Chemical equilibrium

Equilibrium with respect to matter exchange and reactions: no net particle flow and chemical potentials satisfy the appropriate equalities.
Chemical equilibrium

A is in chemical equilibrium when there is no spontaneous tendency for its composition to change through matter transfer or chemical reaction, given the allowed exchanges with its and its constraints.

Two common cases are:

  1. Particle exchange (diffusive equilibrium). If two systems can exchange through a permeable boundary, chemical equilibrium requires equality of the for each exchanged species:

    μi(1)=μi(2)for each species i. \mu_i^{(1)} = \mu_i^{(2)} \quad \text{for each species } i.
  2. Chemical reactions. For a reaction with stoichiometric coefficients νi\nu_i, chemical equilibrium requires that the reaction has no net driving force. In terms of chemical potentials this can be written as

    iνiμi=0, \sum_i \nu_i \mu_i = 0,

    with the sum over all species participating in the reaction.

Chemical equilibrium is a necessary component of , alongside and equilibrium.

Physical interpretation

Chemical potential measures the “escaping tendency” of particles (or, more generally, how the system’s free energy changes with composition). If two regions have different chemical potentials for a species, matter transfer or reaction progress can increase total entropy (or decrease the appropriate free-energy potential), so a net change occurs until the chemical potentials satisfy the equilibrium condition.

In practice, chemical equilibrium is what makes composition stable: once reached, the system may still exchange energy as or perform (depending on constraints), but it has no net tendency to change its particle content or reaction extent.

Key relations and thermodynamic potentials

Entropy maximization with particle exchange. For two subsystems that can exchange particles (but not volume) with fixed totals, maximizing total entropy implies

(S1N1)U1,V1=(S2N2)U2,V2. \left(\frac{\partial S_1}{\partial N_1}\right)_{U_1,V_1} ={} \left(\frac{\partial S_2}{\partial N_2}\right)_{U_2,V_2}.

Using the identity from equilibrium thermodynamics

(SN)U,V=μT, \left(\frac{\partial S}{\partial N}\right)_{U,V} = -\frac{\mu}{T},

this yields μ1/T1=μ2/T2\mu_1/T_1 = \mu_2/T_2. When the subsystems are also in so that T1=T2T_1=T_2, it reduces to μ1=μ2\mu_1=\mu_2.

Equivalent definitions of chemical potential. For a single-component system,

μ=(UN)S,V=(FN)T,V=(GN)T,P, \mu = \left(\frac{\partial U}{\partial N}\right)_{S,V} = \left(\frac{\partial F}{\partial N}\right)_{T,V} = \left(\frac{\partial G}{\partial N}\right)_{T,P},

linking μ\mu to derivatives of UU, FF, and GG in the natural variables of each potential.

Open systems and reservoirs. A system that can exchange particles with a reservoir is an ; at fixed (T,V,μ)(T,V,\mu) the equilibrium state minimizes the .