Hints of a Local Matter Underdensity or Modified Gravity in the Low $z$ Pantheon data

Adam G. Riess, Stefano Casertano, Wenlong Yuan, Lucas M. Macri, and Dan 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,” Astrophys. J. 876

Original

1903

Earlier work this paper cites.

Dong Zhao, Yong Zhou, and Zhe Chang, “Anisotropy of the Universe via the Pantheon supernovae sample revisited,” Mon. Not. Roy. Astron. Soc. 486

Original

1903

Earlier work this paper cites.

Eoin Ó. Colgáin, “A hint of matter underdensity at low z?” JCAP 1909

Original

1903

Earlier work this paper cites.

Fotios K. Anagnostopoulos, David Benisty, Spyros Basilakos, and Eduardo I. Guendelman, “Dark energy and dark matter unification from dynamical space time: observational constraints and cosmological implications,” JCAP 06

Original

1904

Earlier work this paper cites.

Leandros Perivolaropoulos and Lavrentios Kazantzidis, “Hints of modified gravity in cosmos and in the lab?” Int. J. Mod. Phys. D28

Original

1904

Earlier work this paper cites.

David Camarena and Valerio Marra, “Local determination of the Hubble constant and the deceleration parameter,” Phys. Rev. Res. 2

Original

1906

Earlier work this paper cites.

Andrei Cuceu, James Farr, Pablo Lemos, and Andreu Font-Ribera, “Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future,” JCAP 1910

Original

1906

Earlier work this paper cites.

Kenneth 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,” (2019), arXiv:1907.04869 [astro-ph.CO]

Original

1907

Earlier work this paper cites.

Wendy L. Freedman et al. , “The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch,” (2019), 10.3847/1538-4357/ab2f73 , arXiv:1907.05922 [astro-ph.CO]

Original

1907

Earlier work this paper cites.

Lavrentios Kazantzidis and Leandros Perivolaropoulos, “Is gravity getting weaker at low z? Observational evidence and theoretical implications,” (2019), arXiv:1907.03176 [astro-ph.CO]

Original

1907

Earlier work this paper cites.

N. Aghanim et al. (Planck), “Planck 2018 results. V. CMB power spectra and likelihoods,” (2019), arXiv:1907.12875 [astro-ph.CO]

Original

1907

Earlier work this paper cites.

Vladimir V. Luković, Balakrishna S. Haridasu, and Nicola Vittorio, “Exploring the evidence for a large local void with supernovae Ia data,” Mon. Not. Roy. Astron. Soc. 491

Original

1907

Earlier work this paper cites.

Hans Boehringer, Gayoung Chon, and Chris A. Collins, “Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant,” Astron. Astrophys. 633

Original

1907

Earlier work this paper cites.

Alba Quelle and Antonio L. Maroto, “On the tension between growth rate and CMB data,” (2019), arXiv:1908.00900 [astro-ph.CO]

Original

1908

Earlier work this paper cites.

Will Handley, “Curvature tension: evidence for a closed universe,” (2019), arXiv:1908.09139 [astro-ph.CO]

Original

1908

Earlier work this paper cites.

Kai Liao, Arman Shafieloo, Ryan E. Keeley, and Eric V. Linder, “A model-independent determination of the Hubble constant from lensed quasars and supernovae using Gaussian process regression,” Astrophys. J. Lett. 886

Original

1908

Earlier work this paper cites.

Koushik Dutta, Anirban Roy, Ruchika, Anjan A. Sen, and M.M. Sheikh-Jabbari, “Cosmology with low-redshift observations: No signal for new physics,” Phys. Rev. D 100

Original

1908

Earlier work this paper cites.

T. Shanks, L. M. Hogarth, N. Metcalfe, and J. Whitbourn, “Local Hole revisited: evidence for bulk motions and self-consistent outflow,” Mon. Not. Roy. Astron. Soc. 490

Original

1909

Earlier work this paper cites.

Ekim Taylan Hanı meli, Brahim Lamine, Alain Blanchard, and Isaac Tutusaus, “Time-dependent G G in Einstein’s equations as an alternative to the cosmological constant,” Phys. Rev. D 101

Original

1910

Earlier work this paper cites.

Rubén Arjona and Savvas Nesseris, “What can Machine Learning tell us about the background expansion of the Universe?” (2019), arXiv:1910.01529 [astro-ph.CO]

Original

1910

Earlier work this paper cites.

Zhe Chang, Dong Zhao, and Yong Zhou, “Constraining the anisotropy of the Universe via Pantheon supernovae sample,” (2019), arXiv:1910.06883 [astro-ph.CO]

Original

1910

Earlier work this paper cites.

Eleonora Di Valentino, Alessandro Melchiorri, and Joseph Silk, “Planck evidence for a closed Universe and a possible crisis for cosmology,” Nat. Astron. (2019), 10.1038/s41550-019-0906-9 , arXiv:1911.02087 [astro-ph.CO]

Original

1911

Earlier work this paper cites.

