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We assess the consistency of cosmological models that alter the size of the sound horizon at last scattering to resolve the Hubble tension with data from ACT + Planck CMB lensing, Big Bang Nucleosynthesis, and supernova data from Pantheon or Pantheon+.
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V.I. Sabla and R.R. Caldwell, Microphysics of early dark energy , Phys. Rev. D 106
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2024
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