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Similar

J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, “Early dark energy does not restore cosmological concordance,” Phys. Rev
Original
2003
Cited alongside, same era.
H. Desmond and J. Sakstein, “Screened fifth forces lower the TRGB-calibrated Hubble constant too,” Phys. Rev
Original
2003
Cited alongside, same era.
P. J. E. Peebles and B. Ratra, “The Cosmological Constant and Dark Energy,” Rev. Mod. Phys
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,” Astrophys. J
Original
2004
Cited alongside, same era.
J. L. Bernal, T. L. Smith, K. K. Boddy, and M. Kamionkowski, “Robustness of baryon acoustic oscillation constraints for early-Universe modifications of Λ \Lambda CDM cosmology,” Phys. Rev. D

Then

J. Khoury, “Chameleon Field Theories,” Class. Quant. Grav
Original
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A. Heavens, R. Jimenez, and L. Verde, “Standard rulers, candles, and clocks from the low-redshift Universe,” Phys. Rev. Lett
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2014
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B. Audren, “Separate Constraints on Early and Late Cosmology,” Mon. Not. Roy. Astron. Soc
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R. Wojtak, A. Knebe, W. A. Watson, I. T. Iliev, S. Heß, D. Rapetti, G. Yepes, and S. Gottlöber, “Cosmic variance of the local Hubble flow in large-scale cosmological simulations,” Mon. Not. Roy. Astron. Soc
Original
2014
Later among the works it cites.
I. Odderskov, S. Hannestad, and T. Haugbølle, “On the local variation of the Hubble constant,” JCAP

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2021

Chameleon dark energy can resolve the Hubble tension

Cai, Rong-Gen, Guo, Zong-Kuan, Li, Li et al.

Understand

Values of the Hubble constant between the direct measurements from various independent local observations and that inferred from the cosmic microwave background with the $\Lambda$-cold-dark-matter model are in tension with persistent significance.

We propose a late-time inhomogeneous resolution suggesting that a chameleon field coupled to a local overdensity of matter could be trapped at a higher potential energy density as an effective cosmological constant driving the local expansion rate faster than that of the background with lower matter density.
We illustrate this mechanism in a toy model in which a region with only $20\%$ overdensity of matter is sufficient to resolve the Hubble tension, and the Hubble constant measured by the local distance ladders could be accommodated by the chameleon coupled to the observed overdensities from the large-scale structure surveys.