Can an ab initio three-body virial equation describe the mercury gas phase?

We report a sixth-order ab initio virial equation of state (EOS) for mercury. The virial coefficients were determined in the temperature range from 500 to 7750 K using a three-body approximation to the N-body interaction potential.

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Bibliographic Details
Main Authors: Wiebke, Jonas (Author) , Wormit, Michael (Author) , Hellmann, R. (Author) , Pahl, E. (Author) , Schwerdtfeger, P. (Author)
Format: Article (Journal)
Language:English
Published: February 18, 2014
In: The journal of physical chemistry. B, Biophysics, biomaterials, liquids, and soft matter
Year: 2014, Volume: 118, Issue: 12, Pages: 3392-3400
ISSN:1520-5207
DOI:10.1021/jp412260a
Online Access:Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1021/jp412260a
Verlag, lizenzpflichtig, Volltext: https://pubs.acs.org/doi/10.1021/jp412260a
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Author Notes:J. Wiebke, M. Wormit, R. Hellmann, E. Pahl, and P. Schwerdtfeger
Description
Summary:We report a sixth-order ab initio virial equation of state (EOS) for mercury. The virial coefficients were determined in the temperature range from 500 to 7750 K using a three-body approximation to the N-body interaction potential.
Item Description:Gesehen am 01.09.2020
Physical Description:Online Resource
ISSN:1520-5207
DOI:10.1021/jp412260a