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Astronomers Target ‘Dark Dwarfs’ in Galactic Core to Probe Heavy Dark Matter

Research teams are focusing on lithium-7 enrichment as a telltale sign of brown dwarfs warmed by dark matter inside the galaxy’s core.

Overview

  • A July paper in the Journal of Cosmology and Astroparticle Physics formalized a model of ‘dark dwarfs’, brown dwarfs heated continuously by self-annihilating dark matter.
  • High dark matter density near galactic centers could enable sufficient particle capture inside these objects to sustain steady heat output.
  • Dark dwarfs would maintain constant luminosity, radius and temperature and uniquely preserve their initial lithium-7, unlike normal brown dwarfs.
  • Detecting a single dark dwarf through its lithium-7 spectral signature would strongly support the existence of heavy, self-interacting dark matter particles such as WIMPs.
  • Teams are now planning targeted lithium-7 surveys and infrared observations with the James Webb Space Telescope to seek these theoretical sub-stellar objects.