§2.4 Contour Integrals§2.6 Distributional Methods

§ 2.5. Mellin Transform Methods

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Keywords:
asymptotic approximations of integrals
Referenced by:
§2.10(iii), §2.3(ii), §5.19(ii)
Permalink:
http://dlmf.nist.gov/2.5
Contents

§ 2.5(i). Introduction

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Notes:
See Wong (1989, pp. 147–153, 155–157) and Doetsch (1955, §6.5).
Keywords:
locally integrable, Mellin transform, Parseval formula
Referenced by:
§2.3(ii), §2.5(ii)
Permalink:
http://dlmf.nist.gov/2.5.SS1

Let f(t) be a locally integrable function on (0,\infty), that is, \int _{{\rho}}^{{T}}f(t)dt exists for all \rho and T satisfying 0<\rho<T<\infty. The Mellin transform of f(t) is defined by

2.5.1 \mathscr{M}\left(f;z\right)=\int _{{0}}^{{\infty}}t^{{z-1}}f(t)dt,
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Defines:
f(x): locally integrable function
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when this integral converges. The domain of analyticity of \mathscr{M}\left(f;z\right) is usually an infinite strip a<\realpart{z}<b parallel to the imaginary axis. The inversion formula is given by

2.5.2 f(t)=\frac{1}{2\pi i}\int _{{c-i\infty}}^{{c+i\infty}}t^{{-z}}\mathscr{M}\left(f;z\right)dz,
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Defines:
f(x): locally integrable function and c: point
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with a<c<b.

One of the two convolution integrals associated with the Mellin transform is of the form

2.5.3 I(x)=\int _{{0}}^{{\infty}}f(t)\, h(xt)dt, x>0,
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Defines:
I(x): convolution integral and h(x): function
Symbols:
f(x): locally integrable function
Referenced by:
§2.5(ii), §2.5(ii)
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and

2.5.4 \mathscr{M}\left(I;z\right)=\mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right).
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Defines:
I(x): convolution integral and h(x): function
Symbols:
f(x): locally integrable function
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If \mathscr{M}\left(f;1-z\right) and \mathscr{M}\left(h;z\right) have a common strip of analyticity a<\realpart{z}<b, then

2.5.5 I(x)=\frac{1}{2\pi i}\int _{{c-i\infty}}^{{c+i\infty}}x^{{-z}}\mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right)dz,
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Defines:
I(x): convolution integral and h(x): function
Symbols:
f(x): locally integrable function and c: point
Referenced by:
§2.5(i), §2.5(ii), §2.5(iii)
Permalink:
http://dlmf.nist.gov/2.5.E5
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where a<c<b. When x=1, this identity is the Parseval formula.

If \mathscr{M}\left(f;1-z\right) and \mathscr{M}\left(h;z\right) can be continued analytically to meromorphic functions in a left half-plane, and if the contour \realpart{z}=c can be translated to \realpart{z}=d with d<c, then

2.5.6 I(x)=\sum\limits _{{d<\realpart{z}<c}}\Residue\left[x^{{-z}}\mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right)\right]+E(x),
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Defines:
d: point and E(x): function
Symbols:
f(x): locally integrable function, c: point, I(x): convolution integral and h(x): function
Referenced by:
§2.5(i), §2.5(i)
Permalink:
http://dlmf.nist.gov/2.5.E6
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where

2.5.7 E(x)=\frac{1}{2\pi i}\int _{{d-i\infty}}^{{d+i\infty}}x^{{-z}}\mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right)dz.
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Defines:
d: point and E(x): function
Symbols:
f(x): locally integrable function and h(x): function
Referenced by:
§2.5(i)
Permalink:
http://dlmf.nist.gov/2.5.E7
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The sum in (2.5.6) is taken over all poles of x^{{-z}}\mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right) in the strip d<\realpart{z}<c, and it provides the asymptotic expansion of I(x) for small values of x. Similarly, if \mathscr{M}\left(f;1-z\right) and \mathscr{M}\left(h;z\right) can be continued analytically to meromorphic functions in a right half-plane, and if the vertical line of integration can be translated to the right, then we obtain an asymptotic expansion for I(x) for large values of x.

