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.
The DM temperature Tχ in this case is the average of the nucleon temperatures with which the DM is in thermal contact with, weighted by the local inter- action rate
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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.