A Gaussian variational approximation chooses a quadratic trial kernel and minimizes a variational upper bound on the interacting free energy. The optimized kernel often equals the bare kernel plus a self-consistent, wavevector-independent mass shift.
For and an even positive trial kernel , define and using a positive-wavevector sum for a real field. Isserlis theorem gives . The Feynman-Bogoliubov inequality therefore has stationary kernelsThus both the mass and gradient coefficient shift. In the thermodynamic limit, their self-consistency equations areA coarse-graining ultraviolet cutoff is necessary for the first integral in three dimensions: its large- radial integrand tends to a constant. Physical solutions require .
For an exact dimensionless Hamiltonian and trial Hamiltonian , the free energies obeywhere , , and the expectation value uses the normalized trial equilibrium state. A physical Hamiltonian is multiplied by in these formulas; multiplying the bound by restores physical free energy units.
For classical configurations, the identity and the Jensen inequality for the convex exponential function give . Taking minus the logarithm proves the bound.
The same bound holds for finite-dimensional, noncommuting quantum Hamiltonians, although the preceding exponential-factorization identity cannot generally be used. Define the density matrices and . With natural logarithms, nonnegativity of quantum relative entropy givesRearrangement proves the quantum result without requiring . Equality holds when ; in this finite-dimensional setting that means is a scalar multiple of the identity operator.[ref]
The Theory of Quantum Information by John Watrous. Proposition 5.22, Klein's inequality; the displayed thermal-state substitution derives the variational free-energy bound, using natural rather than the book's base-two logarithms
A tractable trial family therefore supplies upper bounds that can be minimized over its parameters. This variational minimum need not reproduce exact correlations or phase transition locations.
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