The Saalfrank Group develops quantum mechanical models for molecular dynamics, spectroscopy, and reactions in complex environments.
In IRAstro, the group works with:
T1: IR spectra from molecules on surfaces under interstellar conditions
• 1A. Theoretical modelling of Laser induced mid-IR spectroscopy of adsorbates
• 1B. Theoretical modelling of Single-molecule IR emission spectroscopy
T2: Energy dissipation on low-T surfaces
• 2A. Theoretical modelling Vibrational dissipation in astrochemical relevant systems
• 2B. Theoretical modelling High-resolution spectroscopy of condensed phase isomerization
T3: Chemical reactivity under interstellar conditions
• 3A. Theoretical modelling Gateway tunneling in reactions of astrochemical significance
• 3B. Theoretical modelling Vibrationally driven interstellar reactions
This work provides the framework needed to interpret and predict experimental results
