Exact Relation for Correlation Functions in Compressible Isothermal Turbulence

被引:125
作者
Galtier, Sebastien [1 ,2 ]
Banerjee, Supratik [1 ]
机构
[1] Univ Paris 11, Inst Astrophys Spatiale, UMR 8617, F-91405 Orsay, France
[2] Inst Univ France, F-75005 Paris, France
关键词
INTERSTELLAR TURBULENCE; SUPERSONIC TURBULENCE; BURGERS TURBULENCE; MOLECULAR CLOUDS; WAVE TURBULENCE; STATISTICS; KOLMOGOROV;
D O I
10.1103/PhysRevLett.107.134501
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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 -2/3 epsilon(eff) r =F-r(r), where F-r is the radial component of the two-point correlation functions and epsilon(eff) is an effective mean total energy injection rate. By dimensional arguments, we predict that a spectrum in k(-5/3) may still be preserved at small scales if the density-weighted fluid velocity rho(1/3) is used.
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页数:5
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