Built on

W. D. Kenworthy, D. Scolnic, and A. Riess, “The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant,” Astrophys. J
Original
1901
Earlier work this paper cites.
M. Martinelli, N. B. Hogg, S. Peirone, M. Bruni, and D. Wands, “Constraints on the interacting vacuum–geodesic CDM scenario,” Mon. Not. Roy. Astron. Soc
Original
1902
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, “The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
K. L. Pandey, T. Karwal, and S. Das, “Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model,” JCAP
Original
1902
Earlier work this paper cites.
M. Raveri, “Reconstructing Gravity on Cosmological Scales,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
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,” Astrophys. J
Original
1903
Earlier work this paper cites.
S. Kumar, R. C. Nunes, and S. K. Yadav, “Dark sector interaction: a remedy of the tensions between CMB and LSS data,” Eur. Phys. J
Original
1903
Earlier work this paper cites.
S. Pan, W. Yang, C. Singha, and E. N. Saridakis, “Observational constraints on sign-changeable interaction models and alleviation of the H 0 H_{0} tension,” Phys. Rev
Original
1903
Earlier work this paper cites.
D. Green et al
Original
1903
Earlier work this paper cites.
K. Vattis, S. M. Koushiappas, and A. Loeb, “Dark matter decaying in the late Universe can relieve the H0 tension,” Phys. Rev
Original
1903
Earlier work this paper cites.
A. Palmese et al
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, “Rock ’n’ Roll Solutions to the Hubble Tension,” arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
W. Yang, S. Pan, A. Paliathanasis, S. Ghosh, and Y. Wu, “Observational constraints of a new unified dark fluid and the H 0 H_{0} tension,” Mon. Not. Roy. Astron. Soc
Original
1904
Earlier work this paper cites.
X. Li, A. Shafieloo, V. Sahni, and A. A. Starobinsky, “Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters,” Astrophys. J
Original
1904
Earlier work this paper cites.
M. Kasai and T. Futamase, “A possible solution to the Hubble constant discrepancy – Cosmology where the local volume expansion is driven by the domain average density,” PTEP
Original
1904
Earlier work this paper cites.
S. Capozziello, R. D’Agostino, and O. Luongo, “Extended Gravity Cosmography,” Int. J. Mod. Phys. D
Original
1904
Earlier work this paper cites.
R. E. Keeley, S. Joudaki, M. Kaplinghat, and D. Kirkby, “Implications of a transition in the dark energy equation of state for the H 0 H_{0} and σ 8 \sigma_{8} tensions,” JCAP
Original
1905
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, “Acoustic Dark Energy: Potential Conversion of the Hubble Tension,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
E. . Colgáin and H. Yavartanoo, “Testing the Swampland: H 0 H_{0} tension,” Phys. Lett
Original
1905
Earlier work this paper cites.
S. Adhikari and D. Huterer, “Super-CMB fluctuations and the Hubble tension,” Phys. Dark Univ
Original
1905
Earlier work this paper cites.
N. Blinov, K. J. Kelly, G. Z. Krnjaic, and S. D. McDermott, “Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension,” Phys. Rev. Lett
Original
1905
Earlier work this paper cites.
S. L. Adler, “Implications of a frame dependent dark energy for the spacetime metric, cosmography, and effective Hubble constant,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
Ö. Akarsu, S. Kumar, S. Sharma, and L. Tedesco, “Constraints on a Bianchi type I spacetime extension of the standard Λ \Lambda CDM model,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
D. Camarena and V. Marra, “Local determination of the Hubble constant and the deceleration parameter,” Phys. Rev. Res
Original
1906
Earlier work this paper cites.
W. Yang, O. Mena, S. Pan, and E. Di Valentino, “Dark sectors with dynamical coupling,” Phys. Rev
Original
1906
Earlier work this paper cites.
W. Yang, S. Pan, E. Di Valentino, A. Paliathanasis, and J. Lu, “Challenging bulk viscous unified scenarios with cosmological observations,” Phys. Rev
Original
1906
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson, “Late time transitions in the quintessence field and the H 0 H_{0} tension,” Phys. Dark Univ
Original
1906
Earlier work this paper cites.
M. Martinelli and I. Tutusaus, “CMB tensions with low-redshift H 0 H_{0} and S 8 S_{8} measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity,” Symmetry
Original
1906
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,” JCAP
Original
1906
Earlier work this paper cites.
G. B. Gelmini, A. Kusenko, and V. Takhistov, “Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter,” arXiv:1906.10136 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
P. Agrawal, G. Obied, and C. Vafa, “ H 0 H_{0} Tension, Swampland Conjectures and the Epoch of Fading Dark Matter,” arXiv:1906.08261 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
M. Rossi, M. Ballardini, M. Braglia, F. Finelli, D. Paoletti, A. A. Starobinsky, and C. Umiltà, “Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity,” Phys. Rev. D
Original
1906
Earlier work this paper cites.
X. Li and A. Shafieloo, “A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension,” Astrophys. J. Lett
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu, and A. Riess, “Tensions between the Early and the Late Universe,” arXiv:1907.10625 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
K. C. Wong et al
Original
1907
Earlier work this paper cites.
W. L. Freedman et al
Original
1907
Earlier work this paper cites.
S. Vagnozzi, “New physics in light of the H 0 H_{0} tension: an alternative view,” Phys. Rev. D
Original
1907
Earlier work this paper cites.
H. Desmond, B. Jain, and J. Sakstein, “Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder,” Phys. Rev
Original
1907
Earlier work this paper cites.
