Beyond Dominated Convergence: Newer Methods of Integration
Patrick Muldowney

TL;DR
This paper explores advanced criteria for integral convergence beyond Lebesgue's dominated convergence theorem, addressing its limitations in modern analysis.
Contribution
It introduces new convergence criteria that extend the applicability of integral convergence theorems beyond traditional dominated convergence.
Findings
Deeper convergence criteria are formulated.
Limitations of Lebesgue's dominated convergence are addressed.
New methods improve understanding of integral convergence.
Abstract
Lebesgue's dominated convergence theorem is a crucial pillar of modern analysis, but there are certain areas of the subject where this theorem is deficient. Deeper criteria for convergence of integrals are described in this article.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Beyond Dominated Convergence:
Newer Methods of Integration
Pat Muldowney
Abstract
Lebesgue’s dominated convergence theorem is a crucial pillar of modern analysis, but there are certain areas of the subject where this theorem is deficient. Deeper criteria for convergence of integrals are described in this article.
1 What Is Integration?
We learn calculus in secondary school: first, differentiation of functions, and later integration as the inverse or opposite of differentiation—the integral is the anti-derivative or primitive function, from which definite integrals can be easily deduced.
In more advanced mathematics courses we learn Riemann’s definition of definite integrals which enables us to integrate more functions. The Riemann method does not make use of differentiation; it is similar to the ancient method of finding areas and volumes “by exhaustion”—that is, estimating the area or volume by dividing it up into pieces which are more easily estimated, and then taking the aggregate of the pieces.
Specialists in mathematical analysis go on from this to study the Lebesgue method of integration. Why? Again, one of the stock answers to this question is that the Lebesgue method enables us to integrate functions which cannot be integrated by more familiar methods such as the calculus integral and the Riemann integral.
The Dirichlet function is sometimes mentioned. In the unit interval this function takes value one at the rational points, and zero at the other points. The Dirichlet function is not the derivative of some other function, so it cannot be integrated by the method we learn at school in calculus lessons. Also, it cannot be integrated by Riemann’s method. But the Lebesgue integral of the Dirichlet function exists: the definite integral of the Dirichlet function on the unit interval is [math].
But—so what? Apart from some specialists and experts, is there anybody else who has any real use for the Dirichlet function, and who really cares whether or not it is amenable to calculus? It cannot be pictured as lines in a graph, it does not have a straightforward formulation in polynomial, trigonometric or exponential terms. Unlike the area and volume calculations of antiquity, and unlike the calculus of Newton and Leibnitz which explained the world in mechanical terms, what difference does the Dirichlet function make to anyone outside the narrow and rarified world of a tiny number of people in pure mathematics?
The same can be said of many of the other arcane and exotic functions, such as the Devil’s Staircase, invented during the long nineteenth century gestation of Lebesgue integration, measure theory and set theory. Such functions have counter-intuitive and challenging qualities that we can admire and wonder at. But they were described by Hermite and Poincaré as unwelcome monsters causing mayhem in the rich and fertile garden of mathematics.
“Does anyone believe that the difference between the Lebesgue and the Riemann integrals can have physical significance, and that whether, say, an airplane would or would not fly could depend on this difference? If such were claimed, I should not care to fly in that plane.” (Richard W. Hamming [5]).
This critique is understandable, but unhistorical. By the early nineteenth century, the rich and fertile garden was on the verge of becoming a barren and dangerous wilderness—and not because of trespassing monster-functions.
2 Monstrous Functions
In the tradition of Newton and Leibnitz, Fourier series representation of functions had opened up the analysis of wave motion, crucial to an understanding of sound, light, electricity and so on. But strange and paradoxical things could happen when the integral of a function was obtained by integrating its Fourier series term by term. Certain questions could no longer be avoided. To what extent, and under what conditions, is a function identical to its corresponding Fourier series representation? When is the integral of a function equal to the series obtained by integrating the terms of the corresponding Fourier series?
This boils down to whether a convergent series of integrable functions has integrable limit, and whether the integral of the limit is equal to the limit of the integrals whenever the latter limit exists.