¶ Example

2.5.8 I(x)=\int _{{0}}^{{\infty}}\frac{{J_{{\nu}}^{{2}}}\!\left(xt\right)}{1+t}dt, \nu>-\tfrac{1}{2},
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Symbols:
I(x): convolution integral
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where J_{{\nu}} denotes the Bessel function (§Ch.10), and x is a large positive parameter. Let h(t)={J_{{\nu}}^{{2}}}\!\left(t\right) and f(t)=1/(1+t). Then from Table Ch.1 and Watson (1944, p. 403)

2.5.9 \mathscr{M}\left(f;1-z\right)=\frac{\pi}{\sin\!\left(\pi z\right)}, 0<\realpart{z}<1,
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Defines:
f(t)=1/(1+t): function
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2.5.10 \mathscr{M}\left(h;z\right)=\frac{2^{{z-1}}\Gamma\!\left(\nu+\frac{1}{2}z\right)}{{\Gamma^{{2}}}\!\left(1-\frac{1}{2}z\right)\Gamma\!\left(1+\nu-\frac{1}{2}z\right)\Gamma\!\left(z\right)}\frac{\pi}{\sin\!\left(\pi z\right)}, -2\nu<\realpart{z}<1.
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Defines:
h(t)={J_{{\nu}}^{{2}}}\!\left(t\right): function
Symbols:
\Gamma\!\left(z\right): Gamma function
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In the half-plane \realpart{z}>\max(0,-2\nu), the product \mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right) has a pole of order two at each positive integer, and

2.5.11 \Residue _{{z=n}}\left[x^{{-z}}\mathscr{M}\left(f;1-z\right)\mathscr{M}\left(h;z\right)\right]=(a_{n}\ln x+b_{n})x^{{-n}},
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Defines:
h(t)={J_{{\nu}}^{{2}}}\!\left(t\right): function and f(t)=1/(1+t): function
Symbols:
a_{n}: coefficients and b_{n}: coefficients
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where

2.5.12 a_{n}=\frac{2^{{n-1}}\Gamma\!\left(\nu+\tfrac{1}{2}n\right)}{{\Gamma^{{2}}}\!\left(1-\tfrac{1}{2}n\right)\Gamma\!\left(1+\nu-\tfrac{1}{2}n\right)\Gamma\!\left(n\right)},
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Defines:
a_{n}: coefficients
Symbols:
\Gamma\!\left(z\right): Gamma function
Referenced by:
§2.5(i)
Permalink:
http://dlmf.nist.gov/2.5.E12
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2.5.13 b_{n}=-a_{n}\left(\ln 2+\tfrac{1}{2}\psi\!\left(\nu+\tfrac{1}{2}n\right)+\psi\!\left(1-\tfrac{1}{2}n\right)+\tfrac{1}{2}\psi\!\left(1+\nu-\tfrac{1}{2}n\right)-\psi\!\left(n\right)\right),
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Defines:
a_{n}: coefficients and b_{n}: coefficients
Symbols:
\psi\!\left(z\right): Psi or digamma function
Referenced by:
§2.5(i)
Permalink:
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and \psi is the logarithmic derivative of the gamma function (§5.2(i)).

We now apply (2.5.5) with \max(0,-2\nu)<c<1, and then translate the integration contour to the right. This is allowable in view of the asymptotic formula

2.5.14 |\Gamma\!\left(x+iy\right)|=\sqrt{2\pi}e^{{-\pi|y|/2}}|y|^{{x-(1/2)}}\left(1+o\!\left(1\right)\right),
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Symbols:
\Gamma\!\left(z\right): Gamma function and o\!\left(x\right): order symbol
Referenced by:
§2.5(iii)
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as y\to\pm\infty, uniformly for bounded |x|; see (5.11.9). Then as in (2.5.6) and (2.5.7), with d=2n+1-\epsilon (0<\epsilon<1), we obtain

2.5.15 I(x)=-\sum _{{s=0}}^{{2n}}(a_{s}\ln x+b_{s})x^{{-s}}+O\!\left(x^{{-2n-1+\epsilon}}\right), n=0,1,2,\dots.
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Defines:
\epsilon: parameter
Symbols:
O\!\left(x\right): order symbol, a_{n}: coefficients, b_{n}: coefficients and I(x): convolution integral
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http://dlmf.nist.gov/2.5.E15
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From (2.5.12) and (2.5.13), it is seen that a_{s}=b_{s}=0 when s is even. Hence

2.5.16 I(x)=\sum _{{s=0}}^{{n-1}}(c_{s}\ln x+d_{s})x^{{-2s-1}}+O\!\left(x^{{-2n-1+\epsilon}}\right),
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Defines:
\epsilon: parameter
Symbols:
O\!\left(x\right): order symbol, c: point, I(x): convolution integral and d: point
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where c_{s}=-a_{{2s+1}}, d_{s}=-b_{{2s+1}}.

