We give a theory of asymptotic expansions of thick distributions of rapid decay at infinity. We show that the moment asymptotic expansion of standard distributions of rapid decay follows by projection of our result. We also study in which spaces of thick test functions the asymptotic Taylor approximation is valid.
We employ our formulas to obtain the asymptotic expansion of several multidimensional integrals that are divergent but are regularized by using the Hadamard method.
The theory of asymptotic expansions of generalized functions was probably initiated by the work of Łojasiewicz [28], and has been studied by several authors in the recent years; see [14,31,32,38] and the references therein. These studies have provided a deep understanding of the local properties of distributions and of their behavior at infinity and have helped us to understand many aspects of Tauberian theory; applications in several areas, particularly in number theory, geometry, and mathematical physics have been developed.
The aim of this article is to present a theory of the asymptotic expansion of thick distributions, a new class of distributions introduced in one variable in [11] and in several variables by us [41]. Thick distributions help us to solve several puzzles, apparent paradoxes in the applications of distribution theory in quantum field theory [5], in engineering [29,37], and in the understanding of singularities in mathematical physics as considered in [4] or in [6]. We consider spaces with one thick point in this article, but it is possible to consider spaces with a finite number of such singular points, or even spaces with a countable number of thick points [43]. Thick distributions are the distributional theory corresponding to the theory of finite part regularizations given by Blanchet and Faye [2], who develop such a scheme in the context of finite parts, pseudofunctions and Hadamard regularization, subjects considered earlier by Sellier [33,34]; their analysis is aimed at the study of the dynamics of point particles in high post-Newtonian approximations of general relativity [3]. Thick distributions also appear in problems that seem well understood: The textbook formula for the second order distributional derivatives of in , was given by Frahm [16]; recently, Franklin [17] gave an alternative formula for certain singular functions,1
It is not clear to which singular test functions the formula of [17] applies.
while we gave the correct generalization that applies in the space of thick distributions [42].
The main result in the approach of [14] is the moment asymptotic expansion, that says that if g is a distribution defined in the whole that decays very fast at infinity2
Technically rapid decay means .
then has the asymptotic expansion
where the constants are the moments of g, .
It should be remarked that if is any sequence indexed by multi-indices, it is possible to consider a corresponding infinite series of Dirac delta functions, ,
Such series of deltas have a long story, starting with the study of orthogonal polynomials [22–24], the solution of differential equations [27,35,39], the asymptotics of such solutions [18], and the boundary layer theory [13], to name a few topics; see especially [8] and [14, Chapter 7]. However, it is important to observe that unless only a finite number of the are different from zero, the series is divergent in any space of distributions, as follows immediately from Borel’s theorem [14, Theorem 1.5.2]; actually one even can construct series of deltas that diverge as hyperfunctions [14, Chapter 7]. Therefore, if g is a distribution, whose moments all exist, one can consider the series of deltas , but this series will not converge, to g or to any other distribution, if the series is infinite. On the other hand, the question of convergence is irrelevant when the extra parameter λ is introduced and the series is considered as an asymptotic series, since only finite sums are needed to understand asymptotic series; interestingly, it is sometimes possible to write certain functions and distributions as finite sums of delta functions plus a remainder term [7].
In this article we prove that thick distributions f that show rapid decay at infinity, in the sense that , satisfy a generalized moment expansion, namely,
where the are the moment functions of f, and where the are thick delta functions as defined in Definition 2.4. Notice that, in general, the formal series of thick delta functions is divergent in .
The plan of the article is as follows. In Section 2 we define the standard thick test functions, , and distributions, . Other spaces of thick distributions, corresponding to the spaces , , and especially , are defined in Section 3. We then study asymptotic Taylor series of thick test functions in Section 4, and this allows us to prove the generalized expansion (1.3) in Section 5; we also show how the ordinary moment asymptotic expansion follows by projection. Section 6 provides some formulas arising in finite part integrals that are needed in Section 7, where we give several illustrations of the generalized moment expansion (1.3).
The spaces and
Let us recall the construction of the space of thick test functions and its dual, , the space of thick distributions [41]. Let a be a fixed point of .
Let denote the vector space of all smooth functions ϕ defined in , with support of the form , where K is compact in , that admit a strong asymptotic expansion of the form
where m is an integer (positive or negative), and where the are smooth functions of w, that is, . The subspace consists of those test functions ϕ whose expansion (2.1) begins at m. For a fixed compact K whose interior contains a, is the subspace formed by those test functions of that vanish in .
