Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond Λ \Lambda CDM
Original
1903
Earlier work this paper cites.
A. Cuceu, J. Farr, P. Lemos, and A. Font-Ribera, Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
Original
1906
Earlier work this paper cites.
K. C. Wong et al., H0LiCOW XIII. A 2.4% measurement of H 0 H_{0} from lensed quasars: 5.3 σ 5.3\sigma tension between early and late-Universe probes
Original
1907
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues, and D. C. Hooper, The BAO+BBN take on the Hubble tension
Original
1907
Earlier work this paper cites.
S. Vagnozzi, New physics in light of the H 0 H_{0} tension: An alternative view
Original
1907
Earlier work this paper cites.
C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano, P. A. Whitelock, S. L. Hoffmann, A. V. Filippenko, and D. Scolnic, Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide
Original
1908
Earlier work this paper cites.
D. W. Pesce et al., The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Original
2001
Earlier work this paper cites.
A. G. Riess, The Expansion of the Universe is Faster than Expected
Original
2001
Earlier work this paper cites.
M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter
2001
Earlier work this paper cites.
W. L. Freedman, B. F. Madore, T. Hoyt, I. S. Jang, R. Beaton, M. G. Lee, A. Monson, J. Neeley, and J. Rich, Calibration of the Tip of the Red Giant Branch (TRGB)
Original
2002
Earlier work this paper cites.

Similar

O. H. Philcox, M. M. Ivanov, M. Simonović, and M. Zaldarriaga, Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
Original
2002
Cited alongside, same era.
A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach
2002
Cited alongside, same era.
E. V. Linder, Exploring the expansion history of the universe
2003
Cited alongside, same era.
E. Kourkchi, R. B. Tully, G. S. Anand, H. M. Courtois, A. Dupuy, J. D. Neill, L. Rizzi, and M. Seibert, Cosmicflows-4: The Calibration of Optical and Infrared Tully–Fisher Relations
Original
2004
Cited alongside, same era.
J. Schombert, S. McGaugh, and F. Lelli, Using the Baryonic Tully–Fisher Relation to Measure H o
Original
2006

Then

D. Foreman-Mackey, D. W. Hogg, D. Lang, and J. Goodman, emcee: The MCMC Hammer
Original
2013
Later among the works it cites.
G. E. Addison, G. Hinshaw, and M. Halpern, Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
Original
2013
Later among the works it cites.
E. Aver, K. A. Olive, and E. D. Skillman, The effects of He I λ \lambda 10830 on helium abundance determinations
Original
2015
Later among the works it cites.
A. Coc, P. Petitjean, J.-P. Uzan, E. Vangioni, P. Descouvemont, C. Iliadis, and R. Longland, New reaction rates for improved primordial D/H calculation and the cosmic evolution of deuterium
Original
2015
Later among the works it cites.
A. G. Riess et al., A 2.4% Determination of the Local Value of the Hubble Constant

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2021

$H_0$ tension without CMB data: beyond the $\Lambda$CDM

Okamatsu, Fumiya, Sekiguchi, Toyokazu, Takahashi, Tomo

Understand

We investigate the $H_0$ tension in a range of extended model frameworks beyond the standard $\Lambda$CDM without the data from cosmic microwave background (CMB).

Specifically, we adopt the data from baryon acoustic oscillation, big bang nucleosynthesis and type Ia supernovae as indirect measurements of $H_0$ to study the tension.
We show that the estimated value of $H_0$ from indirect measurements is overall lower than that from direct local ones regardless of the data sets and a range of extended models to be analyzed, which indicates that, although the significance of the tension varies depending on models, the $H_0$ tension persists in a broad framework beyond the standard $\Lambda$CDM model even without CMB data.