Lattice Hamiltonian
Fix a spin space and a finite region of the lattice (see finite box in the integer lattice ). A lattice Hamiltonian in volume is an energy function that assigns a real number (or in hard-constraint models) to each spin configuration , typically depending also on an exterior configuration (a boundary condition ) .
Given an interaction potential , the standard finite-volume Hamiltonian with boundary condition is
where each depends only on the spins in .
An external field is usually incorporated via single-site terms (see external field coupling ), e.g. by including appropriate .
Key properties
- Locality: If has finite range (see finite-range interaction ), then changing far from (in the boundary condition) does not affect except near the boundary.
- Additivity over interaction sets: The Hamiltonian is a sum of local contributions. For nearest-neighbor models (see nearest-neighbor structure ), the sum reduces to edges and sites.
- Translation invariance: If is translation invariant (see translation-invariant interaction ), then is covariant under lattice shifts (up to boundary effects).
- Boundary dependence: Different boundary conditions encode different ways the exterior influences . This dependence is essential in the study of phase transitions and in defining infinite-volume Gibbs measures via the DLR equation .
- Connection to Gibbs weights: The Hamiltonian generates Boltzmann weights , where is the inverse temperature . These weights define the finite-volume Gibbs measure and the lattice partition function .
Physical interpretation
The lattice Hamiltonian encodes the microscopic energetics: which local patterns are energetically favored (low energy) or suppressed (high energy). Competing terms in (e.g. interaction vs field, ferro- vs antiferromagnetic couplings) determine typical configurations, the presence of order parameters (see order parameter ), and whether multiple equilibrium phases can coexist (see pure phases and mixtures of Gibbs measures ).