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§5.11 Asymptotic Expansions

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§5.11(i) Poincaré-Type Expansions

With the same conditions,

where

5.11.4
g_{0}=1,
g_{1}=\tfrac{1}{12},
g_{2}=\tfrac{1}{288},
g_{3}=-\tfrac{139}{51840},
g_{4}=-\tfrac{571}{24\;88320},
g_{5}=\tfrac{1\;63879}{2090\;18880},
g_{6}=\tfrac{52\;46819}{7\;52467\;96800}.

Also,

where a_{0}=\tfrac{1}{2}\sqrt{2} and

5.11.6a_{0}a_{k}+\frac{1}{2}a_{1}a_{{k-1}}+\frac{1}{3}a_{2}a_{{k-2}}+\dots+\frac{1}{%
k+1}a_{k}a_{0}=\frac{1}{k}a_{{k-1}},k\geq 1.

Wrench (1968) gives exact values of g_{k} up to g_{{20}}. Spira (1971) corrects errors in Wrench’s results and also supplies exact and 45D values of g_{k} for k=21,22,\dots,30. For an asymptotic expansion of g_{k} as k\to\infty see Boyd (1994).

Terminology

The expansion (5.11.1) is called Stirling’s series (Whittaker and Watson (1927, §12.33)), whereas the expansion (5.11.3), or sometimes just its leading term, is known as Stirling’s formula (Abramowitz and Stegun (1964, §6.1), Olver (1997b, p. 88)).

Next, and again with the same conditions,

where a\;(>0) and b\;(\in\Complex) are both fixed, and

where h\;(\in[0,1]) is fixed, and \mathop{B_{{k}}\/}\nolimits\!\left(h\right) is the Bernoulli polynomial defined in §24.2(i).

Lastly, as y\to\pm\infty,

uniformly for bounded real values of x.

§5.11(ii) Error Bounds and Exponential Improvement

If the sums in the expansions (5.11.1) and (5.11.2) are terminated at k=n-1 (k\geq 0) and z is real and positive, then the remainder terms are bounded in magnitude by the first neglected terms and have the same sign. If z is complex, then the remainder terms are bounded in magnitude by {\mathop{\sec\/}\nolimits^{{2n}}}\!\left(\tfrac{1}{2}\mathop{\mathrm{ph}\/}%
\nolimits z\right) for (5.11.1), and {\mathop{\sec\/}\nolimits^{{2n+1}}}\!\left(\tfrac{1}{2}\mathop{\mathrm{ph}\/}%
\nolimits z\right) for (5.11.2), times the first neglected terms.

For the remainder term in (5.11.3) write

Then

where \mathop{\zeta\/}\nolimits\!\left(K\right) is as in Chapter 25. For this result and a similar bound for the sector \frac{1}{2}\pi\leq\mathop{\mathrm{ph}\/}\nolimits z\leq\pi see Boyd (1994).

For further information see Olver (1997b, pp. 293–295), and for other error bounds see Whittaker and Watson (1927, §12.33), Spira (1971), and Schäfke and Finsterer (1990).

For re-expansions of the remainder terms in (5.11.1) and (5.11.3) in series of incomplete gamma functions with exponential improvement (§2.11(iii)) in the asymptotic expansions, see Berry (1991), Boyd (1994), and Paris and Kaminski (2001, §6.4).

§5.11(iii) Ratios

In this subsection a, b, and c are real or complex constants.

If z\to\infty in the sector |\mathop{\mathrm{ph}\/}\nolimits z|\leq\pi-\delta (<\pi), then

Also, with the added condition \realpart{(b-a)}>0,

Here

In terms of generalized Bernoulli polynomials \mathop{B^{{(\ell)}}_{{n}}\/}\nolimits\!\left(x\right)24.16(i)), we have for k=0,1,\ldots,

Lastly, and again if z\to\infty in the sector |\mathop{\mathrm{ph}\/}\nolimits z|\leq\pi-\delta (<\pi), then

For the error term in (5.11.19) in the case z=x\;(>0) and c=1, see Olver (1995).