Microscopic Reversibility
Microscopic reversibility is concerned with the behaviour of matter at the molecular level. To understand this concept clearly,…
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 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.
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 \(f
P\).
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