Chemical potential

Why does water evaporate from an open dish even though nothing is boiling, and why does a drop of ink spread through still water without anyone stirring it? Both are answered by a single quantity: chemical potential, μi\mu_i. It is the Gibbs-energy analogue of temperature or electric potential — matter of species ii flows spontaneously from wherever μi\mu_i is high to wherever it is lower, exactly as heat flows from hot to cold. Chemical potential sits right after entropy in the CY11001 thermodynamics sequence and becomes the pivot for everything that follows: phase equilibrium, reaction equilibrium and the equilibrium constant are all restatements of "chemical potentials are equal" or "the weighted sum of chemical potentials is zero." This article defines μi\mu_i rigorously as a partial molar Gibbs energy, derives its ideal-gas form, and shows how a handful of algebraic steps with μi\mu_i replace the vague CBSE-level statement "ΔG<0\Delta G<0 means spontaneous" with a precise, species-by-species criterion.

The core insight

The chemical potential μi=(∂G/∂ni)T,P,nj≠i\mu_i=(\partial G/\partial n_i)_{T,P,n_{j\ne i}} is the partial molar Gibbs energy of species ii, and matter always moves spontaneously from higher μi\mu_i to lower μi\mu_i until μi\mu_i is equal everywhere that species can go.

The core idea

Definition. In a mixture, adding an infinitesimal amount of species ii while holding TT, PP, and every other mole number fixed changes the total Gibbs energy by an amount per mole equal to μi\mu_i:

μi=(∂G∂ni)T,P,nj≠i\mu_i = \left(\frac{\partial G}{\partial n_i}\right)_{T,P,n_{j\ne i}}

where: GG is total Gibbs energy, nin_i is moles of species ii, and the subscript nj≠in_{j\ne i} means every other component's mole number is held fixed. Because it is a ratio of an extensive change to an infinitesimal mole change, μi\mu_i is intensive — it depends only on composition, TT and PP, never on the total size of the system.

Any potential, same μi\mu_i. GG is the natural choice because T,PT,P are usually the controlled variables in a lab, but μi\mu_i can equally be written as a derivative of UU, HH, or AA under their own natural variables:

μi=(∂U∂ni)S,V,nj=(∂H∂ni)S,P,nj=(∂A∂ni)T,V,nj=(∂G∂ni)T,P,nj\mu_i = \left(\frac{\partial U}{\partial n_i}\right)_{S,V,n_j} = \left(\frac{\partial H}{\partial n_i}\right)_{S,P,n_j} = \left(\frac{\partial A}{\partial n_i}\right)_{T,V,n_j} = \left(\frac{\partial G}{\partial n_i}\right)_{T,P,n_j}

All four expressions describe the same state and give the identical number — μi\mu_i is one physical property of the system, only the bookkeeping (which variables are held fixed) changes.

The mixture rule for an ideal gas. For a pure ideal gas at pressure pp, referenced to a standard pressure p∘p^\circ (1 bar):

μ=μ∘(T)+RTln⁡(pp∘)\mu = \mu^\circ(T) + RT\ln\left(\frac{p}{p^\circ}\right)

where: μ∘(T)\mu^\circ(T) is the standard chemical potential (a function of TT alone, fixed by convention at p=p∘p=p^\circ), R=8.314 J mol−1K−1R=8.314\ \text{J mol}^{-1}\text{K}^{-1}, and TT is absolute temperature. In a mixture of ideal gases, the same formula holds for each component with its own partial pressure pip_i in place of pp — total pressure never appears in this formula.

The flow rule. Starting from the fundamental relation dG=−S dT+V dP+∑iμi dnidG=-S\,dT+V\,dP+\sum_i\mu_i\,dn_i, at constant T,PT,P this collapses to dG=∑iμi dni≤0dG=\sum_i\mu_i\,dn_i\le 0 for any spontaneous change. If species ii can move between two regions without a net change in total moles, transfer proceeds from high μi\mu_i to low μi\mu_i, and stops — reaching equilibrium — exactly when μi\mu_i is equal in every region species ii can reach.

