Lattice pressure (finite volume)

Dimensionless free-energy density: the log partition function per lattice site in a finite region.
Lattice pressure (finite volume)

Let Λ\Lambda be a finite region (see ) and let ZΛ(β,τ)Z_\Lambda(\beta,\tau) be the at inverse temperature β\beta with τ\tau.

The finite-volume (dimensionless) pressure is

pΛ(β,τ)=1ΛlogZΛ(β,τ), p_\Lambda(\beta,\tau) ={} \frac{1}{|\Lambda|}\,\log Z_\Lambda(\beta,\tau),

where Λ|\Lambda| is the number of lattice sites in Λ\Lambda.

Equivalently, the finite-volume Helmholtz free energy is

FΛ(β,τ)=1βlogZΛ(β,τ), F_\Lambda(\beta,\tau) = -\frac{1}{\beta}\log Z_\Lambda(\beta,\tau),

so that pΛ(β,τ)=βFΛ(β,τ)Λp_\Lambda(\beta,\tau) = -\beta\,\frac{F_\Lambda(\beta,\tau)}{|\Lambda|}, matching the statistical-mechanics notion of and the thermodynamic (up to conventions and units).

Key properties

  • Intensive quantity. pΛp_\Lambda is normalized per site and is therefore the natural quantity to send to the .

  • Boundary effects are subextensive. For many short-range models (e.g. ), changing τ\tau changes logZΛ\log Z_\Lambda by at most order Λ|\partial \Lambda|, so pΛ(β,τ)p_\Lambda(\beta,\tau) is often asymptotically independent of τ\tau as Λ|\Lambda|\to\infty.

  • Convexity in parameters. Because it is a log-partition function density, pΛp_\Lambda is typically convex in couplings and fields appearing linearly in the (a finite-volume version of standard convexity for logZ\log Z).

  • Derivatives give observables. If the Hamiltonian includes an external field term (see ), then derivatives of pΛp_\Lambda with respect to that field give magnetization density and susceptibilities (see ).

Physical interpretation

pΛp_\Lambda is the free-energy density in units of kBTk_B T (see and ): it encodes the competition between energy minimization and entropy maximization in a finite region. Non-smooth behavior of its infinite-volume limit is a key diagnostic of .