2 Asymptotic ApproximationsAreas

§2.6 Distributional Methods

Contents
  1. §2.6(i) Divergent Integrals
  2. §2.6(ii) Stieltjes Transform
  3. §2.6(iii) Fractional Integrals
  4. §2.6(iv) Regularization

§2.6(i) Divergent Integrals

Consider the integral

2.6.1 S⁡(x)=∫0∞1(1+t)1/3⁢(x+t)⁢dt,

where x>0. For t>1,

2.6.2 (1+t)−1/3=∑s=0∞(−13s)⁢t−s−(1/3).

Motivated by Watson’s lemma (§2.3(ii)), we substitute (2.6.2) in (2.6.1), and integrate term by term. This leads to integrals of the form

2.6.3 ∫0∞t−s−(1/3)x+t⁢dt,
s=1,2,3,….

Although divergent, these integrals may be interpreted in a generalized sense. For instance, we have

2.6.4 ∫0∞tα−1(x+t)α+β⁢dt=Γ⁡(α)⁢Γ⁡(β)Γ⁡(α+β)⁢1xβ,
ℜ⁡α>0, ℜ⁡β>0.

But the right-hand side is meaningful for all values of α and β, other than nonpositive integers. We may therefore define the integral on the left-hand side of (2.6.4) by the value on the right-hand side, except when α,β=0,−1,−2,…. With this interpretation

2.6.5 ∫0∞t−s−(1/3)x+t⁢dt=2⁢π3⁢(−1)sxs+(1/3),
s=0,1,2,….

Inserting (2.6.2) into (2.6.1) and integrating formally term-by-term, we obtain

2.6.6 S⁡(x)∼2⁢π3⁢∑s=0∞(−1)s⁢(−13s)⁢x−s−(1/3),
x→∞.

However this result is incorrect. The correct result is given by

2.6.7 S⁡(x)∼2⁢π3⁢∑s=0∞(−1)s⁢(−13s)⁢x−s−(1/3)−∑s=1∞3s⁢(s−1)!2⋅5⁢⋯⁢(3⁢s−1)⁢x−s;

see §2.6(ii).

The fact that expansion (2.6.6) misses all the terms in the second series in (2.6.7) raises the question: what went wrong with our process of reaching (2.6.6)? In the following subsections, we use some elementary facts of distribution theory (§1.16) to study the proper use of divergent integrals. An important asset of the distribution method is that it gives explicit expressions for the remainder terms associated with the resulting asymptotic expansions.

For an introduction to distribution theory, see Wong (1989, Chapter 5). For more advanced discussions, see Gel’fand and Shilov (1964) and Rudin (1973).

§2.6(ii) Stieltjes Transform

Let f⁡(t) be locally integrable on [0,∞). The Stieltjes transform of f⁡(t) is defined by

2.6.8 𝒮⁡f⁡(z)=∫0∞f⁡(t)t+z⁢dt.

To derive an asymptotic expansion of 𝒮⁡f⁡(z) for large values of |z|, with |ph⁡z|<π, we assume that f⁡(t) possesses an asymptotic expansion of the form

2.6.9 f⁡(t)∼∑s=0∞as⁢t−s−α,
t→+∞,

with 0<α≤1. For each n=1,2,3,…, set

2.6.10 f⁡(t)=∑s=0n−1as⁢t−s−α+fn⁡(t).

To each function in this equation, we shall assign a tempered distribution (i.e., a continuous linear functional) on the space 𝒯 of rapidly decreasing functions on ℝ. Since f⁡(t) is locally integrable on [0,∞), it defines a distribution by

2.6.11 ⟨f,ϕ⟩=∫0∞f⁡(t)⁢ϕ⁡(t)⁢dt,
ϕ∈𝒯.