Figure
Two boxes connected by an arrow labelled matter flows from high chemical potential to low chemical potential until the two values become equal at equilibrium
Chemical potential drives matter flow, like temperature drives heat flow Region A mu_i higher Region B mu_i lower species i flows this way Flow continues until mu_i(A) equals mu_i(B) — equilibrium
Derivation ADeriving the ideal-gas chemical potential formula

The goal is to show, starting only from the fundamental relation dG=−S dT+V dP+∑iμi dnidG=-S\,dT+V\,dP+\sum_i\mu_i\,dn_i and the ideal-gas law, that at fixed temperature a pure ideal gas's chemical potential must take the exact logarithmic form μ=μ∘(T)+RTln⁡(p/p∘)\mu=\mu^\circ(T)+RT\ln(p/p^\circ) used throughout this article, and to make clear why the logarithm — not pressure itself — is the natural variable for μ\mu.

Step 1. Isolate the pressure dependence at constant TT. For a pure substance with n=1n=1 mole, μ\mu equals the molar Gibbs energy GmG_m, and from dG=−S dT+V dPdG=-S\,dT+V\,dP, holding TT fixed gives dμ=Vm dPd\mu = V_m\,dP, where VmV_m is the molar volume. This says the chemical potential's response to pressure, at fixed TT, is governed purely by how much volume a mole of gas occupies.

Step 2. Substitute the ideal-gas molar volume. Since PVm=RTPV_m=RT for one mole, Vm=RT/PV_m=RT/P, so Step 1 becomes dμ=RTP dPd\mu = \dfrac{RT}{P}\,dP at constant TT. This is now a simple one-variable differential equation in PP.

Step 3. Integrate from the standard pressure p∘p^\circ up to the pressure of interest pp. ∫μ∘μdμ=RT∫p∘pdPP\displaystyle\int_{\mu^\circ}^{\mu} d\mu = RT\int_{p^\circ}^{p}\frac{dP}{P} gives μ−μ∘=RTln⁡(pp∘)\mu-\mu^\circ = RT\ln\left(\dfrac{p}{p^\circ}\right), i.e. μ=μ∘(T)+RTln⁡(p/p∘)\mu=\mu^\circ(T)+RT\ln(p/p^\circ), exactly the formula quoted above. The lower integration limit μ∘\mu^\circ is, by definition, the chemical potential the gas would have if it were at the standard pressure p∘p^\circ — it depends on TT but not on the actual pressure pp.

Step 4. Read off why the pressure dependence must be logarithmic, not linear. Because Vm∝1/PV_m\propto 1/P for an ideal gas, dμd\mu shrinks as PP grows, so equal ratio changes in pressure (doubling, halving) — not equal absolute changes — produce equal changes in μ\mu; that is precisely what a logarithm encodes, and it is why μi−μi∘=RTln⁡(pi/pi∘)\mu_i-\mu_i^\circ=RT\ln(p_i/p_i^\circ) generalises directly to any component of an ideal-gas mixture using its own partial pressure pip_i.

Worked example

For an ideal-gas mixture at 298 K containing N2\text{N}_2 at partial pressure 0.8 bar and O2\text{O}_2 at partial pressure 0.2 bar (standard state p∘=1p^\circ=1 bar), find μN2−μN2∘\mu_{N_2}-\mu_{N_2}^\circ and μO2−μO2∘\mu_{O_2}-\mu_{O_2}^\circ, then use the results to decide which phase water occupies at 25°C, 1 atm in an open dish.

Step 1. Apply μi−μi∘=RTln⁡(pi/p∘)\mu_i-\mu_i^\circ=RT\ln(p_i/p^\circ) to nitrogen. μN2−μN2∘=(8.314)(298)ln⁡(0.8/1)=2477.6×ln⁡(0.8)=2477.6×(−0.2231)=−552.7 J mol−1\mu_{N_2}-\mu_{N_2}^\circ=(8.314)(298)\ln(0.8/1)=2477.6\times\ln(0.8)=2477.6\times(-0.2231)=-552.7\ \text{J mol}^{-1}.

Step 2. Apply the same formula to oxygen, which is more dilute. μO2−μO2∘=(8.314)(298)ln⁡(0.2/1)=2477.6×ln⁡(0.2)=2477.6×(−1.6094)=−3987.4 J mol−1\mu_{O_2}-\mu_{O_2}^\circ=(8.314)(298)\ln(0.2/1)=2477.6\times\ln(0.2)=2477.6\times(-1.6094)=-3987.4\ \text{J mol}^{-1}.

