Cosmology can't understand the expanding universe

Why physicists still haven't solved the Hubble Tension

The Hubble Tension describes the discrepancy between measurements of the early and late universe, of the current rate of cosmic expansion. The initial cause of this tension was assumed to be systematic, with many thinking that some error in our measurements could be eliminated by better telescopes and better data, but following James Webb Space Telescope (JWST) results many believe that something more mysterious might be at play. Do we need new physics outside of cosmology’s standard model? In this piece, Marco Forgione explores recent attempts to resolve the tension and highlights the role of philosophy when science can’t make its mind up.

 

 

The best tool that scientists have for describing the history and structure of our universe is called the Lambda Cold Dark Matter model (ΛCDM). Thanks to this model we can describe (among other things) the acceleration of the universe, its large-scale structures, temporal evolution, and the many different forms of radiation we observe with our telescopes. However, the model is also characterized by six free-parameters that need to be added “manually” since they cannot be determined by theory only. One such parameter is the expansion rate of the universe (also: Hubble’s constant (H0)), which is given by the relationship between the velocity of a cosmological object receding from us and its distance.

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