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Scattering SAXS Stars solar-type Methods data analysis PhDtitle Stars interiors Soutenance2016 Shock waves Photolysis Spectral line shape Titan Potential energy Methods analytical Catalogs Artificial Neuron Networks ANN Kinetics Plasma plume Planetary atmospheres Quantum physics Reaction dynamics Astrophysics laboratory Proper motions Ab initio calculations Potential energy surfaces Astrophysics - Astrophysics of Galaxies Astrophysics Astrophysics - Solar and Stellar Astrophysics Collisional Low temperatures Methane Methods numerical Cold collisions Collisional broadening Vibronic couplings Fretting corrosion Quantum theory Laboratory astrophysics Stars fundamental parameters Quantum Monte Carlo Quantum scattering Fourier transform infrared spectroscopy Molecular collisions Surveys Cold and ultra-cold collisions He Nanoparticles Rotational spectroscopy Reaction kinetics Stars formation Computational chemistry Spectroscopy Molecular processes Linewidths Molecular data Contact resistance ISM abundances Helium clusters Line shape parameters Radial velocities Astrochemistry Low temperature chemistry Nitrogen Radio lines ISM Contact voltage Probes Pressure broadening Chemical kinetics Low temperature chemical kinetics Quantum dynamics Collisions Line profiles Quantum chemistry ISM clouds MCTDH Spectral element methods Stars evolution Microwave spectroscopy Hydrogen Molecules CRESU Combustion Soutenance2022 Molecular physics Reaction products Radiative transfer Rate coefficients Atomic and molecular physics Atomic and molecular collisions Asteroseismology Binaries spectroscopic Astrometry Soot Reaction kinetics and dynamics Soutenance2021 Stars oscillations Soutenance2017 Chemical physics ISM molecules Optical frequency comb spectroscopy Optical-optical double resonance spectroscopy