W. Yang, S. Pan, S. Vagnozzi, E. Di Valentino, D. F. Mota, and S. Capozziello, “Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal,” JCAP
Original
1907
Earlier work this paper cites.
S. Pan, W. Yang, E. Di Valentino, E. N. Saridakis, and S. Chakraborty, “Interacting scenarios with dynamical dark energy: Observational constraints and alleviation of the H 0 H_{0} tension,” Phys. Rev
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson, “Revisiting a negative cosmological constant from low-redshift data,” Symmetry
Original
1907
Earlier work this paper cites.
Y.-F. Cai, M. Khurshudyan, and E. N. Saridakis, “Model-independent reconstruction of f ⁡ ( T ) f(T) gravity from Gaussian Processes,” Astrophys. J
Original
1907
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues, and D. C. Hooper, “The BAO+BBN take on the Hubble tension,” JCAP
Original
1907
Earlier work this paper cites.
S. K. Yadav, “Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy,” Mod. Phys. Lett
Original
1907
Earlier work this paper cites.
S. Pan, W. Yang, E. Di Valentino, A. Shafieloo, and S. Chakraborty, “Reconciling H 0 H_{0} tension in a six parameter space?,” JCAP
Original
1907
Earlier work this paper cites.
K. Abazajian et al
Original
1907
Earlier work this paper cites.
M. Reid, D. Pesce, and A. Riess, “An Improved Distance to NGC 4258 and its Implications for the Hubble Constant,” Astrophys. J. Lett
Original
1908
Earlier work this paper cites.
W. Yuan, A. G. Riess, L. M. Macri, S. Casertano, and D. Scolnic, “Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant,” Astrophys. J
Original
1908
Earlier work this paper cites.
K. Dutta, A. Roy, Ruchika, A. A. Sen, and M. Sheikh-Jabbari, “Cosmology with low-redshift observations: No signal for new physics,” Phys. Rev. D
Original
1908
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,” arXiv:1908.10883 [astro-ph.CO]
Original
1908
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, O. Mena, and S. Vagnozzi, “Interacting dark energy in the early 2020s: a promising solution to the H 0 H_{0} and cosmic shear tensions,” Phys. Dark Univ
Original
1908
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, and J. Silk, “Cosmological constraints in extended parameter space from the Planck 2018 Legacy release,” JCAP
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, “Oscillating scalar fields and the Hubble tension: a resolution with novel signatures,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, “Hubble constant hunter’s guide,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
M. M. Ivanov, M. Simonović, and M. Zaldarriaga, “Cosmological Parameters from the BOSS Galaxy Power Spectrum,” JCAP
Original
1909
Earlier work this paper cites.
G. D’Amico, J. Gleyzes, N. Kokron, D. Markovic, L. Senatore, P. Zhang, F. Beutler, and H. Gil-Marín, “The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure,” JCAP
Original
1909
Earlier work this paper cites.
S.-F. Yan, P. Zhang, J.-W. Chen, X.-Z. Zhang, Y.-F. Cai, and E. N. Saridakis, “Interpreting cosmological tensions from the effective field theory of torsional gravity,” Phys. Rev. D
Original
1909
Earlier work this paper cites.
A. Desai, K. R. Dienes, and B. Thomas, “Constraining Dark-Matter Ensembles with Supernova Data,” Phys. Rev. D
Original
1909
Earlier work this paper cites.
J. Solà Peracaula, A. Gómez-Valent, J. de Cruz Pérez, and C. Moreno-Pulido, “Brans–Dicke Gravity with a Cosmological Constant Smoothes Out Λ \Lambda CDM Tensions,” Astrophys. J. Lett
Original
1909
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, O. Mena, and S. Vagnozzi, “Nonminimal dark sector physics and cosmological tensions,” Phys. Rev. D
Original
1910
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, “New Early Dark Energy,” arXiv:1910.10739 [astro-ph.CO]
Original
1910
Earlier work this paper cites.
L. A. Anchordoqui and S. E. Perez Bergliaffa, “Hot thermal universe endowed with massive dark vector fields and the Hubble tension,” Phys. Rev. D
Original
1910
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G. Choi, M. Suzuki, and T. T. Yanagida, “Quintessence Axion Dark Energy and a Solution to the Hubble Tension,” Phys. Lett. B
Original
1910
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W. Yang, S. Pan, R. C. Nunes, and D. F. Mota, “Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release,” JCAP
Original
1910
Earlier work this paper cites.
M. Benetti and S. Capozziello, “Connecting early and late epochs by f(z)CDM cosmography,” JCAP
Original
1910
Earlier work this paper cites.
K. V. Berghaus and T. Karwal, “Thermal Friction as a Solution to the Hubble Tension,” Phys. Rev. D
Original
1911
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J. Sakstein and M. Trodden, “Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension,” Phys. Rev. Lett
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1911
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Ö. Akarsu, J. D. Barrow, L. A. Escamilla, and J. A. Vazquez, “Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant,” Phys. Rev. D
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1912
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L. Hart and J. Chluba, “Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension,” Mon. Not. Roy. Astron. Soc
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1912
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L. A. Anchordoqui, I. Antoniadis, D. Lüst, J. F. Soriano, and T. R. Taylor, “ H 0 H_{0} tension and the String Swampland,” Phys. Rev. D
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1912
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1912
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Earlier work this paper cites.
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Earlier work this paper cites.

