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The early dark energy (EDE) scenario aims to increase the value of the Hubble constant ($H_0$) inferred from cosmic microwave background (CMB) data over that found in $\Lambda$CDM, via the introduction of a new form of energy density in the early universe.
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A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach , PhRvD 66
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R. M. Neal, Taking Bigger Metropolis Steps by Dragging Fast Variables , arXiv Mathematics e-prints (2005) math/0502099 [ math/0502099 ]
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A. Lewis, Efficient sampling of fast and slow cosmological parameters , PhRvD 87
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W. L. Freedman, Measurements of the Hubble Constant: Tensions in Perspective , Astrophys. J. 919
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