Interaction potential (Φ)
An interaction potential (often denoted ) for a lattice spin system with spin space is a family of functions
indexed by finite subsets of the lattice. Each term is a real-valued function of the spin variables in only; equivalently, it is a function on (measurable with respect to the product sigma-algebra on ).
From one constructs the finite-volume lattice Hamiltonian by summing all interaction terms that intersect the volume, and from those Hamiltonians one builds the Gibbs specification and ultimately infinite-volume Gibbs measures via the DLR equation .
Key properties
- Support and range:
- is finite range if whenever exceeds some fixed range (see finite-range interaction ).
- Nearest-neighbor models are special cases where only single-site and edge terms appear (see nearest-neighbor structure ).
- Translation invariance: is translation invariant if translating and the spins on it does not change the functional form of (see translation-invariant interaction ). This is the lattice analogue of homogeneity.
- Summability/regularity (ensuring well-defined energies): For infinite-volume considerations, one often requires a summability condition (e.g. absolute summability over sets containing the origin) so that energy differences and pressure are well-defined and the Gibbs formalism behaves well.
- Multi-body interactions: Terms with encode genuine many-body couplings. Pair interactions correspond to terms, plus possible on-site fields ().
- Symmetries and constraints: Symmetries of (spin-flip, rotations, permutations of Potts colors) control invariances of the model and are central to spontaneous symmetry breaking .
- Model identification: Standard models correspond to specific choices of , e.g. Ising , Potts , XY , and Heisenberg interactions.
Physical interpretation
The interaction potential specifies how local patterns contribute to energy:
- which alignments are favored (ferromagnetic vs antiferromagnetic tendencies; see ferromagnetic Ising and antiferromagnetic Ising ),
- how strongly and how far spins influence each other (range and decay),
- whether external fields bias single sites (see external field coupling ),
- and whether the system has continuous or discrete symmetry.
In equilibrium, determines the competition between energy minimization and entropic fluctuations, shaping typical configurations and the possible emergence of multiple Gibbs states (see extremal Gibbs measures and phase transitions ).