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We suggest certain effects, caused by interaction between rotation andgravitation with turbulence structure, for the cooling/heating of dispersedphase of non-isothermal particles in rotating turbulent fluid flows. Theseeffects are obtained through the derivation of kinetic or probability densityfunction based macroscopic equations for the particles. In doing so, forone-way temperature coupling, we also show that homogeneous, isotropicnon-isothermal fluid turbulence does not influence the mean temperature (thoughit influences mean velocity) of the dispersed phase of particles settling dueto gravitational force in the isotropic turbulence.

Dispersed Phase of Non-Isothermal Particles in Rotating Turbulent Flows