In particular,

2.6.12 ⟨t−α,ϕ⟩=∫0∞t−α⁢ϕ⁡(t)⁢dt,
ϕ∈𝒯,

when 0<α<1. Since the functions t−s−α, s=1,2,…, are not locally integrable on [0,∞), we cannot assign distributions to them in a similar manner. However, they are multiples of the derivatives of t−α. Motivated by the definition of distributional derivatives, we can assign them the distributions defined by

2.6.13 ⟨t−s−α,ϕ⟩=1(α)s⁢∫0∞t−α⁢ϕ(s)⁡(t)⁢dt,
ϕ∈𝒯,

where (α)s=α⁢(α+1)⁢⋯⁢(α+s−1). Similarly, in the case α=1, we define

2.6.14 ⟨t−s−1,ϕ⟩=−1s!⁢∫0∞(ln⁡t)⁢ϕ(s+1)⁡(t)⁢dt,
ϕ∈𝒯.

To assign a distribution to the function fn⁡(t), we first let fn,n⁡(t) denote the nth repeated integral (§1.4(v)) of fn:

2.6.15 fn,n⁡(t)=(−1)n(n−1)!⁢∫t∞(τ−t)n−1⁢fn⁡(τ)⁢dτ.

For 0<α<1, it is easily seen that fn,n⁡(t) is bounded on [0,R] for any positive constant R, and is O⁡(t−α) as t→∞. For α=1, we have fn,n⁡(t)=O⁡(t−1) as t→∞ and fn,n⁡(t)=O⁡(ln⁡t) as t→0+. In either case, we define the distribution associated with fn⁡(t) by

2.6.16 ⟨fn,ϕ⟩=(−1)n⁢∫0∞fn,n⁡(t)⁢ϕ(n)⁡(t)⁢dt,
ϕ∈𝒯,

since the nth derivative of fn,n is fn.

We have now assigned a distribution to each function in (2.6.10). A natural question is: what is the exact relation between these distributions? The answer is provided by the identities (2.6.17) and (2.6.20) given below.

For 0<α<1 and n≥1, we have

2.6.17 ⟨f,ϕ⟩=∑s=0n−1as⁢⟨t−s−α,ϕ⟩−∑s=1ncs⁢⟨δ(s−1),ϕ⟩+⟨fn,ϕ⟩

for any ϕ∈𝒯, where

2.6.18 cs=(−1)s(s−1)!⁢ℳ⁡f⁡(s),

ℳ⁡f⁡(z) being the Mellin transform of f⁡(t) or its analytic continuation (§2.5(ii)). The Dirac delta distribution in (2.6.17) is given by

2.6.19 ⟨δ(s),ϕ⟩=(−1)s⁢ϕ(s)⁡(0),
s=0,1,2,…;

compare §1.16(iii).

For α=1

2.6.20 ⟨f,ϕ⟩=∑s=0n−1as⁢⟨t−s−1,ϕ⟩−∑s=1nds⁢⟨δ(s−1),ϕ⟩+⟨fn,ϕ⟩

for any ϕ∈𝒯, where

2.6.21 (−1)s+1⁢ds+1=ass!⁢∑k=1s1k+1s!⁢limz→s+1(ℳ⁡f⁡(z)+asz−s−1),

for s=0,1,2,….

To apply the results (2.6.17) and (2.6.20) to the Stieltjes transform (2.6.8), we take a specific function ϕ∈𝒯. Let ε be a positive number, and

2.6.22 ϕε⁡(t)=e−ε⁢tt+z,
t∈(0,∞).

From (2.6.13) and (2.6.14)

2.6.23 limε→0⟨t−s−α,ϕε⟩=πsin⁡(π⁢α)⁢(−1)szs+α,
2.6.24 limε→0⟨t−s−1,ϕε⟩=(−1)s+1zs+1⁢∑k=1s1k+(−1)szs+1⁢ln⁡z,

with s=0,1,2,…. From (2.6.11) and (2.6.16), we also have

2.6.25 limε→0⟨f,ϕε⟩=𝒮⁡f⁡(z),

On substituting (2.6.15) into (2.6.26) and interchanging the order of integration, the right-hand side of (2.6.26) becomes

(−1)nzn⁢∫0∞τn⁢fn⁡(τ)τ+z⁢dτ.

