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or more topics of focus of the evolved star group: 1) the extended atmospheres, 2) the wind-ISM interaction regions (including hydrodynamical modeling), 3) circumstellar magnetic fields, 4) circumstellar
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kinetic models and their hydrodynamic limits. Dispersive phenomena in kinetic theory. Quantum gases. Applicants must hold a PhD degree in mathematics, physics or a related field. We seek candidates with
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Laboratory's activities cover a wide range of fields, from statistical physics to hydrodynamic turbulence, including mathematical physics and signal processing, as well as soft and condensed matter
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ultrafast processes involved in LWFA. You will use the PIC code Smilei to model short time-scale phenomena (plasma ionization, initial heating, and LWFA dynamics within the formed channel). You will also
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including: Magnetohydrodynamics and the mathematical theory of plasmas. Collisional kinetic models and their hydrodynamic limits. Dispersive phenomena in kinetic theory. Quantum gases. Applicants must hold a
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, stochastic calculus, hydrodynamics, numerical simulations Website for additional job details https://emploi.cnrs.fr/Offres/CDD/UMR8237-RAPVOI-006/Default.aspx Work Location(s) Number of offers
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in a wave tank under regular and irregular waves. Develop and document high-fidelity numerical models (e.g., coupled hydrodynamic–structural models and/or FEM workflows). Develop and validate
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of gels with different swelling responses. Specific tasks include: - Perform experimental work on microfluidics and soft condensed matter. - Analysize data. - Use theoretical models to rationalize data