## Abstract The thermodynamic properties of three halocarbon molecules relevant in atmospheric and public health applications are presented from __ab initio__ calculations. Our technique makes use of a reaction path‐like Hamiltonian to couple all the vibrational modes to a large‐amplitude torsion f
Thermodynamic calculations for molecules with asymmetric internal rotors—application to 1,3-butadiene
✍ Scribed by Bryan M. Wong; Sumathy Raman
- Publisher
- John Wiley and Sons
- Year
- 2007
- Tongue
- English
- Weight
- 337 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0192-8651
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✦ Synopsis
Abstract
We present quantum mechanical partition functions, free energies, entropies, and heat capacities of 1,3‐butadiene derived from ab initio calculations. Our technique makes use of a reaction path‐like Hamiltonian to couple all 23 vibrational modes to the large‐amplitude torsion, which involves heavy asymmetric functional groups. Ab initio calculations were performed at the B3LYP, MP2, and CCSD(T) levels of theory and compared with experimental values as a reference case. By using the ab initio potentials and projected frequencies, simple perturbative expressions are presented for computing the couplings of all the vibrational modes to the large‐amplitude torsion. The expressions are particularly suited for programming in the new STAR‐P software platform which automatically parallelizes our codes with distributed memory via a familiar MATLAB interface. Using the efficient parallelization scheme of STAR‐P, we obtain thermodynamic properties of 1,3‐butadiene for temperatures ranging from 50 to 500 K. The free energies, entropies, and heat capacities obtained from our perturbative formulas are compared with conventional approximations and experimental values found in thermodynamic tables. © 2007 Wiley Periodicals, Inc.J Comput Chem 28: 759–766, 2007
📜 SIMILAR VOLUMES
A new IAM approach based on properties of the generalized inertia tensor and its derivatives for the molecules with internal rotation which have symmetry isomorphic to C 3£ (M) has been developed. For solution the torsional-rotational Hamiltonian is divided into parts dependent and independent on th