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Addressing Tensions in ΛCDM Cosmology by an Increase in the Optical Depth to Reionization
01-mathematical-sciences-for02-physical-sciences-for51-physical-sciences-for-20205106-nuclear-and-plasma-physics-for-2020
Recent baryonic acoustic oscillation (BAO) measurements from the Dark Energy Spectroscopic Instrument (DESI) are mildly discrepant (2.2σ) with the cosmic microwave background (CMB) when interpreted within ΛCDM. When analyzing these data with extended cosmologies this inconsistency manifests as a ≃3σ
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