Sort by
Refine Your Search
-
Listed
-
Category
-
Program
-
Field
-
-simulation databases opening up the possibility of interpretations by deep learning techniques. A numerical database is provided by the team at CORIA, which is also in charge of developing the optical models
-
an atomistic model of the electrode/electrolyte interface in the batteries developed by ITEN, at the anode and at the cathode. Both electrodes are based on lithium-based transition metal oxides. These models
-
fundamental understanding of climate change and its impacts, extending to the development of prototype climate services co-designed by stakeholders and climate modeling experts. The goal is to accelerate
-
collaboration with Michelin, is to develop surrogate models capable of rapidly approximating the simulator's results while accounting for uncertainty. Particular attention will be paid to the model's lightness
-
preparation to conduct the experiments (lamination by thermocompression, …) by working closely on an internal Lab-platform. The postdoctoral fellow will develop her/his activity at the LAPLACE Institute, within
-
evaluated for the reduction of CO2 to C1 molecules (MeOH, formate, CO). In addition to the development of new catalysts, the successful candidate will study the influence of different host structures
-
interventions, creating environmentally sustainable devices, and developing simulators to reduce reliance on in vivo testing. The training network is interdisciplinary, integrating various fields such as
-
to date. We contribute a multidisciplinary research effort aiming at developing biomimetic LH materials - i.e. efficient at transporting EEE within thousands of dyes - for applications to light energy
-
action. The project will focus on the use of natural polymers derived from biomass (such as pectin, cellulose, and hemicellulose). Activities and Methodology Development of experimental setups in (micro
-
project is to develop the next generation of solar jet propagation models from the lower atmosphere to the inner heliosphere, and to allow a direct comparison with real in-situ data of the early solar wind