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We examine further the ability of the New Early Dark Energy model (NEDE) to resolve the current tension between the Cosmic Microwave Background (CMB) and local measurements of $H_0$ and the consequences for inflation.
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V. Poulin, T.L. Smith, T. Karwal and M. Kamionkowski, Early Dark Energy can Resolve the Hubble Tension , Phys. Rev. Lett. 122
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F. Niedermann and M.S. Sloth, Resolving the Hubble tension with new early dark energy , Phys. Rev. D 102
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2009
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2011
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2011
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D.A. Easson and B.A. Powell, Optimizing future experimental probes of inflation , Phys. Rev. D 83
2011
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2012
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R. Wojtak, A. Knebe, W.A. Watson, I.T. Iliev, S. Heß, D. Rapetti et al., Cosmic variance of the local Hubble flow in large-scale cosmological simulations , Mon. Not. R. Astron Soc. 438
2014
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2014
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2021
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2021
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F. Niedermann and M.S. Sloth, New early dark energy , Phys. Rev. D 103
2021
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2021
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2021
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2022
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