Lagrange and Cauchy Forms of the Remainder
How well does a Taylor polynomial approximate a function? Can we pin down the error exactly? A student who has met Taylor's Theorem with Remainder knows the remainder can be written as an integral. But integrals are not always easy to estimate by hand. What is needed is a single point where the "error" of the approximation is captured exactly by a derivative value. This works the same way the ordinary Mean Value Theorem captures the error of a linear approximation. This article derives two such exact expressions. These are the Lagrange form and the Cauchy form of the Taylor remainder. Both are consequences of the Cauchy Mean Value Theorem applied to auxiliary functions built for this purpose. These two forms look different but say the same thing from different angles. The Lagrange form generalizes the familiar mean value theorem remainder to higher order. It expresses the error after terms as a single -th derivative. This derivative is evaluated at some intermediate point, multiplied by a power of the interval length. The Cauchy form instead keeps track of how far that intermediate point is from the two endpoints. It does this via an extra factor that vanishes at one end. That factor equals the full interval length at the other end. This finer bookkeeping matters. There are classical series, notably the binomial series for exponents outside , where the Lagrange remainder fails to reveal convergence. In these cases, the Cauchy remainder succeeds. The big picture is that Taylor's theorem is not one theorem but a family of theorems. These are distinguished by which "form of the remainder" one uses. Each form is suited to different estimation tasks. Lagrange's form is the workhorse for elementary error bounds. It looks exactly like evaluating one more derivative at an unknown point. Cauchy's form is a specialized tool. It is indispensable when the remainder must be tracked as the interval shrinks in a lopsided way. Both are derived from the same generalized mean value machinery. Both also reduce, at , to the ordinary Mean Value Theorem. This article gives complete, self-contained proofs of both forms. It applies the Cauchy Mean Value Theorem to a single well-chosen pair of auxiliary functions. It states the precise hypotheses under which each form is valid. It compares their strengths with worked numerical examples. It also shows, via a genuine counterexample, why the differentiability hypotheses cannot be relaxed. It sets the stage for the broader study of Taylor Polynomials and Local Approximation.
- Both remainder forms express the exact error of the degree- Taylor polynomial, using the -th derivative at an unspecified intermediate point.
- Lagrange form: for some strictly between and .
- Cauchy form: for some (generally different) strictly between and .
- Both follow from applying the Cauchy Mean Value Theorem to minus its Taylor polynomial, against two different comparison functions: for Lagrange, for Cauchy.
- Setting recovers the ordinary Mean Value Theorem in both cases, confirming these are genuine generalizations.
- Key idea: the same generalized mean value argument, run against different comparison functions, yields remainder formulas with different sensitivity — Cauchy's form tracks the location of more precisely and controls some series (e.g. the binomial series) that Lagrange's form cannot.
Where this lives today
The Lagrange remainder is the standard tool for numerical error bounds: calculators and computer algebra systems computing , , , and via truncated Taylor series use Lagrange-type bounds to decide how many terms are needed for a target precision. In numerical analysis, error terms in interpolation formulas (e.g. polynomial interpolation error, Simpson's rule error in numerical integration) are derived by essentially the same Cauchy-mean-value-theorem technique used here. In complex analysis and the study of power series, the Cauchy remainder is the classical route to proving convergence of the binomial series for all and all real , a case where the Lagrange form's bound diverges near while the Cauchy form's bound stays controlled — exactly the phenomenon illustrated in Example 2. In physics and engineering, both forms justify truncating perturbative expansions (small-oscillation approximations, first-order error propagation) with a guaranteed error bound rather than a merely heuristic one. In statistics, Taylor remainder bounds underlie the rigorous justification of the delta method and asymptotic normality arguments, where a function of an estimator is linearized and the remainder must be shown to vanish in probability. The underlying technique — comparing two functions via the Cauchy Mean Value Theorem — reappears throughout analysis whenever an "exact form of an error term" is sought, including in the proof of L'Hôpital's rule itself.
Ask the tutor: How does the integral form of the Taylor remainder relate to these two explicit forms, and can it be used to derive both at once?
Let be an interval, let , and let be an integer. Suppose has derivatives on . The -th Taylor polynomial of centered at is
For , the remainder is defined by
Any formula expressing in closed form, typically involving at an unspecified point between and , is called a form of the Taylor remainder.
Intuition
Think of the ordinary Mean Value Theorem as the case : it says
for some strictly between and . This is exactly , an expression for the error of the constant approximation in terms of the first derivative at an unknown intermediate point. The Lagrange remainder is the natural continuation of this pattern: replacing the constant approximation by the degree- Taylor polynomial, the error is captured by the -th derivative at an unknown point, scaled by — exactly the next term the Taylor series would have, except evaluated at instead of . The Cauchy remainder tells the same qualitative story but keeps a second piece of information: not just that there is an intermediate point , but a factor recording how close sits to the far endpoint . Geometrically, imagine sweeping a parameter from to and watching the "residual" , where is the Taylor polynomial of centered at the moving point . Both remainder formulas arise from applying the Cauchy Mean Value Theorem to this same residual function, but paired against two different "rulers": Lagrange uses the ruler , Cauchy uses the ruler . Different rulers place the mean-value point in different (generally non-equal) locations, and yield algebraically different — but equally correct — closed forms for the same number .
