Small-scale clustering of nano-dust grains in turbulent interstellar molecular clouds [Extended version]

Clustering and dynamics of nano-sized particles (nano dust) is investigated using high-resolution (${1024}^3$) simulations of compressible isothermal hydrodynamic turbulence, intended to mimic the conditions inside cold molecular clouds in the interstellar medium. Nano-sized grains may cluster in a turbulent flow (small-scale clustering), which increases the local grain density significantly. Together with the increased interaction rate due to turbulent motions, aggregation of interstellar nano-dust may be plausible.