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Aspen Physical Property System - Physical Property Models

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Where:<br />

Parameter<br />

Name/Element<br />

2 Thermodynamic <strong>Property</strong> <strong>Models</strong> 17<br />

Symbol Default MDS Lower<br />

Limit<br />

Upper<br />

Limit<br />

Units<br />

TCBWR T ci TC X 5.0 2000.0 TEMPERATURE<br />

VCBWR V ci *<br />

BWRGMA � i<br />

BWRKV � ij<br />

BWRKT � ij<br />

VC X 0.001 3.5 MOLE-<br />

VOLUME<br />

OMEGA X -0.5 3.0 —<br />

0 X -5.0 1.0 —<br />

0 X -5.0 1.0 —<br />

Binary interaction parameters BWRKV and BWRKT are available in the <strong>Aspen</strong><br />

<strong>Physical</strong> <strong>Property</strong> <strong>System</strong> for a large number of components from Brulé et al.<br />

(1982) and from Watanasiri et al. (1982). (See <strong>Physical</strong> <strong>Property</strong> Data,<br />

Chapter 1).<br />

References<br />

M.R. Brulé, C.T. Lin, L.L. Lee, and K.E. Starling, AIChE J., Vol. 28, (1982) p.<br />

616.<br />

Brulé et al., Chem. Eng., (Nov., 1979) p. 155.<br />

Watanasiri et al., AIChE J., Vol. 28, (1982) p. 626.<br />

Benedict-Webb-Rubin-Starling<br />

The Benedict-Webb-Rubin-Starling equation-of-state is the basis of the BWRS<br />

property method. It is a modification by Han and Starling of the virial<br />

equation-of-state for pure fluids by Benedict, Webb and Rubin. This equationof-state<br />

can be used for hydrocarbon systems that include the common light<br />

gases, such as H2S, CO2 and N2.<br />

The form of the equation-of-state is:

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