Instanton calculus in shell models of turbulence

Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics

Volumn 62, Issue 3 A, 2000, Pages 3592-3610

  Daumont, Isabelle ^a,b   Dombre, Thierry ^a   Gilson, Jean Louis ^a  

^a UNIV GRENOBLE ALPES   (France)

^b UNIVERSITÉ DE LYON   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EQUATIONS OF MOTION; MATHEMATICAL MODELS; PROBABILITY DENSITY FUNCTION; RANDOM PROCESSES;

GLEDZER-OHKITANI-YAMADA MODEL; INSTANTONS;

TURBULENCE;

EID: 0034272220     PISSN: 1063651X     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevE.62.3592     Document Type: Article

References (37)

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35. Actually, this change of variable is not strictly necessary. It may be shown to roughly "square root" the range of values spanned by the coefficients of matrices U and W introduced in Sec. V A. The ensuing reduction of numerical stiffness allows computations at larger sizes of the shell lattice. However, the switch from δb to h gets totally impracticable when the matrix B cannot be easily inverted.
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