Such issues motivated decades of investigation of the notion of integration, until a satisfactory resolution was found in the convergence theorems—uniform, monotone, and dominated convergence—of Lesbesgue integration theory. In particular the dominated convergence theorem tells us that if a sequence of integrable functions converges to , and if the sequence satisfies for all , where is integrable, then is integrable and converges to as .
The integral here is the definite Lebesgue integral on some domain. But the theorem holds for functions which are integrable in the older and more familiar senses of Riemann, Cauchy, and Newton/Leibnitz, since, broadly speaking, functions which are integrable in the latter senses are, a fortiori, integrable in the Lebesgue sense.
From this point onwards somebody—not necessarily expert in Lebesgue’s integration—who is contentedly doing some familiar integral operations, and who encounters some issue of convergence such as term-wise integration of a Fourier series, can proceed in safety if a dominant integrable function can be found for the convergence.
This is the practical significance of Lebesgue’s theory. It is a reason why “it is safe to fly in airplanes”, so to speak. It is why the fertile garden did not turn into a barren wilderness. And the “monster-functions” were in reality guard dogs that played their part in protecting the garden.
3 A Non-monstrous Function
But is this the end of the story? Did Lebesgue’s 1901 and 1902 papers [12, 13] give the last word on the subject?
Here is a sequence of non-monstrous functions formed by combining some familiar polynomial with trigonometric functions. For , let if and [math] if .
An impression of function can be obtained from Figure 3 below, which contains the graph of for . Figure 2 resembles Figure 3 in the neighbourhood of . The difference between the two is , whose graph is in Figure 1.
But the values of the latter function are very small in the neighbourhood of . Figure 1 demonstrates its “visual insignificance”, so to speak. Note that the vertical scale of Figure 1 is much more magnified than the vertical scales of Figures 2 and 3.
Figure 4 is the graph of the primitive function or anti-derivative of , which will play a big part in our discussion.
Each has a single discontinuity (at ), but is differentiable at every other point. Each is integrable (in the sense of Riemann and Lebesgue), and the sequence is convergent at each to , , whose graph is Figure 3.
The limit function has a single discontinuity (from the right) at ; and it has a primitive function (), (Figure 4); so in fact has a definite integral on the domain provided the Newton-Leibnitz definition of the integral is used.
But is unbounded on and therefore is not Riemann integrable on . And, though clearly non-monstrous, and understandable to a beginning calculus student, the function is not Lebesgue integrable. See below for discussion of this point.
On the face of it, this example indicates a step backwards, as it were, where the old school method of Newton/Leibnitz is actually more effective than more modern methods. Lebesgue’s theory of the integral threw up anomalies of this kind, and accordingly investigation of the theory continued through the twentieth century.
To recapitulate, Lebesgue’s dominated convergence theorem can be said to be the cutting edge of modern integration theory. But it fails to capture the convergence of sequences such as and . The graph in Figure 3 suggests as a conceivable candidate for dominating function for the terms , , at least in a neighbourhood of the critical point . But is not integrable in a neighbourhood of [math], and it seems that the dominated convergence theorem is not applicable here.
This failure must sound some alarm bells, because while many working mathematicians can get by without the Lebesgue integral, we cannot really do without convergence theorems which allow us, for instance, to perform routine operations on Fourier series; or, more generally, to safely find the integral of the limit of a sequence of integrable functions by taking the limit of the corresponding sequence of integrals.
The purpose of this essay is to dip into some aspects of modern integration theory in order to introduce Theorems 1, 2, and 3 below, which are delicate enough to deal with, for instance, the convergence of the functions above and their integrals; while also covering the ground already captured by the convergence theorems of Lebesgue’s theory.
For ease of reference, here again are the sequence and related functions, :
[TABLE]
Figures 3 and 4 are, respectively, the graphs of the functions and . The graphs of and are easily substituted—just insert a horizontal line segment at height [math] from to .
The function has a single discontinuity at , while is continuous. The reader should verify that is differentiable, including at the point (from the right), and that . The fact that for is easily verified.
