University of Chinese Academy of Sciences
Topics & keywords
- Dark energy
- Hubble's law
- Cosmic microwave background
- Planck
- Equation of state
- Cosmology
- Baryon acoustic oscillations
- Markov chain Monte Carlo