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| * [[animation:workshops:2013:accueil|Workshops 2013]] | * [[animation:workshops:2013:accueil|Workshops 2013]] | ||
| - | ====== ====== | + | ====== Influence of Interfacial Interactions on Structural and Rheological Properties of Confined Liquids ====== |
| - | {{:animation:workshops:2013:plasmalogo.jpeg?nolink&200 |}} | + | {{:animation:workshops:2013:confine.png?nolink&200 |}}Centre Blaise Pascal, ENS-Lyon, France \\ |
| - | Centre Blaise Pascal, ENS-Lyon, France \\ | + | September 23, 2013 \\ |
| - | June 20-21, 2013 \\ | + | [[http://confine.sciencesconf.org/|Website of the workshop]] |
| - | [[http://plasma2013.sciencesconf.org/|Website of the workshop]] | + | |
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| - | Organizing committee: | + | |
| - | * **Rolf Walder**, CRAL, École normale supérieure de Lyon | + | |
| - | * **Alexandre Marcowith**, LUPM, Laboratoire Univers et Particules, Université Montpellier 2, France | + | |
| - | * **Andrei Bykov**, Ioffe Institute, Russian Academy of Sciences, St. Petersburg, Russia | + | |
| - | * **Christophe Winisdoerffer**, CRAL, École normale supérieure de Lyon, France | + | |
| - | * **Mickaël Melzani**, CRAL, École normale supérieure de Lyon, France | + | |
| - | Administrative coordination: | + | Organizing committee: **Claire Loison**, Lasim, UCBL-CNRS, France |
| - | * **Samantha Barendson**, CBP, ENS de Lyon, France (samantha.barendson @ ens-lyon.fr) | + | |
| + | Administrative coordination: **Samantha Barendson**, CBP, ENS de Lyon, France (samantha.barendson @ ens-lyon.fr) | ||
| The workshop is supported by: | The workshop is supported by: | ||
| * **CBP** - Centre Blaise Pascal, Lyon, France | * **CBP** - Centre Blaise Pascal, Lyon, France | ||
| - | * **FLMSN** - Fédération Lyonnaise de Modélisation et Sciences Numériques | + | * **FLMSN** - Fédération Lyonnaise de Modélisation et Sciences Numérique |
| - | * **CRAL** - Centre de Recherche Astrophysique de Lyon | + | |
| - | * **ENSL** - École normale supérieure de Lyon | + | |
| - | * **Université de Lyon** | + | |
| - | * **CNRS** - Centre National de la Recherche Scientifique | + | |
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| ===== Summary ===== | ===== Summary ===== | ||
| - | The acceleration of non-thermal particles in large scale flows is of prime importance in astrophysics and beyond. Cosmic accelerators can energize particles up to 10²⁰ eV. The flux of high-energy cosmic rays has a strong impact on Earth, on its climate and weather. | + | The structure of a liquid may drastically change if it is confined within a narrow space. This affects many phenomena in nature and technology such as diffusion through narrow pores, viscosity, swelling of clay and lubrication. However, an understanding of the fluid ordering induced by the confining surfaces is still lacking. |
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| - | However, accelerators embedded in large scale MHD flows within astrophysical objects still remain enigmatic in various ways. The aim of the workshop is to bring together people of different communities and approaches: modelers of large scale flows, scientists scrutinizing fundamental processes, people who are deriving observable signatures, and numerical specialists. We also aim at bringing together the French with the European community and strengthen the collaboration between them, specially emphasizing the Rhône-Alpes region. | + | |
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| - | The first day concentrates on theoretical questions of plasma physics, particle acceleration, magnetic reconnection, and turbulence in plasma fluids. This includes open questions of how to model these phenomena and how to realize such models numerically. | + | |
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| - | The second day presents results of modeling concrete astrophysical objects: microquasars and X-ray binaries, pulsars and their winds, gamma-ray bursts, solar wind, supernova remnants and superbubbles, the interstellar medium. | + | |
| + | During this workshop, experimental and theoretical results shall be presented on the impact of confinement on the structure and rheological properties of colloidal fluids, ie liquids which spontaneously show nanometer-scale ordering even in a bulk phase. | ||