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Recently it has been noted by Di Valentino, Melchiorri and Silk (2019) that the enhanced lensing signal relative to that expected in the spatially flat $\Lambda$CDM model poses a possible crisis for the Friedmann-Lema\^{\i}tre-Robertson-Walker (FLRW) class of models usually used to interpret cosmological data.
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Rameez M and Sarkar S (2020) Is there really a ‘Hubble tension’? [ arXiv:1911.06456 ]
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