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Field
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. Extension to non-stationary acoustic fields: The study will initially focus on stationary fields and will then be extended to time-varying situations. The objective is to develop a time-dependent formulation
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own resonant frequency. MKIDs are an innovative detection technology that will open up a wide range of applications in astronomy et astrophysics. Since 2020, we have been developing at Paris Observatory
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atmospheric aging. These simplifications constrain the reliability of projections and weaken policy assessment capabilities. The thesis will develop an improved representation of MP/NP in GEOS-Chem. The size
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. The unit develops interdisciplinary research at the interface of physiology, cell biology, biochemistry and medicine, hosts state-of-the art scientific technological platforms. It is a stimulating and highly
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of atomic nuclei. It played an important role in the early evolution of the Universe and is crucial for the structure of compact stellar objects such as neutron stars. Understanding the properties of matter
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to develop the following research project : Reverse-engineered concrete formulations to evaluate the risk of Alkali-Silica Reaction in case of extended life Nuclear Power Plant This postdoctoral position is
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for the development of critical systems. However, there has not yet been a lot of effort in formalizing these languages, their semantics or their execution model. The goal of this research project is to
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have been developed in the linear framework for several decades, the current challenge remains their extension to the nonlinear framework, which is necessary for an accurate description of complex
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Sorbonne Université SIS (Sciences, Ingénierie, Santé) | Palaiseau, le de France | France | 2 months ago
the relevant expertise in the development of such CRM on various planetary environments, most recently on Uranus, Neptune and mini-Neptunes (exoplanets) [Leconte et al., 2024, Clément et al., 2024]. The PhD
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cosmology. In this context, we have developed a multi-scale detection method specifically designed to identify galaxy clusters based only on their gravitational lensing signal, which has been pre-selected