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PRL Study Links Dark Energy to Black Holes Using DESI Data

A peer‑reviewed DESI–CMB analysis links dark energy to black hole formation to explain a neutrino‑mass mismatch.

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Overview

  • Researchers report in Physical Review Letters on August 21 that a cosmologically coupled black hole model fits recent DESI observations alongside cosmic microwave background data.
  • The model proposes that when stars collapse, black holes convert some infalling matter into dark energy, causing the dark energy density to evolve in step with the cosmic star‑formation history.
  • Applying this framework to DESI results resolves a matter‑budget tension by restoring positive neutrino masses consistent with terrestrial measurements.
  • DESI’s international, Department of Energy–managed survey of millions of galaxies supplied the precision large‑scale structure data needed to test the model.
  • Authors describe the findings as promising but provisional and call for independent checks and future DESI data to validate or refute the hypothesis.