Background field method

Background field method

In theoretical physics, background field method is a useful procedure to calculate the effective action of a quantum field theory by expanding a quantum field around a classical "background" value "B":: phi(x) = B(x) + eta (x).After this is done, the Green's functions are evaluated as a function of the background. This approach has the advantage that the gauge invariance is manifestly preserved if the approach is applied to gauge theory.

Method

We typically want to calculate expressions like: Z [J] = int mathcal D phi e^{i int d^d x (mathcal L [phi(x)] + J(x) phi(x))} where "J"("x") is a source, mathcal L(x) is the Lagrangian density of the system, "d" is the number of dimensions and φ("x") is a field.

In the background field method, one starts by splitting this field in a classical background field "B"("x") and a field η("x") containing additional quantum fluctuations:: phi(x) = B(x) + eta(x) .Typically, "B"("x") will be a solution of the classical equations of motion: left.frac{delta S}{delta phi} ight|_{phi = B} = 0 where "S" is the action, i.e. the space integral of the Lagrangian density. Fields obeying these equations typically yield the greatest contribution in a path integral, so it is natural to expand around them. Switching on a source "J"("x") will change the equations into δ"S"/δφ|φ = "B" + "J" = 0.

Then the action is expanded around the background "B"("x"):: int d^d x (mathcal L [phi(x)] + J(x) phi(x)) = int d^d x (mathcal L [B(x)] + J(x) B(x)) + int d^d x left(frac{deltamathcal L}{delta phi(x)} [B] + J(x) ight) eta(x) + frac12 int d^d x d^d y frac{delta^2mathcal L}{delta phi(x) deltaphi(y)} [B] eta(x) eta(y) + cdots The second term in this expansion is zero by the equations of motion. The first term does not depend on any fluctuating fields, so that it can be brought out of the path integral. The result is: Z [J] = e^{i int d^d x (mathcal L [B(x)] + J(x) B(x))} int mathcal D eta e^{frac i2 int d^d x d^d y frac{delta^2mathcal L}{delta phi(x) deltaphi(y)} [B] eta(x) eta(y) + cdots}. The path integral which now remains is (neglecting the corrections in the dots) of Gaussian form and can be integrated exactly:: Z [J] = C e^{i int d^d x (mathcal L [B(x)] + J(x) B(x))} left(det frac{delta^2mathcal L}{delta phi(x) deltaphi(y)} [B] ight)^{-1/2} + cdots where "det" signifies a functional determinant and "C" is a constant. The power of minus one half will naturally be plus one for Grassmann fields.

The above derivation gives the Gaussian approximation to the functional integral. Corrections to this can be computed, producing a diagrammatic expansion.

ee also

BF theory

References

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