van der Waals equation

File:VdWaalsLeiden2020.jpg

One explicit way to write the van der Waals equation is:{{sfn|ps=|Epstein|1937|p=9}}{{sfn|ps=|Boltzmann|1995|p=231}}

{{NumBlk||$$p=\backslash frac\{RT\}\{v-b\}-\backslash frac\{a\}\{v^2\},$$|{{EquationRef|1a}}}}

where $p$ is pressure, $T$ is temperature, and $v=V/n=N\_\backslash text\{A\}V/N$ is molar volume, the ratio of volume, $V$, to quantity of matter, $n$ ($N\_\backslash text\{A\}$ is the Avogadro constant and $N$ the number of molecules). Also $a$ and $b$ are experimentally determinable, substance-specific constants, and $R=kN\_\backslash text\{A\}$ is the universal gas constant. This form is useful for plotting isotherms (constant temperature curves).

Van der Waals wrote it in an equivalent, explicit in temperature, form in his Thesis{{sfn|ps=|van der Waals|1873|p=56}}{{sfn|ps=|Sommerfeld|1956|p=55}} (although he could not denote absolute temperature by its modern form in 1873)

{{NumBlk||$$\backslash left(p+\backslash frac\{a\}\{v^2\}\backslash right)(v-b)\; =\; RT.$$|{{EquationRef|1b}}}}

This form is useful for plotting isobars (constant pressure curves). Writing $v=V/n$, and multiplying both sides by $n$ it becomes the form that appears in Figure A.{{sfn|ps=|Goodstein|1985|p=446}}

When van der Waals created his equation, few scientists believed that fluids were composed of rapidly moving particles. Moreover, those who thought so did not know the atomic/molecular structure. The simplest conception of a particle, and the easiest to model mathematically, was a hard sphere of volume $V\_0$; this is what van der Waals used, and he found the total excluded volume was {{tmath|1= B=4NV_0 }}, namely 4 times the volume of all the particles.{{sfn|ps=|van der Waals|2004|pp=168-172}}{{sfn|ps=|Boltzmann|1995|p=221–224}}

The constant {{tmath|1= b = B N_\text{A} /N }}, has the dimension of molar volume, [v]. The constant $a$ expresses the strength of the hypothesized inter-particle attraction. Van der Waals only had Newton's law of gravitation, in which two particles are attracted in proportion to the product of their masses, as a model. Thus he argued that, in his case, the attractive pressure was proportional to the density squared.{{sfn|ps=|van der Waals|2004|p=173}} The proportionality constant, {{mvar|a}}, when written in the form used above, has the dimension [pv²] (pressure times molar volume squared).

file:pair potentials.png (black) represents the induced-dipole–induced-dipole interaction of two non-polar molecules. Both are simple realistic molecular models.{{sfn|ps=|Hirschfelder|Curtis|Bird|1964|pp=31-34}}]]

The force magnitude between two spherically symmetric molecules is written as $F=-d\backslash varphi/dr$, where $\backslash varphi(r)$ is the pair potential function, and the force direction is along the line connecting the two mass centers. The specific functional relation is most simply characterized by a single length, {{tmath|1= \sigma }}, and a minimum energy, $-\backslash varepsilon$ (with {{tmath|1= \varepsilon\ge 0 }}). Two of the many such functions that have been suggested are shown in Fig. B.{{sfn|ps=|Hirschfelder|Curtis|Bird|1964|pp=31-34}}

A modern theory based on statistical mechanics produces the same result for $b=4N\_\backslash text\{A\}[(4\backslash pi/3)(\backslash sigma/2)^3]$ obtained by van der Waals and his contemporaries. It also produces a constant value for $a/N\_\backslash text\{A\}\backslash varepsilon\; b$ when $\backslash varepsilon/kT$ is small enough.{{sfn|ps=|Goodstein|1985|pp=250,263}}{{sfn|ps=|Tien|Lienhard|1979|pp=250,251}}

Once the constants $a$ and $b$ are known for a given substance, the van der Waals equation can be used to predict attributes like the boiling point at any given pressure, and the critical point.{{sfn|ps=|Boltzmann|1995|pp=231-234, 236-240}} These predictions are accurate for only a few substances. Most simple fluids are only a valuable approximation.{{sfn|ps=|Dong and Lienhard|1986|pp=158-159}}{{sfn|ps=|Lienhard|1986|pp=172-173}}

The ideal gas law follows from the van der Waals equation whenever the molar volume $v$ is sufficiently large (when {{tmath|1= v\gg b }}, so {{tmath|1= v-b\approx v }}), or equivalently whenever the molar density, {{tmath|1= \rho=1/v }}, is sufficiently small (when {{tmath|1= v\gg (a/p)^{1/2} }}, so {{tmath|1= p+a/v^2\approx p }}).{{sfn|ps=|Epstein|1937|p=10}}

When $v$ is large enough that both inequalities are satisfied, these two approximations reduce the van der Waals equation to {{tmath|1= p=RT/v }}, or $pv=RT$. With $R=N\_\backslash text\{A\}k$, where $k$ is the Boltzmann constant, and using the definition $v=V/n$ given after Eq (1a), this becomes {{tmath|1= pV=NkT }}; either of these forms expresses the ideal gas law.{{sf|ps=|Epstein|1937|p=10}} This is unsurprising since the van der Waals equation was constructed from the ideal gas equation to obtain an equation valid beyond the low-density limit of ideal gas behavior.

What is truly remarkable is the extent to which van der Waals succeeded. Indeed, Epstein in his classic thermodynamics textbook began his discussion of the van der Waals equation by writing, "Despite its simplicity, it comprehends both the gaseous and the liquid state and brings out, in a most remarkable way, all the phenomena pertaining to the continuity of these two states".{{sfn|ps=|Epstein|1937|p=10}} Also, in Volume 5 of his Lectures on Theoretical Physics, Sommerfeld, in addition to noting that "BoltzmannBoltzmann, L. Enzykl. der Mathem. Wiss., V, (1), 550 described van der Waals as the Newton of real gases",{{sfn|ps=|Sommerfeld|1956|p=55}} also wrote "It is very remarkable that the theory due to van der Waals is in a position to predict, at least qualitatively, the unstable [referring to superheated liquid, and subcooled vapor, now called metastable] states" that are associated with the phase change process.{{sfn|ps=|Sommerfeld|1956|p=66}}

The first to propose a volume correction to Boyle's law was Daniel Bernoulli in his microscopic theory in Hydrodynamica, however this model was mostly ignored in 1738.{{sfn|Grattan-Guinness|2005}}

In 1857 Rudolf Clausius published The Nature of the Motion which We Call Heat. In it he derived the relation $p=(N/V)m\backslash overline\{c^2\}/3$ for the pressure $p$ in a gas, composed of particles in motion, with number density {{tmath|1= N/V }}, mass {{tmath|1= m }}, and mean square speed {{tmath|1=\overline{c^2} }}. He then noted that using the classical laws of Boyle and Charles, one could write $m\backslash overline\{c^2\}/3=kT$ with a constant of proportionality {{tmath|1= k }}. Hence temperature was proportional to the average kinetic energy of the particles.{{sfn|ps=|Weinberg|2021|pp=4–5}} This article inspired further work based on the twin ideas that substances are composed of indivisible particles, and that heat is a consequence of the particle motion; movement that evolves according to Newton's laws. The work, known as the kinetic theory of gases, was done principally by Clausius, James Clerk Maxwell, and Ludwig Boltzmann. At about the same time, Josiah Willard Gibbs advanced the work by converting it into statistical mechanics.{{sfn|ps=|Weinberg|2021|p=33}}{{sfn|ps=|Gibbs|1948|pp=vii–xii}}

This environment influenced Johannes Diderik van der Waals. After initially pursuing a teaching credential, he was accepted for doctoral studies at the University of Leiden under Pieter Rijke.{{sfn|ps=|Brush|1973|pp=262-263}} This led, in 1873, to a dissertation that provided a simple, particle-based equation that described the gas-liquid change of state, the origin of a critical temperature, and the concept of corresponding states.{{sfn|ps=|van der Waals|1873}}{{sfn|ps=|van der Waals|2004|pp=121–240}} The equation is based on two premises: first, that fluids are composed of particles with non-zero volumes, and second, that at a large enough distance each particle exerts an attractive force on all other particles in its vicinity. Boltzmann called these forces van der Waals cohesive forces.{{sfn|ps=|Boltzmann|1995|p=218}}

