Molecular Calculation of the Critical Parameters of Classical Helium

Richard A. Messerly, Navneeth Gokul, Andrew J. Schultz, David A. Kofke, Allan H. Harvey

Research output: Contribution to journalArticlepeer-review

8 Scopus citations

Abstract

We compute the vapor-liquid critical coordinates of a model of helium in which nuclear quantum effects are absent. We employ highly accurate ab initio pair and three-body potentials and calculate the critical parameters rigorously in two ways. First, we calculate the virial coefficients up to seventh order and find the point where an isotherm satisfies the critical conditions. Second, we use Gibbs ensemble Monte Carlo (GEMC) to calculate the vapor-liquid equilibrium and extrapolate the phase envelope to the critical point. Both methods yield results that are consistent within their uncertainties. The critical temperature of "classical helium" is 13.0 K (compared to 5.2 K for real helium), the critical pressure is 0.93 MPa, and the critical density is 28.4 mol·L-1, with expanded uncertainties (corresponding to a 95% confidence interval) on the order of 0.1 K, 0.02 MPa, and 0.5 mol·L-1, respectively. The effect of three-body interactions on the location of the critical point is small (lowering the critical temperature by roughly 0.1 K), suggesting that we are justified in ignoring four-body and higher interactions in our calculations. This work is motivated by the use of corresponding-states models for mixtures containing helium (such as some natural gases) at higher temperatures where quantum effects are expected to be negligible. In these situations, the distortion of the critical properties by quantum effects causes problems for the corresponding-states treatment.

Original languageEnglish
Pages (from-to)1028-1037
Number of pages10
JournalJournal of Chemical and Engineering Data
Volume65
Issue number3
DOIs
StatePublished - Mar 12 2020
Externally publishedYes

Funding

We are grateful to Eliseo Marin-Rimoldi of the Molecular Sciences Software Institute for invaluable support in modifying the Cassandra code and to Alta Fang of NIST for a careful reading of the manuscript. Support for University at Buffalo authors is provided by the U.S. National Institute of Standards and Technology, award no. 70NANB17H334, and by the U.S. National Science Foundation, grant CBET-1510017. This research was performed while R.A.M. held a National Research Council (NRC) Postdoctoral Research Associateship at NIST.

FundersFunder number
National Science FoundationCBET-1510017
National Institute of Standards and Technology70NANB17H334

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