Built on

C. D. Kreisch, F. Y. Cyr-Racine and O. Doré, arXiv:1902.00534 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, Astrophys. J. 876
Original
1903
Earlier work this paper cites.
E. Ó Colgáin, JCAP 09
Original
1903
Earlier work this paper cites.
P. Agrawal, F. Y. Cyr-Racine, D. Pinner and L. Randall, arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
R. E. Keeley, S. Joudaki, M. Kaplinghat and D. Kirkby, JCAP 12
Original
1905
Earlier work this paper cites.
X. Li and A. Shafieloo, Astrophys. J. Lett. 883
Original
1906
Earlier work this paper cites.
P. Agrawal, G. Obied and C. Vafa, [arXiv:1906.08261 [astro-ph.CO]]
Original
1906
Earlier work this paper cites.
D. Camarena and V. Marra, Phys. Rev. Res. 2
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu and A. G. Riess, doi:10.1038/s41550-019-0902-0 [arXiv:1907.10625 [astro-ph.CO]]
Original
1907
Earlier work this paper cites.
K. C. Wong, S. H. Suyu et al
Original
1907
Earlier work this paper cites.
W. L. Freedman, B. F. Madore, D. Hatt, T. J. Hoyt, I. S. Jang, R. L. Beaton, C. R. Burns, M. G. Lee, A. J. Monson and J. R. Neeley, et al
Original
1907
Earlier work this paper cites.
S. Vagnozzi, Phys. Rev. D 102
Original
1907
Earlier work this paper cites.
S. Pan, W. Yang, E. Di Valentino, A. Shafieloo and S. Chakraborty, JCAP 06
Original
1907
Earlier work this paper cites.
L. Kazantzidis and L. Perivolaropoulos, [arXiv:1907.03176 [astro-ph.CO]]
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, doi:10.3847/1538-4357/ab5dbd [arXiv:1908.10883 [astro-ph.CO]]
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
G. Choi, M. Suzuki and T. T. Yanagida, Phys. Lett. B 805
Original
1910
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, [arXiv:1910.10739 [astro-ph.CO]]
Original
1910
Earlier work this paper cites.
J. Sakstein and M. Trodden, Phys. Rev. Lett. 124
Original
1911
Earlier work this paper cites.
M. Millon, A. Galan, F. Courbin, T. Treu, S. H. Suyu, X. Ding, S. Birrer, G. C. F. Chen, A. J. Shajib and D. Sluse, et al
Original
1912
Earlier work this paper cites.
Ö. Akarsu, J. D. Barrow, L. A. Escamilla and J. A. Vazquez, Phys. Rev. D 101
Original
1912
Earlier work this paper cites.
D. W. Pesce, J. A. Braatz, M. J. Reid, A. G. Riess, D. Scolnic, J. J. Condon, F. Gao, C. Henkel, C. M. V. Impellizzeri and C. Y. Kuo, et al
Original
2001
Earlier work this paper cites.
S. Dhawan, D. Brout, D. Scolnic, A. Goobar, A. G. Riess and V. Miranda, Astrophys. J. 894
Original
2001
Earlier work this paper cites.
C. Krishnan, E. Ó Colgáin, Ruchika, A. A. Sen, M. M. Sheikh-Jabbari, and T. Yang, arXiv: 2002.06044 [astro-ph.CO]
2002
Earlier work this paper cites.

Similar

R. Jimenez and A. Loeb, Astrophys. J. 573
2002
Cited alongside, same era.
R. D’Agostino and R. C. Nunes, Phys. Rev. D 101
Original
2002
Cited alongside, same era.
A. De Felice, C. Q. Geng, M. C. Pookkillath and L. Yin, JCAP 08
Original
2002
Cited alongside, same era.
G. D’Amico, L. Senatore and P. Zhang, JCAP 01
Original
2003
Cited alongside, same era.
J. C. Hill, E. McDonough, M. W. Toomey and S. Alexander, Phys. Rev. D 102
Original
2003
Cited alongside, same era.

Then

K. Jedamzik, L. Pogosian and G. B. Zhao, [arXiv:2010.04158 [astro-ph.CO]]
Original
2010
Later among the works it cites.
A. Shafieloo, A. G. Kim and E. V. Linder, Phys. Rev. D 85
Original
2012
Later among the works it cites.
M. Seikel, C. Clarkson and M. Smith, JCAP 06
Original
2012
Later among the works it cites.
A. Shafieloo, V. Sahni and A. A. Starobinsky, Phys. Rev. D 86
Original
2012
Later among the works it cites.
M. Betoule et al
Original
2014
Later among the works it cites.

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…

2020

Running Hubble Tension and a H0 Diagnostic

Krishnan, Chethan, Colgáin, Eoin Ó, Sheikh-Jabbari, M. M. et al.

Understand

Hubble tension is routinely presented as a mismatch between the Hubble constant $H_0$ determined locally and a value inferred from the flat $\Lambda$CDM cosmology.

In essence, the tension boils down to a disagreement between two numbers.
Here, assuming the tension is cosmological in origin, we predict that within flat $\Lambda$CDM there should be other inferred values of $H_0$, and that a "running of $H_0$ with redshift" can be expected.
These additional determinations of $H_0$ may be traced to a difference between the effective equation of state (EoS) of the Universe within the Friedmann-Lema\^itre-Robertson-Walker (FLRW) cosmology framework and the current standard model.