In 1869 Irish professor of chemistry Thomas Andrews at Queen's University Belfast, in a paper entitled On the Continuity of the Gaseous and Liquid States of Matter,{{sfn|ps=|Andrews|1869}} displayed an experimentally obtained set of isotherms of carbonic acid, {{Chem2|H2CO3}}, that showed at low temperatures a jump in density at a certain pressure, while at higher temperatures there was no abrupt change (the figure can be seen here). Andrews called the isotherm at which the jump disappears the critical point. Given the similarity of the titles of this paper and van der Waals' subsequent thesis, one might think that van der Waals set out to develop a theoretical explanation of Andrews' experiments; however, this is not what happened. Van der Waals began work by trying to determine a molecular attraction that appeared in Laplace's theory of capillarity, and only after establishing his equation he tested it using Andrews' results.{{sfn|ps=|Klein|1974|p=31}}{{sfn|ps=|van der Waals|2004|pp=125,191–194}}

By 1877 sprays of both liquid oxygen and liquid nitrogen had been produced, and a new field of research, low-temperature physics, had been opened. The van der Waals equation played a part in all this, especially for the liquefaction of hydrogen and helium which was finally achieved in 1908.{{sfn|ps=|Goodstein|1985|pp=450–451}} From measurements of $p\_1,\; T\_1$ and $p\_2,\; T\_2$ in two states with the same density, the van der Waals equation produces the values{{sfn|ps=|Boltzmann|1995|pp=232–233}}

$$b\; =\; v\; -\; \backslash frac\{R\; \backslash left(T\_2\; -\; T\_1\backslash right)\}\{p\_2\; -\; p\_1\}\; \backslash qquad\; \backslash text\{and\}\; \backslash qquad\; a\; =\; v^2\; \backslash frac\{p\_2\; T\_1\; -\; p\_1\; T\_2\}\{T\_2\; -\; T\_1\}.$$

Thus from two such measurements of pressure and temperature, one could determine $a$ and $b$, and from these values calculate the expected critical pressure, temperature, and molar volume. Goodstein summarized this contribution of the van der Waals equation as follows:{{sfn|ps=|Goodstein|1985|p=452}}

All this labor required considerable faith in the belief that gas–liquid systems were all basically the same, even if no one had ever seen the liquid phase. This faith arose out of the repeated success of the van der Waals theory, which is essentially a universal equation of state, independent of the details of any particular substance once it has been properly scaled. [...] As a result, not only was it possible to believe that hydrogen could be liquefied, but it was even possible to predict the necessary temperature and pressure.

The van der Waals equation has been, and remains, useful because:{{sfn|ps=|Sommerfeld|1956|pp=55–68}}

• Its coefficient of thermal expansion has a simple analytic expression
• It explains the existence of the critical point, and establishes the theorem of corresponding states
• Its internal energy and entropy have simple analytic expressions
• Its specific heat at constant volume $c\_v$ is a function of $T$ only
• Its specific heat at constant pressure, $c\_p$ has a simple relationship with $c\_v$
• Its Joule–Thomson coefficient and associated inversion curve, which are instrumental in the commercial liquefaction of gases, have simple analytic expressions
• Together with the Maxwell construction it explains the existence of the liquid–vapor phase transition, including the observed metastable states

In addition{{sfn|ps=|Johnston|2014|pp=5,7, 12,18,25}}

• Its enthalpy and free energies all have simple analytic expressions
• Its isothermal compressibility has a simple analytic expression
• Its saturation curve has a simple analytic parametric solution
• It is an intermediate mathematical model that is useful as a pedagogical tool when teaching physics, chemistry, and engineering

and

• It plays an important role in the modern theory of phase transitions{{sfn|ps=|Goodstein|1985|pp=443–452}}
• It is the completely accurate equation of state for substances whose intermolecular potential matches the Sutherland potential{{sfn|ps=|Dong|Lienhard|1986|pp=158-159}}

File:vdW isotherms+2log.png of the van der Waals equation along with the spinodal curve (black dash-dot curve) and the coexistence (saturation) curve (red dash-dot curve), plotted using reduced (dimensionless) variables. The critical point lies at the inflection point on the orange isotherm.]]

Figure 1 shows four isotherms of the van der Waals equation (abbreviated as vdW) on a $p,\; v$ (pressure, molar volume) plane. The essential character of these curves is that they come in three forms:

1. At some critical temperature $T\_\backslash text\{c\}$ (orange isotherm), the slope is negative everywhere except at a single inflection point: the critical point {{tmath|1= ( p_\text{c}, v_\text{c} ) }}, where both the slope and curvature are zero, {{tmath|1= \left.\frac{\partial p}{\partial v}\right \vert_{T} = \left. \frac{\partial^2p}{\partial v^2}\right \vert_{T}=0 }}.
2. At higher temperatures (red isotherm), the isotherm's slope is negative everywhere. (This corresponds to values of $p,\; T$ for which the vdW equation has one real root for {{tmath|1= v }}).
3. At lower temperatures (green and blue isotherms), all isotherms have two points with zero slope. (This corresponds to values of {{tmath|1= p }}, $T$ for which the vdW equation has three real roots for {{tmath|1= v }}).

The critical point can be analytically determined by equating the two partial derivatives of the vdW equation, created by differentiating Eq (1a), to zero. This produces the critical values $v\_\backslash text\{c\}=3b$ and {{tmath|1= T_\text{c}=8a/(27Rb) }}. Finally, using these values in Eq (1a) gives {{tmath|1= p_\text{c}=a/27b^2 }}.{{sfn|ps=|Sommerfeld|1956|pp=56–57}} These results can also be obtained algebraically by noting that at the critical point the three roots are equal. Hence, Eqs (1) can be written as either $v^3-(b+RT\_\backslash text\{c\}/p\_\backslash text\{c\})v^2+(a/p\_\backslash text\{c\})v-ab/p\_\backslash text\{c\}=0$, or $(v-v\_\backslash text\{c\})^3=0$; two forms with the same coefficients.{{sfn|ps=|Goodstein|1985|p=449}}{{sfn|ps=|Boltzmann|1995|pp=237-238}}

Above the critical temperature $T\_\backslash text\{c\}$, van der Waals isotherms satisfy the stability criterion that . Below the critical temperature, each isotherm contains an interval where this condition is violated. This unstable region is the genesis of the phase change; there is a range $v\_\{\backslash rm\; min\}\backslash le\; v\backslash le\; v\_\{\backslash rm\; max\}$, for which no observable states exist. The states for spinodal points.{{sfn|ps=|Lienhard|Shamsundar|Biney|1986|pp=297-298}} Their locus is the spinodal curve, a boundary that separates the regions of the plane for which liquid, vapor, and gas exist from a region where no observable homogeneous states exist. This spinodal curve is obtained here from the vdW equation by differentiation (or equivalently from $\backslash kappa\_T=\backslash infty$) as

$$T\_\{\backslash rm\; sp\}=2a\backslash frac\{(v-b)^2\}\{Rv^3\}\backslash qquad\; p\_\{\backslash rm\; sp\}=\; \backslash frac\{a(v-2b)\}\{v^3\}$$

A projection of the spinodal curve is plotted in Figure 1 as the black dash-dot curve. It passes through the critical point, which is also a spinodal point.

Using the critical values to define reduced (dimensionless) variables {{tmath|1= p_r=p/p_\text{c} }}, {{tmath|1= T_r=T/T_\text{c} }}, and $v\_r=v/v\_\backslash text\{c\}$ renders the vdW equation in the dimensionless form (used to construct Fig. 1):

$$p\_r=\backslash frac\{8T\_r\}\{3v\_r-1\}-\backslash frac\{3\}\{v\_r^2\}$$

This dimensionless form is a similarity relation; it indicates that all vdW fluids at the same $T\_r$ will plot on the same curve. It expresses the law of corresponding states which Boltzmann described as follows:{{sfn|ps=|Boltzmann|1995|pp=239–240}}

All the constants characterizing the gas have dropped out of this equation. If one bases measurements on the van der Waals units [Boltzmann's name for the reduced quantities here], then he obtains the same equation of state for all gases. [...] Only the values of the critical volume, pressure, and temperature depend on the nature of the particular substance; the numbers that express the actual volume, pressure, and temperature as multiples of the critical values satisfy the same equation for all substances. In other words, the same equation relates the reduced volume, reduced pressure, and reduced temperature for all substances.

Obviously such a broad general relation is unlikely to be correct; nevertheless, the fact that one can obtain from it an essentially correct description of actual phenomena is very remarkable.

