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New Early Dark Energy (NEDE) is a component of vacuum energy at the electron volt scale, which decays in a first-order phase transition shortly before recombination [arXiv:1910.10739].
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C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455
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W. Hu, Structure formation with generalized dark matter, The Astrophysical Journal 506
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D. Baumann, D. Green, J. Meyers, and B. Wallisch, Phases of new physics in the cmb, Journal of Cosmology and Astroparticle Physics 2016
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R. Kappl, H. P. Nilles, and M. W. Winkler, Modulated Natural Inflation, Phys. Lett. B 753
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D. J. E. Marsh, Axion Cosmology, Phys. Rept. 643
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J. Evslin, A. A. Sen, and Ruchika, Price of shifting the Hubble constant, Phys. Rev. D 97
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M. Raveri and W. Hu, Concordance and Discordance in Cosmology, Phys. Rev. D 99
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N. Schöneberg, J. Lesgourgues, and D. C. Hooper, The bao+bbn take on the hubble tension, Journal of Cosmology and Astroparticle Physics 2019
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A. Kosowsky, M. S. Turner, and R. Watkins, Gravitational waves from first order cosmological phase transitions, Phys. Rev. Lett. 69
2026
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