Similar

D. Pesce et al
Original
2001
Cited alongside, same era.
A. G. Riess, “The Expansion of the Universe is Faster than Expected,” Nature Rev. Phys
Original
2001
Cited alongside, same era.
H. Amirhashchi and A. K. Yadav, “Interacting Dark Sectors in Anisotropic Universe: Observational Constraints and H 0 H_{0} Tension,” arXiv:2001.03775 [astro-ph.CO]
Original
2001
Cited alongside, same era.
A. Perez, D. Sudarsky, and E. Wilson-Ewing, “Resolving the H 0 H_{0} tension with diffusion,” arXiv:2001.07536 [astro-ph.CO]
Original
2001
Cited alongside, same era.
W. Yang, E. Di Valentino, S. Pan, S. Basilakos, and A. Paliathanasis, “Metastable dark energy models in light of Planck 2018: Alleviating the H 0 H_{0} tension,” arXiv:2001.04307 [astro-ph.CO]

Then

L. A. Anchordoqui, H. Goldberg, and G. Steigman, “Right-Handed Neutrinos as the Dark Radiation: Status and Forecasts for the LHC,” Phys. Lett. B
Original
2013
Later among the works it cites.
P. Di Bari, S. F. King, and A. Merle, “Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck,” Phys. Lett. B
Original
2013
Later among the works it cites.
V. Pettorino, L. Amendola, and C. Wetterich, “How early is early dark energy?,” Phys. Rev. D
Original
2013
Later among the works it cites.
V. Pettorino, “Testing modified gravity with Planck: the case of coupled dark energy,” Phys. Rev. D
Original
2013
Later among the works it cites.
R. Allahverdi, M. Cicoli, B. Dutta, and K. Sinha, “Correlation between Dark Matter and Dark Radiation in String Compactifications,” JCAP

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2020

Cosmology Intertwined II: The Hubble Constant Tension

Di Valentino, Eleonora, Anchordoqui, Luis A., Akarsu, Ozgur et al.

