A MOLECULAR DYNAMICS STUDY OF THE PRESSURE-VOLUME-TEMPERATURE PROPERTIES OF SUPERCRITICAL FLUIDS: II. CO2, CH4, CO, O2, AND H2

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dc.contributor.author Belonoshko A.
dc.contributor.author Saxena S.K.
dc.date.accessioned 2020-11-06T09:16:12Z
dc.date.available 2020-11-06T09:16:12Z
dc.date.issued 1991
dc.identifier https://elibrary.ru/item.asp?id=31673418
dc.identifier.citation Geochimica et Cosmochimica Acta, 1991, , 11, 3191-3208
dc.identifier.issn 0016-7037
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/18581
dc.description.abstract The method of molecular dynamics (MD) has been used to simulate the pressure-volume-temperature (PVT) properties of COâ, CHâ, CO, Oâ, and Hâ. For the MD simulation, the exponential-6 form of the intermolecular potential has been adopted. The parameters of the potential are calculated from the available experimental PVT data. The MD-simulated results fit the experimental (static) PVT data well and are in reasonable agreement with the shock-wave P-V data. Based on both the experimental PVT and the MD-simulated data, equations of the type: P + a/V + b/V² + c/Vâ ¿ have been formulated for each of the five fluids in the pressure range of 5 Kbar to 1 Mbar at temperatures from 400 to 4,000 K. The calculated fugacity of Coâ has been used to show the consistency of the modeled data with the experimental phase equilibrium data on the reactions involving magnesite.
dc.title A MOLECULAR DYNAMICS STUDY OF THE PRESSURE-VOLUME-TEMPERATURE PROPERTIES OF SUPERCRITICAL FLUIDS: II. CO2, CH4, CO, O2, AND H2
dc.type Статья


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