Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis

dc.creatorCalzetta, Esteban Adolfo
dc.date.accessioned2018-10-01T16:30:36Z
dc.date.available2018-10-01T16:30:36Z
dc.date.created2018-10-01T16:30:36Z
dc.date.issued2009-05
dc.identifierCalzetta, Esteban Adolfo; Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis; American Physical Society; Physical Review E: Statistical, Nonlinear and Soft Matter Physics; 79; 5; 5-2009; 1-7
dc.identifier1539-3755
dc.identifierhttp://hdl.handle.net/11336/61360
dc.identifierCONICET Digital
dc.identifierCONICET
dc.description.abstractWe 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.
dc.languageeng
dc.publisherAmerican Physical Society
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevE.79.056311
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectTurbulence
dc.titleFriction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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