§ 2.5(ii). Extensions

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Notes:
See Wong (1989, pp. 157–162).
Keywords:
asymptotic approximations of integrals
Referenced by:
§2.6(ii)
Permalink:
http://dlmf.nist.gov/2.5.SS2

Let f(t) and h(t) be locally integrable on (0,\infty) and

2.5.17 f(t)\sim\sum _{{s=0}}^{{\infty}}a_{s}t^{{\alpha _{s}}}, t\to 0+,
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Defines:
f(x): locally integrable function and a_{s}: coefficients
Symbols:
\sim: asymptotically equal
Referenced by:
§2.5(ii)
Permalink:
http://dlmf.nist.gov/2.5.E17
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where \realpart{\alpha _{s}}>\realpart{\alpha _{{s^{{\prime}}}}} for s>s^{{\prime}}, and \realpart{\alpha _{s}}\to+\infty as s\to\infty. Also, let

2.5.18 h(t)\sim\exp\!\left(i\kappa t^{p}\right)\sum _{{s=0}}^{{\infty}}b_{s}t^{{-\beta _{s}}}, t\to+\infty,
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Defines:
h(x): locally integrable function, \kappa: real and p: positive
Symbols:
\sim: asymptotically equal and b: right endpoint
Referenced by:
§2.5(iii), §2.5(ii), §2.5(iii), §2.5(iii)
Permalink:
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where \kappa is real, p>0, \realpart{\beta _{s}}>\realpart{\beta _{{s^{{\prime}}}}} for s>s^{{\prime}}, and \realpart{\beta _{s}}\to+\infty as s\to\infty. To ensure that the integral (2.5.3) converges we assume that

2.5.19 f(t)=O\!\left(t^{{-b}}\right), t\to+\infty,
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Defines:
f(x): locally integrable function
Symbols:
O\!\left(x\right): order symbol and b: right endpoint
Referenced by:
§2.5(ii)
Permalink:
http://dlmf.nist.gov/2.5.E19
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with b+\realpart{\beta _{0}}>1, and

2.5.20 h(t)=O\!\left(t^{c}\right), t\to 0+,
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Defines:
h(x): locally integrable function
Symbols:
O\!\left(x\right): order symbol and c: point
Referenced by:
§2.5(iii), §2.5(ii), §2.5(ii), §2.5(iii), §2.5(iii)
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with c+\realpart{\alpha _{0}}>-1. To apply the Mellin transform method outlined in §2.5(i), we require the transforms \mathscr{M}\left(f;1-z\right) and \mathscr{M}\left(h;z\right) to have a common strip of analyticity. This, in turn, requires -b<\realpart{\alpha _{0}}, -c<\realpart{\beta _{0}}, and either -c<\realpart{\alpha _{0}}+1 or 1-b<\realpart{\beta _{0}}. Following Handelsman and Lew (1970, 1971) we now give an extension of this method in which none of these conditions is required.

First, we introduce the truncated functions f_{1}(t) and f_{2}(t) defined by

2.5.21 f_{1}(t)=\begin{cases}f(t),&0<t\leq 1,\\
0,&1<t<\infty,\end{cases}
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Defines:
f_{j}(t): truncated functions
Symbols:
f(x): locally integrable function
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2.5.22 f_{2}(t)=f(t)-f_{1}(t).
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Defines:
f_{j}(t): truncated functions
Symbols:
f(x): locally integrable function
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Similarly,

2.5.23 h_{1}(t)=\begin{cases}h(t),&0<t\leq 1,\\
0,&1<t<\infty,\end{cases}
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Symbols:
h(x): locally integrable function
Referenced by:
§2.5(iii)
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2.5.24 h_{2}(t)=h(t)-h_{1}(t).
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Symbols:
h(x): locally integrable function
Referenced by:
§2.5(iii)
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With these definitions and the conditions (2.5.17) – (2.5.20) the Mellin transforms converge absolutely and define analytic functions in the half-planes shown in Table 2.5.1.

