English

Exact relation for correlation functions in compressible isothermal turbulence

Solar and Stellar Astrophysics 2015-05-30 v1 Fluid Dynamics

Abstract

Compressible isothermal turbulence is analyzed under the assumption of homogeneity and in the asymptotic limit of a high Reynolds number. An exact relation is derived for some two-point correlation functions which reveals a fundamental difference with the incompressible case. The main difference resides in the presence of a new type of term which acts on the inertial range similarly as a source or a sink for the mean energy transfer rate. When isotropy is assumed, compressible turbulence may be described by the relation, 23ϵeffr=Fr(r)- {2 \over 3} \epsilon_{\rm{eff}} r = {\cal F}_r(r), where Fr{\cal F}_r is the radial component of the two-point correlation functions and ϵeff\epsilon_{\rm{eff}} is an effective mean total energy injection rate. By dimensional arguments we predict that a spectrum in k5/3k^{-5/3} may still be preserved at small scales if the density-weighted fluid velocity, ρ1/3\uu\rho^{1/3} \uu, is used.

Keywords

Cite

@article{arxiv.1108.4529,
  title  = {Exact relation for correlation functions in compressible isothermal turbulence},
  author = {Sebastien Galtier and Supratik Banerjee},
  journal= {arXiv preprint arXiv:1108.4529},
  year   = {2015}
}

Comments

10 pages, 1 figures, will appear in PRL

R2 v1 2026-06-21T18:54:01.373Z