This "law" is just a special case of dimensional analysis in which an equation containing 6 dimensional quantities, {{tmath|1= p, v, T, a, b, R }}, and 3 independent dimensions, [p], [v], [T], must be expressible in terms of 6 − 3 = 3 dimensionless groups.{{sfn|ps=|Barenblatt|1979|pp=13–23}} Here $v^*=b$ is a characteristic molar volume, $p^*=a/b^2$ a characteristic pressure, and $T^*\; =\; a/(Rb)$ a characteristic temperature, and the 3 dimensionless groups are {{tmath|1= p/p^*, v/v^*,T/T^* }}. According to dimensional analysis the equation must then have the form {{tmath|1= p/p^*=\Phi(v/v^*,T/T^*) }}, a general similarity relation. In his discussion of the vdW equation, Sommerfeld also mentioned this point.{{sfn|ps=|Sommerfeld|1956|p=57}} The reduced properties defined previously are {{tmath|1= p_r=27(p/p^*) }}, {{tmath|1= v_r=(1/3)(v/v^*) }}, and {{tmath|1= T_r=(27/8)(T/T^*) }}. Recent research has suggested that there is a family of equations of state that depend on an additional dimensionless group, and this provides a more exact correlation of properties.{{sfn|ps=|Peck|1982| p=446}} Nevertheless, as Boltzmann observed, the van der Waals equation provides an essentially correct description.

The vdW equation produces the critical compressibility factor {{tmath|1= Z_\text{c}=p_\text{c}v_\text{c}/(RT_\text{c})=3/8=0.375 }}, while for most real fluids {{tmath|1= 0.23acentric) factor, {{tmath|1= \omega }}, and the liquid metals (mercury and cesium) are well approximated by it.{{sfn|ps=|Lienhard|1986|pp=172-173}}{{sfn|ps=|Dong|Lienhard|1986|pp=158-159}}

The properties molar internal energy, $u$, and entropy, $s$, are defined by the first and second laws of thermodynamics. From these laws, they, and all other thermodynamic properties of a simple compressible substance, can be specified, up to a constant of integration, by two measurable functions. These are a mechanical equation of state, $p=p(v,T)$, and a constant volume specific heat, $c\_v(v,T)$.{{sfn|ps=|Whitman|2023|pp=155, 202-204}}{{sfn|ps=|Moran and Shapiro|2000|pp=574}}

When $u(v,T)$ represents a continuous surface, it must be a continuous function with continuous partial derivatives, and its second mixed partial derivatives must be equal, $\backslash partial\_\{v\}\backslash partial\_Tu=\backslash partial\_T\backslash partial\_v\; u$. Then with $c\_v=\backslash partial\_Tu$ this condition can be written simply as $\backslash partial\_vc(v,T)=\; \backslash partial\_T[T^2\backslash partial\_T(p/T)]$. Differentiating $p/T$ for the vdW equation gives $T^2\backslash partial\_T(p/T)]=a/v^2$, so $\backslash partial\_vc\_v=0$. Consequently $c\_v=c\_v(T)$ for a vdW fluid exactly as it is for an ideal gas.{{sfn|ps=|Sommerfeld|pp=58-59}} To keep things simple, it is regarded as a constant in the following, $c\_v=cR$, with $c$ a number.

The energetic equation of state gives the internal energy, and the entropic equation of state gives the entropy as{{sfn|ps=|Whitman|2023|pp=155,204}}{{sfn|ps=|Moran and Shapiro|2000|pp=574}}

$$\backslash begin\{align\}$$

u - C_u &= \int c_v(v,T) \, dT + \int T^2 \, \frac{\partial (p/T)}{\partial T} \, dv \\

s - C_s &= \int c_v(T) \, \frac{dT}{T} + \int \frac{\partial p}{\partial T} \, dv

\end{align}

where $C\_u,\; C\_s$ are arbitrary constants of integration.

Both integrals for $u$ can be easily evaluated and the result is, {{sfn|ps=|Johnston|2014|p=7}}{{sfn|ps=|Whitman|2023|p=192}}

{{NumBlk||$$u-C\_u=cRT-a/v$$|{{EquationRef|2}}}}

Likewise both integrals for $s$ can be evaluated with the result,{{sfn|ps=|Johnston|2014|p=6}}{{sfn|ps=|Whitman|2023|p=257}}

{{NumBlk||$$s-C\_s=R\backslash ln[T^c(v-b)]$$|{{EquationRef|3}}}}

The Helmholtz free energy is $f=u-Ts$. Subtracting $T$ times Eq (3) from Eq (2) gives $f$ as{{sfn|sp=|Johnston|2014|p=5}}

{{NumBlk||$$f\; =\; C\_u\; +\; c\; T\; -\; a\; /\; v\; -\; T\; \backslash \{C\_s\; +\; R\; \backslash ln[T^c\; (v\; -\; b)]\backslash \}$$| {{EquationRef|4a}}}}

The enthalpy is $h=u+pv$, and the product $pv$ is, using Eq (1a), $pv=RTv/(v-b)-a/v$. Adding Eq (2) gives $h$ as {{sfn|ps=|Johnston|2014|p=7}}{{sfn|ps=|Whitman|2023|p=192}}

$$h-C\_u=RT[c+v/(v-b)]-2a/v$$

The Gibbs free energy is $g=h-Ts$ so subtracting $T$ times Eq (3) from $h$ produces $g$ as{{sfn|ps=|Johnston|2014|p=12}}

{{NumBlk||$$g-C\_u\; =\; \backslash left(c+\{v\; \backslash over\; v-b\}-C\_\backslash text\{s\}-\backslash ln[T^c(v-b)]\backslash right)RT-\{2a\; \backslash over\; v\}$$|{{EquationRef|4b}}}}

All these results can be rendered in reduced form by using the characteristic energy $RT\_\backslash text\{c\}$.

Any derivative of any thermodynamic property can be expressed in terms of any three of them.{{sfn|ps=|Callen|1962|pp=117-130}} A standard set is composed of $\backslash alpha,\; \backslash kappa\_T,\; c\_v$. For a vdW fluid $c\_v(T)$ is a known function, and the other two are obtained from the first partial derivatives of the vdW equation as,

$$\backslash left(\backslash frac\{\backslash partial\; p\}\{\backslash partial\; T\}\backslash right)\_v\; =\; \backslash frac\{R\}\{v-b\}\; =\; \backslash frac\{\backslash alpha\}\{\backslash kappa\_T\}$$

\quad\text{and}\quad

\left(\frac{\partial p}{\partial v}\right)_T = -\frac{RT}{(v-b)^2} + \frac{2a}{v^3} = -\frac{1}{v\kappa_T}

Here $\backslash kappa\_T=-v^\{-1\}\backslash partial\_pv$, is the isothermal compressibility, and $\backslash alpha=v^\{-1\}\backslash partial\_Tv\_p$, is the coefficient of thermal expansion.{{sfn|ps=|Moran and Shapiro|2000|p=578}}{{sfn|ps=|Whitman|2014|pp=43-45, 98}} Therefore,{{sfn|ps=|Sommerfeld|1956|p=56}}{{sfn|ps=|Johnston|2014| p=11}}

{{NumBlk||$$\backslash kappa\_T=\backslash frac\{v^2(v-b)^2\}\{RTv^3-2a(v-b)^2\}\backslash quad\backslash text\{and\}\; \backslash quad\backslash alpha=\backslash frac\{Rv^2(v-b)\}\{RTv^3-2a(v-b)^2\}.$$|{{EquationRef|5}}}}

In the limit $v\backslash to\backslash infty$, $\backslash alpha=\; 1/T$ and $\backslash kappa\_T=\; v/(RT)$.{{sfn|ps=|Johnston|2014|p=11}}{{sfn|ps=|Moran and Shapiro|2000|p=580}} Since the vdW equation in this limit becomes $p=\; RT/v$, finally $\backslash kappa\_T=\; 1/p$. Both of these are the ideal gas values.

