A deformed uncertainty relation for the universe scale factor modifies the Friedmann equation to yield late-universe acceleration or a bounce according to the sign of a single free exponent.
Hou et al., The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD mea- surements from anisotropic clustering analysis of the quasar sample , Mon
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A Cosmological Uncertainty Relation and Late-Universe Acceleration
A deformed uncertainty relation for the universe scale factor modifies the Friedmann equation to yield late-universe acceleration or a bounce according to the sign of a single free exponent.