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New BAO Study Intensifies Evidence for Giant Local Void Shaping Cosmic Expansion

Twenty years of BAO measurements have made a local void model vastly more likely than a uniform cosmos with upcoming cosmic chronometer studies poised to test its predictions.

© Moritz Haslbauer and Zarija Lukic
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Overview

  • BAO analyses incorporating two decades of data find a local void scenario is about 100 million times more likely than a homogeneous Planck cosmology model
  • Direct galaxy counts reveal our region has roughly 20% fewer galaxies within a billion-light-year radius, consistent with a deep underdensity
  • A giant void centered on the Milky Way would gravitationally pull matter outward, boosting apparent local expansion rates and potentially resolving the Hubble tension
  • Such a vast underdensity conflicts with the Lambda CDM assumption of large-scale uniformity and would demand revisions to standard cosmological frameworks
  • Researchers plan to validate the void hypothesis by comparing its expansion-history predictions with independent cosmic chronometer measurements