Results 101 to 110 of about 6,292 (199)
Measurements of the Hubble Constant: Tensions in Perspective*
Abstract Measurement of the distances to nearby galaxies has improved rapidly in recent decades. The ever-present challenge is to reduce systematic effects, especially as greater distances are probed and the uncertainties become larger. In this paper, we combine several recent calibrations of the tip of the red giant branch (TRGB) method.
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The Pursuit of the Hubble Constant Using Type II Supernovae
Part of the book series: Springer Series in Astrophysics and CosmologyThe use of multiple independent methods with their own systematic uncertainties is crucial for resolving the ongoing tension between local and distant measurements of the Hubble ...
Jaeger, T. de, Galbany, Lluís
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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
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Hubble Constant and Strong Gravitational Lensing [PDF]
The persistent tension between early and late universe measurements of the Hubble constant (H0) represents one of the most significant challenges in modern cosmology, with implications for our understanding of fundamental physics.
Schmidt, Thomas
core
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
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On the cosmological and Hubble constants
The values of the cosmological constant, $\Lambda$, and the Hubble constant, $H_0$, are determined using the vacuum energy density, $-\Delta e$, equal to $-1.016124 \times 10^{113} J m^{-3}$ and the age of the universe, $t_0$, equal to $1.380 \times 10^{10}~years$.
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Golden and Silver Dark Sirens for Precise H0 Measurement with HETDEX
Gravitational waves (GWs) from compact binary coalescences are standard sirens that provide a direct measure of the source’s luminosity distance, enabling an independent measurement of the Hubble constant ( H _0 ).
Yixuan Dang +14 more
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On the Hubble constant and the cosmological constant [PDF]
F. Hoyle, G. Burbidge, J. V. Narlikar
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Estimating the Hubble constant on a base of observed values of the Hubble parameter H(z) in a model without expansion [PDF]
In the model of low-energy quantum gravity by the author, the ratio H(z)/(1 + z) should be equal to the Hubble constant. Here, the weighted average value of the Hubble constant has been found using 29 observed values of the Hubble parameter H(z): ±σ0
Ivanov, M. A.
core
This replacement corrects the method of separating components of red ...
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