Put and integrate by parts using . The exponential cutoff has derivative , so the endpoint at infinity vanishes and the lower endpoint gives
With this becomes
The mass of the transformed integral lies at , where
To control this asymptotic expansion, split at and . On the central interval the geometric-series remainder is bounded by , whose integral against is finite. The lower tail has length and denominator at least ; the upper tail is exponentially small in , with the original denominator at least one. The omitted tails of the logarithmic moments are likewise negligible. Thus extending the moments to is justified.
The Gamma function gives , and the first logarithmic moment is , with Euler's constant. Therefore
This is the moving Gumbel cutoff in an inverse-power tail: replacing the original cutoff by a sharp step at gives the first term, but its smooth transition supplies the Euler-constant correction.
The phase is nonnegative on the interval and vanishes only at its two endpoints. An interval away from both endpoints contributes exponentially little, so both endpoint contributions must be expanded before their orders are ranked.
At the left endpoint,
The Laplace's method scale is . Hence its leading contribution is
The substitution evaluates the integral by the Gamma function. Since there is no quartic term in the phase, the next left-end correction is relatively , and thus absolutely .
At the right endpoint put . There
so gives
The leading right-end integral is a Gaussian integral. Its first correction is also absolutely . The mixed cubic and quadratic Laplace endpoints therefore produce the first two global terms
Keeping only the dominant cubic endpoint would miss the second term, which is larger than that endpoint's own first correction.

Articles by others on the same topic (0)

There are currently no matching articles.