The central theorem
Let with , let be the closed interval with endpoints and , and let be an integer. Suppose: 1. are continuous on ; 2. exists at every point of the open interval between and . Then there exist points strictly between and (generally different from one another) such that, writing as above:
(Lagrange form.)
(Cauchy form.)
Fix and with (the case is identical with all inequalities reversed; the interval throughout, or in the reversed case). Define, for , the function
This is the "residual" mentioned in the Intuition section: it is minus the degree- Taylor polynomial of centered at the moving point , evaluated at the fixed point . Note two facts immediately from the definition:
(The first equality holds because when every term with has factor , leaving only the term .)
Step 1: Compute . By hypothesis, is continuous on for and differentiable on the open interval for (since exists there), so is continuous on and differentiable on . Differentiate the sum term by term using the product rule on each :
and for the derivative is simply . Summing over , the sum telescopes: the negative term at index is
which is exactly the negative of the positive term produced at index ... let us verify this telescoping explicitly rather than merely asserting it. Write . Then
The second sum, re-indexed, is
The second of these two sums, re-indexed with running from to , equals . So
The term of the subtracted sum is , which cancels the leading . All other terms of the two sums (indices appear in both) cancel identically, leaving only the term of the first sum:
Since is constant minus ,
Step 2 (Lagrange form): compare against . The function is continuous on , differentiable on with , and for since there. Also and . By the Cauchy Mean Value Theorem applied to on , there exists with
(This is the standard determinant form of the Cauchy Mean Value Theorem, valid without dividing by or ; we verify below that both these quantities are in fact nonzero here, so the more familiar quotient form applies too.) Substituting , , , :
Using for :
Since , , so we may divide both sides by :
This is precisely the Lagrange form.
Step 3 (Cauchy form): compare against . The function is continuous on , differentiable everywhere with , and , . Apply the Cauchy Mean Value Theorem to on : there exists with
Substitute , , , :
i.e. . Using :
This is precisely the Cauchy form.
∎For , both formulas reduce to for some between and — the ordinary Mean Value Theorem. Indeed with : Lagrange gives ; Cauchy gives . Since , both reduce to the same classical statement (with and each simply a mean-value point, not necessarily equal).
Worked examples
Example 1 (Lagrange remainder: bounding using , centered at ). Let , , , . All derivatives of equal , certainly continuous everywhere, so the hypotheses of the theorem hold on . The Taylor polynomial is
At :
By the Lagrange form with , there is with
Since , (using , a standard bound since ). Hence
i.e.
So , giving
The true value is , comfortably inside this window, confirming the bound is correct and reasonably tight — a genuine numerical error estimate produced with no knowledge of the exact value.
Example 2 (Cauchy remainder: the binomial series at a point where Lagrange's bound is uninformative). Let so that (the Taylor series of about has , so ). Fix (an asymmetric, negative value close to , where the series is delicate) and take . We have
so . All derivatives are continuous on the interval between and (i.e. ), since never vanishes there; hypotheses of the theorem hold. Lagrange form gives with
Since , , so . This bound is essentially useless: it only tells us , while the true remainder is small (we compute it below). The Lagrange form, because it only uses the endpoint distance and not the position of relative to , cannot see that being close to (where is huge) is compensated by another factor — because Lagrange's formula has no such compensating factor. Cauchy form gives with
Simplify: , so
Here the crucial point: as (i.e. approaches the far endpoint, where is largest), the factor , exactly compensating the blow-up of . This is the mechanism by which the Cauchy form remains a useful, bounded estimate even when the Lagrange form is not. Concretely, since and , we get the crude bound
which is also not tight as a crude bound, but the point of this example is structural, not to produce the tightest bound by hand — the exact value can be checked directly: , and , so
an exact, finite, moderate number — consistent with both formulas (each merely expresses using an intermediate point, and Cauchy's formula does so with better-behaved individual factors). This example illustrates the classical fact that for the binomial series with near , the Cauchy remainder is the one used to prove convergence rigorously, since the Lagrange remainder's bound -type expressions blow up while the Cauchy form's ratio can be shown to stay bounded by using .