2.5.1. Domains of convergence for Mellin transforms.
Transform Domain of Convergence
\mathscr{M}\left(f_{1};z\right) \realpart{z}>-\realpart{\alpha _{0}}
\mathscr{M}\left(f_{2};z\right) \realpart{z}<b
\mathscr{M}\left(h_{1};z\right) \realpart{z}>-c
\mathscr{M}\left(h_{2};z\right) \realpart{z}<\realpart{\beta _{0}}
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Symbols:
h(x): locally integrable function, f_{j}(t): truncated functions, b: right endpoint and c: point
Referenced by:
§2.5(ii), §2.5(ii), §2.5(ii), §2.5(ii)
Permalink:
http://dlmf.nist.gov/2.5.T1

Furthermore, \mathscr{M}\left(f_{1};z\right) can be continued analytically to a meromorphic function on the entire z-plane, whose singularities are simple poles at -\alpha _{s}, s=0,1,2,\dots, with principal part

2.5.25 a_{s}/\left(z+\alpha _{s}\right).
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Symbols:
a_{s}: coefficients
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By Table 2.5.1, \mathscr{M}\left(f_{2};z\right) is an analytic function in the half-plane \realpart{z}<b. Hence we can extend the definition of the Mellin transform of f by setting

2.5.26 \mathscr{M}\left(f;z\right)=\mathscr{M}\left(f_{1};z\right)+\mathscr{M}\left(f_{2};z\right)
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Symbols:
f(x): locally integrable function and f_{j}(t): truncated functions
Referenced by:
§2.5(ii)
Permalink:
http://dlmf.nist.gov/2.5.E26
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for \realpart{z}<b. The extended transform \mathscr{M}\left(f;z\right) has the same properties as \mathscr{M}\left(f_{1};z\right) in the half-plane \realpart{z}<b.

Similarly, if \kappa=0 in (2.5.18), then \mathscr{M}\left(h_{2};z\right) can be continued analytically to a meromorphic function on the entire z-plane with simple poles at \beta _{s}, s=0,1,2,\dots, with principal part

2.5.27 -b_{s}/\left(z-\beta _{s}\right).
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Symbols:
b: right endpoint
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Alternatively, if \kappa\neq 0 in (2.5.18), then \mathscr{M}\left(h_{2};z\right) can be continued analytically to an entire function.

Since \mathscr{M}\left(h_{1};z\right) is analytic for \realpart{z}>-c by Table 2.5.1, the analytically-continued \mathscr{M}\left(h_{2};z\right) allows us to extend the Mellin transform of h via

2.5.28 \mathscr{M}\left(h;z\right)=\mathscr{M}\left(h_{1};z\right)+\mathscr{M}\left(h_{2};z\right)
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Symbols:
h(x): locally integrable function
Referenced by:
§2.5(iii), §2.5(ii)
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in the same half-plane. From (2.5.26) and (2.5.28), it follows that both \mathscr{M}\left(f;1-z\right) and \mathscr{M}\left(h;z\right) are defined in the half-plane \realpart{z}>\max(1-b,-c).

We are now ready to derive the asymptotic expansion of the integral I(x) in (2.5.3) as x\to\infty. First we note that

2.5.29 I(x)=\sum\limits _{{j,k=1}}^{{2}}I_{{jk}}(x),
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Symbols:
I(x): convolution integral
Referenced by:
§2.5(ii)
Permalink:
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where

2.5.30 I_{{jk}}(x)=\int _{{0}}^{{\infty}}f_{j}(t)h_{k}(xt)dt.
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Symbols:
h(x): locally integrable function, f_{j}(t): truncated functions and I(x): convolution integral
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By direct computation

2.5.31 I_{{21}}(x)=0, for x\ge 1.
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Symbols:
I(x): convolution integral
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Next from Table 2.5.1 we observe that the integrals for the transform pair \mathscr{M}\left(f_{j};1-z\right) and \mathscr{M}\left(h_{k};z\right) are absolutely convergent in the domain D_{{jk}} specified in Table 2.5.2, and these domains are nonempty as a consequence of (2.5.19) and (2.5.20).

