Abstract:
We show that the main results of the analysis of the friction factor for turbulent pipe flow reported by Gioia and Chakraborty [Phys. Rev. Lett. 96, 044502 (2006)] can be recovered by assuming the Heisenberg closure hypothesis for the turbulent spectrum. This highlights the structural features of the turbulent spectrum underlying the analysis of Gioia and Chakraborty. © 2009 The American Physical Society.
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Citas:
---------- APA ----------
(2009)
. Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis. Physical Review E - Statistical, Nonlinear, and Soft Matter Physics, 79(5).
http://dx.doi.org/10.1103/PhysRevE.79.056311---------- CHICAGO ----------
Calzetta, E.
"Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis"
. Physical Review E - Statistical, Nonlinear, and Soft Matter Physics 79, no. 5
(2009).
http://dx.doi.org/10.1103/PhysRevE.79.056311---------- MLA ----------
Calzetta, E.
"Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis"
. Physical Review E - Statistical, Nonlinear, and Soft Matter Physics, vol. 79, no. 5, 2009.
http://dx.doi.org/10.1103/PhysRevE.79.056311---------- VANCOUVER ----------
Calzetta, E. Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis. Phys. Rev. E Stat. Nonlinear Soft Matter Phys. 2009;79(5).
http://dx.doi.org/10.1103/PhysRevE.79.056311