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Earlier studies have conjectured that redshift drift is described by spatially averaged quantities and thus becomes positive if the average expansion of the Universe accelerates.
Raul Jimenez et al., Measuring the Homogeneity of the Universe, arXiv:1902.11298v1 [astro-ph.CO]
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Marie-Noelle Celerier, Do we really see a cosmological constant in the supernovae data?, Astron.Astrophys.353:63-71,2000, arXiv:astro-ph/9907206v4
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Thomas Buchert, On average properties of inhomogeneous fluids in general relativity II: perfect fluid cosmologies, Gen.Rel.Grav.33:1381-1405,2001 , arXiv:gr-qc/0102049v2
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L. Pasquini et al., CODEX: Measuring the Expansion of the Universe (and beyond), The Messenger 122, 10 (2005)
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G.F.R. Ellis, T. Buchert, The universe seen at different scales, Phys.Lett. A347 (2005) 38-46, arXiv:gr-qc/0506106v2
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Syksy Rasanen, Accelerated expansion from structure formation, JCAP0611:003,2006, arXiv:astro-ph/0607626v3
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Syksy Rasanen, Cosmological acceleration from structure formation, Int.J.Mod.Phys.D15:2141-2146,2006, arXiv:astro-ph/0605632v1
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Pier-Stefano Corasaniti, Dragan Huterer, Alessandro Melchiorri, Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test, Phys.Rev.D75:062001,2007, arXiv:astro-ph/0701433v1
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Aseem Paranjape, T. P. Singh, Explicit Cosmological Coarse Graining via Spatial Averaging, Gen.Rel.Grav.40:139-157,2008, arXiv:astro-ph/0609481v4
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Ming-Jian Zhang, Jing-Zhao Qi, Wen-Biao Liu, Cosmic Expansion History from the Distance Indicator and Redshift Drift, Int J Theor Phys (2015) 54:2456-2466
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