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0.5 eV QCD Axion Cosmology
high-energy-physics-experimenthigh-energy-physics-phenomenologyhigh-energy-physics-theorystrongly-correlated-electrons
The best available determination of the present expansion rate of the universe using late-universe observations, by the SH0ES collaboration in 2025, differs by more than seven standard deviations from the value of the Hubble constant determined by the Planck collaboration in 2018 using early-univers
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