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A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension.
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Lloyd Knox and Marius Millea, “The Hubble Hunter’s Guide,” (2019), arXiv:1908.03663 [astro-ph.CO]
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Larry McLerran, Emil Mottola, and Mikhail E. Shaposhnikov, “Sphalerons and axion dynamics in high-temperature qcd,” Phys. Rev. D 43
1991
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Arjun Berera, “Warm inflation,” Phys. Rev. Lett. 75
1995
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Arjun Berera and Li-Zhi Fang, “Thermally induced density perturbations in the inflation era,” Phys. Rev. Lett. 74
1995
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Wayne Hu, “Structure formation with generalized dark matter,” Astrophys. J. 506
1998
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Arjun Berera, Marcelo Gleiser, and Rudnei O. Ramos, “A First principles warm inflation model that solves the cosmological horizon / flatness problems,” Phys. Rev. Lett. 83
1999
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2016
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Mikko Laine and Aleksi Vuorinen, “Basics of Thermal Field Theory,” Lect. Notes Phys. 925
2016
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Arjun Berera, “Warm inflation at arbitrary adiabaticity: A Model, an existence proof for inflationary dynamics in quantum field theory,” Nucl. Phys. B585
2000
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Wayne Hu, Masataka Fukugita, Matias Zaldarriaga, and Max Tegmark, “CMB observables and their cosmological implications,” Astrophys. J. 549
2001
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2009
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Guy D. Moore and Marcus Tassler, “The Sphaleron Rate in SU(N) Gauge Theory,” JHEP 02
2011
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2011
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Diego Blas, Julien Lesgourgues, and Thomas Tram, “The cosmic linear anisotropy solving system (class). part ii: Approximation schemes,” Journal of Cosmology and Astroparticle Physics 2011
2011
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2011
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2016
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Wendy L. Freedman, “Cosmology at a Crossroads,” Nat. Astron. 1
2017
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