To summarize,

2.6.27 𝒮⁡f⁡(z)=πsin⁡(π⁢α)⁢∑s=0n−1(−1)s⁢aszs+α−∑s=1n(s−1)!⁢cszs+Rn⁡(z),

if α∈(0,1) in (2.6.9), or

2.6.28 𝒮⁡f⁡(z)=ln⁡z⁢∑s=0n−1(−1)s⁢aszs+1+∑s=0n−1(−1)s⁢d~szs+1+Rn⁡(z),

if α=1 in (2.6.9). Here cs is given by (2.6.18),

2.6.29 d~s=limz→s+1(ℳ⁡f⁡(z)+asz−s−1),

and

2.6.30 Rn⁡(z)=(−1)nzn⁢∫0∞τn⁢fn⁡(τ)τ+z⁢dτ.

The expansion (2.6.7) follows immediately from (2.6.27) with z=x and f⁡(t)=(1+t)−(1/3); its region of validity is |ph⁡x|≤π−δ (<π). The distribution method outlined here can be extended readily to functions f⁡(t) having an asymptotic expansion of the form

2.6.31 f⁡(t)∼ei⁢c⁢t⁢∑s=0∞as⁢t−s−α,
t→+∞,

where c (≠0) is real, and 0<α≤1. For a more detailed discussion of the derivation of asymptotic expansions of Stieltjes transforms by the distribution method, see McClure and Wong (1978) and Wong (1989, Chapter 6). Corresponding results for the generalized Stieltjes transform

2.6.32 ∫0∞f⁡(t)(t+z)ρ⁢dt,
ρ>0,

can be found in Wong (1979). An application has been given by López (2000) to derive asymptotic expansions of standard symmetric elliptic integrals, complete with error bounds; see §19.27(vi).

§2.6(iii) Fractional Integrals

The Riemann–Liouville fractional integral of order μ is defined by

2.6.33 𝐼μf⁡(x)=1Γ⁡(μ)⁢∫0x(x−t)μ−1⁢f⁡(t)⁢dt,
μ>0;

see §1.15(vi). We again assume f⁡(t) is locally integrable on [0,∞) and satisfies (2.6.9). We now derive an asymptotic expansion of 𝐼μf⁡(x) for large positive values of x.

In terms of the convolution product

2.6.34 (f∗g)⁢(x)=∫0xf⁡(x−t)⁢g⁡(t)⁢dt

of two locally integrable functions on [0,∞), (2.6.33) can be written

2.6.35 𝐼μf⁡(x)=1Γ⁡(μ)⁢(tμ−1∗f)⁢(x).

The replacement of f⁡(t) by its asymptotic expansion (2.6.9), followed by term-by-term integration leads to convolution integrals of the form

2.6.36 (tμ−1∗t−s−α)⁢(x)=∫0x(x−t)μ−1⁢t−s−α⁢dt,
s=0,1,2,….

Of course, except when s=0 and 0<α<1, none of these integrals exists in the usual sense. However, the left-hand side can be considered as the convolution of the two distributions associated with the functions tμ−1 and t−s−α, given by (2.6.12) and (2.6.13).

To define convolutions of distributions, we first introduce the space K+ of all distributions of the form 𝐷nf, where n is a nonnegative integer, f is a locally integrable function on ℝ which vanishes on (−∞,0], and 𝐷nf denotes the nth derivative of the distribution associated with f. For F=𝐷nf and G=𝐷mg in K+, we define

It is easily seen that K+ forms a commutative, associative linear algebra. Furthermore, K+ contains the distributions H, δ, and tλ, t>0, for any real (or complex) number λ, where H is the distribution associated with the Heaviside function H⁡(t) (§1.16(iv)), and tλ is the distribution defined by (2.6.12)–(2.6.14), depending on the value of λ. Since δ=𝐷H, it follows that for μ≠1,2,…,

2.6.38 tμ−1∗δ(s−1)=Γ⁡(μ)Γ⁡(μ+1−s)⁢tμ−s,
t>0.

