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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.

Concept image of brown dwarf.
Astronomers now propose that “failed stars” known as brown dwarfs could be powered by dark matter
Image

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.