2.5.2. Domains of analyticity.
Transform Pair Domain D_{{jk}}
\mathscr{M}\left(f_{1};1-z\right),\;\mathscr{M}\left(h_{1};z\right) -c<\realpart{z}<1+\realpart{\alpha _{0}}
\mathscr{M}\left(f_{1};1-z\right),\;\mathscr{M}\left(h_{2};z\right) \realpart{z}<\min(1+\realpart{\alpha _{0}},\realpart{\beta _{0}})
\mathscr{M}\left(f_{2};1-z\right),\;\mathscr{M}\left(h_{1};z\right) \max(-c,1-b)<\realpart{z}
\mathscr{M}\left(f_{2};1-z\right),\;\mathscr{M}\left(h_{2};z\right) 1-b<\realpart{z}<\realpart{\beta _{0}}
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Symbols:
h(x): locally integrable function, f_{j}(t): truncated functions, D_{{jk}}: domain, b: right endpoint and c: point
Referenced by:
§2.5(ii), §2.5(ii)
Permalink:
http://dlmf.nist.gov/2.5.T2

For simplicity, write

2.5.32 G_{{jk}}(z)=\mathscr{M}\left(f_{j};1-z\right)\mathscr{M}\left(h_{k};z\right).
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Defines:
G_{{jk}}(z): function
Symbols:
h(x): locally integrable function and f_{j}(t): truncated functions
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From Table 2.5.2, we see that each G_{{jk}}(z) is analytic in the domain D_{{jk}}. Furthermore, each G_{{jk}}(z) has an analytic or meromorphic extension to a half-plane containing D_{{jk}}. Now suppose that there is a real number p_{{jk}} in D_{{jk}} such that the Parseval formula (2.5.5) applies and

2.5.33 I_{{jk}}(x)=\frac{1}{2\pi i}\int _{{p_{{jk}}-i\infty}}^{{p_{{jk}}+i\infty}}x^{{-z}}G_{{jk}}(z)dz.
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Defines:
G_{{jk}}(z): function and p_{{jk}}: real number
Symbols:
I(x): convolution integral
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Encodings:
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If, in addition, there exists a number q_{{jk}}>p_{{jk}} such that

2.5.34 \sup _{{p_{{jk}}\leq x\leq q_{{jk}}}}\left|G_{{jk}}(x+iy)\right|\to 0, y\to\pm\infty,
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Defines:
G_{{jk}}(z): function, p_{{jk}}: real number and q_{{jk}}>p_{{jk}}: real number
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then

2.5.35 I_{{jk}}(x)=\sum _{{p_{{jk}}<\realpart{z}<q_{{jk}}}}\Residue\left[-x^{{-z}}G_{{jk}}(z)\right]+E_{{jk}}(x),
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Defines:
G_{{jk}}(z): function, p_{{jk}}: real number, q_{{jk}}>p_{{jk}}: real number and E_{{jk}}(x): function
Symbols:
I(x): convolution integral
Permalink:
http://dlmf.nist.gov/2.5.E35
Encodings:
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where

2.5.36 E_{{jk}}(x)=\frac{1}{2\pi i}\int _{{q_{{jk}}-i\infty}}^{{q_{{jk}}+i\infty}}x^{{-z}}G_{{jk}}(z)dz=o\!\left(x^{{-q_{{jk}}}}\right)
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Defines:
G_{{jk}}(z): function, q_{{jk}}>p_{{jk}}: real number and E_{{jk}}(x): function
Symbols:
o\!\left(x\right): order symbol
Permalink:
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as x\to+\infty. (The last order estimate follows from the Riemann-Lebesgue lemma, §Ch.1.) The asymptotic expansion of I(x) is then obtained from (2.5.29).

For further discussion of this method and examples, see Wong (1989, Chapter 3), Paris and Kaminski (2001, Chapter 5), and Bleistein and Handelsman (1975, Chapters 4 and 6). The first reference also contains explicit expressions for the error terms, as do Soni (1980) and Carlson and Gustafson (1985).

The Mellin transform method can also be extended to derive asymptotic expansions of multidimensional integrals having algebraic or logarithmic singularities, or both; see Wong (1989, Chapter 3), Paris and Kaminski (2001, Chapter 7), and McClure and Wong (1987). See also Brüning (1984) for a different approach.

