Let . Near the interior minimum, Taylor expansion gives
On the scale , the leading exponent is and . If the integral is localized at this minimum, the rescaled integration endpoints tend to infinity in both directions, so the Gaussian integral gives Laplace's method:
Formally expanding the cubic term gives an order- correction odd in , whose Gaussian integral is zero. Quartic terms and the square of the cubic term produce the order- correction. Sufficient smoothness near the minimum and control of the exterior integral justify this formal calculation.
The printed local assumptions alone do not guarantee localization. A useful localization condition for Laplace's method is that outside each sufficiently small fixed neighbourhood of , for some , and that for some . For , the exterior contribution is at most
which is exponentially smaller than the displayed local term. To see why something of this kind is needed, take on . Its unique minimum is at zero and , yet on we have . This boundary interval alone contributes at least , dominating the proposed local approximation. The Laplace formula therefore has its usual implicit tail assumption, rather than following from uniqueness of the interior minimum alone.
For the Gamma function, set to obtain
Here has its unique minimum at , with and . It tends to infinity at both endpoints, and its integral is finite for positive exponents, so localization holds. Laplace's method yields Stirling's formula:
For a prior density and independent observations, Bayes' theorem writes the desired posterior expectation as a ratio of integrals:
Suppose the log-posterior kernel has a unique concentrating interior mode , with curvature of order , and the smoothness and tail conditions hold for both integrals. Expanding quadratically gives a common Gaussian factor . Replacing the smooth amplitude by gives
This approximation does not require to be positive: it treats as an amplitude, without taking its logarithm. For more accuracy, expand the amplitude and the cubic term in the log-posterior kernel. With , the Gaussian moments are and . Terms multiplying cancel between numerator and denominator; the two remaining first corrections are
under the stronger smoothness, derivative-scaling and integrability assumptions needed for this expansion. The first term accounts for the curvature of the amplitude and the second for posterior skewness. This is posterior expectation by Laplace approximation. If there are several modes, boundary modes, or nonconcentrating tails, the appropriate separate contributions must be included; a single interior Gaussian approximation cannot then be assumed.