Using (5.12.1), we can also show that when μ≠1,2,… and μ−α is not a nonnegative integer,

2.6.39 tμ−1∗t−s−α=Γ⁡(μ)⁢Γ⁡(1−s−α)Γ⁡(μ+1−s−α)⁢tμ−s−α,
t>0,

and

2.6.40 tμ−1∗t−s−1=(−1)sμ⋅s!⁢𝐷s+1(tμ⁢(ln⁡t−γ−ψ⁡(μ+1))),
t>0,

where γ is Euler’s constant (§5.2(ii)).

To derive the asymptotic expansion of 𝐼μf⁡(x), we recall equations (2.6.17) and (2.6.20). In the sense of distributions, they can be written

2.6.41 f=∑s=0n−1as⁢t−s−α−∑s=1ncs⁢δ(s−1)+fn,

and

2.6.42 f=∑s=0n−1as⁢t−s−1−∑s=1nds⁢δ(s−1)+fn.

Substituting into (2.6.35) and using (2.6.38)–(2.6.40), we obtain

2.6.43 tμ−1∗f=∑s=0n−1as⁢Γ⁡(μ)⁢Γ⁡(1−s−α)Γ⁡(μ+1−s−α)⁢tμ−s−α−∑s=1ncs⁢Γ⁡(μ)Γ⁡(μ−s+1)⁢tμ−s+tμ−1∗fn

when 0<α<1, or

2.6.44 tμ−1∗f=∑s=0n−1(−1)s⁢asμ⋅s!⁢𝐷s+1(tμ⁢(ln⁡t−γ−ψ⁡(μ+1)))−∑s=1nds⁢Γ⁡(μ)Γ⁡(μ−s+1)⁢tμ−s+tμ−1∗fn

when α=1. These equations again hold only in the sense of distributions. Since the function tμ⁢(ln⁡t−γ−ψ⁡(μ+1)) and all its derivatives are locally absolutely continuous in (0,∞), the distributional derivatives in the first sum in (2.6.44) can be replaced by the corresponding ordinary derivatives. Furthermore, since fn,n(n)⁡(t)=fn⁡(t), it follows from (2.6.37) that the remainder terms tμ−1∗fn in the last two equations can be associated with a locally integrable function in (0,∞). On replacing the distributions by their corresponding functions, (2.6.43) and (2.6.44) give

2.6.45 𝐼μf⁡(x)=∑s=0n−1as⁢Γ⁡(1−s−α)Γ⁡(μ+1−s−α)⁢xμ−s−α−∑s=1ncsΓ⁡(μ+1−s)⁢xμ−s+1xn⁢δn⁡(x),

when 0<α<1, or

2.6.46 𝐼μf⁡(x)=∑s=0n−1(−1)s⁢ass!⁢Γ⁡(μ+1)⁢ds+1dxs+1⁡(xμ⁢(ln⁡x−γ−ψ⁡(μ+1)))−∑s=1ndsΓ⁡(μ−s+1)⁢xμ−s+1xn⁢δn⁡(x),

when α=1, where

2.6.47 δn⁡(x)=∑j=0n(nj)⁢Γ⁡(μ+1)Γ⁡(μ+1−j)⁢𝐼μ(tn−j⁢fn,j)⁡(x),

fn,j⁡(t) being the jth repeated integral of fn; compare (2.6.15).

Example

Let f⁡(t)=t1−α/(1+t), 0<α<1. Then

2.6.48 𝐼μf⁡(x)=1Γ⁡(μ)⁢∫0x(x−t)μ−1⁢t1−α⁢(1+t)−1⁢dt,

where μ>0. For 0<t<∞

2.6.49 f⁡(t)=∑s=0n−1(−1)s⁢t−s−α+(−1)n⁢t1−n−α1+t.

In the notation of (2.6.10), as=(−1)s and

2.6.50 fn⁡(t)=(−1)n⁢t1−n−α1+t.