§ 2.5(iii). Laplace Transforms with Small Parameters

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Notes:
See Wong (1989, pp. 167–171).
Keywords:
Laplace transforms
Permalink:
http://dlmf.nist.gov/2.5.SS3

Let h(t) satisfy (2.5.18) and (2.5.20) with c>-1, and consider the Laplace transform

2.5.37 \mathscr{L}\left(h;\zeta\right)=\int _{{0}}^{{\infty}}h(t)e^{{-\zeta t}}dt.
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Symbols:
h(x): locally integrable function
Permalink:
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Encodings:
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Put x=1/\zeta and break the integration range at t=1, as in (2.5.23) and (2.5.24). Then

2.5.38 \zeta\mathscr{L}\left(h;\zeta\right)=I_{1}(x)+I_{2}(x),
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Defines:
I_{j}(x): integral
Symbols:
h(x): locally integrable function
Referenced by:
§2.5(iii)
Permalink:
http://dlmf.nist.gov/2.5.E38
Encodings:
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where

2.5.39 I_{j}(x)=\int _{{0}}^{{\infty}}e^{{-t}}h_{j}(xt)dt, j=1,2.
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Defines:
I_{j}(x): integral
Symbols:
h(x): locally integrable function
Permalink:
http://dlmf.nist.gov/2.5.E39
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Since \mathscr{M}\left(e^{{-t}};z\right)=\Gamma\!\left(z\right), by the Parseval formula (2.5.5), there are real numbers p_{1} and p_{2} such that -c<p_{1}<1, p_{2}<\min(1,\realpart{\beta _{0}}), and

2.5.40 I_{j}(x)=\frac{1}{2\pi i}\int _{{p_{j}-i\infty}}^{{p_{j}+i\infty}}x^{{-z}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h_{j};z\right)dz, j=1,2.
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Defines:
I_{j}(x): integral and p_{j}: real numbers
Symbols:
\Gamma\!\left(z\right): Gamma function and h(x): locally integrable function
Permalink:
http://dlmf.nist.gov/2.5.E40
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Since \mathscr{M}\left(h;z\right) is analytic for \realpart{z}>-c, by (2.5.14),

2.5.41 I_{1}(x)=\mathscr{M}\left(h_{1};1\right)x^{{-1}}+\frac{1}{2\pi i}\int _{{\rho-i\infty}}^{{\rho+i\infty}}x^{{-z}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h_{1};z\right)dz,
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Defines:
I_{j}(x): integral and \rho: parameter
Symbols:
\Gamma\!\left(z\right): Gamma function and h(x): locally integrable function
Referenced by:
§2.5(iii)
Permalink:
http://dlmf.nist.gov/2.5.E41
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for any \rho satisfying 1<\rho<2. Similarly, since \mathscr{M}\left(h_{2};z\right) can be continued analytically to a meromorphic function (when \kappa=0) or to an entire function (when \kappa\neq 0), we can choose \rho so that \mathscr{M}\left(h_{2};z\right) has no poles in 1<\realpart{z}\leq\rho<2. Thus

2.5.42 I_{2}(x)=\sum _{{\realpart{\beta _{0}}\leq\realpart{z}\leq 1}}\Residue\left[-x^{{-z}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h_{2};z\right)\right]+\frac{1}{2\pi i}\int _{{\rho-i\infty}}^{{\rho+i\infty}}x^{{-z}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h_{2};z\right)dz.
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Defines:
I_{j}(x): integral and \rho: parameter
Symbols:
\Gamma\!\left(z\right): Gamma function and h(x): locally integrable function
Referenced by:
§2.5(iii)
Permalink:
http://dlmf.nist.gov/2.5.E42
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On substituting (2.5.41) and (2.5.42) into (2.5.38), we obtain

2.5.43 \mathscr{L}\left(h;\zeta\right)=\mathscr{M}\left(h_{1};1\right)+\sum _{{\realpart{\beta _{0}}\leq\realpart{z}\leq 1}}\Residue\left[-\zeta^{{z-1}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h_{2};z\right)\right]+\sum\limits _{{1<\realpart{z}<l}}\Residue\left[-\zeta^{{z-1}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h;z\right)\right]+\frac{1}{2\pi i}\int _{{l-\delta-i\infty}}^{{l-\delta+i\infty}}\zeta^{{z-1}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h;z\right)dz,
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Defines:
\delta: arbitrary small positive constant
Symbols:
\Gamma\!\left(z\right): Gamma function and h(x): locally integrable function
Referenced by:
§2.5(iii), §2.5(iii)
Permalink:
http://dlmf.nist.gov/2.5.E43
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where l (\ge 2) is an arbitrary integer and \delta is an arbitrary small positive constant. The last term is clearly O\!\left(\zeta^{{l-\delta-1}}\right) as \zeta\to 0+.

