HAL will be down for maintenance from Friday, June 10 at 4pm through Monday, June 13 at 9am.
More information
Skip to Main content
Skip to Navigation
Toggle navigation
Sign in
Sign in
Sign in with ORCID
se connecter avec Fédération
Create account
Forgot your password?
Have you forgotten your login?
fr
en
Institute of Physics - RennesMolecular physics Team
Home
Browse
All items
Latest additions
Subject
Document type
Authors
Year
Simple search
Browse by keywords
Browse by Journals
IPR Collection
Home
Browse all deposits
here.
Latest Additions
Search
Full Text Publications
229
Bibliographic Records
936
Resources
How to deposit in HAL?
Do I have the right to deposit?
Contact support Rennes 1
Contact support CCSD
Keywords
Stars oscillations
Cold and ultra-cold collisions
Atomic and molecular physics
Quantum theory
ISM clouds
Microwave spectroscopy
Planetary atmospheres
SAXS
Radial velocities
Molecular collisions
Collisional broadening
Catalogs
Quantum scattering
Stimulated Raman spectroscopy
Atmospheric chemistry
Reaction kinetics
Linewidths
Shock waves
CRESUCHIRP
Atomic and molecular collision
ISM abundances
Stars fundamental parameters
Astrochemistry
Soot
Helium clusters
Photolysis
CRESU
Molecular processes
Collisional
Stars evolution
Optical-optical double resonance spectroscopy
Low temperature chemistry
He
MCTDH
Kinetics
Quantum physics
Spectroscopy
Astrophysics
Cold collisions
X-ray scattering
Low temperature chemical kinetics
Nanoparticles
Chemical physics
Spectrometers
Astrophysics laboratory
Tropospheric lifetimes
Acetylene
Titan
Pressure broadening
Potential energy
Chemical kinetics
Vibronic couplings
Molecular data
Fretting corrosion
Stars formation
Methods numerical
Proper motions
Astrophysics - Solar and Stellar Astrophysics
Nitrogen
Spectral element methods
Probes
Ab initio calculations
Artificial Neuron Networks ANN
Binaries spectroscopic
Combustion
Astrophysics - Astrophysics of Galaxies
Fourier transform infrared spectroscopy
Stars solar-type
Methane
Spectral line shape
Laboratory astrophysics
Radio lines ISM
Collisions
Quantum chemistry
Asteroseismology
Hydrogen
Stars interiors
Rate coefficients
Methods data analysis
Atomic and molecular collisions
Line shape parameters
Quantum dynamics
Plasma plume
Molecules
Contact voltage
Line profiles
Methods analytical
ISM molecules
Contact resistance
Astrometry
Surveys
Reaction dynamics
Reaction kinetics and dynamics
Atmospheres
Quantum Monte Carlo
Low temperatures
Potential energy surfaces
Molecular physics
Optical frequency comb spectroscopy
Reaction products