This establishes that , , has a primitive or anti-derivative, and is the calculus- or Newton-indefinite integral of . Also the calculus- or Newton-definite integral on is
[TABLE]
For each both and have a discontinuity at , but provided , we have . Thus, for each , is Riemann and Lebesgue integrable on , but not calculus- or Newton-integrable on . However is calculus-integrable on for each , and
[TABLE]
provided we interpret as a Riemann (or Lebesgue) integral. Thus, as ,
[TABLE]
provide we interpret the left hand integrals in the sense of Riemann or Lebesgue, and the right hand one as a calculus or Newton/Leibnitz integral.
Unless we can interpret it in some other way, (13) is deficient as it stands, since we cannot ascribe the same meaning to the symbol in the left- and right-hand terms. In fact we will establish later that (13) is valid for an adapted111That is, the Riemann-complete integral, also known as the generalized Riemann or Henstock-Kurzweil integral. version of the Riemann integral; and that the convergence—including integrability of the limit function —though unrelated to any kind of dominated convergence, satisfies a new kind of Riemann sum convergence criterion which goes beyond the Lebesgue dominated convergence theorem.
To recapitulate, for the function is bounded and continuous—except for a discontinuity at . Also it is differentiable except at . It has anti-derivative —except at .
By familiar standard results, is Riemann integrable and Lebesgue integrable on domain . But, as discussed above, its limit function is not Lebesgue (or Riemann) integrable.
There are theorems which tell us when to expect Lebesgue integrability of the limit function of Lebesgue integrable functions. If the convergence of the functions to the function is uniform, monotone, or dominated by a Lebesgue integrable function, then Lebesgue integrability of the functions implies Lebesgue integrability of their limit function , with
[TABLE]
Inspection of the graphs indicates that convergence of functions is not uniform, monotone or dominated. And, even though each is Lebesgue integrable, the limit function is not Lebesgue integrable—as demonstrated below.
Is this a big problem for the garden of mathematics, or is it just a minor incursion by, not a monster, but an atypical creature which is easily contained? This article attempts to provide some perspective.
The names of Denjoy, Perron, Kolmogorov and others are associated with twentieth century efforts [4] to pursue the implications of problems such as the convergence of functions and their integrals. This article will examine the Riemann sum approach of R. Henstock and J. Kurzweil.
4 Riemann-complete Integration
Kurzweil came to this subject through his investigations of differential equations. Henstock was interested in convergence issues in integration. Independently, each of them focussed on careful construction of Riemann sums for integrands .
Here is a broad outline of Riemann sum construction. A partition of a domain such as is a set of points . Identify with the corresponding set of disjoint intervals :
[TABLE]
For each let denote the length of . Given a function defined for , evaluation points are selected for the intervals in accordance with certain rules (such as ), and then a Riemann sum for is
[TABLE]
The integral of on the domain , denoted by , exists if satisfies a condition which is broadly of the following form. Given , partitions can be chosen such that
[TABLE]
This inequality is reminiscent of the Riemann integral of , but it is not the full definition that is required here. There must be some rule (sometimes called a gauge) for selecting the elements (corresponding to the partition or ) that can be admitted in the inequality.
For Riemann integration, the rule is that, given there exists a constant such that, for every partition for which and for each , the above222If is continuous on then its Riemann integral exists there. inequality (14) holds. Denote such a rule by , and denote a partition which satisfies an appropriate instance of the rule by .
An integral constructed from such a rule can be identified by notation . Then the definition of the integral is as follows. There is a number for which, given any , there exists a corresponding333For the ordinary Riemann integral, read “there exists a corresponding number ”. instance of such that every partition satisfies
[TABLE]
We will omit the γ in , and allow the context to demonstrate which version of the integral is being discussed.
While the Riemann sum rule for ordinary Riemann integration is “”, the primary innovations of Kurzweil and Henstock were:
to replace selection of intervals by selection of linked pairs in constructing Riemann sums,444The familiar condition is sometimes altered. Also the new approach often gives priority to the evaluation points ; and then it can be a more subtle and difficult task to determine the linked partitioning elements . See [9] and [14]. and 2. 2.
to replace the constant by variable , where is the evaluation point in the term of the Riemann sum in (15).
