Dark Matter And The Habitability of Planets
arXiv:1103.5086 · doi:10.1088/1475-7516/2012/07/046
Abstract
In many models, dark matter particles can elastically scatter with nuclei in planets, causing those particles to become gravitationally bound. While the energy expected to be released through the subsequent annihilations of dark matter particles in the interior of the Earth is negligibly small (a few megawatts in the most optimistic models), larger planets that reside in regions with higher densities of slow moving dark matter could plausibly capture and annihilate dark matter at a rate high enough to maintain liquid water on their surfaces, even in the absence of additional energy from starlight or other sources. On these rare planets, it may be dark matter rather than light from a host star that makes it possible for life to emerge, evolve, and survive.
9 pages, 3 figures, updated calculations with a larger velocity dispersion for the central portion of the Milky Way
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Cited by in corpus (4)
- The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. II. Framework, Strategy, and First Result
- Exoplanets as Sub-GeV Dark Matter Detectors
- Novel constraints on fifth forces and ultralight dark sector with asteroidal data
- Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk