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Updated: May 29, 2026

Thermochemical Studies of Ni(II) and Zn(II) Ternary Complexes Using Ion Mobility-Mass Spectrometry
Published on: June 8, 2022
First-principles simulation of molecular dissociation-recombination equilibrium.
Ilkka Kylänpää1, Tapio T Rantala
1Department of Physics, Tampere University of Technology, P.O. Box 692, FI-33101 Tampere, Finland. ilkka.kylanpaa@tut.fi
This study presents the first first-principles simulation of chemical dissociation-recombination reactions, incorporating nuclear quantum effects and electron-nuclear coupling for the H(3)(+) ion. Results cover a wide temperature range, detailing reaction balance and thermal ionization.
Area of Science:
- Quantum chemistry
- Chemical physics
- Computational physics
Background:
- Accurate simulation of chemical reactions requires considering nuclear quantum effects and electron-nuclear coupling.
- Previous ab initio methods often neglect these dynamics, limiting their applicability at extreme temperatures.
Purpose of the Study:
- To perform the first first-principles simulation of chemical dissociation-recombination reactions.
- To consistently include nuclear quantum dynamics and nonadiabatic coupling.
- To investigate the H(3)(+) ion's behavior across a broad temperature spectrum.
Main Methods:
- Path integral Monte Carlo simulations were employed for full NVT quantum statistics.
- Ab initio quantum chemistry calculations were performed.
- Simulations covered temperatures from below room temperature to those relevant for planetary atmospheres.
Main Results:
- The study presents the equilibrium composition of dissociation-recombination reactions.
- Temperature and density-dependent reaction balance of the molecular ion and its fragments above 4000 K was determined.
- The density dependence of thermal ionization above 10,000 K was demonstrated.
Conclusions:
- This work provides a comprehensive, first-principles understanding of H(3)(+) ion chemistry.
- The inclusion of nuclear quantum effects and electron-nuclear coupling is crucial for accurate simulations.
- The findings are relevant for understanding planetary atmospheric physics.
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