To distinguish this from the Riemann integral, call it555It is also called the Henstock-Kurzweil integral, generalized Riemann integral, and gauge integral. the Riemann-complete integral. Clearly, every Riemann integrable function is also integrable in the Riemann-complete sense.
A Stieltjes-type definition of the integral of a function can be expressed as follows. Suppose and are point functions defined on the domain . The Riemann-Stieltjes integral of with respect to is got by replacing the length function by the increment function in the above definitions. A standard result is that if is continuous and is monotone (or has bounded variation), then the Riemann-Stieltjes integral exists. If the constant in the definition is replaced by the function of the Riemann-complete construction, call the resulting integral the Stieltjes-complete integral of with respect to .
To see how the Riemann-complete integral matches the calculus or Newton/Leibnitz integral, suppose a point function has an anti-derivative or primitive function for , so its definite integral in the Newton/Leibnitz sense is . Proceeding as follows, it is easy to deduce that is Riemann-complete integrable.
If is a partition of with partition points , , and if , then
[TABLE]
Let be given. Then, for each , , there exists a number such that, for ,
[TABLE]
Now choose a partition so that each term satisfies
[TABLE]
The existence of such partitions is a consequence of the Heine-Borel theorem. For such a partition (16) implies
[TABLE]
with corresponding inequalities for and . Writing and ,
[TABLE]
Thus the Riemann-complete integral of exists and equals the Newton/Leibnitz definite integral .
In the case that is given by (3), while the Newton/Leibnitz and Riemann-complete integrals exist, it has been asserted above that the Lesbesgue integral does not exist.666In that case the Riemann integral of does not exist either. This assertion remains to be demonstrated.
The definition of the Lebesgue integral of a function can be addressed in various equivalent ways, e.g. [18]. For instance, given a real-valued, measurable function defined on an arbitrary measurable space , with measure defined on the family of measurable subsets of , [15] shows how to define the Lebesgue integral of on as a Riemann-Stieltjes integral in , the set of real numbers. In fact, writing
[TABLE]
the Lebesgue integral is the Riemann-Stieltjes integral . If and is Lebesgue measure in , and if the Lebesgue integral of exists, then the Riemann-complete integral of exists and the two integrals are equal. Every Lebesgue integrable function is integrable in the Riemann-complete sense (see [14]).
A key point is that the Lebesgue integral is an absolute integral, while the Riemann-complete is non-absolute. Writing if , with otherwise, and , absolute integrability implies that is Lebesgue integrable if and only if both and are Lebesgue integrable.777This restriction does not apply to the Riemann-complete integral of , which does not require the Riemann-complete integrability of and . We use this point to demonstrate that the function defined by (3) is not Lebesgue integrable.
With that in mind, Figure 3 provides an indication of how the function defined by (3)
- •
fails to be Lebesgue integrable, while
- •
its Riemann-complete integral exists.
In fact Figure 3 shows that, in neighbourhoods of , the graph of oscillates increasingly rapidly, in positive (, above the -axis) loops and negative (, below the -axis) loops whose amplitude (or height/depth) increases without limit as . This creates the suspicion, or expectation, that the sum of areas of the positive loops diverges to , while the sum of areas of the negative loops diverges to .
But if, instead of treating positive and negative loops separately, we add up their areas in their natural sequence, then positive and negative areas will tend to cancel each other out, and the resulting sequence of net values may converge.888For example, with , the series converges, but the series consisting of only the positive terms (or only negative terms) diverges; so diverges. The latter is what happens in the Riemann sum construction of the Riemann-complete integral of .
The following discussion seeks to add substance to these speculations. In any interval, not including zero, but with small values of , Figure 1 shows that the contribution from the term to the area under the graph of is vanishingly small in neighbourhoods of , while the corresponding contribution from the term in is relatively large. Therefore, disregarding the term , the zeros of (3) can, for present purposes, be estimated approximately as
[TABLE]
Accordingly we may estimate that, for large, even values of ,
[TABLE]
while for large and odd values of
[TABLE]
Writing
[TABLE]
each of the two series
[TABLE]
diverges, so it is clear that is not Lebesgue integrable in . But it is easy to see that the series
[TABLE]
is non-absolutely convergent, even if we did not already know, from existence of the primitive function for , that is Riemann-complete integrable.
