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 f(b)−f(a)=f′(ξ)(b−a)f(b)-f(a) = f'(\xi)(b-a) to higher order. It expresses the error after nn terms as a single (n+1)(n+1)-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 [0,1][0,1], 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 n=0n=0, 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.

Key takeaways
  • Both remainder forms express the exact error Rn(x)=f(x)−Pn(x)R_n(x) = f(x) - P_n(x) of the degree-nn Taylor polynomial, using the (n+1)(n+1)-th derivative at an unspecified intermediate point.
  • Lagrange form: Rn(x)=f(n+1)(ξ)(n+1)!(x−a)n+1R_n(x) = \dfrac{f^{(n+1)}(\xi)}{(n+1)!}(x-a)^{n+1} for some ξ\xi strictly between aa and xx.
  • Cauchy form: Rn(x)=f(n+1)(ξ)n!(x−ξ)n(x−a)R_n(x) = \dfrac{f^{(n+1)}(\xi)}{n!}(x-\xi)^n(x-a) for some (generally different) ξ\xi strictly between aa and xx.
  • Both follow from applying the Cauchy Mean Value Theorem to ff minus its Taylor polynomial, against two different comparison functions: (x−t)n+1(x-t)^{n+1} for Lagrange, (x−t)(x-t) for Cauchy.
  • Setting n=0n=0 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 ξ\xi 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 sin⁡\sin, cos⁡\cos, exp⁡\exp, and log⁡\log 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 (1+x)α=∑(αk)xk(1+x)^\alpha = \sum \binom{\alpha}{k} x^k for all x∈(−1,1)x \in (-1,1) and all real α\alpha, a case where the Lagrange form's bound diverges near x→−1x \to -1 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?

DefinitionTaylor Polynomial and Remainder

Let I⊂RI \subset \mathbb{R} be an interval, let a∈Ia \in I, and let n≥0n \ge 0 be an integer. Suppose f:I→Rf : I \to \mathbb{R} has derivatives f′,f′′,…,f(n)f', f'', \dots, f^{(n)} on II. The nn-th Taylor polynomial of ff centered at aa is

Pn(x)=∑k=0nf(k)(a)k!(x−a)k.P_n(x) = \sum_{k=0}^{n} \frac{f^{(k)}(a)}{k!}(x-a)^k .

For x∈Ix \in I, the remainder is defined by

Rn(x):=f(x)−Pn(x).R_n(x) := f(x) - P_n(x).

Any formula expressing Rn(x)R_n(x) in closed form, typically involving f(n+1)f^{(n+1)} at an unspecified point between aa and xx, is called a form of the Taylor remainder.

Intuition

Think of the ordinary Mean Value Theorem as the case n=0n = 0: it says

f(x)−f(a)=f′(ξ)(x−a)f(x) - f(a) = f'(\xi)(x-a)

for some ξ\xi strictly between aa and xx. This is exactly R0(x)=f′(ξ)(x−a)R_0(x) = f'(\xi)(x-a), an expression for the error of the constant approximation P0(x)=f(a)P_0(x) = f(a) 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-nn Taylor polynomial, the error is captured by the (n+1)(n+1)-th derivative at an unknown point, scaled by (x−a)n+1/(n+1)!(x-a)^{n+1}/(n+1)! — exactly the next term the Taylor series would have, except evaluated at ξ\xi instead of aa. The Cauchy remainder tells the same qualitative story but keeps a second piece of information: not just that there is an intermediate point ξ\xi, but a factor (x−ξ)n(x-\xi)^n recording how close ξ\xi sits to the far endpoint xx. Geometrically, imagine sweeping a parameter tt from aa to xx and watching the "residual" f(x)−Pn(t)(x)f(x) - P_n^{(t)}(x), where Pn(t)P_n^{(t)} is the Taylor polynomial of ff centered at the moving point tt. 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 (x−t)n+1(x-t)^{n+1}, Cauchy uses the ruler (x−t)(x-t). Different rulers place the mean-value point ξ\xi in different (generally non-equal) locations, and yield algebraically different — but equally correct — closed forms for the same number Rn(x)R_n(x).

