Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, Astrophys. J. 876
Original
1903
Earlier work this paper cites.
E. Palti, Fortsch. Phys. 67
Original
1903
Earlier work this paper cites.
C. van de Bruck and C. C. Thomas, Phys. Rev. D 100
Original
1904
Earlier work this paper cites.
E. Ó Colgáin and H. Yavartanoo, Phys. Lett. B 797
Original
1905
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.
E. Di Valentino, R. Z. Ferreira, L. Visinelli and U. Danielsson, Phys. Dark Univ. 26
Original
1906
Earlier work this paper cites.
S. Joudaki et al
Original
1906
Earlier work this paper cites.
K. C. Wong et al
Original
1907
Earlier work this paper cites.
W. L. Freedman, B. F. Madore, D. Hatt, T. J. Hoyt, I. Jang, R. L. Beaton, C. R. Burns, M. G. Lee, A. J. Monson, J. R. Neeley, M. M. Phillips, J. A. Rich and M. Seibert, [arXiv:1907.05922 [astro-ph.CO]]
Original
1907
Earlier work this paper cites.
L. Verde, T. Treu and A. Riess, [arXiv:1907.10625 [astro-ph.CO]]
Original
1907
Earlier work this paper cites.
S. Vagnozzi, [arXiv:1907.07569 [astro-ph.CO]]
Original
1907
Earlier work this paper cites.
A. Hebecker, T. Skrzypek and M. Wittner, JHEP 11
Original
1909
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, O. Mena and S. Vagnozzi, Phys. Rev. D 101
Original
1910
Earlier work this paper cites.
L. A. Anchordoqui, I. Antoniadis, D. Lï¿œst, J. F. Soriano and T. R. Taylor, arXiv:1912.00242 [hep-th]
Original
1912
Earlier work this paper cites.
S. Ferrara, M. Tournoy and A. Van Proeyen, Fortsch. Phys. 68
Original
1912
Earlier work this paper cites.
S. Tsujikawa, Class. Quant. Grav. 30
Original
1961
Earlier work this paper cites.
Physics Today 23, 2, 34 (1970)
1970
Earlier work this paper cites.
C. Wetterich, Astron. Astrophys. 301
1995
Earlier work this paper cites.
A. G. Riess et al
1998
Earlier work this paper cites.
S. Perlmutter et al
1999
Earlier work this paper cites.
P. Brax and J. Martin, Phys. Lett. B 468
1999
Earlier work this paper cites.
L. Amendola, Phys. Rev. D 62
2000
Earlier work this paper cites.

Similar

D. Pesce, J. Braatz, M. Reid, A. Riess, D. Scolnic, J. Condon, F. Gao, C. Henkel, C. Impellizzeri, C. Kuo and K. Lo, Astrophys. J. 891
Original
2001
Cited alongside, same era.
M. Chevallier and D. Polarski, Int. J. Mod. Phys. D 10
2001
Cited alongside, same era.
E. V. Linder, Phys. Rev. Lett. 90
2003
Cited alongside, same era.
R. Jiménez, L. Verde, T. Treu and D. Stern, Astrophys. J. 593 (2003) 622 [arXiv:astro-ph/0302560]
2003
Cited alongside, same era.
G. Alestas, L. Kazantzidis and L. Perivolaropoulos, [arXiv:2004.08363 [astro-ph.CO]]
Original
2004
Cited alongside, same era.
A. Gómez-Valent, V. Pettorino and L. Amendola, [arXiv:2004.00610 [astro-ph.CO]]

Then

T. D. Brennan, F. Carta and C. Vafa, PoS TASI2017
Original
2017
Later among the works it cites.
A.L. Ratsimbazafy et al
Original
2017
Later among the works it cites.
S. Alam et al
Original
2017
Later among the works it cites.
P. Agrawal, G. Obied, P. J. Steinhardt and C. Vafa, Phys. Lett. B 784
Original
2018
Later among the works it cites.
D. Andriot, Phys. Lett. B 785
Original
2018
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

Hubble Sinks In The Low-Redshift Swampland

Banerjee, Aritra, Cai, Haiying, Heisenberg, Lavinia et al.

Understand

Local determinations of the Hubble constant $H_0$ favour a higher value than Planck based on CMB and $\Lambda$CDM.

Through a model-independent expansion, we show that low redshift ($z \lesssim 0.7$) data comprising baryon acoustic oscillations (BAO), cosmic chronometers and Type Ia supernovae has a preference for Quintessence models that lower $H_0$ relative to $\Lambda$CDM.
In addition, we confirm that an exponential coupling to dark matter cannot alter this conclusion in the same redshift range.
Our results leave open the possibility that a coupling in the matter-dominated epoch, potentially even in the dark ages, may yet save $H_0$ from sinking in the string theory Swampland.