This is because the Riemann-complete convergence is obtained from the cancellation effects produced by successively summing the positive and negative parts in their natural sequence.
We can ensure this by choosing as follows. When lies between adjacent roots and let
[TABLE]
and if is one of the roots , take
[TABLE]
and when let be arbitrary. Any partition corresponding to this definition of () will contain a term with , and the terms for non-zero will each contain an arbitrarily close estimate of the area of the corresponding positive or negative loop in Figure 3. This provides the required cancellation and convergence of Riemann sums, since the alternating loops are monotone decreasing in area as approaches [math].
In the case of the Lebesgue integral this cancellation effect is absent, and convergence fails.
This establishes that, just as there are Lebesgue integrable functions that are not Riemann integrable, there are Riemann-complete integrable functions that are not Lebesgue integrable.
5 Convergence Criteria
Anybody experienced in the theory of integration will be aware that most of the preceding discussion covers fairly well-worn ground which has already been worked through in many excellent publications, such as [2].
But at the outset of this article it was stated that, while Lebesgue’s dominated convergence theorem is a crucial pillar of modern analysis, there are certain areas of the subject where this theorem is deficient. The sequence of (6) demonstrates that the dominated convergence theorem provides no illumination in this particular instance of converging non-absolute integrals. This section addresses the deficit.
There are convergence conditions and criteria which encompass and surpass the dominated convergence, monotone and uniform convergence theorems of standard integration theory. These are the convergence criteria of Theorems 1, 2, and 3 below. They are valid for Riemann-complete integrals (which include integrals of the Newton/Leibnitz, Riemann, and Lebesgue kinds). Measurability of the integrand functions is not assumed.
Theorem 1
Suppose is integrable on and converges to for . Suppose, given arbitrary , there exist a number and, for , a gauge , and integers depending on , so that, for every partition of with linked elements satisfying (), the condition
[TABLE]
holds for all choices of () in the Riemann sum. Then the limit function is integrable on , with .
Theorem 2
Suppose is integrable on and converges to for . Suppose, given arbitrary , there exist a number and a positive integer depending only on , so that, for every partition of with linked elements satisfying (), the condition
[TABLE]
holds for every choice of with constant for each term of the Riemann sum. Then converges as .
Theorems 1 and 2 can be expressed in converse form (see [14]), so they are criteria for their respective conclusions. Apart from the opening sentence of each they apply independently of each other; in the sense that either one of them may hold for particular integrands while the other one does not hold.
Theorem 3
If both of Theorems 1 and 2 hold (so both of and exist), then
[TABLE]
if and only if .
For anybody more familiar with the classical integration theorems on passage to a limit, these theorems or criteria may appear somewhat indigestible at first sight.
Their starting point is that a convergent sequence of functions is given. These function are assumed to be Riemann-complete integrable, which is a weaker assumption than Lebesgue integrability. There is no assumption of properties like continuity or measurability.
To answer questions about convergence of the corresponding sequence of Riemann-complete integrals, and about the Riemann-complete integrability of the limit function, from previous experience of integration we might be led to expect some condition, not about Riemann sums, but only about the functions —such as monotonicity, domination by a fixed integrable function ; or the like. But nothing like this appears in the above convergence criteria. Instead we have various statements about Riemann sums.
However, setting aside for a moment the conception of integral as primitive function, or anti-derivative, the original and more durable meaning of integral involves slicing up (partitioning), followed by summation, followed by taking a limit of the sums.
From this perspective, it may be less of a surprise that Riemann sums appear in the formulation of conditions for limits of integrals, since Riemann sums are central to the concept of integral.
Consider Theorem 1. Given integrability of the terms in the sequence, this theorem addresses the integrability of the limit function , which, essentially, involves the question of convergence of Riemann sums .