Step 3. Interpret the sizes. Both shifts are negative, as expected below standard pressure, but the O2\text{O}_2 shift is roughly seven times larger even though its pressure is only four times smaller than N2\text{N}_2's — because μ\mu depends on PP logarithmically, the more dilute species is pulled down disproportionately far from its reference value. This same logarithmic sensitivity is what later produces the −RTln⁡K-RT\ln K relation between Gibbs energy and the equilibrium constant.

Step 4. Apply the flow rule to water in an open dish at 25°C, 1 atm. For a pure substance, μ(l)=Gm(l)\mu^{(l)}=G_m^{(l)} and μ(v)=Gm(v)\mu^{(v)}=G_m^{(v)}. At the normal boiling point (100°C, 1 atm) the two phases coexist, so μ(l)=μ(v)\mu^{(l)}=\mu^{(v)} there by definition. At 25°C in an open dish, water vapour never accumulates to its saturation partial pressure, so using μ(v)=μ∘(v)+RTln⁡(pH2O/p∘)\mu^{(v)}=\mu^{\circ(v)}+RT\ln(p_{H_2O}/p^\circ), the lower actual pH2Op_{H_2O} makes μ(v)\mu^{(v)} smaller than the value at which μ(v)=μ(l)\mu^{(v)}=\mu^{(l)} would hold. Answer: hence μ(l)>μ(v)\mu^{(l)}>\mu^{(v)} under open-dish conditions, so liquid water spontaneously converts to vapour — the dish evaporates — until it empties or (in a closed container) pH2Op_{H_2O} rises enough to restore equality.

Common traps

  • Writing μi=G/ni\mu_i=G/n_i (Gibbs energy per mole of the mixture) instead of the correct partial derivative (∂G/∂ni)T,P,nj(\partial G/\partial n_i)_{T,P,n_j} — the two coincide only for a single pure substance, never for a genuine mixture where cross-terms between components matter.
  • Using total pressure PP instead of the component's own partial pressure pip_i in the ideal-gas chemical potential formula for a mixture — a very common substitution error.
  • Assuming μi\mu_i has some absolute zero or must be positive — like GG itself, μi\mu_i is only meaningfully defined relative to a reference/standard state μi∘\mu_i^\circ; only differences and equalities between phases carry physical meaning.
  • Thinking equilibrium requires μi=0\mu_i=0 — the correct condition is μi\mu_i equal across every phase or location species ii can access, not equal to zero.

Ask the tutor: If "matter flows from high mu to low mu" still feels like a hand-wavy analogy, ask the AI tutor to connect it back to dG=∑iμi dni≤0dG=\sum_i\mu_i\,dn_i\le0 algebraically so you can see the inequality itself force the direction of flow.

Why is chemical potential called a partial molar quantity instead of just molar Gibbs energy?

Because in a mixture, adding a mole of species ii changes the total Gibbs energy by an amount that also depends on what else is already present — the interactions between components matter. Only for a single pure substance does adding a mole of it change GG by exactly G/nG/n, so μ=Gm\mu=G_m there. In any real mixture the partial derivative (∂G/∂ni)T,P,nj(\partial G/\partial n_i)_{T,P,n_j} is the only correct definition, which is why it is called "partial" molar Gibbs energy.

Does chemical potential only apply to gases, or also to liquids and solids?

It applies to every phase and every species — gases, liquids, solids, and dissolved solutes all have a well-defined μi\mu_i. This article derives the ideal-gas form because it is algebraically the simplest case and the one you need first in CY11001. Liquids and solids, and non-ideal gases, get corrected formulas (using fugacity or activity in place of pressure) in later articles, but the underlying definition μi=(∂G/∂ni)T,P,nj\mu_i=(\partial G/\partial n_i)_{T,P,n_j} and the flow rule "high mu to low mu" never change.

How does chemical potential connect to the equilibrium constant K that I already know from JEE-level chemistry?

At equilibrium in a reacting mixture, the weighted sum of chemical potentials of products equals that of reactants (each weighted by its stoichiometric coefficient) rather than a simple pairwise equality. Substituting the ideal-gas form μi=μi∘+RTln⁡(pi/p∘)\mu_i=\mu_i^\circ+RT\ln(p_i/p^\circ) into that condition and rearranging produces exactly ΔG∘=−RTln⁡K\Delta G^\circ=-RT\ln K — the familiar equilibrium-constant relation is just the reaction version of the same "chemical potentials balance" idea used here for phases. That derivation is covered in the next article on reaction equilibria.

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