Figure
Two rulers sweeping from aa to xx, same residual, different remainder formulas
a x ξ₁ ξ₂ t sweeps a → x ruler (x−t)ⁿ⁺¹ → Lagrange gives ξ₁ ruler (x−t) → Cauchy gives ξ₂ R_n(x) same value, two exact formulas

The central theorem

TheoremLagrange and Cauchy Forms of the Taylor Remainder

Let a,x∈Ra, x \in \mathbb{R} with a≠xa \ne x, let II be the closed interval with endpoints aa and xx, and let n≥0n \ge 0 be an integer. Suppose: 1. f,f′,f′′,…,f(n)f, f', f'', \dots, f^{(n)} are continuous on II; 2. f(n+1)f^{(n+1)} exists at every point of the open interval between aa and xx. Then there exist points ξL,ξC\xi_L, \xi_C strictly between aa and xx (generally different from one another) such that, writing Rn(x)=f(x)−Pn(x)R_n(x) = f(x) - P_n(x) as above:

(Lagrange form.)

Rn(x)=f(n+1)(ξL)(n+1)! (x−a)n+1.R_n(x) = \frac{f^{(n+1)}(\xi_L)}{(n+1)!}\,(x-a)^{n+1}.

(Cauchy form.)

Rn(x)=f(n+1)(ξC)n! (x−ξC)n(x−a).R_n(x) = \frac{f^{(n+1)}(\xi_C)}{n!}\,(x-\xi_C)^n (x-a).
Proof

Fix aa and xx with a<xa<x (the case x<ax<a is identical with all inequalities reversed; the interval I=[a,x]I=[a,x] throughout, or [x,a][x,a] in the reversed case). Define, for t∈It \in I, the function

φ(t):=f(x)−∑k=0nf(k)(t)k!(x−t)k.\varphi(t) := f(x) - \sum_{k=0}^{n} \frac{f^{(k)}(t)}{k!}(x-t)^k .

This is the "residual" mentioned in the Intuition section: it is f(x)f(x) minus the degree-nn Taylor polynomial of ff centered at the moving point tt, evaluated at the fixed point xx. Note two facts immediately from the definition:

φ(x)=f(x)−f(x)=0,φ(a)=f(x)−Pn(x)=Rn(x).\varphi(x) = f(x) - f(x) = 0, \qquad \varphi(a) = f(x) - P_n(x) = R_n(x).

(The first equality holds because when t=xt=x every term with k≥1k\ge1 has factor (x−t)k=0(x-t)^k=0, leaving only the k=0k=0 term f(x)f(x).)

Step 1: Compute φ′(t)\varphi'(t). By hypothesis, f(k)f^{(k)} is continuous on II for 0≤k≤n0 \le k \le n and differentiable on the open interval (a,x)(a,x) for k≤nk \le n (since f(n+1)f^{(n+1)} exists there), so φ\varphi is continuous on [a,x][a,x] and differentiable on (a,x)(a,x). Differentiate the sum term by term using the product rule on each f(k)(t)k!(x−t)k\frac{f^{(k)}(t)}{k!}(x-t)^k:

ddt[f(k)(t)k!(x−t)k]=f(k+1)(t)k!(x−t)k−f(k)(t)(k−1)!(x−t)k−1,k≥1,\frac{d}{dt}\left[\frac{f^{(k)}(t)}{k!}(x-t)^k\right] = \frac{f^{(k+1)}(t)}{k!}(x-t)^k - \frac{f^{(k)}(t)}{(k-1)!}(x-t)^{k-1}, \qquad k \ge 1,

and for k=0k=0 the derivative is simply f′(t)f'(t). Summing over k=0,…,nk=0,\dots,n, the sum telescopes: the negative term at index kk is

−f(k)(t)(k−1)!(x−t)k−1,-\frac{f^{(k)}(t)}{(k-1)!}(x-t)^{k-1},

which is exactly the negative of the positive term produced at index k−1k-1... let us verify this telescoping explicitly rather than merely asserting it. Write S(t)=∑k=0nf(k)(t)k!(x−t)kS(t) = \sum_{k=0}^n \frac{f^{(k)}(t)}{k!}(x-t)^k. Then

S′(t)=f′(t)+∑k=1n[f(k+1)(t)k!(x−t)k−f(k)(t)(k−1)!(x−t)k−1].S'(t) = f'(t) + \sum_{k=1}^{n}\left[\frac{f^{(k+1)}(t)}{k!}(x-t)^k - \frac{f^{(k)}(t)}{(k-1)!}(x-t)^{k-1}\right].

The second sum, re-indexed, is

∑k=1nf(k+1)(t)k!(x−t)k  −  ∑k=1nf(k)(t)(k−1)!(x−t)k−1.\sum_{k=1}^{n}\frac{f^{(k+1)}(t)}{k!}(x-t)^k \;-\; \sum_{k=1}^{n}\frac{f^{(k)}(t)}{(k-1)!}(x-t)^{k-1}.