The specific heat at constant pressure, $c\_p$ is defined as the partial derivative $c\_p=\backslash partial\_Th|\_p$. It is related to $c\_v$ by the Mayer equation, $c\_p-c\_v=-T(\backslash partial\_Tp)^2/\backslash partial\_vp=Tv\backslash alpha^2/\backslash kappa\_T$.{{sfn|ps=|Whitman|2023|p= 204}}{{sfn|ps=|Johnston|2014|p=3}} Then the two partials of the vdW equation can be used to express $c\_p$ as,{{sfn|ps=|Johnston|2014|p=12}}

{{NumBlk|:|$$c\_p(v,T)-c\_v(T)=\backslash frac\{R^2Tv^3\}\{RTv^3-2a(v-b)^2\}\backslash ge\; R$$|{{EquationRef|6}}}}

Here in the limit $v\backslash to\backslash infty$, $c\_p-c\_v=\; R$, which is also the ideal gas result;{{sfn|ps=|Johnston|2014|p=12}} however the limit $v\backslash rightarrow\; b$ gives the same result, which does not agree with experiments on liquids.{{sfn|ps=|Moran and Shapiro|2000|p=580}}

Finally $c\_p,\; \backslash alpha$, and $\backslash kappa\_T$ are all infinite on the curve $T=2a(v-b)^2/(Rv^3)=T\_\backslash text\{c\}(3v\_r-1)^2/(4v\_r^3)$.{{sfn|ps=|Johnston|2014|p=12}} This is the spinodal curve defined by $\backslash kappa\_T^\{-1\}=0$,{{sfn|ps=|Lienhard, Shamsundahr and Biney|1986|p=299}} that was discussed in the subsection The course of the isotherms.

Although the gap in $v$ delimited by the two spinodal points on an isotherm (e.g. $T\_\backslash text\{r\}=7/8$ in Fig. 1) is the origin of the phase change, the change occurs at some intermediate value of pressure. This can be understood by considering that the saturated liquid and vapor states can coexist in equilibrium, with the same pressure and temperature.{{sfn|ps=|Callen|1960|pp=37–44}} However, the minimum and maximum spinodal points are not at the same pressure. Therefore, at a temperature $T\_\backslash text\{s\}$, the phase change is characterized by the pressure $p\_\backslash text\{s\}$, which lies within the range of $p$ set by the spinodal points (

Applying Eq (1a) to the saturated liquid and saturated vapor states gives:

{{NumBlk||$$p\_\backslash text\{s\}=\backslash frac\{RT\_\backslash text\{s\}\}\{v\_\backslash text\{f\}-b\}-\backslash frac\{a\}\{\{v\_\backslash text\{f\}\}^2\}\backslash quad\backslash text\{and\}\backslash quad\; p\_\backslash text\{s\}=\backslash frac\{RT\_\backslash text\{s\}\}\{v\_\backslash text\{g\}-b\}-\backslash frac\{a\}\{\{v\_\backslash text\{g\}\}^2\}.$$

|{{EquationRef|7}}}}

Equations (7) contain four variables $p\_\backslash text\{s\},\; T\_\backslash text\{s\},\; v\_\backslash text\{f\},\; v\_\backslash text\{g\}$), so a third equation is required to uniquely specify three of these variables in terms of the fourth. In this case of a single substance, the equation is provided by the condition of equal Gibbs free energy,{{sfn|ps=|Callen|1960|pp=37–44}}

$$g\_\backslash text\{g\}\; =\; g\_\backslash text\{f\}$$

Using Eq (4b) applied to each state in this equation produces

{{NumBlk||$$RT\_\backslash text\{s\}\backslash left[\backslash frac\{v\_\backslash text\{g\}\}\{v\_\backslash text\{g\}-b\}-\backslash frac\{v\_\backslash text\{f\}\}\{v\_\backslash text\{f\}-b\}-\backslash ln\backslash left(\backslash frac\{v\_\backslash text\{g\}-b\}\{v\_\backslash text\{f\}-b\}\backslash right)\backslash right]\; -2a\backslash left(\backslash frac\{1\}\{v\_\backslash text\{g\}\}-\backslash frac\{1\}\{v\_\backslash text\{f\}\}\backslash right)=0$$|{{EquationRef|8}}}}

This is a third equation that, along with {{EquationNote|7|Eqs. 7}} can be solved numerically. This has been done given a value for either $T\_\backslash text\{s\}$ or $p\_\backslash text\{s\}$, and tabular results presented;{{sfn|ps=|Shamsundar|Lienhard|1983|pp=878,879}}{{sfn|ps=|Barrufet|Eubank|1989|p=170}} however, the equations also admit an analytic parametric solution obtained by Lekner.{{sfn|ps=|Lekner|1982|pp=161-162}} Details of this solution may be found in the Maxwell construction, and the dimensionless results are:

$$\backslash begin\{align\}$$

T_\text{rs}(y) &= \frac{27}{8} \cdot \frac{2f(y) \left[\cosh y + f(y)\right]}{g(y)^2}, &

p_\text{rs} &= 27\frac{f(y)^2 \left[1 - f(y)^2\right]}{g(y)^2}, \\[1ex]

v_\text{rf} &= \frac{1 + f(y) e^y}{3 f(y) e^y}, &

v_\text{rg} &= \frac{1 + f(y) e^{-y}}{3 f(y) e^{-y}}

\end{align}

where

$$\backslash begin\{align\}$$

f(y) &= \frac{y \cosh y - \sinh y}{\sinh y \cosh y - y}, &

g(y) &= 1 + 2f(y) \cosh y + f(y)^2

\end{align}

The parameter is given physically by $y=(s\_\backslash text\{g\}-s\_\backslash text\{f\})/(2R)$. This solution also produces values of all other property discontinuities across the saturation curve.{{sfn|ps=|Johnston|2014|pp=16-18}} These functions define the coexistence curve (or saturation curve), which is the locus of the saturated liquid and saturated vapor states of the vdW fluid. Projections of this saturation curve are plotted in Figures 1 and 2.

File:Vdw stability-saturation.png

Referring back to Figure 1, the isotherms for are discontinuous. For example, the $T\_\backslash text\{r\}=7/8$ (green) isotherm consists of two separate segments. The solid green lines are composed of stable states. They terminate at dots representing the saturated liquid and vapor states forming the phase change. The dashed green lines represent metastable states (superheated liquid and subcooled vapor). They are created in the phase transition, have a finite lifetime, and then devolve into their lower energy stable alternative.

At every point in the region between the two curves in Figure 2, there are two states: one stable and one metastable. The coexistence of these states can be seen in Figure 1—for discontinuous isotherms, there are values of $p\_\backslash text\{r\}$ which correspond to two points on the isotherm: one on a solid line (the stable state) and one on a dashed region (the metastable state).

In his treatise of 1898, in which he described the van der Waals equation in great detail, Boltzmann discussed these metastable states in a section titled "Undercooling, Delayed evaporation".{{sfn|ps=|Boltzmann|1995|pp=248–250}} (Today, these states are now denoted "subcooled vapor" and "superheated liquid".) Moreover, it has now become clear that these metastable states occur regularly in the phase transition process. In particular, processes that involve very high heat fluxes create large numbers of these states, and transition to their stable alternative with a corresponding release of energy that can be dangerous. Consequently, there is a pressing need to study their thermal properties.{{sfn|ps=|Lienhard|Shamsundar|Biney|1986|p=297}}

In the same section, Boltzmann also addressed and explained the negative pressures which some liquid metastable states exhibit (for example, the blue isotherm $T\_\backslash text\{r\}=4/5$ in Fig. 1). He concluded that such liquid states of tensile stresses were real, as did Tien and Lienhard many years later who wrote "The van der Waals equation predicts that at low temperatures liquids sustain enormous tension [...] In recent years measurements have been made that reveal this to be entirely correct."{{sfn|ps=|Tien|Lienhard|1979|p=254}}

Even though the phase change produces a mathematical discontinuity in the homogeneous fluid properties (for example $v$), there is no physical discontinuity.{{sfn|ps=|Callen|1960|pp=146–156}} As the liquid begins to vaporize, the fluid becomes a heterogeneous mixture of liquid and vapor whose molar volume varies continuously from $v\_\backslash text\{f\}$ to $v\_\backslash text\{g\}$ according to the equation of state $v=v\_\backslash text\{f\}+x(v\_\backslash text\{g\}-v\_\backslash text\{f\})$ where $x=N\_\backslash text\{g\}/(N\_\backslash text\{f\}+N\_\backslash text\{g\})$ and $0\backslash le\; x\backslash le\; 1$ is the mole fraction of the vapor. This equation is called the lever rule and applies to other properties as well.{{sfn|ps=|Sommerfeld|1956|p=66}}{{sfn|ps=|Callen|1960|pp=146–156}} The states it represents form a horizontal line bridging the discontinuous region of an isotherm (not shown in Fig. 1 because it is a different equation from the vdW equation).

