# Maxwell relations

Flow chart showing the paths between the Maxwell relations. ${\displaystyle P}$ is pressure, ${\displaystyle T}$ temperature, ${\displaystyle V}$ volume, ${\displaystyle S}$ entropy, ${\displaystyle \alpha }$ coefficient of thermal expansion, ${\displaystyle \kappa }$ compressibility, ${\displaystyle C_{V}}$ heat capacity at constant volume, ${\displaystyle C_{P}}$ heat capacity at constant pressure.

Maxwell's relations are a set of equations in thermodynamics which are derivable from the symmetry of second derivatives and from the definitions of the thermodynamic potentials. These relations are named for the nineteenth-century physicist James Clerk Maxwell.

## Equations

The structure of Maxwell relations is a statement of equality among the second derivatives for continuous functions. It follows directly from the fact that the order of differentiation of an analytic function of two variables is irrelevant (Schwarz theorem). In the case of Maxwell relations the function considered is a thermodynamic potential and ${\displaystyle x_{i}}$ and ${\displaystyle x_{j}}$ are two different natural variables for that potential, we have

Schwarz' theorem (general)

${\displaystyle {\frac {\partial }{\partial x_{j}}}\left({\frac {\partial \Phi }{\partial x_{i}}}\right)={\frac {\partial }{\partial x_{i}}}\left({\frac {\partial \Phi }{\partial x_{j}}}\right)}$

where the partial derivatives are taken with all other natural variables held constant. For every thermodynamic potential there are ${\displaystyle {\frac {n(n-1)}{2}}}$ possible Maxwell relations where ${\displaystyle n}$ is the number of natural variables for that potential. The substantial increase in the entropy will be verified according to the relations satisfied by the laws of thermodynamics.

## The four most common Maxwell relations

The four most common Maxwell relations are the equalities of the second derivatives of each of the four thermodynamic potentials, with respect to their thermal natural variable (temperature ${\displaystyle T}$, or entropy ${\displaystyle S}$) and their mechanical natural variable (pressure ${\displaystyle P}$, or volume ${\displaystyle V}$):

Maxwell's relations (common)

{\displaystyle {\begin{aligned}+\left({\frac {\partial T}{\partial V}}\right)_{S}&=&-\left({\frac {\partial P}{\partial S}}\right)_{V}&=&{\frac {\partial ^{2}U}{\partial S\partial V}}\\+\left({\frac {\partial T}{\partial P}}\right)_{S}&=&+\left({\frac {\partial V}{\partial S}}\right)_{P}&=&{\frac {\partial ^{2}H}{\partial S\partial P}}\\+\left({\frac {\partial S}{\partial V}}\right)_{T}&=&+\left({\frac {\partial P}{\partial T}}\right)_{V}&=&-{\frac {\partial ^{2}F}{\partial T\partial V}}\\-\left({\frac {\partial S}{\partial P}}\right)_{T}&=&+\left({\frac {\partial V}{\partial T}}\right)_{P}&=&{\frac {\partial ^{2}G}{\partial T\partial P}}\end{aligned}}\,\!}

where the potentials as functions of their natural thermal and mechanical variables are the internal energy ${\displaystyle U(S,V)}$, enthalpy ${\displaystyle H(S,P)}$, Helmholtz free energy ${\displaystyle F(T,V)}$, and Gibbs free energy ${\displaystyle G(T,P)}$. The thermodynamic square can be used as a mnemonic to recall and derive these relations. The usefulness of these relations lies in their quantifying entropy changes, which are not directly measurable, in terms of measurable quantities like temperature, volume, and pressure.

Each equation can be re-expressed using the relationship

${\displaystyle \left({\frac {\partial y}{\partial x}}\right)_{z}=1\left/\left({\frac {\partial x}{\partial y}}\right)_{z}\right.}$

which are sometimes also known as Maxwell relations.

### Derivation

Maxwell relations are based on simple partial differentiation rules, in particular the total differential of a function and the symmetry of evaluating second order partial derivatives.

## Derivation based on Jacobians

If we view the first law of thermodynamics,

{\displaystyle {\begin{aligned}dU&=TdS-PdV\\\end{aligned}}\,\!}

as a statement about differential forms, and take the exterior derivative of this equation, we get

${\displaystyle 0=dTdS-dPdV}$

since ${\displaystyle d(dU)=0}$. This leads to the fundamental identity

${\displaystyle dPdV=dTdS.}$

The physical meaning of this identity can be seen by noting that the two sides are the equivalent ways of writing the work done in an infinitesimal Carnot cycle. An equivalent way of writing the identity is

${\displaystyle {\frac {\partial (T,S)}{\partial (P,V)}}=1.}$

The Maxwell relations now follow directly. For example,

${\displaystyle {\Bigl (}{\frac {\partial S}{\partial V}}{\Bigr )}_{T}={\frac {\partial (T,S)}{\partial (T,V)}}={\frac {\partial (P,V)}{\partial (T,V)}}={\Bigl (}{\frac {\partial P}{\partial T}}{\Bigr )}_{V},}$

The critical step is the penultimate one. The other Maxwell relations follow in similar fashion. For example,

${\displaystyle {\Bigl (}{\frac {\partial T}{\partial V}}{\Bigr )}_{S}={\frac {\partial (T,S)}{\partial (V,S)}}={\frac {\partial (P,V)}{\partial (V,S)}}=-{\Bigl (}{\frac {\partial P}{\partial S}}{\Bigr )}_{V}.}$

## General Maxwell relationships

The above are not the only Maxwell relationships. When other work terms involving other natural variables besides the volume work are considered or when the number of particles is included as a natural variable, other Maxwell relations become apparent. For example, if we have a single-component gas, then the number of particles N  is also a natural variable of the above four thermodynamic potentials. The Maxwell relationship for the enthalpy with respect to pressure and particle number would then be:

${\displaystyle \left({\frac {\partial \mu }{\partial P}}\right)_{S,N}=\left({\frac {\partial V}{\partial N}}\right)_{S,P}\qquad ={\frac {\partial ^{2}H}{\partial P\partial N}}}$

where μ is the chemical potential. In addition, there are other thermodynamic potentials besides the four that are commonly used, and each of these potentials will yield a set of Maxwell relations. For example, the grand potential ${\displaystyle \Omega (\mu ,V,T)}$ yields:[1]

{\displaystyle {\begin{aligned}\left({\frac {\partial N}{\partial V}}\right)_{\mu ,T}&=&\left({\frac {\partial P}{\partial \mu }}\right)_{V,T}&=&-{\frac {\partial ^{2}\Omega }{\partial \mu \partial V}}\\\left({\frac {\partial N}{\partial T}}\right)_{\mu ,V}&=&\left({\frac {\partial S}{\partial \mu }}\right)_{V,T}&=&-{\frac {\partial ^{2}\Omega }{\partial \mu \partial T}}\\\left({\frac {\partial P}{\partial T}}\right)_{\mu ,V}&=&\left({\frac {\partial S}{\partial V}}\right)_{\mu ,T}&=&-{\frac {\partial ^{2}\Omega }{\partial V\partial T}}\end{aligned}}\,\!}