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