File:vapor pressure vs temperature1.png

The idea of corresponding states originated when van der Waals cast his equation in the dimensionless form, $p\_\backslash text\{r\}=p(v\_\backslash text\{r\},T\_\backslash text\{r\})$. However, as Boltzmann noted, such a simple representation could not correctly describe all substances. Indeed, the saturation analysis of this form produces $p\_\backslash text\{rs\}=p\_\backslash text\{s\}(T\_\backslash text\{r\})$; namely, that all substances have the same dimensionless coexistence curve, which is not true.{{sfn|ps=|Rowlinson (ed) in van der Waals|2004|p=22}} To avoid this paradox, an extended principle of corresponding states has been suggested in which $p\_\backslash text\{r\}=p(v\_\backslash text\{r\},T\_\backslash text\{r\},\backslash phi)$ where $\backslash phi$ is a substance-dependent dimensionless parameter related to the only physical feature associated with an individual substance: its critical point.

File:Tr vs Pitzer factor.jpg

One candidate for $\backslash phi$ is the critical compressibility factor $Z\_\backslash text\{c\}=p\_\backslash text\{c\}v\_\backslash text\{c\}/(RT\_\backslash text\{c\})$; however, because $v\_\backslash text\{c\}$ is difficult to measure accurately, the acentric factor developed by Kenneth Pitzer,{{sfn|ps=|Pitzer|Lippman|Curl|Huggins|1955|p=3433}} $\backslash omega=-\backslash log\_\{10\}[p\_\backslash text\{r\}(T\_\backslash text\{r\}=0.7)]-1$, is more useful. The saturation pressure in this situation is represented by a one-parameter family of curves: $p\_\backslash text\{rs\}=p\_\backslash text\{s\}(T\_\backslash text\{r\},\backslash omega)$. Several investigators have produced correlations of saturation data for several substances; Dong and Lienhard give{{sfn|ps=|Dong|Lienhard|1986|pp=158-159}}

$$\backslash begin\{align\}$$

\ln p_\text{rs} = 5.37270 (1 - 1/T_\text{r}) + \omega

(& 7.49408 - 11.181777\ {T_\text{r}}^3 + \\

& 3.68769 \ {T_\text{r}}^6+17.92998\,\ln T_\text{r})

\end{align}

which has an RMS error of $\backslash pm\; 0.42$ over the range $1\backslash le\; T\_\backslash text\{r\}\backslash le0.3$.

Figure 3 is a plot of $p\_\backslash text\{rs\}$ vs. $T\_\backslash text\{r\}$ for various values of the Pitzer factor $\backslash omega$ as given by this equation. The vertical axis is logarithmic to show the behavior at pressures closer to zero, where differences among the various substances (indicated by varying values of $\backslash omega$) are more pronounced.

Figure 4 is another plot of the same equation showing $T\_\backslash text\{r\}$ as a function of $\backslash omega$ for various values of $p\_\backslash text\{rs\}$. It includes data from 51 substances, including the vdW fluid, over the range . This plot shows that the vdW fluid ($\backslash omega=-0.302$) is a member of the class of real fluids; indeed, the vdW fluid can quantitatively approximate the behavior of the liquid metals cesium ($\backslash omega=-0.267$) and mercury ($\backslash omega=-0.21$), which share similar values of $\backslash omega$. However, in general it can describe the behavior of fluids of various $\backslash omega$ only qualitatively.

The Joule–Thomson coefficient, $\backslash mu\_\backslash text\{JT\}=\backslash partial\_pT|\_h$, is of practical importance because the two end states of a throttling process ($h\_2=h\_1$) lie on a constant enthalpy curve. Although ideal gases, for which $h=h(T)$, do not change temperature in such a process, real gases do, and it is important in applications to know whether they heat up or cool down.{{sfn|ps=|Sommerfeld|1956|pp=61–63}}

This coefficient can be found in terms of the previously derived $\backslash alpha$ and $c\_p$ as{{sfn|ps=|Sommerfeld|1956|pp=60-62}}

$$\backslash mu\_\backslash text\{JT\}=\backslash frac\{v(\backslash alpha\; T-1)\}\{c\_p\}.$$

When $\backslash mu\_\backslash text\{JT\}$ is positive, the gas temperature decreases as it passes through a throttling process, and when it is negative, the temperature increases. Therefore, the condition $\backslash mu\_\backslash text\{JT\}=0$ defines a curve that separates the region of the $T,p$ plane where $\backslash mu\_\backslash text\{JT\}>0$ from the region where . This curve is called the inversion curve, and its equation is $\backslash alpha\; T-1=0$. Evaluating this using the expression for $\backslash alpha$ derived in {{EquationNote|4|Eq. 5}} produces,{{sfn|ps=|Sommerfeld|1956|p=61}}

File:Vdw inversion2.png

$$2a(v-b)^2-RTv^2b=0$$

Note that for $v\backslash gg\; b$ there will be cooling for $2a>RTb$ (or, in terms of the critical temperature, ). As Sommerfeld noted, "This is the case with air and with most other gases. Air can be cooled at will by repeated expansion and can finally be liquified."{{sfn|ps=|Sommerfeld|1956|p=61}}

Solving for $b/v>0$, and using this to eliminate $v$ from Eq (1a) gives the inversion curve as

$$\backslash frac\{p\}\{p^*\}\; =\; -1\; +\; 4\; \backslash left(\backslash frac\{T\}\{2T^*\}\backslash right)^\{1/2\}\; -\; 3\; \backslash left(\backslash frac\{T\}\{2T^*\}\backslash right)$$

where, for simplicity, $a,b,R$ have been replaced by $p^*,T^*$.

A plot of the curve, in reduced variables, is shown in green in Figure 5. Sommerfeld also displays this plot,{{sfn|ps=|Sommerfeld|1956|p=62|loc=Fig.8}} together with a curve drawn using experimental data from H₂. The two curves agree qualitatively, but not quantitatively.

Figure 5 shows an overlap between the saturation curve and the inversion curve plotted in the same region. This crossover means a van der Waals gas can be liquified by passing it through a throttling process under the proper conditions; real gases are liquified in this way.

File:Vdw Z rho.png File:Vdw Z p_r 1.png

Real gases are characterized by their difference from ideal gases by writing $pv=ZRT$, where $Z$, called the compressibility factor. It is expressed either as $Z(p,T)$ or $Z(\backslash rho,T)$, because in either case (pressure, $p$, or density, $\backslash rho$) the limit as $p$ or $\backslash rho$ approaches zero is 1, and $Z$ takes the ideal gas value. In the second case $Z(\backslash rho,T)=p(\backslash rho,T)/\backslash rho\; RT$,{{sfn|ps=|Van Wylen|Sonntag|1973|p=49}} so for a van der Waals fluid from Eq (‘’’1’’’) the compressibility factor is

{{Numblk|:|$Z=\{1\; \backslash over\; 1-b\backslash rho\}-\{a\backslash rho\; \backslash over\; RT\}$|{{EquationRef|9}}}}

or in terms of reduced variables

$$Z=\backslash frac\{3\}\{3-\backslash rho\_r\}-\backslash frac\{9\backslash rho\_r\}\{8T\_r\}$$

where $0\backslash le\backslash rho\_r=1/v\_r\backslash le\; 3$. At the critical point, $T\_r=\backslash rho\_r=1$ and $Z=Z\_\backslash text\{c\}=3/2-9/8=3/8$.

In the limit $\backslash rho\backslash rightarrow\; 0$, $Z=1$; the fluid behaves like an ideal gas, as mentioned before. The derivative $\backslash left(\backslash frac\{\backslash partial\; Z\}\{\backslash partial\; \backslash rho\}\backslash right)\_T\; =\; b\backslash left(\; \{\backslash left(1\; -\; b\backslash rho\backslash right)\}^\{-2\}\; -\; \backslash frac\{a\}\{bRT\}\backslash right)$ is never negative when $\{a\; \backslash over\; bRT\}=T^*/T\backslash le\; 1$; that is, when $T/T^*\backslash ge\; 1$ (which corresponds to $T\_r\backslash ge27/8$). Alternatively, the initial slope is negative when , is zero at $b\backslash rho=1-(T/T^*)^\{1/2\}$, and is positive for larger $b\backslash rho\backslash le\; 1$ (see Fig. 6). In this case, the value of $Z$ passes through $1$ when $b\backslash rho\_B=1-T\_B/T^*$. Here $T\_B=(27T\_\backslash text\{c\}/8)(1-b\backslash rho\_B)$ is called the Boyle temperature. It ranges between $0\; \backslash le\; T\_B\; \backslash le\; 27T\_\backslash text\{c\}/8$, and denotes a point in $T,\backslash rho$ space where the equation of state reduces to the ideal gas law. However, the fluid does not behave like an ideal gas there, because neither its derivatives $(\backslash alpha,\; \backslash kappa\_T)$

nor $c\_p$

reduce to their ideal gas values, other than where $b\backslash rho\_B\backslash ll\; 1,\backslash ,T\_B\backslash sim\; 27T\_\backslash text\{c\}/8$ the actual ideal gas region.{{sfn|ps=|Johnston|2014|p=10}}

Figure 6 plots various isotherms of $Z(\backslash rho,T\_r)$ vs $\backslash rho\_r$. Also shown are the spinodal and coexistence curves described previously. The subcritical isotherm consists of stable, metastable, and unstable segments (identified in the same way as in Fig. 1). Also included are the zero initial slope isotherm and the one corresponding to infinite temperature.

