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R. Jimenez, R. Maartens, A. R. Khalifeh, R. R. Caldwell, A. F. Heavens and L. Verde, “Measuring the Homogeneity of the Universe Using Polarization Drift,” JCAP 1905
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Similar

A. G. Riess et al
Original
2016
Cited alongside, same era.
P. Bull, “Extending cosmological tests of General Relativity with the Square Kilometre Array,” Astrophys. J. 817
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2016
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F. Lepori, E. Di Dio, M. Viel, C. Baccigalupi and R. Durrer, “The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys,” JCAP 1702
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2017
Cited alongside, same era.
F. Villaescusa-Navarro, D. Alonso and M. Viel, “Baryonic acoustic oscillations from 21 cm intensity mapping: the Square Kilometre Array case,” Mon. Not. Roy. Astron. Soc. 466

Then

D. Camarena and V. Marra, “Impact of the cosmic variance on H 0 H_{0} on cosmological analyses,” Phys. Rev. D 98
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2018
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H. Y. Chen, M. Fishbach and D. E. Holz, “A two per cent Hubble constant measurement from standard sirens within five years,” Nature 562
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2019

The Hubble constant tension with next-generation galaxy surveys

Bengaly, Carlos A. P., Clarkson, Chris, Maartens, Roy

Understand

The rate at which the universe is expanding today is a fundamental parameter in cosmology which governs our understanding of structure formation and dark energy.

However, current measurements of the Hubble constant, $H_0$, show a significant tension ($\sim 4-6\sigma$) between early- and late-Universe observations.
There are ongoing efforts to check the diverse observational results and also to investigate possible theoretical ways to resolve the tension~-- which could point to radical extensions of the standard model.
Here we demonstrate the potential of next-generation spectroscopic galaxy surveys to shed light on the Hubble constant tension.