If \kappa=0 in (2.5.18) and c>-1 in (2.5.20), and if none of the exponents in (2.5.18) are positive integers, then the expansion (2.5.43) gives the following useful result:

2.5.44 \mathscr{L}\left(h;\zeta\right)\sim\sum _{{n=0}}^{{\infty}}b_{n}\Gamma\!\left(1-\beta _{n}\right)\zeta^{{\beta _{n}-1}}+\sum\limits _{{n=0}}^{{\infty}}\frac{(-\zeta)^{n}}{n!}\mathscr{M}\left(h;n+1\right), \zeta\to 0+.
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Symbols:
\Gamma\!\left(z\right): Gamma function, \sim: asymptotically equal, h(x): locally integrable function and b: right endpoint
Permalink:
http://dlmf.nist.gov/2.5.E44
Encodings:
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¶ Example

2.5.45 \mathscr{L}\left(h;\zeta\right)=\int _{{0}}^{{\infty}}\frac{e^{{-\zeta t}}}{1+t}dt, \realpart{\zeta}>0.
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Symbols:
h(x): locally integrable function
Permalink:
http://dlmf.nist.gov/2.5.E45
Encodings:
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With h(t)=1/(1+t), we have \mathscr{M}\left(h;z\right)=\pi\csc\!\left(\pi z\right) for 0<\realpart{z}<1. In the notation of (2.5.18) and (2.5.20), \kappa=0, \beta _{s}=s+1, and c=0. Straightforward calculation gives

2.5.46 \Residue _{{z=k}}\left[-\zeta^{{z-1}}\Gamma\!\left(1-z\right)\pi\csc\!\left(\pi z\right)\right]=\left(-\ln\zeta+\psi\!\left(k\right)\right)\dfrac{\zeta^{{k-1}}}{(k-1)!},
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Symbols:
\Gamma\!\left(z\right): Gamma function and \psi\!\left(z\right): Psi or digamma function
Permalink:
http://dlmf.nist.gov/2.5.E46
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where \psi\!\left(z\right)={{\Gamma}^{{\prime}}}\!\left(z\right)/\Gamma\!\left(z\right). From (2.5.28)

2.5.47 \Residue _{{z=1}}\left[-\zeta^{{z-1}}\Gamma\!\left(1-z\right)\mathscr{M}\left(h_{2};z\right)\right]=\left(-\ln\zeta-\EulerConstant\right)-\mathscr{M}\left(h_{1};1\right),
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Symbols:
\Gamma\!\left(z\right): Gamma function, \EulerConstant: Euler's constant and h(x): locally integrable function
Permalink:
http://dlmf.nist.gov/2.5.E47
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where \EulerConstant is Euler's constant (§5.2(ii)). Insertion of these results into (2.5.43) yields

2.5.48 \mathscr{L}\left(h;\zeta\right)\sim(-\ln\zeta)\sum _{{k=0}}^{{\infty}}\frac{\zeta^{k}}{k!}+\sum _{{k=0}}^{{\infty}}\psi\!\left(k+1\right)\frac{\zeta^{k}}{k!}, \zeta\to 0+.
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Symbols:
\psi\!\left(z\right): Psi or digamma function, \sim: asymptotically equal and h(x): locally integrable function
Referenced by:
§2.5(iii)
Permalink:
http://dlmf.nist.gov/2.5.E48
Encodings:
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To verify (2.5.48) we may use

2.5.49 \mathscr{L}\left(h;\zeta\right)=e^{\zeta}E_{1}\!\left(\zeta\right);
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Symbols:
h(x): locally integrable function
Permalink:
http://dlmf.nist.gov/2.5.E49
Encodings:
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compare (5.4.14) and (6.6.?).

For examples in which the integral defining the Mellin transform \mathscr{M}\left(h;z\right) does not exist for any value of z, see Wong (1989, Chapter 3), Bleistein and Handelsman (1975, Chapter 4), and Handelsman and Lew (1970).