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.
[4, 8] ( mχ = 1 kg, R⋆ = 2.4 m), and a realistic solar model using temperature, density and composition data from the AGS05 Standard Solar Model
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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.