Understand

The current cosmological probes have provided a fantastic confirmation of the standard $\Lambda$ Cold Dark Matter cosmological model, that has been constrained with unprecedented accuracy.

However, with the increase of the experimental sensitivity a few statistically significant tensions between different independent cosmological datasets emerged.
While these tensions can be in portion the result of systematic errors, the persistence after several years of accurate analysis strongly hints at cracks in the standard cosmological scenario and the need for new physics.
In this Letter of Interest we will focus on the $4.4\sigma$ tension between the Planck estimate of the Hubble constant $H_0$ and the SH0ES collaboration measurements.

Built on

W. D. Kenworthy, D. Scolnic, and A. Riess, “The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant,” Astrophys. J
Original
1901
Earlier work this paper cites.
M. Martinelli, N. B. Hogg, S. Peirone, M. Bruni, and D. Wands, “Constraints on the interacting vacuum–geodesic CDM scenario,” Mon. Not. Roy. Astron. Soc
Original
1902
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, “The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
K. L. Pandey, T. Karwal, and S. Das, “Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model,” JCAP
Original
1902
Earlier work this paper cites.
M. Raveri, “Reconstructing Gravity on Cosmological Scales,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
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,” Astrophys. J
Original
1903
Earlier work this paper cites.
S. Kumar, R. C. Nunes, and S. K. Yadav, “Dark sector interaction: a remedy of the tensions between CMB and LSS data,” Eur. Phys. J
Original
1903
Earlier work this paper cites.
S. Pan, W. Yang, C. Singha, and E. N. Saridakis, “Observational constraints on sign-changeable interaction models and alleviation of the H 0 H_{0} tension,” Phys. Rev
Original
1903
Earlier work this paper cites.
D. Green et al
Original
1903
Earlier work this paper cites.
K. Vattis, S. M. Koushiappas, and A. Loeb, “Dark matter decaying in the late Universe can relieve the H0 tension,” Phys. Rev
Original
1903
Earlier work this paper cites.
A. Palmese et al
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, “Rock ’n’ Roll Solutions to the Hubble Tension,” arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
W. Yang, S. Pan, A. Paliathanasis, S. Ghosh, and Y. Wu, “Observational constraints of a new unified dark fluid and the H 0 H_{0} tension,” Mon. Not. Roy. Astron. Soc
Original
1904
Earlier work this paper cites.
X. Li, A. Shafieloo, V. Sahni, and A. A. Starobinsky, “Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters,” Astrophys. J
Original
1904
Earlier work this paper cites.
M. Kasai and T. Futamase, “A possible solution to the Hubble constant discrepancy – Cosmology where the local volume expansion is driven by the domain average density,” PTEP
Original
1904
Earlier work this paper cites.
S. Capozziello, R. D’Agostino, and O. Luongo, “Extended Gravity Cosmography,” Int. J. Mod. Phys. D
Original
1904
Earlier work this paper cites.
R. E. Keeley, S. Joudaki, M. Kaplinghat, and D. Kirkby, “Implications of a transition in the dark energy equation of state for the H 0 H_{0} and σ 8 \sigma_{8} tensions,” JCAP
Original
1905
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, “Acoustic Dark Energy: Potential Conversion of the Hubble Tension,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
E. . Colgáin and H. Yavartanoo, “Testing the Swampland: H 0 H_{0} tension,” Phys. Lett
Original
1905
Earlier work this paper cites.
S. Adhikari and D. Huterer, “Super-CMB fluctuations and the Hubble tension,” Phys. Dark Univ
Original
1905
Earlier work this paper cites.
N. Blinov, K. J. Kelly, G. Z. Krnjaic, and S. D. McDermott, “Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension,” Phys. Rev. Lett
Original
1905
Earlier work this paper cites.
S. L. Adler, “Implications of a frame dependent dark energy for the spacetime metric, cosmography, and effective Hubble constant,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
