Page 2: 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.

A slowly spinning universe could solve the Hubble tension

A new study in Monthly Notices of the Royal Astronomical Society by researchers including István Szapudi of the University of Hawaiʻi at Mānoa Institute for Astronomy suggests the universe may rotate—just extremely slowly. ...

Gravitational lens confirms the Hubble tension

We've known the universe is expanding for a long time. The first solid paper demonstrating cosmic expansion was published by Edwin Hubble in 1929, based on observations made by Vesto Slipher, Milton Humason, and Henrietta ...

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