Rogue Worlds and the Power of the Dark Side

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Many models for WIMP dark matter (Weakly Interacting Massive Particles) have both weak-scale couplings to nucleons and the capacity to annihilate into standard-model particles. A consequence of these properties is that dark matter particles near the cores of galaxies can, through nuclear scattering in a planet interior, lose energy and become gravitationally bound to the planet. These dark matter particles can then annihilate into energetic standard model particles providing a significant source of internal heat. In some situations, dark matter annihilations and a modest greenhouse effect can raise the surface temperature of a super-Earth planet above the melting point of water. These temperatures can be sustained for many trillions of years. Thus, it may be possible for even rogue super-Earths, with no stellar host, to sustain habitable conditions almost indefinitely.

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