Ö. Akarsu, S. Kumar, S. Sharma, and L. Tedesco, “Constraints on a Bianchi type I spacetime extension of the standard Λ \Lambda CDM model,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
D. Camarena and V. Marra, “Local determination of the Hubble constant and the deceleration parameter,” Phys. Rev. Res
Original
1906
Earlier work this paper cites.
W. Yang, O. Mena, S. Pan, and E. Di Valentino, “Dark sectors with dynamical coupling,” Phys. Rev
Original
1906
Earlier work this paper cites.
W. Yang, S. Pan, E. Di Valentino, A. Paliathanasis, and J. Lu, “Challenging bulk viscous unified scenarios with cosmological observations,” Phys. Rev
Original
1906
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson, “Late time transitions in the quintessence field and the H 0 H_{0} tension,” Phys. Dark Univ
Original
1906
Earlier work this paper cites.
M. Martinelli and I. Tutusaus, “CMB tensions with low-redshift H 0 H_{0} and S 8 S_{8} measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity,” Symmetry
Original
1906
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,” JCAP
Original
1906
Earlier work this paper cites.
G. B. Gelmini, A. Kusenko, and V. Takhistov, “Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter,” arXiv:1906.10136 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
P. Agrawal, G. Obied, and C. Vafa, “ H 0 H_{0} Tension, Swampland Conjectures and the Epoch of Fading Dark Matter,” arXiv:1906.08261 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
M. Rossi, M. Ballardini, M. Braglia, F. Finelli, D. Paoletti, A. A. Starobinsky, and C. Umiltà, “Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity,” Phys. Rev. D
Original
1906
Earlier work this paper cites.
X. Li and A. Shafieloo, “A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension,” Astrophys. J. Lett
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu, and A. Riess, “Tensions between the Early and the Late Universe,” arXiv:1907.10625 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
K. C. Wong et al
Original
1907
Earlier work this paper cites.
W. L. Freedman et al
Original
1907
Earlier work this paper cites.
S. Vagnozzi, “New physics in light of the H 0 H_{0} tension: an alternative view,” Phys. Rev. D
Original
1907
Earlier work this paper cites.
H. Desmond, B. Jain, and J. Sakstein, “Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder,” Phys. Rev
Original
1907
Earlier work this paper cites.
W. Yang, S. Pan, S. Vagnozzi, E. Di Valentino, D. F. Mota, and S. Capozziello, “Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal,” JCAP
Original
1907
Earlier work this paper cites.
S. Pan, W. Yang, E. Di Valentino, E. N. Saridakis, and S. Chakraborty, “Interacting scenarios with dynamical dark energy: Observational constraints and alleviation of the H 0 H_{0} tension,” Phys. Rev
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson, “Revisiting a negative cosmological constant from low-redshift data,” Symmetry
Original
1907
Earlier work this paper cites.
Y.-F. Cai, M. Khurshudyan, and E. N. Saridakis, “Model-independent reconstruction of f ⁡ ( T ) f(T) gravity from Gaussian Processes,” Astrophys. J
Original
1907
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues, and D. C. Hooper, “The BAO+BBN take on the Hubble tension,” JCAP
Original
1907
Earlier work this paper cites.
S. K. Yadav, “Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy,” Mod. Phys. Lett
Original
1907
Earlier work this paper cites.
S. Pan, W. Yang, E. Di Valentino, A. Shafieloo, and S. Chakraborty, “Reconciling H 0 H_{0} tension in a six parameter space?,” JCAP
Original
1907
Earlier work this paper cites.
K. Abazajian et al
Original
1907
Earlier work this paper cites.
M. Reid, D. Pesce, and A. Riess, “An Improved Distance to NGC 4258 and its Implications for the Hubble Constant,” Astrophys. J. Lett
Original
1908
Earlier work this paper cites.
W. Yuan, A. G. Riess, L. M. Macri, S. Casertano, and D. Scolnic, “Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant,” Astrophys. J
Original
1908
Earlier work this paper cites.
K. Dutta, A. Roy, Ruchika, A. A. Sen, and M. Sheikh-Jabbari, “Cosmology with low-redshift observations: No signal for new physics,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
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