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dc.contributor.author
Calzetta, Esteban Adolfo  
dc.date.available
2018-10-01T16:30:36Z  
dc.date.issued
2009-05  
dc.identifier.citation
Calzetta, 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.identifier.issn
1539-3755  
dc.identifier.uri
http://hdl.handle.net/11336/61360  
dc.description.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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
American Physical Society  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Turbulence  
dc.subject.classification
Astronomía  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Friction factor for turbulent flow in rough pipes from Heisenberg's closure hypothesis  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2018-10-01T14:23:15Z  
dc.journal.volume
79  
dc.journal.number
5  
dc.journal.pagination
1-7  
dc.journal.pais
Estados Unidos  
dc.journal.ciudad
Nueva York  
dc.description.fil
Fil: Calzetta, Esteban Adolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina  
dc.journal.title
Physical Review E: Statistical, Nonlinear and Soft Matter Physics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevE.79.056311  

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