Since

2.6.51 ℳ⁡f⁡(s)=(−1)s⁢π/sin⁡(π⁢α),

from (2.6.45) it follows that

2.6.52 𝐼μf⁡(x)=∑s=0n−1(−1)s⁢Γ⁡(1−s−α)Γ⁡(μ+1−s−α)⁢xμ−s−α−πsin⁡(π⁢α)⁢∑s=1n1Γ⁡(μ+1−s)⁢xμ−s(s−1)!+1xn⁢δn⁡(x).

Moreover,

2.6.53 |δn⁡(x)|≤Γ⁡(μ+1)⁢Γ⁡(1−α)Γ⁡(μ+1−α)⁢Γ⁡(n+α)⁢∑j=0n(nj)⁢Γ⁡(n+α−j)|Γ⁡(μ+1−j)|⁢xμ−α

for x>0.

It may be noted that the integral (2.6.48) can be expressed in terms of the hypergeometric function F12⁡(1,2−α;2−α+μ;−x); see §15.2(i).

For proofs and other examples, see McClure and Wong (1979) and Wong (1989, Chapter 6). If both f and g in (2.6.34) have asymptotic expansions of the form (2.6.9), then the distribution method can also be used to derive an asymptotic expansion of the convolution f∗g; see Li and Wong (1994).

§2.6(iv) Regularization

The method of distributions can be further extended to derive asymptotic expansions for convolution integrals:

2.6.54 I⁡(x)=∫0∞f⁡(t)⁢h⁡(x⁢t)⁢dt.

We assume that for each n=1,2,3,…,

2.6.55 f⁡(t)=∑s=0n−1as⁢ts+α−1+fn⁡(t),

where 0<α≤1 and fn⁡(t)=O⁡(tn+α−1) as t→0+. Also,

2.6.56 h⁡(t)=∑s=0n−1bs⁢t−s−β+hn⁡(t),

where 0<β≤1, and hn⁡(t)=O⁡(t−n−β) as t→∞. Multiplication of these expansions leads to

2.6.57 f⁡(t)⁢h⁡(x⁢t)=∑j=0n−1∑k=0n−1aj⁢bk⁢tj+α−1−k−β⁢x−k−β+∑j=0n−1aj⁢tj+α−1⁢hn⁡(x⁢t)+∑k=0n−1bk⁢x−k−β⁢t−k−β⁢fn⁡(t)+fn⁡(t)⁢hn⁡(x⁢t).

On inserting this identity into (2.6.54), we immediately encounter divergent integrals of the form

2.6.58 ∫0∞tλ⁢dt,
λ∈ℝ.

However, in the theory of generalized functions (distributions), there is a method, known as “regularization”, by which these integrals can be interpreted in a meaningful manner. In this sense

2.6.59 ∫0∞tλ⁢dt=0,
λ∈ℂ.

From (2.6.55) and (2.6.59)

2.6.60 ℳ⁡f⁡(z)=ℳ⁡fn⁡(z),

where ℳ⁡f⁡(z) is the Mellin transform of f or its analytic continuation. Also, when α≠β,

2.6.61 ℳ⁡hx⁡(j+α)=x−j−α⁢ℳ⁡h⁡(j+α),

where hx⁡(t)=h⁡(x⁢t). Inserting (2.6.57) into (2.6.54), we obtain from (2.6.59)–(2.6.61)

2.6.62 I⁡(x)=∑j=0n−1aj⁢ℳ⁡h⁡(j+α)⁢x−j−α+∑k=0n−1bk⁢ℳ⁡f⁡(1−k−β)⁢x−k−β+δn⁡(x)

when α≠β, where

δn⁡(x)=∫0∞fn⁡(t)⁢hn⁡(x⁢t)⁢dt.

There is a similar expansion, involving logarithmic terms, when α=β. For rigorous derivations of these results and also order estimates for δn⁡(x), see Wong (1979) and Wong (1989, Chapter 6).