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Updated: Jul 15, 2025

Computation of Atmospheric Concentrations of Molecular Clusters from ab initio Thermochemistry
Published on: April 8, 2020
The Challenge of ab Initio Calculations in Small Neon Clusters
Ignacio Ema1, Guillermo Ramírez1, Rafael López1
1Departamento de Química Física Aplicada, Universidad Autónoma de Madrid.
This study investigates weakly bound neon clusters, determining their binding energies and structures using advanced computational methods. New SIGMA-s basis sets were developed for accurate analysis of these small neon systems.
Area of Science:
- Computational Chemistry
- Quantum Chemistry
- Atomic and Molecular Physics
Background:
- Weakly bound clusters are fundamental in understanding intermolecular forces.
- Accurate theoretical descriptions of noble gas clusters are challenging due to weak interactions.
Purpose of the Study:
- To investigate the ground-state binding energies and structural properties of neon dimer, trimer, and tetramers.
- To develop and validate new SIGMA-s basis sets for studying weakly bound systems.
- To assess the accuracy of different basis sets and computational levels for these systems.
Main Methods:
- High-level ab initio calculations using Hartree-Fock (HF) and Coupled Cluster with Singles and Doubles and perturbative Triples (CCSD(T)) methods.
- Utilized Dunning, Augmented Near-Optimized (ANO), and newly developed SIGMA-s basis sets of varying sizes.
- Computed total energies, atomization energies, correlation energies, and equilibrium distances.
Main Results:
- Determined ground-state binding energies and structural parameters for neon clusters (Ne2, Ne3, Ne4).
- Demonstrated the effectiveness of the SIGMA-s basis sets for accurately describing weak interactions.
- Evaluated the impact of basis set size and augmentation on calculated properties.
Conclusions:
- The developed SIGMA-s basis sets provide accurate results for weakly bound neon systems.
- Extrapolation methods can reliably predict stabilization energies for larger systems.
- This work offers a benchmark for future studies on noble gas clusters.
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