The second of these two sums, re-indexed with j=k−1j = k-1 running from 00 to n−1n-1, equals ∑j=0n−1f(j+1)(t)j!(x−t)j\sum_{j=0}^{n-1} \frac{f^{(j+1)}(t)}{j!}(x-t)^j. So

S′(t)=f′(t)+∑k=1nf(k+1)(t)k!(x−t)k−∑j=0n−1f(j+1)(t)j!(x−t)j.S'(t) = f'(t) + \sum_{k=1}^n \frac{f^{(k+1)}(t)}{k!}(x-t)^k - \sum_{j=0}^{n-1}\frac{f^{(j+1)}(t)}{j!}(x-t)^j.

The j=0j=0 term of the subtracted sum is f′(t)f'(t), which cancels the leading f′(t)f'(t). All other terms of the two sums (indices 1,…,n−11,\dots,n-1 appear in both) cancel identically, leaving only the k=nk=n term of the first sum:

S′(t)=f(n+1)(t)n!(x−t)n.S'(t) = \frac{f^{(n+1)}(t)}{n!}(x-t)^n.

Since φ(t)=f(x)−S(t)\varphi(t) = f(x) - S(t) is constant minus S(t)S(t),

φ′(t)=−S′(t)=−f(n+1)(t)n!(x−t)n,t∈(a,x).(∗)\varphi'(t) = -S'(t) = -\frac{f^{(n+1)}(t)}{n!}(x-t)^n, \qquad t \in (a,x). \tag{$\ast$}

Step 2 (Lagrange form): compare φ\varphi against ψ(t)=(x−t)n+1\psi(t) = (x-t)^{n+1}. The function ψ\psi is continuous on [a,x][a,x], differentiable on (a,x)(a,x) with ψ′(t)=−(n+1)(x−t)n\psi'(t) = -(n+1)(x-t)^n, and ψ′(t)≠0\psi'(t) \ne 0 for t∈(a,x)t \in (a,x) since x−t≠0x - t \ne 0 there. Also ψ(x)=0\psi(x) = 0 and ψ(a)=(x−a)n+1≠0\psi(a) = (x-a)^{n+1} \ne 0. By the Cauchy Mean Value Theorem applied to φ,ψ\varphi, \psi on [a,x][a,x], there exists ξL∈(a,x)\xi_L \in (a,x) with

[φ(x)−φ(a)]ψ′(ξL)=[ψ(x)−ψ(a)]φ′(ξL).\bigl[\varphi(x)-\varphi(a)\bigr]\psi'(\xi_L) = \bigl[\psi(x)-\psi(a)\bigr]\varphi'(\xi_L).

(This is the standard determinant form of the Cauchy Mean Value Theorem, valid without dividing by ψ(x)−ψ(a)\psi(x)-\psi(a) or ψ′(ξL)\psi'(\xi_L); we verify below that both these quantities are in fact nonzero here, so the more familiar quotient form applies too.) Substituting φ(x)=0\varphi(x)=0, φ(a)=Rn(x)\varphi(a) = R_n(x), ψ(x)=0\psi(x) = 0, ψ(a)=(x−a)n+1\psi(a) = (x-a)^{n+1}:

−Rn(x)⋅[−(n+1)(x−ξL)n]=−(x−a)n+1⋅φ′(ξL).-R_n(x)\cdot\bigl[-(n+1)(x-\xi_L)^n\bigr] = -(x-a)^{n+1}\cdot\varphi'(\xi_L).

Using (∗)(\ast) for φ′(ξL)\varphi'(\xi_L):

Rn(x)(n+1)(x−ξL)n=(x−a)n+1⋅f(n+1)(ξL)n!(x−ξL)n.R_n(x)(n+1)(x-\xi_L)^n = (x-a)^{n+1}\cdot \frac{f^{(n+1)}(\xi_L)}{n!}(x-\xi_L)^n.

Since ξL∈(a,x)\xi_L \in (a,x), x−ξL≠0x - \xi_L \ne 0, so we may divide both sides by (n+1)(x−ξL)n(n+1)(x-\xi_L)^n:

Rn(x)=f(n+1)(ξL)(n+1)!(x−a)n+1.R_n(x) = \frac{f^{(n+1)}(\xi_L)}{(n+1)!}(x-a)^{n+1}.

This is precisely the Lagrange form.

