Dark matter is one of nature’s most confounding mysteries. It keeps particle physicists up at night and cosmologists glued to their supercomputer simulations. We know it’s real because its mass prevents galaxies from falling apart. But we don’t know what it is.
Dark matter doesn’t like other matter and may prefer its own company. While it doesn’t seem to interact with regular baryonic matter, it could possibly react with itself and self-annihilate. It needs a tightly-packed environment to do that, and that may lead to a way astrophysicists can finally detect it.
New theoretical research outlines how this could happen and states that sub-stellar objects, basically brown dwarfs, could host the process. The research is titled “Dark dwarfs: dark matter-powered sub-stellar objects awaiting discovery at the galactic center,” and it’s published in the Journal of Cosmology and Astroparticle Physics. The lead author is Djuna Croon, a theoretical physicist and assistant professor in the Institute for Particle Physics Phenomenology in the Department of Physics at Durham University.