Figure 7 shows a generalized compressibility chart for a vdW gas. Like all other vdW properties, this is not quantitatively correct for most gases, but it has the correct qualitative features.{{sfn|ps=|Su|1946|p=803}}{{sfn|ps=|Moran|Shapiro|2000|p=113}} Note the caustic generated by the crossing isotherms.

Kammerlingh Onnes first suggested the virial expansion as an empirical alternative to the vdW equation. Subsequently, it was proven to result from Statistical mechanics,{{sfn|ps=|Hirschfelder, Curtis, and Bird|1964|pp=137-145}}{{sfn|ps=|Hill|1986|pp=261-266}} in the form

$$Z(\backslash rho,T)=1+\backslash sum\_\{k=2\}^\backslash infty\backslash ,B\_k(T)(\backslash rho)^\{k-1\}$$ where $Z=p/(\backslash rho\; RT)$ and the functions $B\_k(T)$ are the virial coefficients. The $k$th term represents a $k$-particle interaction.

Expanding the term $(1-b\backslash rho)^\{-1\}$ in the definition of $Z$, Eq ({{EquationNote|9|9}}), into an infinite series, absolutely convergent for , produces

$$Z(\backslash rho,T)=1+\backslash left(1-\{a\; \backslash over\; bRT\}\backslash right)b\backslash rho+\backslash sum\_\{k=3\}^\backslash infty\; (b\backslash rho)^\{k-1\}.$$

The second virial coefficient is the slope of $Z(\backslash rho,T)$ at $\backslash rho=0$. It is positive when $T/T^*>1$ and negative when (), in agreement with the result found by differentiation. Its vdW value, $B\_2=b-a/RT$ agrees with a statistical mechanical calculation; however, the higher order coefficients are in error. This means that the vdW virial expansion, hence the vdW equation itself, is equivalent to a two term asymptotic approximation to the virial equation.{{sfn|ps=|Tien|Lienhard|1979|pp=250,251}}

{{sfn|ps=|Hirschfelder, Curtis, and Bird|1964|pp=156-157, 158-159}}

For molecules modeled as non-attracting hard spheres, $a=0$, and the vdW virial expansion becomes

$$Z(\backslash rho)=(1-b\backslash rho)^\{-1\}=1+\backslash sum\_\{k=2\}^\backslash infty\; (b\backslash rho)^\{k-1\},$$

which illustrates the effect of the excluded volume alone. It was recognized early on that this was in error beginning with the term $(b\backslash rho)^2$. Boltzmann calculated its correct value as $\backslash frac\{5\}\{8\}\; (b\backslash rho)^2$, and used the result to propose an enhanced version of the vdW equation:

$$\backslash left(p+\{a\; \backslash over\; v^2\}\backslash right)\backslash left(v-\{b\; \backslash over\; 3\}\backslash right)=RT\backslash left(1+\{2b\; \backslash over\; 3v\}+\{\{7b^2\}\; \backslash over\; \{24v^2\}\}\backslash right).$$

On expanding $(v-b/3)^\{-1\}$, this produced the correct coefficients through $(b/v)^2$ and also gave infinite pressure at $b/3$, which is approximately the close-packing distance for hard spheres.{{sfn|ps=|Boltzmann|1995|pp=353-356}} This was one of the first of many equations of state proposed over the years that attempted to make quantitative improvements to the remarkably accurate explanations of real gas behavior produced by the vdW equation.{{sfn|ps=|Rowlinson (ed) in van der Waals|2004|pp=20-22}}

In 1890 van der Waals published an article that initiated the study of fluid mixtures. It was subsequently included as Part III of a later published version of his thesis.{{sfn|ps=|van der Waals|2004|pp=243-282}} His essential idea was that in a binary mixture of vdW fluids described by the equations

p_1=\frac{RT}{v-b_{11}}-\frac{a_{11}}{v^2}\quad\text{and}\quad p_2=\frac{RT}{v-b_{22}}-\frac{a_{22}}{v^2}

the mixture is also a vdW fluid given by

$$p=\backslash frac\{RT\}\{v-b\_x\}-\backslash frac\{a\_x\}\{v^2\}$$

where

$$\backslash begin\{align\}$$

a_x &= a_{11} x_1^2 + 2a_{12} x_1 x_2 + a_{22} x_2^2, \\[2pt]

b_x &= b_{11} x_1^2 + 2b_{12} x_1 x_2 + b_{22} x_2^2.

\end{align}

Here $x\_1=N\_1/N$ and $x\_2=N\_2/N$, with $N=N\_1+N\_2$ (so that $x\_1+x\_2=1$), are the mole fractions of the two fluid substances. Adding the equations for the two fluids shows that $p\backslash ne\; p\_1+p\_2$, although for $v$ sufficiently large $p\backslash approx\; p\_1+p\_2$ with equality holding in the ideal gas limit. The quadratic forms for $a\_x$ and $b\_x$ are a consequence of the forces between molecules. This was first shown by Lorentz,{{sfn|ps=|Lorentz|1881|pp=127,134,600}} and was credited to him by van der Waals. The quantities $a\_\{11\},\backslash ,a\_\{22\}$ and $b\_\{11\},\backslash ,b\_\{22\}$ in these expressions characterize collisions between two molecules of the same fluid component, while $a\_\{12\}=a\_\{21\}$ and $b\_\{12\}=b\_\{21\}$ represent collisions between one molecule of each of the two different fluid components. This idea of van der Waals' was later called a one fluid model of mixture behavior.{{sfn|ps=|Rowlinson (ed) in van der Waals|2004|p=68}}

Assuming that $b\_\{12\}$ is the arithmetic mean of $b\_\{11\}$ and $b\_\{22\}$, $b\_\{12\}=(b\_\{11\}+b\_\{22\})/2$, substituting into the quadratic form and noting that $x\_1+x\_2=1$ produces

$$b=b\_\{11\}x\_1+b\_\{22\}x\_2$$

Van der Waals wrote this relation, but did not make use of it initially.{{sfn|ps=|van der Waals|2004|p=244}} However, it has been used frequently in subsequent studies, and its use is said to produce good agreement with experimental results at high pressure.{{sfn|ps=|Redlich|Kwong|1949}}

In this article, van der Waals used the Helmholtz potential minimum principle to establish stability conditions. This principle states that in a system in diathermal contact with a heat reservoir $T=T\_R$, $DF=0$, and $D^2F>0$, namely at equilibrium, the Helmholtz potential is a minimum.{{sfn|ps=|Callen|1986|p=105}} Since, like $g(p,T)$, the molar Helmholtz function $f(v,T)$ is also a potential function whose differential is

$$df\; =\; \backslash left(\backslash frac\{\backslash partial\; f\}\{\backslash partial\; v\}\backslash right)\_T\; dv+\; \backslash left(\backslash frac\{\backslash partial\; f\}\{\backslash partial\; T\}\backslash right)\_v\; dT\; =\; -p\; \backslash ,\; dv\; -\; s\; \backslash ,\; dT,$$

this minimum principle leads to the stability condition $\backslash partial^2f/\backslash partial\; v^2|\_T=-\backslash partial\; p/\backslash partial\; v|\_T>\; 0$. This condition means that the function, $f(v,T)$, is convex at all stable states of the system. Moreover, for those states the previous stability condition for the pressure is also necessarily satisfied.{{sfn|ps=|van der Waals|2004|pp=245-247}}