The asymptotic development of as has to be “strong”. This means [14, Chapter 1] that for any differentiation operator , , the asymptotic development of as exists and is equal to the term-by-term differentiation of . Observe that saying that the expansion exists as is the same as saying that it exists as , uniformly with respect to w.
We call the space of standard test functions on with a thick point located at . We denote as . The topology of this space is constructed as follows.
Let m be a fixed integer and K a compact subset of whose interior contains a. The topology of is given by the seminorms defined as
where and3
Formulas for the coefficients can be found in [41].
. The topology of is the inductive limit topology of the as . The topology of is the inductive limit topology of the as .
A sequence in converges to ψ if and only there exists , an integer m, and a compact set K with a in its interior, such that for and as if . Notice that if converges to ψ in then and the corresponding derivatives converge uniformly to ψ and its derivatives in any set of the form , where B is a ball with center at a; in fact, converges uniformly to over all . Furthermore, if are the coefficients of the expansion of and are those for ψ, then in the space for each .
We can now consider standard distributions in a space with one thick point, the standard thick distributions.
The space of distributions on with a thick point at is the dual space of . We denote it , or just as when .
Observe that , the space of standard test functions, is a closed subspace of ; we denote by
the projection operator, dual of the inclusion .
Let
be the surface area of the unit sphere of .
Let be a distribution in . The thick delta function of degree q, denoted as , or as , acts on a thick test function as
where , as .
Thick deltas of order 0 are called just thick deltas, and we shall use the notation instead of . If is an arbitrary sequence of distributions of , then the series converges in , and such series are the most general thick distributions whose support is the set .
Other spaces of thick distributions
Let be a space of test functions in and let be the corresponding space of distributions.4
In the sense of Zemanian [44]; we assume that densely and continuously and that differentiation is a continuous map of .
Our aim in this section is to construct the corresponding spaces of thick test functions and distributions, and .
Our construction will apply in multiple cases. For instance, can be , the space of all smooth functions and thus becomes , the space of distributions with compact support; or can be , so that becomes the space of tempered distributions . In this study the case of and plays a central role. Other possibilities include the spaces , , or . We shall recall the properties of these spaces when needed, but more details can be found in the textbooks [14,20,21,36].
Let be a space of test functions in . The space consists of those functions ϕ defined in that can be written as , where and where . The topology of is the final topology induced by the map , . The space of thick distributions is the corresponding dual space.
Similarly one can consider the spaces for any integer m; the space is the inductive limit of the as .
The topology of can actually be described in several ways. Suppose for instance that is a test function that satisfies that in a neighborhood of . If is a continuous seminorm of while is a continuous seminorm of , then5
Technically does not belong to since it is not defined at but naturally one can extend the domain of by asking that ; we shall not mention such clear situations any more.
is a continuous seminorm of and the collection of seminorms so constructed form a basis for the continuous seminorms of . We shall consider alternative constructions of basis of seminorms for various spaces below.
The elements of can be described as those smooth functions defined in that show the behavior of thick test functions near while at infinity show the behavior of the elements of . Similar considerations apply to the dual spaces.
The spaces and
The space is the space of multipliers of [41]. Its elements are smooth functions defined in that behave like elements of near but without any restriction at infinity. No topology for the space was considered in [41]; with the topology given in the Definition 3.1 then the dual space is the subspace of formed by those thick distributions whose support, a subset of , is of the form where K is compact. For a fixed m the family of seminorms defined in (2.2), for , and K a compact set of that contains a, form a basis of seminorms for the topology of .
The spaces and
Let us employ the notation
The spaces and play a rather important role in the theory of asymptotic expansions of distributions [14]. The space is the inductive limit of the spaces as , where is the space of all smooth functions in that satisfy
for all multi-indices ; the topology of is defined by the family of seminorms
We can construct a family of seminorms of as follows; the general case of is then obtained by a change of variables. If , put
where
The spaces and
The family of seminorms
where is given by (3.6) and where
defines the topology of the space .
Taylor series in spaces of test functions
If ϕ is a smooth function in then we can consider its Taylor series
Naturally does not have to converge for any and even if convergent it may not converge to . However, is an asymptotic series6
Asymptotic series do not have to be divergent, but many such series used in applied problems are [14, Chapter 1].
as :
for any .
Similarly, if ϕ is a thick test function of a space then the series
provides an asymptotic approximation of as , and, likewise, the series is usually divergent or if convergent it does not have to converge to .
