Results 101 to 110 of about 114,518 (203)
Can Inflation Resolve the Hubble Tension?
In this work, we investigate how a change in the sound horizon due to inflation may affect the value of H0. Performing an analysis using the measurements of BAO, SN Ia, H(z), CMB, and the local H0, we show that the modification in the sound horizon ...
Ione A. Silva, Edésio M. Barboza
doaj +1 more source
A nuclear data approach for the Hubble constant measurements
An extraordinary number of Hubble constant measurements challenges physicists with selection of the best numerical value. The standard U.S. Nuclear Data Program (USNDP) codes and procedures have been applied to resolve this issue.
Pritychenko Boris
doaj +1 more source
The Hubble constant troubled by dark matter in non-standard cosmologies. [PDF]
Alcaniz JS +5 more
europepmc +1 more source
Observational Constraint on Spherical Inhomogeneity with CMB and Local Hubble Parameter
We derive an observational constraint on a spherical inhomogeneity of the void centered at our position from the angular power spectrum of the cosmic microwave background(CMB) and local measurements of the Hubble parameter. The late time behaviour of the
Ichiki, Kiyotomo +2 more
core +1 more source
Author Correction: The Hubble constant troubled by dark matter in non-standard cosmologies. [PDF]
Alcaniz JS +4 more
europepmc +1 more source
Gravitational wave sources are standard sirens that provide an independent way to map the cosmic expansion history by combining with an independent redshift measurement, either from an electromagnetic counterpart for a bright siren or using different ...
Aman Agarwal +20 more
doaj +1 more source
This replacement corrects the method of separating components of red ...
openaire +2 more sources
The dispersion measure–redshift relation of fast radio bursts (FRBs) provides a valuable cosmological probe for constraining the Hubble constant, offering an independent measurement that could help resolve the ongoing Hubble tension.
Chenyuan Xu, Yi Feng, Jiaying Xu
doaj +1 more source
Running Hubble constant: Evolutionary Dark Energy
8 pages, 3 ...
G. Montani, N. Carlevaro, M.G. Dainotti
openaire +2 more sources
Domain Walls and Hubble constant Tension
We present the idea that replacing the cosmological constant $Λ$ in the $Λ$CDM model by a distribution of walls, with very low tension compared to what one would expect from new physics, could help explaining the tension in the Hubble constant fits in the Standard Cosmological Model. Using parameters from our model for dark matter as macroscopic pearls,
Froggatt, Colin D., Nielsen, Holger Bech
openaire +2 more sources