Step 3 (Cauchy form): compare φ\varphi against χ(t)=x−t\chi(t) = x - t. The function χ\chi is continuous on [a,x][a,x], differentiable everywhere with χ′(t)=−1≠0\chi'(t) = -1 \ne 0, and χ(x)=0\chi(x) = 0, χ(a)=x−a≠0\chi(a) = x - a \ne 0. Apply the Cauchy Mean Value Theorem to φ,χ\varphi,\chi on [a,x][a,x]: there exists ξC∈(a,x)\xi_C \in (a,x) with

[φ(x)−φ(a)]χ′(ξC)=[χ(x)−χ(a)]φ′(ξC).\bigl[\varphi(x)-\varphi(a)\bigr]\chi'(\xi_C) = \bigl[\chi(x)-\chi(a)\bigr]\varphi'(\xi_C).

Substitute φ(x)=0\varphi(x)=0, φ(a)=Rn(x)\varphi(a)=R_n(x), χ′(ξC)=−1\chi'(\xi_C) = -1, χ(x)−χ(a)=−(x−a)\chi(x)-\chi(a) = -(x-a):

−Rn(x)⋅(−1)=−(x−a)⋅φ′(ξC),-R_n(x)\cdot(-1) = -(x-a)\cdot \varphi'(\xi_C),

i.e. Rn(x)=−(x−a)φ′(ξC)R_n(x) = -(x-a)\varphi'(\xi_C). Using (∗)(\ast):

Rn(x)=−(x−a)⋅[−f(n+1)(ξC)n!(x−ξC)n]=f(n+1)(ξC)n!(x−ξC)n(x−a).R_n(x) = -(x-a)\cdot\left[-\frac{f^{(n+1)}(\xi_C)}{n!}(x-\xi_C)^n\right] = \frac{f^{(n+1)}(\xi_C)}{n!}(x-\xi_C)^n(x-a).

This is precisely the Cauchy form. ■\blacksquare

∎
Corollaryn=0n=0 recovers the Mean Value Theorem

For n=0n=0, both formulas reduce to f(x)−f(a)=f′(ξ)(x−a)f(x)-f(a) = f'(\xi)(x-a) for some ξ\xi between aa and xx — the ordinary Mean Value Theorem. Indeed with n=0n=0: Lagrange gives R0(x)=f′(ξL)(x−a)R_0(x) = f'(\xi_L)(x-a); Cauchy gives R0(x)=f′(ξC)(x−ξC)0(x−a)=f′(ξC)(x−a)R_0(x) = f'(\xi_C)(x-\xi_C)^0(x-a) = f'(\xi_C)(x-a). Since R0(x)=f(x)−f(a)R_0(x) = f(x)-f(a), both reduce to the same classical statement (with ξL\xi_L and ξC\xi_C each simply a mean-value point, not necessarily equal).

Worked examples

Example 1 (Lagrange remainder: bounding e0.6e^{0.6} using n=3n=3, centered at a=0a=0). Let f(x)=exf(x) = e^x, a=0a=0, x=0.6x=0.6, n=3n=3. All derivatives of ff equal exe^x, certainly continuous everywhere, so the hypotheses of the theorem hold on [0,0.6][0, 0.6]. The Taylor polynomial is

P3(x)=1+x+x22+x36.P_3(x) = 1 + x + \frac{x^2}{2} + \frac{x^3}{6}.

At x=0.6x = 0.6:

P3(0.6)=1+0.6+0.18+0.036=1.816.P_3(0.6) = 1 + 0.6 + 0.18 + 0.036 = 1.816.

By the Lagrange form with n=3n=3, there is ξL∈(0,0.6)\xi_L \in (0, 0.6) with

R3(0.6)=f(4)(ξL)4!(0.6)4=eξL24(0.1296).R_3(0.6) = \frac{f^{(4)}(\xi_L)}{4!}(0.6)^4 = \frac{e^{\xi_L}}{24}(0.1296).

Since ξL∈(0,0.6)\xi_L \in (0,0.6), 1=e0<eξL<e0.6<e0.7<2.021 = e^0 < e^{\xi_L} < e^{0.6} < e^{0.7} < 2.02 (using e0.7<2.02e^{0.7}<2.02, a standard bound since e0.7≈2.0138e^{0.7} \approx 2.0138). Hence

0.129624≤R3(0.6)<2.02×0.129624,\frac{0.1296}{24} \le R_3(0.6) < \frac{2.02 \times 0.1296}{24},

i.e.

0.00540≤R3(0.6)<0.01090.0.00540 \le R_3(0.6) < 0.01090.