Tao Yang, Aritra Banerjee, and Eoin Ó. Colgáin, “On cosmography and flat Λ \Lambda CDM tensions at high redshift,” (2019a), arXiv:1911.01681 [astro-ph.CO]

Original

1911

Earlier work this paper cites.

F. Skara and L. Perivolaropoulos, “Tension of the E G E_{G} statistic and redshift space distortion data with the Planck - Λ ​ C ​ D ​ M \Lambda CDM model and implications for weakening gravity,” Phys. Rev. D 101

Original

1911

Earlier work this paper cites.

Georges Lemaître, “L’Univers en expansion,” Annales de la Société Scientifique de Bruxelles 53

1933

Earlier work this paper cites.

H. Bondi, “Spherically symmetrical models in general relativity,” Mon. Not. Roy. Astron. Soc. 107

1947

Earlier work this paper cites.

Steven Weinberg, “The Cosmological Constant Problem,” Rev. Mod. Phys. 61

1988

Earlier work this paper cites.

Steinhardt P.J, Critical Problems in Physics (Princeton University Press, 1997)

1997

Earlier work this paper cites.

Richard C. Tolman, “Effect of imhomogeneity on cosmological models,” Proc. Nat. Acad. Sci. 20

1997

Earlier work this paper cites.

Adam G. Riess et al. (Supernova Search Team), “Observational evidence from supernovae for an accelerating universe and a cosmological constant,” Astron. J. 116

1998

Earlier work this paper cites.

S. Perlmutter et al. (Supernova Cosmology Project), “Measurements of Ω \Omega and Λ \Lambda from 42 high redshift supernovae,” Astrophys. J. 517

1999

Earlier work this paper cites.

E. Garcia-Berro, E. Gaztanaga, J. Isern, O. Benvenuto, and L. Althaus, “On the evolution of cosmological type ia supernovae and the gravitational constant,” (1999), arXiv:astro-ph/9907440 [astro-ph]

1999

Earlier work this paper cites.

C. Armendariz-Picon, Viatcheslav F. Mukhanov, and Paul J. Steinhardt, “A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration,” Phys. Rev. Lett. 85

2000

Earlier work this paper cites.

Sean M. Carroll, “The Cosmological constant,” Living Rev. Rel. 4

2001

Earlier work this paper cites.

Winfried Zimdahl, Dominik J. Schwarz, Alexander B. Balakin, and Diego Pavon, “Cosmic anti-friction and accelerated expansion,” Phys. Rev. D 64

2001

Earlier work this paper cites.

Rubén Arjona and Savvas Nesseris, “Hints of dark energy anisotropic stress using Machine Learning,” (2020), arXiv:2001.11420 [astro-ph.CO]

Original

2001

Earlier work this paper cites.

Adam G. Riess, “The Expansion of the Universe is Faster than Expected,” Nature Rev. Phys. 2

Original

2001

Earlier work this paper cites.

Xiaolei Li and Arman Shafieloo, “Generalised Emergent Dark Energy Model: Confronting Λ \Lambda and PEDE,” (2020), arXiv:2001.05103 [astro-ph.CO]

Original

2001

Earlier work this paper cites.

Varun Sahni, “The Cosmological constant problem and quintessence,” The early universe and cosmological observations: A critical review. Proceedings, Conference, Cape Town, South Africa, July 23-25, 2001 , Class. Quant. Grav. 19

2002

Cited alongside, same era.

Kai Liao, Arman Shafieloo, Ryan E. Keeley, and Eric V. Linder, “Determining H 0 H_{0} Model-Independently and Consistency Tests,” Astrophys. J. 895

Original

2002

Cited alongside, same era.

Chethan Krishnan, Eoin Ó. Colgáin, Ruchika, Anjan A. Sen, M.M. Sheikh-Jabbari, and Tao Yang, “Is there an early Universe solution to Hubble tension?” (2020), arXiv:2002.06044 [astro-ph.CO]

Original

2002

Cited alongside, same era.

E. Gaztanaga, E. Garcia-Berro, J. Isern, E. Bravo, and I. Dominguez, “Bounds on the possible evolution of the gravitational constant from cosmological type Ia supernovae,” Phys. Rev. D65

2002

Cited alongside, same era.

P. A. R. Ade et al. (Planck), “Planck 2015 results. XIII. Cosmological parameters,” Astron. Astrophys. 594

Original

2015

Later among the works it cites.

Éric Aubourg et al. , “Cosmological implications of baryon acoustic oscillation measurements,” Phys. Rev. D92

Original

2015

Later among the works it cites.

P. A. R. Ade et al. (Planck), “Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts,” Astron. Astrophys. 594

Original

2015

Later among the works it cites.

Shinji Tsujikawa, “Possibility of realizing weak gravity in redshift space distortion measurements,” Phys. Rev. D92

Original

2015

Later among the works it cites.

Zhe Chang and Hai-Nan Lin, “Comparison between hemisphere comparison method and dipole-fitting method in tracing the anisotropic expansion of the Universe use the Union2 dataset,” Mon. Not. Roy. Astron. Soc. 446