For a single substance, the definition of the molar Gibbs free energy can be written in the form $f=g-pv$. Thus when $p$ and $g$ are constant, the function $f(v)$ is a straight line with slope $-p$, and intercept $g$. Since the curve $f(T\_R,\; v)$ has positive curvature everywhere when $T\_R\backslash ge\; T\_\backslash text\{c\}$, the curve and the straight line will have a single tangent. However, for a subcritical $T\_R,\backslash ,\; f(T\_R,v)$ is not everywhere convex. With $p=p\_\backslash text\{s\}(T\_R)$ and a suitable value of $g$, the line will be tangent to $f(T\_R,v)$ at the molar volume of each coexisting phase: saturated liquid $v\_f(T\_R)$ and saturated vapor $v\_g(T\_R)$; there will be a double tangent. Furthermore, each of these points is characterized by the same values of $g$, $p$, and $T\_R.$ These are the same three specifications for coexistence that were used previously.{{sfn|ps=|van der Waals|2004|pp=245-247}}

file:Vdw helmholtz1.png

Figure 8 depicts an evaluation of $f(T\_R,v)$ as a green curve, with $v\_f$ and $v\_g$ marked by the left and right green circles, respectively. The region on the green curve for $v\backslash le\; v\_f$ corresponds to the liquid state. As $v$ increases past $v\_f$, the curvature of $f$ (proportional to $\backslash partial\_v\backslash partial\_vf=-\backslash partial\_vp$) continually decreases. The inflection point, characterized by zero curvature, is a spinodal point; between $v\_f$ and this point is the metastable superheated liquid. For further increases in $v$ the curvature decreases to a minimum then increases to another (zero curvature) spinodal point; between these two spinodal points is the unstable region in which the fluid cannot exist in a homogeneous equilibrium state (represented by the dotted grey curve). With a further increase in $v$ the curvature increases to a maximum at $v\_g$, where the slope is $p\_\backslash text\{s\}$; the region between this point and the second spinodal point is the metastable subcooled vapor. Finally, the region $v\backslash ge\; v\_g$ is the vapor. In this region the curvature continually decreases until it is zero at infinitely large $v$. The double tangent line (solid black) that runs between $v\_f$ and $v\_g$ represents states that are stable but heterogeneous, not homogeneous solutions of the vdW equation.{{sfn|ps=|van der Waals|2004|pp=245-247}} The states above this line (with larger Helmholtz free energy) are either metastable or unstable.{{sfn|ps=|van der Waals|2004|pp=245-247}} The combined solid green-black curve in Figure 8 is the convex envelope of $f(T\_R,v)$, which is defined as the largest convex curve that is less than or equal to the function.{{sfn|ps=|Lebowitz|1974|p=52}}

For a vdW fluid, the molar Helmholtz potential is given by Eq (4a). This is, in reduced form,

$$f\_r\; =\; \backslash frac\{f\}\{RT\_\backslash text\{c\}\}\; =\; C\_u\; +\; T\_\backslash text\{r\}(c\; -\; C\_\backslash text\{s\}\; -\; \backslash ln[T\_\backslash text\{r\}^c\; (3v\_\backslash text\{r\}\; -\; 1)])\; -\; \backslash frac\{9\}\{8v\_\backslash text\{r\}\}$$

with derivative $\backslash partial\_\{v\_\backslash text\{r\}\}f\_\backslash text\{r\}\; =\; -3T\_\backslash text\{r\}\}/\; (\{3v\_\backslash text\{r\}-1)\; +\; 9/(8v\_\backslash text\{r\})^2\; =\; -p\_\backslash text\{r\}$. A plot of this function $f\_\backslash text\{r\}$, whose slope at each point is given by $p\_\backslash text\{r\}$ of the vdW equation, for the subcritical isotherm $T\_\backslash text\{r\}=7/8$ is shown in Figure 8 along with the line tangent to it at its two coexisting saturation points. The data illustrated in Figure 8 is the same as that shown in Figure 1 for this isotherm.{{sfn|ps=|van der Waals|2004|pp=245-247}}

This double tangent construction thus provides a graphical alternative to the Maxwell construction to establish the saturated liquid and vapor points on an isotherm.{{sfn|ps=|van der Waals|2004|pp=245-247}}

Van der Waals used the Helmholtz function because its properties could be easily extended to the binary fluid situation. In a binary mixture of vdW fluids, the Helmholtz potential is a function of two variables, $f(T\_R,v,x)$, where $x$ is a composition variable (for example $x=x\_2$ so $x\_1=1-x$). In this case, there are three stability conditions:{{sfn|ps=|van der Waals|2004|pp=247-250}}

$$\backslash frac\{\backslash partial^2f\}\{\backslash partial\; v^2\}>0\backslash qquad\backslash frac\{\backslash partial^2f\}\{\backslash partial\; x^2\}>0\backslash qquad\backslash frac\{\backslash partial^2f\}\{\backslash partial\; v^2\}\backslash frac\{\backslash partial^2f\}\{\backslash partial\; x^2\}-\backslash left(\backslash frac\{\backslash partial^2f\}\{\backslash partial\; x\backslash partial\; v\}\backslash right)^2>0$$

and the Helmholtz potential is a surface (of physical interest in the region $0\backslash le\; x\backslash le\; 1$). The first two stability conditions show that the curvature in each of the directions $v$ and $x$ are both non-negative for stable states, while the third condition indicates that stable states correspond to elliptic points on this surface.{{sfn|ps=|Kreyszig|1959|pp=124-128}} Moreover, its limit

$$\backslash frac\{\backslash partial^2f\}\{\backslash partial\; v^2\}\backslash frac\{\backslash partial^2f\}\{\backslash partial\; x^2\}$$

-\frac{\partial^2f}{\partial x\partial v}=0

specifies the spinodal curves on the surface.

For a binary mixture, the Euler equation{{sfn|ps=|Callen|1960|pp=47-48}} can be written in the form

$$\backslash begin\{align\}$$

f &= - p v + \mu_1 x_1 + \mu_2 x_2 \\

&= - p v + (\mu_2 - \mu_1) x + \mu_1

\end{align}

where $\backslash mu\_j=\backslash partial\_\{x\_j\}f$ are the molar chemical potentials of each substance, $j=1,2$. For constant values of $p$, $\backslash mu\_1$, and $\backslash mu\_2$, this equation is a plane with slopes $-p$ in the $v$ direction, $\backslash mu\_2-\backslash mu\_1$ in the $x$ direction, and intercept $\backslash mu\_1$. As in the case of a single substance, here the plane and the surface can have a double tangent, and the locus of the coexisting phase points forms a curve on each surface. The coexistence conditions are that the two phases have the same $T$, $p$, $\backslash mu\_2-\backslash mu\_1$, and $\backslash mu\_1$; the last two are equivalent to having the same $\backslash mu\_1$ and $\backslash mu\_2$ individually, which are just the Gibbs conditions for material equilibrium in this situation. The two methods of producing the coexistence surface are equivalent.{{sfn|ps=|van der Waals|2004|pp=247-250}}

Although this case is similar to that of a single fluid, here the geometry can be much more complex. The surface can develop a wave (called a plait or fold) in the $x$ direction as well as the one in the $v$ direction. Therefore, there can be two liquid phases that can be either miscible, or wholly or partially immiscible, as well as a vapor phase.{{sfn|ps=|Rowlinson (ed) in van der Waals|2004|pp=23-27}}{{sfn|ps=|van der Waals|2004|pp=253-258}} Despite a great deal of both theoretical and experimental work on this problem by van der Waals and his successors—work which produced much useful knowledge about the various types of phase equilibria that are possible in fluid mixtures{{sfn|ps=|DeBoer|1974|pp=7-16}}—complete solutions to the problem were only obtained after 1967, when the availability of modern computers made calculations of mathematical problems of this complexity feasible for the first time.{{sfn|ps=|Rowlinson (ed) in van der Waals|2004|pp=23-27,64-66}} The results obtained were, in Rowlinson's words,{{sfn|ps=|Rowlinson (ed) in van der Waals|1984|p=66}}

a spectacular vindication of the essential physical correctness of the ideas behind the van der Waals equation, for almost every kind of critical behavior found in practice can be reproduced by the calculations, and the range of parameters that correlate with the different kinds of behavior are intelligible in terms of the expected effects of size and energy.

