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. They present a strong spin-orbit coupling, a relatively long spin relaxation times, and an optical accessibly for spin generation and detection. The objective of the PhD is to explore the exciton and spin
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into account — for the first time — the cognitive processes related to peripheral vision and their evolution with age. Relying on a multidisciplinary approach that combines psychophysics, eye tracking, and
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PhD on 2D quantum photonics : towards neuromorphic applications with 2D ferroelectrics materials M/F
-of-plane ferroelectric domains. The goal of this PhD is to optically detect, track, and ultimately control the ferroelectric state in such materials. Key objectives include imaging ferroelectric domains in a
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, which has around 20 members (including a dozen doctoral students and fixed-term contract researchers) conducting research in the fields of mass spectrometry and optical spectroscopy. Candidates should
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team, which has around 20 members (including a dozen doctoral students and fixed-term contract researchers) conducting research in the fields of mass spectrometry and optical spectroscopy. The thesis
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create different chiral nanomaterials that will be studied by optical spectroscopy (circular dichroism, photoluminescence, circularly polarised nonlinear optics). The PhD student will acquire expertise in
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and draping singularities resulting from the manufacturing process on the thermomechanical damage and permeability of thermoplastic composites used for liquid hydrogen storage. With the energy
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both fundamental and applied studies in photonics, turbulence, atomization, and reactive flows. The recruited person will join the Optics and Lasers Department of CORIA. The position falls within a
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. Experimental characterization of Hall effect thrusters using combination of diagnostic techniques such as optical emission and absorption, Langmuir probes, etc. enhanced by the application of machine learning
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crucial applications in astronomy and geodesy. Today, two fundamental CRF realizations coexist: the ICRF3 realized by geodetic very long baseline interferometry (VLBI), and the optical ESA's Gaia-CRF3