The Named Integrals
for continuous with finite limits at and .
Every integral of the form "difference of two scalings, divided by " is Frullani: , , . The makes each piece diverge alone; only the difference converges, and the value depends on only through its two endpoint values — which is why it looks like magic and is really Feynman's trick in disguise.
, with and . .
Gamma interpolates the factorial ( by one integration by parts) and evaluates every . Beta evaluates every polynomial-times-polynomial integral on in one line () and, via , every — the Wallis integrals are Beta values. The reflection formula is why .
rationalizes any . Expanding the integrand in a series and swapping and turns hard integrals into known sums.
Weierstrass: , , — so . Series: , and . The swap is legal under uniform convergence on the interval — say so.
Symmetry first (it costs nothing). Then look for a parameter (Feynman). Then match a NAMED shape: difference-over- is Frullani; is Gamma; is Beta; a rational function of sine and cosine is Weierstrass; a log or arctan over a simple denominator is a series. Only then reach for parts or partial fractions. The Putnam rewards recognition, not endurance.
"Split into and substitute in the second: it becomes , the same as the first, so the answer is ." Each piece diverges at , and the split is . Do it with a cutoff instead: , which lies between and and tends to . The whole value lives in the sliver near that the careless substitution threw away — this cutoff argument is in fact a proof of Frullani's theorem.
Evaluate .
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With this is . (Or substitute , : ✓.)
Proofs & Why It Matters
Assume continuous with , finite and .
Write (fundamental theorem in ; assume continuous for the clean version). Then , swapping the order of integration (Fubini, justified by absolute convergence). Significance: the proof IS Feynman's trick — the was hiding an integral over a parameter. Once you see that, Frullani stops being a formula to memorize.
Two famous constants, one computation.
Substituting in gives . Square it and go polar: . So . No one-variable method evaluates this integral; the plane does. Every normal-distribution constant in statistics traces back to this square.
Going Deeper: Worked Problems
Evaluate .
Step 1 — recognize with , ; but has no limit at , so the plain theorem does not apply.
Step 2 — the fix: Frullani holds if is replaced by the CESÀRO mean , which for cosine is .
Step 3 — the value is .
Step 4 — verify with the damping trick: as ✓. Knowing the theorem's exact hypotheses — and how to repair them — is the difference between a and a .
Evaluate .
Step 1 — on (convergent at by the alternating series test; uniform on by Abel).
Step 2 — divide by and integrate term by term: .
Step 3 — this is .
Step 4 — numeric check: and ✓.
Improper Integrals: When They Converge
An integral is improper at an infinite endpoint or at a point where the integrand blows up. Define it as a LIMIT of proper integrals, and if there are several bad points, split so that each piece has exactly one.
converges iff ; converges iff . Those two facts, plus splitting, settle most convergence questions on sight: diverges for EVERY , because no single can satisfy both conditions at once. A Putnam answer that integrates through a singularity without splitting is marked down even when the number is right.
If and converges, so does . If and , the two integrals converge or diverge together.
Limit comparison is the practical tool: near , compare with ; near a singularity at , compare with . So behaves like and converges, while behaves like a harmonic sum and diverges — substituting makes that one exact.
convergent implies convergent. The converse fails: converges, while .
For a symmetric singularity the CAUCHY PRINCIPAL VALUE takes the symmetric limit, , but the integral itself does not converge — saying which one you are computing is part of the answer. Dirichlet-type integrals converge because of cancellation, which is why Feynman's trick and Dirichlet's test, not comparison, are the tools that handle them.
For which does converge?
Step 1 — split at : the integrand is improper at and at .
Step 2 — near , , so the piece on converges iff .
Step 3 — near , , so the piece on converges iff , i.e. .
Step 4 — both together: . (For those the value is , the Beta-function evaluation.)
Two bad points in one limit can cancel each other and produce a finite number for a divergent integral — exactly the trap the principal value formalises. Split first, evaluate each piece, and only then add.
Does converge?
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Yes. Substituting turns it into , which converges to .
More Named Results
— one integration by parts each, landing on .
With and the boundary term vanishes and the remainder is , which rescales to Dirichlet. The same move on gives Dirichlet directly. A whole family — — follows by repeated parts and is a Putnam regular for ().
, hence (substitute ) and .
The tangent substitution converts every rational-times-log integrand on into a log-trig integral on , where King and Queen apply. Feynman handles the arctangent cousin: via the parameter .
; ; ; .
Fresnel is the Mellin integral at . The reflection formula is why and hence . Wallis comes from the sine-power reduction formula squeezed between consecutive terms; is the series method landing on .
Every result on this shelf involves an interchange — of limit and integral, of sum and integral, of the order of a double integral. On the Putnam, one sentence naming the justification (dominated convergence with a named dominating function, uniform convergence on the interval, absolute convergence for Fubini) is the difference between a and a . Say it every time.
Given , evaluate .
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Step 1 — integrate by parts twice, differentiating and integrating . Near , and , so both boundary terms vanish at and at , leaving .
Step 2 — from , .
Step 3 — for every (substitute ), so .
Step 4 — halve it: .
Proofs & Why It Matters
Parts onto Dirichlet.
Let , , : . The boundary term is at both ends ( near ; bounded over at infinity). The remaining integrand is ; substituting gives . Significance: the equality of and is not a coincidence but a one-line consequence of parts — and the pattern extends to the Fourier transform of a triangle function.
Via the Beta function and a contour-free evaluation.
; substitute to get . This last integral equals — provable without complex analysis by expanding as a geometric series on and using on , which yields , the partial-fraction expansion of . Significance: gives — the Gaussian integral yet again — and the formula evaluates every .