To obtain these numerical results, the values of the constants of the individual component fluids $a\_\{11\},\; a\_\{22\},b\_\{11\},\; b\_\{22\}$ must be known. In addition, the effect of collisions between molecules of the different components, given by $a\_\{12\}$ and $b\_\{12\}$, must also be specified. In the absence of experimental data, or computer modeling results to estimate their value, the empirical combining rules, geometric and algebraic means can be used, respectively:{{sfn|ps=|Hirschfelder|Curtis|Bird|1964|pp=252-253}}

$$a\_\{12\}=(a\_\{11\}a\_\{22\})^\{1/2\}\backslash qquad\backslash text\{and\}\backslash qquad\; b\_\{12\}^\{1/3\}=(b\_\{11\}^\{1/3\}+b\_\{22\}^\{1/3\})/2.$$

These relations correspond to the empirical combining rules for the intermolecular force constants,

$$\backslash epsilon\_\{12\}=(\backslash epsilon\_\{11\}\backslash epsilon\_\{22\})^\{1/2\}\backslash qquad\backslash text\{and\}\backslash qquad\backslash sigma\_\{12\}=(\backslash sigma\_\{11\}+\backslash sigma\_\{22\})/2,$$

the first of which follows from a simple interpretation of the dispersion forces in terms of polarizabilities of the individual molecules, while the second is exact for rigid molecules.{{sfn|ps=|Hirschfelder|Curtis|Bird|1964|pp=168-169}} Using these empirical combining rules to generalize for $n$ fluid components, the quadratic mixing rules for the material constants are:{{sfn|ps=|Redlich|Kwong|1949}}

$$\backslash begin\{align\}$$

a_x &= \sum_{i=1}^n \sum_{j=1}^n {\left(a_{ii} a_{jj}\right)}^{1/2} x_i x_j = {\left(\sum_{i=1}^n a_{ii}^{1/2} x_i \right)}^2 \\

b_x &= \tfrac{1}{8} \sum_{i=1}^n \sum_{j=1}^n {\left(b_{ii}^{1/3} + b_{jj}^{1/3}\right)}^3 x_i x_j

\end{align}

These expressions come into use when mixing gases in proportion, such as when producing tanks of air for diving{{sfn|ps=|Hewitt}} and managing the behavior of fluid mixtures in engineering applications. However, more sophisticated mixing rules are often necessary, to obtain satisfactory agreement with reality over the wide variety of mixtures encountered in practice.{{sfn|ps=|Valderrama|2003|pp=1308-1312}}{{sfn|ps=|Kontogeorgis|Privat|Jaubert|2019|pp=4626-4633}}

Another method of specifying the vdW constants, pioneered by W.B. Kay and known as Kay's rule,{{sfn|ps=|Niemeyer|}} specifies the effective critical temperature and pressure of the fluid mixture by

$$T\_\{\backslash text\{c\}x\}=\backslash sum\_\{i=1\}^nT\_\{\backslash text\{c\}i\}x\_i\backslash qquad\backslash text\{and\}\backslash qquad\; p\_\{\backslash text\{c\}x\}=\backslash sum\_\{i=1\}^n\backslash ,p\_\{\backslash text\{c\}i\}x\_i.$$

In terms of these quantities, the vdW mixture constants are

$$a\_x=\backslash left(\backslash frac\{3\}\{4\}\backslash right)^3\; \backslash frac\{(RT\_\{\backslash text\{c\}x\})^2\}\{p\_\{\backslash text\{c\}x\}\},\; \backslash qquad\backslash qquad\; b\_x\; =\; \backslash left(\backslash frac\{1\}\{2\}\backslash right)^3\; \backslash frac\{RT\_\{\backslash text\{c\}x\}\}\{p\_\{\backslash text\{c\}x\}\}$$

which Kay used as the basis for calculations of the thermodynamic properties of mixtures. Kay's idea was adopted by T. W. Leland, who applied it to the molecular parameters $\backslash epsilon,\; \backslash sigma$, which are related to $a,\; b$ through $T\_\backslash text\{c\},\; p\_\backslash text\{c\}$ by $a\backslash propto\backslash epsilon\backslash sigma^3$ and $b\backslash propto\backslash sigma^3$. Using these together with the quadratic mixing rules for $a,\; b$ produces

$$\backslash sigma\_x^3=\backslash sum\_\{i=i\}^n\backslash sum\_\{j=1\}^n\backslash ,\; \backslash sigma\_\{ij\}^3x\_ix\_j\backslash qquad\backslash text\{and\}\backslash qquad\; \backslash epsilon\_x=\backslash left[\backslash sum\_\{i=1\}^n\backslash sum\_\{j=1\}^n\backslash epsilon\_\{ij\}\backslash sigma\_\{ij\}^3x\_ix\_j\backslash right]\backslash left[\backslash sum\_\{i=i\}^n\backslash sum\_\{j=1\}^n\backslash ,\; \backslash sigma\_\{ij\}^3x\_ix\_j\backslash right]^\{-1\}$$

which is the van der Waals approximation expressed in terms of the intermolecular constants.{{sfn|ps=|Leland|Rowlinson|Sather|1968|p=1447}}{{sfn|ps=|Rowlinson (ed) in van der Waals|1984|pp=69-70}} This approximation, when compared with computer simulations for mixtures, are in good agreement over the range , namely for molecules of similar diameters. Rowlinson said of this approximation, "It was, and indeed still is, hard to improve on the original van der Waals recipe when expressed in [this] form".{{sfn|ps=|Rowlinson (ed) in van der Waals|1984|p=70}}

Since van der Waals presented his thesis, "[m]any derivations, pseudo-derivations, and plausibility arguments have been given" for it.{{sfn|ps=|Goodstein|1985|p=443}} However, no mathematically rigorous derivation of the equation over its entire range of molar volume that begins from a statistical mechanical principle exists. Indeed, such a proof is not possible, even for hard spheres.{{sfn|ps=|Korteweg|1891b|p=277}}{{sfn|ps=|Tonks|1936|pp=962-963}}{{sfn|ps=|van Hove|1949|pp=957-959}}{{sfn|ps=|Kac|Uhlenbeck|Hemmer|1963|p=224}}{{sfn|ps=|Lebowitz|1974|pp=50, 52-57}} Goodstein writes, "Obviously the value of the van der Waals equation rests principally on its empirical behavior rather than its theoretical foundation."{{sfn|ps=|Goodstein|1985|p=446}}

Although the use of the vdW equation is not justified mathematically, it has empirical validity. Its various applications in this region that attest to this, both qualitative and quantitative, have been described previously in this article. This point was also made by Alder, et al. who, at a conference marking the 100th anniversary of van der Waals' thesis, noted that:{{sfn|ps=|Alder|Alley|Rigby|1974|p=143}}

It is doubtful whether we would celebrate the centennial of the Van der Waals equation if it were applicable only under circumstances where it has been proven to be rigorously valid. It is empirically well established that many systems whose molecules have attractive potentials that are neither long-range nor weak conform nearly quantitatively to the Van der Waals model. An example is the theoretically much studied system of Argon, where the attractive potential has only a range half as large as the repulsive core.

Engineers have made extensive use of this empirical validity, modifying the equation in numerous ways (by one account there have been some 400 cubic equations of state produced){{sfn|ps=|Valderrama|2003|p=1606}} to manage the liquids,{{sfn|ps=|Vera|Prausnitz|1972|p=7-10}} and gases of pure substances and mixtures,{{sfn|ps=|Kontogeorgis|Privat|Jaubert|2019|pp=4626-4629}} that they encounter in practice.

This situation has been aptly described by Boltzmann:{{sfn|ps=|Boltzmann|1995|p=356}}

... van der Waals has given us such a valuable tool that it would cost us much trouble to obtain by the subtlest deliberations a formula that would really be more useful than the one that van der Waals found by inspiration, as it were.

{{reflist}}

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| access-date = 2 April 2024

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| url-status = live

}}

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• Gas laws
• Ideal gas
• Inversion temperature
• Iteration
• Maxwell construction
• Real gas
• Theorem of corresponding states
• Van der Waals constants (data page)
• Redlich–Kwong equation of state

• {{cite book | first = David | last = Chandler | year = 1987 | title = Introduction to Modern Statistical Mechanics | pages = 287–295 | location = Oxford | publisher = Oxford University Press | isbn = 0195042778}}
• {{citation | first = Michael | last = Cross | year = 2004 | chapter-url = http://www.pmaweb.caltech.edu/~mcc/Ph127/b/Lecture3.pdf | chapter = Lecture 3: First Order Phase Transitions | url = http://www.pmaweb.caltech.edu/~mcc/Ph127/b/index.html | title = Physics 127: Statistical Physics, Second Term | location = Pasadena, California | publisher = Division of Physics, Mathematics, and Astronomy, California Institute of Technology}}.
• {{cite journal | first1 = A. | last1 = Dalgarno | first2 = W.D. | last2 = Davison | year = 1966 | title = The Calculation of Van Der Waals Interactions | journal = Advances in Atomic and Molecular Physics | volume = 2 | pages = 1–32 | doi = 10.1016/S0065-2199(08)60216-X| bibcode = 1966AdAMP...2....1D | isbn = 9780120038022 }}
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Category:Eponymous equations of physics

Category:Equations of state

Category:Gas laws

Category:Engineering thermodynamics

Equation