If then, in general, the Taylor series cannot provide an asymptotic series in the topology of since actually, in many cases, the individual terms, the monomials , do not even belong to ; consider the spaces or , for instance. It follows from the results of [9] (see [14, Chapter 6]) that in the space the series gives an asymptotic expansion of as , and actually is the smallest space of test functions with this property. Our aim is to show that a similar result holds for thick test functions of the space , but before we do so we would like to give an example.
Let be the space of polynomials in n variables, with the LF topology as an inductive limit of finite dimensional spaces [36]. Consider the space of test functions , with the direct sum topology. Then the series makes sense as a formal series in since belongs to for any M. However, in general, does not give an asymptotic expansion of as (just take ϕ as any non-zero element of ).
Our aim is to prove an asymptotic Taylor formula in the space . In order to do so we first need an auxiliary result.
Let. Suppose that. Then for each continuous seminormofthere exists a constant M such that
Indeed, it is enough to prove the result for the norms defined in (3.5).
In fact, observe that if then for each multi-index p there exists a constant such that
Hence if ,
for some constant . □
We therefore obtain the ensuing Taylor formula.
Letwith expansion, as. Thenin the topology of the space.
The proof of the theorem follows from the Lemma 4.2 by observing that if and , then belongs to . □
It is worth pointing out that we can express the result of the theorem by saying that if then
as in the topology of . Naturally the asymptotic character of the series is as since the terms vanish if for some m.
The moment asymptotic expansion
If the distribution f belongs to then its moments are the numbers
for . For thick distributions we employ the following definition.
Let . Then its moments are the distributions defined as
for .
Observe that if is a thick distribution and is the usual distribution obtained by projection, then the moments of g are related to the moment functions of f by the formula
where .
Any distribution of satisfies the moment asymptotic expansion [14]. We now prove that the thick distributions of also satisfy a generalized moment asymptotic expansion.
Let, with moment functions, thenwhere, given by (2.4), is the surface area of the unit sphere. This means that, for some m.
We shall prove that (5.4) holds in the strong topology of , but to do so it is enough to show that it holds in the weak sense, since weak and strong convergence of sequences are equivalent in spaces of distributions [20]. Thus, we need to show that if , say , with expansion , as , then for each N,
where
However, is given as
where
belongs to , and thus (5.6) follows from the Lemma 4.2. □
It is interesting to observe that the standard moment asymptotic expansion in the space can be obtained by applying the projection operator (2.3) to the generalized expansion (5.4). Indeed, it was shown in [41] that if , while if then
Thus, using (5.3) we obtain the following corollary [14, Theorem 4.3.1].
If, with moments, then
Expansion of radial distributions
The moment asymptotic expansion takes a rather simple form when applied to radial thick distributions, as we now explain. A radial distribution is one that is invariant with respect to rotations; if is radial then , where has support in , but is not unique [10].
Letbe radial,, wherehas support in. Then the moment functions of f,are constants, given bywhere.
Indeed, if then is given as
as required. □
If we employ the Theorem 5.2 we obtain the ensuing asymptotic expansion of radial thick distributions.
Ifis radial, thenwhere the constantsare given in the Lemma5.4.
Let us now apply the projection operator , and recall [41] that unless , while
where is the kth power of the Laplacian. We thus obtain the following form of the moment asymptotic expansion.
Letbe radial,,with support in. Letbe the moments of. Thenwhere
Finite parts and pseudofunctions
In order to give illustrations of our formulas, we need to consider several important properties of Hadamard finite part integrals and of the associated pseudofunctions.
Let us recall the notion of the finite part of a limit [14, Section 2.4]. Let be a function defined for that satisfies . Suppose , the basic functions, is a family of strictly positive functions defined in the same interval such that all of them tend to infinity at 0 and such that given two different elements then is either 0 or ∞. Then the finite part of the limit of as with respect to exists and equals A if we can write , where , the infinite part, is a linear combination of the basic functions and where , the finite part, has the property that the limit exists; such a decomposition is unique if it exists since any finite number of elements of has to be linearly independent. We then employ the notation
In the standard Hadamard finite part limit one takes as the family of functions , where and or where and and uses the simpler notation .
Consider now a function f defined in that is probably not integrable over the whole space but which is integrable in the region for any . Then the radial7
Other, non-radial finite part integrals can be considered, of course, but the results would be different, in general [40].
finite part integral is defined as
if the finite part limit exists.