To make an initial stab at this question, we might consider sequences of Riemann sums , . We know that, for each , the sequence of values converges to as . We also know that, for each , Riemann sums of the form converge to the integral of . Can we somehow put these two facts together to deduce, as an immediate consequence, convergence of Riemann sums to the integral of ?
Of course, we know that the answer to this is no. The answer is yes if the terms satisfy some conditions such as where is integrable. But if we want a condition expressed in the form of a condition on Riemann sums, clearly something more delicate than convergence of is required.
For instance, with given, the condition we need is not that, for all greater than some , every Riemann sum will be contained within some ball of the form .
This is too crude for our purpose. All it says is that is integrable—which we already know. The convergence of to may be very fast at some points , and very slow at other points . This behaviour is provided for in Theorem 1, by choosing, not , but different for each .
This formulation is sufficient, and necessary, for integrability of the limit function . Once this point is established, the criteria of Theorems 2 and 3 are fairly obvious, and less subtle. But are these conditions of Theorems 1, 2 and 3 “workable” in the way that the dominated convergence condition is?
After all, Riemann sums are fine for defining the meaning of the integral of a function. But when we actually want to find the value of an integral we do not typically work with Riemann sums. Instead we revert to the integral as primitive or anti-derivative, using the substitution method or integration by parts. Or we use some less direct method, such as solving a related differential equation; or a myriad of other999Which is not to say that Riemann sums are “merely” a device of fundamental theory, and nothing else. Versions of them have had other uses; such as the ancient techniques of quadrature; or computer programs for estimating numerical values of an integral. Simpson’s rule is another example. ad hoc methods.
To respond to such questions, and to demonstrate that Riemann sums can actually be of use here, we can as an example take the sequence defined in (6). Remember, for each the function is Riemann integrable and Lebesgue integrable, but not Newton/Leibnitz integrable, and their limit function is Newton/Leibnitz integrable but not Riemann or Lebesgue integrable. For each , is Riemann-complete integrable.101010As is , from earlier discussion. But for present purposes we wish to deduce Riemann-complete integrability of from Theorem 1. This discussion of the convergence criteria of Theorems 1, 2 and 3 is set in the context of Riemann-complete integrability.
The subject of the first criterion is the (Riemann-complete) integrability of the limit function , and it is established by examining Riemann sums of the form
[TABLE]
We already know, by various means, including a direct investigation of the Riemann sums , that is (Riemann-complete) integrable on .
The function is the limit of functions . Is it possible to confirm further the integrability of by direct examination, not just of , but of Riemann sums involving functions instead of , where the factor in the sum has variable index , depending on the element of the division used to construct the Riemann sum?
This is the essence of Theorem 1. And according to Theorem 1 the answer to this question should be yes. Given , and with a suitable gauge , provided factors are chosen appropriately we should be able to demonstrate that the value of each corresponding Riemann sum will lie within some ball of radius where is arbitrarily small.
Since we are already convinced of the integrability of in this case, what we are really trying to do here is to get a sense of the behaviour of sums . So, given the integrability of , write and choose a gauge so that, for every -fine partition of ,
[TABLE]
the ball with centre and radius .
Consider any one of these Riemann sums , corresponding to a particular -fine partition with . For each choose
[TABLE]
Then, by definition of , if ,
[TABLE]
so, for all choices ,
[TABLE]
as required by Theorem 1.
In general, the convenient equation cannot be appealed to. But if, with suitable choices of , the differences
[TABLE]
can make sufficiently small contributions to the Riemann sum, then it may be plausible that
[TABLE]
so is integrable. This is the intuitive content of Theorem 1.
Now to Theorem 2. The preceding remarks are concerned with the integrability of . The fundamental assumption is that each function in the sequence is integrable. In the case of our example (6) the anti-derivatives (12) are the sequence , giving a sequence of integrals
[TABLE]
which can be denoted by . Note that continuity of implies as . In this case it is already clear that the sequence of integrals converges as , the limit being (in this case) ; what we want is confirmation, including intuitive confirmation, that Theorem 2 actually works.
