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The current expansion rate of the Universe, the Hubble constant $H_0$, is an important cosmological quantity.
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I. M. H. Etherington, On the Definition of Distance in General Relativity., Philosophical Magazine 15
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A. G. Riess et al. (Supernova Search Team), Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116
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D. J. Eisenstein and W. Hu, Baryonic features in the matter transfer function, Astrophys. J. 496
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S. Perlmutter et al. (Supernova Cosmology Project), Measurements of Ω \Omega and Λ \Lambda from 42 high redshift supernovae, Astrophys. J. 517
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B. A. Bassett and M. Kunz, Cosmic distance-duality as a probe of exotic physics and acceleration, Phys. Rev. D 69
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M. Kunz, The dark degeneracy: On the number and nature of dark components, Phys. Rev. D 80
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E. V. Linder, A Whole Cosmology View of the Hubble Constant, (2023), arXiv:2301.09695 [astro-ph.CO]
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