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New BAO Data Bolster Local Void Model as Key to Hubble Tension

Scientists plan independent tests using cosmic chronometers to verify a local underdensity that BAO measurements make about 100 million times more likely than a homogeneous cosmos.

If we’re situated in a low-density region like the green dot, gravity from the denser areas around us would pull matter outward, causing it to flow away from our location, as illustrated by the red arrows.
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Overview

  • BAO analyses presented at the National Astronomy Meeting show a billion-light-year void around the Milky Way is roughly 100 million times more probable than a uniform Planck cosmology
  • Direct galaxy counts reveal the local universe’s density is about 20 percent below the cosmic average, matching predictions of the void hypothesis
  • The proposed void would place Earth near its center, causing matter to flow outward and boosting apparent local expansion rates
  • A vast underdensity on this scale conflicts with the Lambda-CDM framework’s principle of large-scale homogeneity
  • Researchers will use cosmic chronometers—galaxies that have ceased star formation—to independently chart expansion history and test the void scenario