The question of the shape of the density PDF for supersonic turbulence is adressed, using both analytical and numerical methods. For isothermal supersonic turbulence, the PDF is Log-Normal, with a width that scales approximately linearly with the Mach number. For a polytropic equation of state, with an effective gamma smaller than one, the PDF becomes skewed and becomes reminiscent of (but not equal to) a power law on the high density side.
CITATION STYLE
Nordlund, Å., & Padoan, P. (2010). The Density PDFs of Supersonic Random Flows. In Interstellar Turbulence (pp. 218–222). Cambridge University Press. https://doi.org/10.1017/cbo9780511564666.034
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