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 kernels
Thus both the mass and gradient coefficient shift. In the thermodynamic limit, their self-consistency equations are
A 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 obey
where , , 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 gives
Rearrangement 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]
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.

Articles by others on the same topic (0)

There are currently no matching articles.