Research news on Hubble constant

The Hubble constant, within cosmological research, denotes the present-day proportionality factor relating the recession velocity of extragalactic objects to their proper distance in the expanding universe, and thus operationally defines the local expansion rate. As a research area, work on the Hubble constant encompasses precision measurement via distance-ladder methods (e.g., Cepheids, Type Ia supernovae), early-universe inferences from cosmic microwave background anisotropies and baryon acoustic oscillations, and associated statistical and systematic error analyses. This field currently focuses on resolving tensions between independent determinations, refining calibration strategies, and constraining cosmological models and new physics through improved estimates of this parameter.

How old is the universe? The oldest stars give us a clue

Researchers from the University of Bologna and the Leibniz Institute for Astrophysics Potsdam (AIP) along with other institutes have proposed a new way to address the Hubble tension by comparing estimates of the universe's ...

page 1 from 3