The 1% Concordance Hubble Constant
C. L. Bennett (1), D. Larson (1), J. L. Weiland (1), G., Hinshaw (2) ((1) Johns Hopkins University, (2) University of British, Columbia)

TL;DR
This paper analyzes the tension between different measurements of the Hubble constant, finding they are consistent within statistical expectations and determining a combined value of 69.6 km/s/Mpc with 1% precision, showing no evidence for new physics.
Contribution
It provides a comprehensive analysis of the consistency between CMB, BAO, and distance ladder measurements, and combines them to refine the Hubble constant estimate.
Findings
Measurements are consistent within statistical expectations.
Best-fit Hubble constant is 69.6+/-0.7 km/s/Mpc.
No evidence for physics beyond the standard cosmological model.
Abstract
The determination of the Hubble constant has been a central goal in observational astrophysics for nearly 100 years. Extraordinary progress has occurred in recent years on two fronts: the cosmic distance ladder measurements at low redshift and cosmic microwave background (CMB) measurements at high redshift. The CMB is used to predict the current expansion rate through a best-fit cosmological model. Complementary progress has been made with baryon acoustic oscillation (BAO) measurements at relatively low redshifts. While BAO data do not independently determine a Hubble constant, they are important for constraints on possible solutions and checks on cosmic consistency. A precise determination of the Hubble constant is of great value, but it is more important to compare the high and low redshift measurements to test our cosmological model. Significant tension would suggest either…
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