Dark Matter (H)eats Young Planets
arXiv:2309.02495 · doi:10.1088/1475-7516/2024/11/046
Abstract
We study the effect of dark matter annihilation on the formation of Jovian planets. We show that dark matter heat injections can slow or halt Kelvin-Helmholtz contraction, preventing the accretion of hydrogen and helium onto the solid core. The existence of Jupiter in our solar system can therefore be used to infer constraints on dark matter with relatively strong interaction cross sections. We derive novel constraints on the cross section for both spin-dependent and spin-independent dark matter. We highlight the possibility of a positive detection using future observations by JWST, which could reveal strongly varying planet morpholoiges close to our Galactic Center.
arXiv comment8 pages, 4 figures, includes astronomical observations made with the naked eye. V2: improved analysis, updated constraints. V3: version published in JCAP
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Cited by in corpus (5)
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