Impact of the Hubble tension on the − contour
Tension (geology)
DOI:
10.1016/j.physletb.2024.138588
Publication Date:
2024-03-21T23:15:50Z
AUTHORS (3)
ABSTRACT
The injection of early dark energy (EDE) before the recombination, a possible resolution Hubble tension, will not only shift scalar spectral index ns towards ns=1, but also be likely to tighten current upper limit on tensor-to-scalar ratio r. In this work, with latest CMB datasets (Planck PR4, ACT, SPT and BICEP/Keck), as well BAO SN, we confirm result, discuss its implication inflation. We show that if happen live EDE, how different inflation models currently allowed would distinguished by planned observations, such CMB-S4 LiteBIRD.
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