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Dark Energy at early times and ACT: a larger Hubble constant without late-time priors

, , and . (2021)cite arxiv:2109.06229Comment: 20 pages, 15 figures, comments welcome.

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Cosmology Intertwined II: The Hubble Constant Tension, , , , , , , , , and 68 other author(s). (2020)cite arxiv:2008.11284Comment: Snowmass2021 - Letter of Interest.Cosmology Intertwined I: Perspectives for the Next Decade, , , , , , , , , and 68 other author(s). (2020)cite arxiv:2008.11283Comment: Snowmass2021 - Letter of Interest.Dark Energy at early times and ACT: a larger Hubble constant without late-time priors, , and . (2021)cite arxiv:2109.06229Comment: 20 pages, 15 figures, comments welcome.Insights into searches for anisotropies in the nanohertz gravitational-wave background, , and . (2020)cite arxiv:2010.13958Comment: 20 pages, 14 figures.CMB-S4 Science Book, First Edition, , , , , , , , , and 76 other author(s). (2016)cite arxiv:1610.02743.On the consistency of effective field theory analyses of BOSS power spectrum, , , and . (2022)cite arxiv:2208.05929Comment: 17+5 pages, 10 figures. Comments welcome!.Robustness of baryon acoustic oscillations constraints to beyond-$Łambda$CDM cosmologies, , , and . (2020)cite arxiv:2004.07263Comment: 21 pages, 4 figures.Cosmology Intertwined III: $f \sigma_8$ and $S_8$, , , , , , , , , and 68 other author(s). (2020)cite arxiv:2008.11285Comment: Snowmass2021 - Letter of Interest.How sound are our ultra-light axion approximations?, , and . (2019)cite arxiv:1909.11094Comment: 22 pages, 16 figures, comments are welcome.Exact treatment of weak dark matter-baryon scattering for linear-cosmology observables, , and . (2023)