Density and Velocity Correlations in Isothermal Supersonic Turbulence

Abstract

In star-forming clouds, high velocity flow gives rise to large fluctuations of density. In this work we explore the correlation between velocity magnitude (speed) and density. We develop an analytic formula for the joint probability distribution (PDF) of density and speed, and discuss its properties. In order to develop an accurate model for the joint PDF, we first develop improved models of the marginalized distributions of density and speed. We confront our results with a suite of 12 supersonic isothermal simulations with resolution of $1024^3$ cells in which the turbulence is driven by 3 different forcing modes (solenoidal, mixed and compressive) and 4 r.m.s. Mach numbers (1, 2, 4, 8). We show, that for transsonic turbulence, density and speed are correlated to a considerable degree and the simple assumption of independence fails to accurately describe their statistics. In the supersonic regime, the correlations tend to weaken with growing Mach number. Our new model of the joint and marginalized PDFs are a factor of 3 better than uncorrelated, and provides insight into this important process.

arXiv commentSubmitted to MNRAS

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• The Formation of Protoplanetary Disks through Pre-Main Sequence Bondi-Hoyle Accretion
• Supersonic turbulence simulations with GPU-based high-order Discontinuous Galerkin hydrodynamics
• Impact of the shape of the prestellar density fluctuations on the core mass function
• An Improved Fit to the Density Distribution in Supersonic Isothermal Turbulence