The theorem requires continuous on the closed interval between and , not merely on the open interval. Weaken this hypothesis and the conclusion can fail. Let , , , and define
Here is continuous on and differentiable there with , but is not continuous at the left endpoint (since but ). This violates hypothesis (1) of the theorem (continuity of on the closed interval ), while the derivative exists and is even continuous (constantly ) on the open interval . The conclusion (the Mean Value Theorem, i.e. case) asserts the existence of with
Compute the left side: . But for every , so the right side is . No such exists — the conclusion genuinely fails. The failure is entirely due to the discontinuity at the endpoint : it destroys the hypothesis of continuity on the closed interval used at the very first step of the Cauchy Mean Value Theorem argument (which requires continuous on to guarantee attains its extrema and Rolle's theorem-type reasoning applies inside the proof of the Cauchy Mean Value Theorem itself). This shows that the endpoint-continuity hypothesis cannot be dropped from the Lagrange/Cauchy remainder theorem, since even the base case (the ordinary Mean Value Theorem) fails without it.
Scope, edge cases & common traps
| Situation | What holds | What can go wrong |
|---|---|---|
| on all of (closed) | Both Lagrange and Cauchy forms valid, 's may differ | — |
| exists only on open interval, discontinuous at an endpoint | Neither form guaranteed | See counterexample above |
| Both formulas still hold, with between and | Sign of , must be tracked carefully | |
| Estimating remainder near large relative to radius of convergence | Cauchy form often gives convergence when Lagrange does not | Applying Lagrange's crude bound blindly, as in Example 2 |
| and | Both exist, both lie strictly between and | Assuming — false in general |
The mathematician behind it
Origins · 1 minJoseph-Louis Lagrange and how this was discovered
Lagrange, born in Turin, made foundational contributions to mechanics, the calculus of variations, and the algebraic theory of equations. His attempt to found calculus on power series and Taylor expansions — without appeal to infinitesimals — led him to seek an exact, algebraic expression for the remainder of a truncated Taylor series, the form that now bears his name. Augustin-Louis Cauchy, working a generation later during the rigorization of analysis in the 1820s, gave the alternative remainder form together with the rigorous –-style foundations that made statements like the Cauchy Mean Value Theorem precise; his form of the remainder emerged naturally from his broader mean-value-theorem framework.
Do the Lagrange and Cauchy remainder formulas always give the same numerical value for ?
Yes — both are exact formulas for the same number ; they must agree numerically once you plug in the actual value of or that makes each formula true. What differs is the intermediate point: the that makes the Lagrange formula correct is generally not the same real number as the that makes the Cauchy formula correct, since they arise from two separate applications of the Cauchy Mean Value Theorem to two different comparison functions. Both formulas are correct descriptions of the same remainder; they simply parametrize it differently through different (and non-interchangeable) unknowns.
Why do we need the Cauchy Mean Value Theorem rather than just Rolle's theorem to derive these formulas?
The proof compares two auxiliary functions, (the residual) and a "ruler" function such as or , simultaneously. The Cauchy Mean Value Theorem is precisely the tool that relates the ratio of derivatives of two functions to the ratio of their increments at a single common point . Using Rolle's theorem alone on would only give a point where , which is not what we want (indeed is generally never zero here); we need the ratio of 's increment to the ruler's increment, matched to the ratio of their derivatives, which is exactly the content of the Cauchy Mean Value Theorem.
Is the Cauchy form ever strictly better for producing numerical bounds, or is it purely of theoretical interest?
It is genuinely useful, not just theoretical. In the binomial series example, bounding the Lagrange remainder for close to requires bounding where could be arbitrarily close to , giving no useful bound. The Cauchy form's extra factor vanishes exactly where the derivative term blows up, and a short computation shows the ratio stays below , giving a genuine geometric decay bound. This is the standard textbook route to proving the binomial series converges on all of for every real exponent.
Does the theorem require to be continuous?
No — only that exists at every point of the open interval between and ; continuity of is not assumed or used in the proof. What is required is that be continuous on the closed interval, since the proof applies the Cauchy Mean Value Theorem to , which is built from these lower derivatives and needs to be continuous on the closed interval and differentiable on the open interval — exactly the hypotheses of the Cauchy Mean Value Theorem itself.
How does this relate to the integral form of the remainder taught alongside Taylor's theorem?
The integral form, , requires to be integrable (commonly, continuous) on the closed interval, and follows from repeated integration by parts. The Lagrange and Cauchy forms can each be recovered from the integral form via the (first and second, respectively) Mean Value Theorems for integrals, but the derivation given here is self-contained and uses only the Cauchy Mean Value Theorem, requiring only that exist (not necessarily be integrable or continuous) on the open interval — a strictly weaker hypothesis than the integral form demands.
Why does the proof define using the moving-center Taylor polynomial rather than working directly with ?
Because is a fixed number once are fixed — it has no "" to differentiate with respect to. The trick is to replace the fixed center by a variable center , forming , which is a genuine function of satisfying and . Differentiating this function in is what produces the telescoping sum collapsing to the single clean expression , which is the engine driving both remainder formulas.