Monte Carlo simulations show the corrected Spergel and Press formalism reproduces dark matter heat transport in realistic Sun, brown dwarf, and Earth models, but with per-scenario fitted parameters.
This is achieved by randomly choosing an optical depth τ , where dτ = X i ωi(⃗ v)dt
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Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets
Monte Carlo simulations show the corrected Spergel and Press formalism reproduces dark matter heat transport in realistic Sun, brown dwarf, and Earth models, but with per-scenario fitted parameters.