Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:
| Indexado |
|
||||
| DOI | 10.1103/PHYSREVLETT.128.204502 | ||||
| Año | 2022 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Verifying nonlinear stability of a laminar fluid flow against all perturbations is a central challenge in fluid dynamics. Past results rely on monotonic decrease of a perturbation energy or a similar quadratic generalized energy. None show stability for the many flows that seem to be stable despite these energies growing transiently. Here a broadly applicable method to verify global stability of such flows is presented. It uses polynomial optimization computations to construct nonquadratic Lyapunov functions that decrease monotonically. The method is used to verify global stability of 2D plane Couette flow at Reynolds numbers above the the energy stability threshold found by Orr in 1907 [The stability or instability of the steady motions of a perfect liquid and of a viscous liquid. Part II: A viscous liquid, Proc. R. Ir. Acad. Sect. A 27, 69 (1907)]. This is the first global stability result for any flow that surpasses the energy method.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Fuentes, Federico | Hombre |
Cornell University - Estados Unidos
Pontificia Universidad Católica de Chile - Chile CORNELL UNIV - Estados Unidos |
| 2 | Goluskin, David | Hombre |
University of Victoria - Canadá
Univ Victoria - Canadá |
| 3 | Chernyshenko, Sergei | Hombre |
Imperial College London - Reino Unido
Imperial Coll London - Reino Unido |
| Fuente |
|---|
| National Science Foundation |
| Natural Sciences and Engineering Research Council of Canada |
| National Science Foundation (NSF) |
| Engineering and Physical Sciences Research Council |
| NSERC |
| UK Engineering and Physical Sciences Research Council |
| Agradecimiento |
|---|
| We thank the Geophysical Fluid Dynamics program at Woods Hole Oceanographic Institution, which hosted two of us (F. F. and D. G.) during much of this work. Many helpful discussions with Giovanni Fantuzzi are appreciated, and one of us (F. F.) thanks A. Townsend for computer resources provided at Cornell University. During this work, F. F. was supported by the National Science Foundation (NSF) Grant No. 2012658, D. G. was supported by the NSERC Discovery Grants Program through Grants No. RGPIN-2018-04263, No. RGPAS-2018-522657, and No. DGECR-2018-00371, and S. C. was supported by the UK Engineering and Physical Sciences Research Council Grant No. EP/J011126/1. |
| We thank the Geophysical Fluid Dynamics program at Woods Hole Oceanographic Institution, which hosted two of us (F. F. and D. G.) during much of this work. Many helpful discussions with Giovanni Fantuzzi are appreciated, and one of us (F. F.) thanks A. Townsend for computer resources provided at Cornell University. During this work, F. F. was supported by the National Science Foundation (NSF) Grant No. 2012658, D. G. was supported by the NSERC Discovery Grants Program through Grants No. RGPIN-2018-04263, No. RGPAS-2018-522657, and No. DGECR-2018-00371, and S. C. was supported by the UK Engineering and Physical Sciences Research Council Grant No. EP/J011126/1. |