Results 21 to 30 of about 114,791 (199)

Determination of the Hubble constant. [PDF]

open access: yesProc Natl Acad Sci U S A, 1999
Establishing accurate extragalactic distances has provided an immense challenge to astronomers since the 1920s. The situation has improved dramatically as better detectors have become available, and as several new, promising techniques have been developed. For the first time in the history of this difficult field, relative distances to
Freedman WL, Feng LL.
europepmc   +4 more sources

Easing the Hubble constant tension [PDF]

open access: yesModern Physics Letters A, 2022
In this paper, we show how a modified Friedmann equation, originating from a model of the universe built from a certain [Formula: see text] algebra, has the potential to explain the difference between the Hubble constants extracted from CMB data and from supernova data.
Ambjørn, Jan, Watabiki, Y.
openaire   +3 more sources

Crowded No More: The Accuracy of the Hubble Constant Tested with High-resolution Observations of Cepheids by JWST

open access: yesThe Astrophysical Journal Letters, 2023
High-resolution James Webb Space Telescope (JWST) observations can test confusion-limited Hubble Space Telescope (HST) observations for a photometric bias that could affect extragalactic Cepheids and the determination of the Hubble constant.
Adam G. Riess   +9 more
doaj   +1 more source

Using Unruh temperature and generalized chemical potential as alternative pathway to determine the Hubble parameter

open access: yesPhysics Letters B, 2023
Hubble constant is found relating velocities and distances of galaxies. Actually Cepheid stars and cosmic background radiation present two distinct values for the Hubble constant.
Bráulio Batista Soares   +3 more
doaj   +1 more source

The Hubble constant. [PDF]

open access: yesProc Natl Acad Sci U S A, 1993
Five methods of estimating distances have demonstrated internal reproducibility at the level of 5-20% rms accuracy. The best of these are the cepheid (and RR Lyrae), planetary nebulae, and surface-brightness fluctuation techniques. Luminosity-line width and Dn-sigma methods are less accurate for an individual case but can be applied to large numbers of
Tully RB.
europepmc   +4 more sources

Hubble constant in the axi-Higgs universe

open access: yesPhysical Review Research, 2023
The Λ-cold-dark-matter (ΛCDM) model provides an excellent fit to the cosmic microwave background (CMB) data. However, a statistically significant tension emerges when its determination of the Hubble constant H_{0} is compared to the local distance ...
Leo W. H. Fung   +5 more
doaj   +1 more source

Supernova calibration by gravitational waves

open access: yesEuropean Physical Journal C: Particles and Fields, 2023
Hubble tension is one of the most important problems in cosmology. Although the local measurements on the Hubble constant with Type Ia supernovae (SNe Ia) are independent of cosmological models, they suffer the problem of zero-point calibration of the ...
Xuchen Lu, Yungui Gong
doaj   +1 more source

Anthropic Principle and the Hubble-Lemaître Constant

open access: yesGalaxies, 2022
According to the weak formulation of the anthropic principle, all fundamental physical constants have just such values that they enabled the origin of life.
Michal Křížek, Lawrence Somer
doaj   +1 more source

CATS: The Hubble Constant from Standardized TRGB and Type Ia Supernova Measurements

open access: yesThe Astrophysical Journal Letters, 2023
The tip of the red giant branch (TRGB) provides a luminous standard candle for constructing distance ladders to measure the Hubble constant. In practice, its measurements via edge-detection response (EDR) are complicated by the apparent fuzziness of the ...
D. Scolnic   +9 more
doaj   +1 more source

THE 1% CONCORDANCE HUBBLE CONSTANT [PDF]

open access: yesThe Astrophysical Journal, 2014
9 pages, 4 figures, v2 reformatted in emulateapj, updated to match accepted ...
Bennett, C. L.   +3 more
openaire   +2 more sources

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