The convergence of a sequence of integrals is the subject of Theorem 2, and it is again expressed in terms of Riemann sums. The criterion implies that, with arbitrarily small given, there is a ball with centre and radius , and a corresponding integer depending only on , so that for each , a gauge can be found such that for every -fine partition of the corresponding Riemann sum is contained in ; so for every -fine ,
[TABLE]
whenever . Unlike Theorem 1, here is the same for each term of any particular Riemann sum.
Again, this is easy to demonstrate since we already know in this case that the integrals converge to the value as . Just take
[TABLE]
and choose so that implies
[TABLE]
For each choose a gauge () so that, for any -fine partition of ,
[TABLE]
Then, by the triangle inequality,
[TABLE]
for all and all -fine partitions of . In other words, the criterion of Theorem 2 confirms the convergence of the sequence of integrals
[TABLE]
and this demonstration illustrates the intuitive content of Theorem 2.
Finally, the question arises whether the integral of the limit
[TABLE]
equals the limit of the integrals
[TABLE]
For the sequence of (6), we already know by direct evaluation that these two quantities have the same value, namely . This agrees with the criterion of Theorem 3, which requires that and have the same value. In this case
[TABLE]
so the intuitive content of Theorem 3 is clear in the context of this example.
6 Conclusion
So, does it really matter whether aviation designers work out their aerodynamic equations using old-fashioned Riemann integrals or the latest fancy Lebesgue integrals?
Probably not much. But it matters a lot if the value 22/7 for were hard-wired into every computer in the world. Or if the wrong value for elasticity of O-rings at freezing temperature was used in space shuttle design. And it certainly matters whether our aviation designers make tricky, unjustifiable calculations involving, for instance, term-by-term integration of Fourier series.
It is thanks to the intellectual diligence of the nineteenth century, not to mention its monster-functions, that we have the dominated convergence theorem to keep the garden of mathematics safe and fertile—and, indeed, to keep airplanes flying safely.
But do we really need anything more than the dominated convergence theorem for absolutely convergent integrals? Why bring up the convergence criteria of Theorems 1, 2, and 3? Is the sequence described in (6) above just an exceptional one-off, or is it representative of something more significant? If the latter, where are all these non-absolute integrals?
In fact they are very widespread. Modern stochastic calculus [16, 17] is based on integrals for which absolute convergence fails, but which may converge weakly or, in some cases, non-absolutely. These are described in [14, 15].
A very significant formulation of quantum mechanics is in terms of path integrals [3] which also fail to converge absolutely. Famously, the dominated convergence theorem does not work for these integrals, and, as described in [14], the non-absolute convergence criteria must be invoked.
“Does anyone believe … I would not care to fly in that plane.” A healthy scepticism must be welcomed. But what is certain is that, while integration is central to mathematical analysis, there are no certain and definite ways of tackling any problem of integration, and even a beginning student has to exercise imagination and ingenuity. From the ancient methods of quadrature, to the methods of Newton/Leibnitz, Cauchy, Riemann, Lebesgue, Denjoy, Perron, Kolmogorov, Kurzweil, or Henstock, it is unwise to disregard any resource or insight that can be called upon.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[1] Bartle, R.G., Return to the Riemann integral , American Mathematical Monthly 103(8) (1980), 625–632.
- 2[2] Bartle, R.G., A Modern Theory of Integration , John Wiley & Sons, Hoboken, 2001.
- 3[3] Feynman, R., Space-time approach to non-relativistic quantum mechanics , Reviews of Modern Physics 20 (1948), 367–387.
- 4[4] Gordon, R.A., The Integrals of Lebesgue, Denjoy, Perron, and Henstock , American Mathematical Society, Providence, 1994.
- 5[5] Paraphrased in N. Rose’s Mathematical Maxims and Minims , Raleigh NC, Rome Press Inc., 1988.
- 6[6] Hardy, G.H., Divergent Series Clarendon Press, Oxford, 1949.
- 7[7] Henstock, R., Theory of Integration , Butterworth, London, 1963.
- 8[8] Henstock, R., The General Theory of Integration , Clarendon Press, Oxford, 1991.
