Results 21 to 30 of about 546,296 (162)

Quantum origin of dark energy and the Hubble tension

open access: yesPhysics Letters B, 2022
Local measurements of the Hubble parameter obtained from the distance ladder at low redshift are in tension with global values inferred from cosmological standard rulers. A key role in the tension is played by the assumptions on the cosmological history,
Enis Belgacem, Tomislav Prokopec
doaj   +1 more source

Is non-particle dark matter equation of state parameter evolving with time?

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
Recently, the so-called Hubble Tension, i.e. the mismatch between the local and the cosmological measurements of the Hubble parameter, has been resolved when non-particle dark matter is considered which has a negative equation of state parameter ...
Souvik Ghose, Arunava Bhadra
doaj   +1 more source

Low-Redshift Observational Constraints on Dark Energy Cosmologies [PDF]

open access: yesIranian Journal of Astronomy and Astrophysics, 2023
Applying the Markov chain Monte Carlo algorithm and using low-redshift observational data, we put cosmological constraints on dark energy cosmologies. Our main aim is to show the influence of each data sample on the procedure of constraining.
Mohammad Malekjani
doaj   +1 more source

Fab-Four Cosmography to Tackle the Hubble Tension

open access: yesUniverse, 2023
In the context of the Fab-Four theory of gravity in a Friedmann-Lemaître-Robertson-Walker background, in this work we use the cosmography approach to study a particular self-tuning filter solution focused on a zero-curvature fixed point to study the H0 ...
Celia Escamilla-Rivera   +2 more
doaj   +1 more source

Axion-dilaton destabilization and the Hubble tension

open access: yesPhysics Letters B, 2019
The discrepancy in measurements of the Hubble constant indicates new physics in dark energy, dark matter, or both. Drawing inspiration from string theory, where axions interact with the other moduli fields, including the dilaton, here we demonstrate that
Stephon Alexander, Evan McDonough
doaj   +1 more source

A review of the Hubble tension [PDF]

open access: yes, 2023
The Hubble constant H0 is the rate of expansion of the universe today. The discrepancy between the early universe H0 value, inferred using ΛCDM from Planck observations of the CMB, and the late universe H0 value, obtained using luminosity and distance ...
Houliston, Rebecca
core   +1 more source

The impact of dust on Cepheid and Type Ia supernova distances [PDF]

open access: yes, 2023
Milky-Way and intergalactic dust extinction and reddening must be accounted for in measurements of distances throughout the universe. This work provides a comprehensive review of the various impacts of cosmic dust focusing specifically on its effects on ...
Brout, Dillon, Riess, Adam
core   +1 more source

The role of CMB spectral distortions in the Hubble tension: A proof of principle

open access: yesPhysics Letters B, 2020
Although both early and late-time modifications of the ΛCDM model have been proposed to address the Hubble tension, compelling arguments suggest that for a solution to be successful it needs to modify the expansion history of the universe prior to ...
Matteo Lucca
doaj   +1 more source

Addressing H0 tension by means of VCDM

open access: yesPhysics Letters B, 2021
In this letter we propose a reduction of the H0 tension puzzle by means of a theory of minimally modified gravity which is dubbed VCDM. After confronting the theory with the data, a transition in the expansion history of the universe in the low-redshift ...
Antonio De Felice   +2 more
doaj   +1 more source

Evidence for dynamical dark energy with an evolving Hubble constant

open access: yesAstronomy & Astrophysics
Context. Hubble constant tension, together with the recent indications of dynamical dark energy proposed from the Dark Energy Spectroscopic Instrument (DESI) baryon acoustic oscillation (BAO) measurements, poses significant challenges for the standard ...
Wang Yi-Ying, Li Yin-Jie, Fan Yi-Zhong
doaj   +1 more source

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