If g is a locally integrable function in such that the radial finite part integral of exists for each ϕ belonging to a space of thick test functions , then we can define a thick8
The same notation is employed for standard distributions.
distribution as
The distribution is sometimes called a pseudofunction. One may usually employ the notation when the variable of the pseudofunction is important, but when considering the transformation properties of the association it is convenient to employ the more detailed notation . Indeed, since g and are not exactly the same object, then applying an operation to g does not give the same result as applying the same operation to ; in particular, as we shall presently see, if , then and are related, but do not coincide, in general.
The transformation formulas for dilatations of were given in [41], namely, for any , but for only, while if then
where C is given in (2.4). If we take and evaluate this formula at we obtain the ensuing result.9
Clearly, formula (6.5) will hold under much weaker conditions on ϕ.
We can consider (6.6) as a transformation formula for the pseudofunction .
If, with, as, andthen
Indeed,
while
and thus (6.7) follows from (6.6) by taking . □
Computation of finite part integrals
We shall now compute some finite part integrals whose results are available in the literature [14,30], but for which the computation of the results does not seem generally known.
Suppose, to fix the ideas, that one needs to compute
the Hadamard finite part of the (probably) divergent integral, where and where . The definition [14, Section 2.4] requires that we decompose , , as a sum of its infinite and finite parts, and while doing this is many times possible, it is sometimes easier to proceed in a different way, as we now explain.
Indeed, let
The function is analytic in its semiplane of definition and it is well known that it admits an analytic continuation to the region ; this continuation is unique and we denote it as F. The singularities at , are simple poles, with residues
Observe now that any analytic function defined in a punctured disc , with an isolated singularity at has a well defined regular part, – the sum of the terms with positive powers in its Laurent series – which has a removable singularity at ω; the value is the regularized value of W at . Actually is the finite part of the limit of as if the singularity is a pole (but not if it is an essential singularity). For our function F this gives values for . We then obtain,
Alternatively [14, Section 2.4], we can say that , the regular distribution of λ for , defined by the integral , admits an analytic continuation to , also denoted as , and given as . The parametrically analytic distribution has simple poles at the negative integers, with residues . The regularized values10
These regularizations are called Riesz regularizations in [30].
are well defined distributions of . The distributions defined for any as
that is, as , can also be computed as [12]
Interestingly, this approach can also be employed for radial finite part integrals in several variables [12], however, it does not work at the singularities for other shapes [40], not even for principal value integrals, a result that has important implications in the numerical solutions of integral equations [15], and in other calculations in Mathematical Physics [19].
We are particularly interested in the finite part integrals
for any . In this case, with the above notation, we have that , where Γ is the well known gamma function [25, Chapter 1]. We immediately obtain from (6.12) that whenever .
Let us now compute the values for . Observe first that (6.11) yields that the residue of the gamma function at equals . Thus, the functional equation gives
Euler’s constant, or in other words,
In fact, since
where is the digamma function, the logarithmic derivative of the gamma function [25], so that [14, Example 60]
The proof of (6.19) is by induction. Indeed, (6.18) says that it is true for , while if we assume that it is true for k then we obtain that equals
Hence, for ,
Illustrations
We shall now give several illustrations of our formulas.
Let be the delta function on the unit sphere of , that is, . Observe that equals
so that
Denote by the sphere of center and radius t. Then, , so that the generalized moment asymptotic expansion yields
in the space .
The projection is the distribution , with the obvious abuse of notation, and thus in the space ,
where , in agreement with [14, Example 94].
Evaluation of (7.3) at a test function yields the well known Pizzetti’s formula [1,26],
as . Therefore, (7.3) can be called the distributional form of Pizzetti’s formula, while (7.2) becomes the thick distributional form of Pizzetti’s formula.
If is a radial distribution of , with constant moment functions , and , then belongs to and the expansion of as follows from (5.12) as
In particular, if , then , for all k, and so
or, equivalently,
The distribution does not belong to for any , and thus does not satisfy the moment asymptotic expansion, as (6.4) shows. However, if , where H is the Heaviside function, then . Using the Lemma 5.4, it follows that the moment functions are constant functions, given as , if , whereas if then , if , while . Thus, as ,
It follows that if , , then as ,
if . If , then (6.6) and (6.7) yield
Let us now consider the asymptotic expansion of the integral
where , . The result is a generalized form of Watson’s lemma, used in the approximation of Laplace integrals [14, Example 58].
Notice that , and while this is not a moment expansion, we can use the Proposition 6.4 with to write
and observe that can be computed from the moment asymptotic expansion,
where we employ (5.12) and (6.21). Thus,
Naturally the expansion of also follows from the analysis of the previous example.
Footnotes
Acknowledgements
The authors gratefully acknowledge support from NSF, through grant number 0968448.
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