Skip to content
OwlStudy Owl OwlStudy
Note

Determination of Fugacity by Virial Equation

Study context

University
Veer Bahadur Singh Purvanchal University
Faculty
Faculty of Science
Degree
Master of Science
Semester
Semester 1
Subject
Chemistry
Branch
Physical Chemistry

About this note

The fugacity of a real gas can also be determined with the help of the virial equation of state. This method is particularly useful at low and moderate pressures, where the virial equation gives a satisfactory representation of the behaviour of real gases.

For one mole of a gas, the virial equation may be written in terms of pressure as

$$
Z=1+B’P+C’P^2+D’P^3+\cdots
$$

where \(B’\), \(C’\), \(D’\), etc. are the pressure-form virial coefficients and may depend upon temperature.

The fugacity coefficient of a real gas is related to the compressibility factor by

$$
\ln\phi=\int_0^P\frac{Z-1}{P}\,dP
$$

For the virial equation,

$$
Z-1=B’P+C’P^2+D’P^3+\cdots
$$

Therefore,

$$
\frac{Z-1}{P}
=
B’+C’P+D’P^2+\cdots
$$

Substitution in the fugacity expression gives

$$
\ln\phi
=
\int_0^P
\left(B’+C’P+D’P^2+\cdots\right)dP
$$

At constant temperature, the virial coefficients are constants with respect to pressure. Hence, integration gives

$$
\ln\phi
=
B’P+\frac{C’P^2}{2}
+\frac{D’P^3}{3}+\cdots
$$

Thus,

$$
\boxed{
\ln\phi
=
B’P+\frac{C’P^2}{2}
+\frac{D’P^3}{3}+\cdots
}
$$

Since the fugacity coefficient is defined by

$$
\phi=\frac{f}{P},
$$

we have

$$
\ln\left(\frac{f}{P}\right)
=
B’P+\frac{C’P^2}{2}
+\frac{D’P^3}{3}+\cdots
$$

Taking the exponential of both sides,

$$
\boxed{
f
=
P\exp\left(
B’P+\frac{C’P^2}{2}
+\frac{D’P^3}{3}+\cdots
\right)
}
$$

At Low Pressure

At sufficiently low pressure, the higher-order terms become very small and may be neglected. The virial equation can then be approximated by

$$
Z=1+B’P
$$

Thus,

$$
Z-1=B’P
$$

and therefore

$$
\frac{Z-1}{P}=B’.
$$

The fugacity coefficient then becomes

$$
\ln\phi=\int_0^P B’\,dP
$$

giving

$$
\boxed{\ln\phi=B’P}
$$

or

$$
\boxed{\phi=e^{B’P}}
$$

Since \(f=\phi P\),

$$
\boxed{f=Pe^{B’P}}
$$

For very low pressures, \(B’P\) is small. Using the approximation \(e^x\approx1+x\) for small \(x\),

$$
f\approx P(1+B’P)
$$

Thus, at sufficiently low pressure, \(f\) approaches \(P\), as expected for a gas approaching ideal behaviour.

Relation with the Virial Coefficient in Volume Form

The virial equation is also commonly expressed in terms of molar volume as

$$
Z=1+\frac{B}{V}+\frac{C}{V^2}+\cdots
$$

where \(B\), \(C\), etc. are the virial coefficients in the volume form.

At low pressure, the pressure-form and volume-form coefficients are related approximately by

$$
B’= \frac{B}{RT}.
$$

Therefore, when only the second virial coefficient is significant,

$$
\boxed{
\ln\phi=\frac{BP}{RT}
}
$$

and hence

$$
\boxed{
f=P\exp\left(\frac{BP}{RT}\right)
}
$$

The sign of the second virial coefficient determines the direction of deviation from ideal behaviour. A negative \(B\) generally indicates predominance of attractive interactions and gives \(fP\).

Related Notes

More notes from the same unit.

View All
Unit-1 Thermodynamics

Microscopic Reversibility

Microscopic reversibility is concerned with the behaviour of matter at the molecular level. To understand this concept clearly,…

September 14, 2026 Written guide
Open details
↓Download PDF