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Propagating modes in a binary liquid mixture under thermal stress

Authors :
Henri Bataller
Alberto Vailati
José M. Ortiz de Zárate
Fabrizio Croccolo
L. García-Fernández
European Space Agency
Centre National D'Etudes Spatiales (France)
Universidad Complutense de Madrid
Ministerio de Ciencia, Innovación y Universidades (España)
Laboratoire des Fluides Complexes et leurs Réservoirs (LFCR)
Centre National de la Recherche Scientifique (CNRS)-Université de Pau et des Pays de l'Adour (UPPA)-TOTAL FINA ELF
Thermodynamique et Energétique des fluides complexes (TEFC)
Université de Pau et des Pays de l'Adour (UPPA)-TOTAL SA-Centre National de la Recherche Scientifique (CNRS)
Source :
E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid, E-Prints Complutense. Archivo Institucional de la UCM, instname, Physical Review E, Physical Review E, American Physical Society (APS), 2019, 99 (1), ⟨10.1103/physreve.99.012602⟩, Digital.CSIC. Repositorio Institucional del CSIC
Publication Year :
2019
Publisher :
Amer Physical Soc, 2019.

Abstract

8 pags., 4 figs.<br />Nonequilibrium temperature and concentration fluctuations inside a binary liquid mixture under the action of a temperature gradient relax back to equilibrium either due to conduction and diffusion at large wave numbers, or due to the quenching determined by gravity at small wave numbers. We investigate the dynamics of nonequilibrium fluctuations in a binary liquid mixture of polystyrene and toluene heated from above under stationary conditions in a thermodiffusion experiment. We show that the strong gravitational stabilization at small wave numbers determines the appearance of propagating modes of nonequilibrium fluctuations as detected through the structure function of shadowgraph images. The propagating modes are the combined effect of temperature and velocity nonequilibrium fluctuations induced by the buoyancy force. The experimental results are in good agreement with a fluctuating hydrodynamics theroretical model including the coupling of fluctuations of velocity, temperature and concentration.<br />We gratefully acknowledge support from the European Space Agency (ESA) and the Centre National d’Etudes Spatiales (CNES) of France, specifically for supporting the acquisition of the fast camera that made it possible to observe the propagating mode described in this paper. F.C., L.G.F., and H.B. would like to thank E2S-UPPA for financial support. The research at the Complutense University was supported by Grant No. ESP2017-83544-C3-2-P of the Spanish Agencia Estatal de Investigación.

Details

ISSN :
24700045 and 24700053
Database :
OpenAIRE
Journal :
E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid, E-Prints Complutense. Archivo Institucional de la UCM, instname, Physical Review E, Physical Review E, American Physical Society (APS), 2019, 99 (1), ⟨10.1103/physreve.99.012602⟩, Digital.CSIC. Repositorio Institucional del CSIC
Accession number :
edsair.doi.dedup.....a464374f60bbde63c0be75f40ef85de3