So 1.816+0.00540≤e0.6<1.816+0.010901.816 + 0.00540 \le e^{0.6} < 1.816 + 0.01090, giving

1.8214≤e0.6<1.8269.1.8214 \le e^{0.6} < 1.8269.

The true value is e0.6=1.822118…e^{0.6} = 1.822118\ldots, 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 f(x)=(1+x)−1f(x) = (1+x)^{-1} so that f(x)=∑k=0n(−1)kxk+Rn(x)f(x) = \sum_{k=0}^n (-1)^k x^k + R_n(x) (the Taylor series of (1+x)−1(1+x)^{-1} about a=0a=0 has f(k)(0)=(−1)kk!f^{(k)}(0) = (-1)^k k!, so f(k)(0)k!=(−1)k\frac{f^{(k)}(0)}{k!} = (-1)^k). Fix x=−0.8x = -0.8 (an asymmetric, negative value close to −1-1, where the series is delicate) and take n=2n = 2. We have

f(k)(t)=(−1)kk!(1+t)−(k+1),f^{(k)}(t) = (-1)^k k! (1+t)^{-(k+1)},

so f(3)(t)=−6(1+t)−4f^{(3)}(t) = -6(1+t)^{-4}. All derivatives are continuous on the interval between 00 and −0.8-0.8 (i.e. [−0.8,0][-0.8, 0]), since 1+t∈[0.2,1]1+t \in [0.2, 1] never vanishes there; hypotheses of the theorem hold. Lagrange form gives ξL∈(−0.8,0)\xi_L \in (-0.8, 0) with

R2(−0.8)=f(3)(ξL)3!(−0.8)3=−6(1+ξL)−46(−0.512)=0.512 (1+ξL)−4.R_2(-0.8) = \frac{f^{(3)}(\xi_L)}{3!}(-0.8)^3 = \frac{-6(1+\xi_L)^{-4}}{6}(-0.512) = 0.512\,(1+\xi_L)^{-4}.

Since ξL∈(−0.8,0)\xi_L \in (-0.8, 0), 1+ξL∈(0.2,1)1+\xi_L \in (0.2, 1), so (1+ξL)−4∈(1,625)(1+\xi_L)^{-4} \in (1, 625). This bound is essentially useless: it only tells us R2(−0.8)∈(0.512,320)R_2(-0.8) \in (0.512, 320), while the true remainder is small (we compute it below). The Lagrange form, because it only uses the endpoint distance (x−a)3=(−0.8)3(x-a)^3 = (-0.8)^3 and not the position of ξ\xi relative to xx, cannot see that ξL\xi_L being close to x=−0.8x=-0.8 (where (1+ξL)−4(1+\xi_L)^{-4} is huge) is compensated by another factor — because Lagrange's formula has no such compensating factor. Cauchy form gives ξC∈(−0.8,0)\xi_C \in (-0.8,0) with

R2(−0.8)=f(3)(ξC)2!(−0.8−ξC)2(−0.8)=−6(1+ξC)−42(−0.8−ξC)2(−0.8).R_2(-0.8) = \frac{f^{(3)}(\xi_C)}{2!}(-0.8-\xi_C)^2(-0.8) = \frac{-6(1+\xi_C)^{-4}}{2}(-0.8-\xi_C)^2(-0.8).

Simplify: −62⋅(−0.8)=2.4\frac{-6}{2}\cdot(-0.8) = 2.4, so

R2(−0.8)=2.4 (1+ξC)−4(0.8+ξC)2=2.4(0.8+ξC1+ξC)2(1+ξC)−2.R_2(-0.8) = 2.4\,(1+\xi_C)^{-4}(0.8+\xi_C)^2 = 2.4\left(\frac{0.8+\xi_C}{1+\xi_C}\right)^2 (1+\xi_C)^{-2}.

Here the crucial point: as ξC→−0.8+\xi_C \to -0.8^+ (i.e. ξC\xi_C approaches the far endpoint, where (1+ξC)−1(1+\xi_C)^{-1} is largest), the factor (0.8+ξC)2→0(0.8+\xi_C)^2 \to 0, exactly compensating the blow-up of (1+ξC)−4(1+\xi_C)^{-4}. This is the mechanism by which the Cauchy form remains a useful, bounded estimate even when the Lagrange form is not. Concretely, since (1+ξC)∈(0.2,1)(1+\xi_C) \in (0.2,1) and (0.8+ξC)∈(0,0.8)(0.8+\xi_C) \in (0, 0.8), we get the crude bound

0≤(0.8+ξC)2(1+ξC)−4≤0.640.0016=400,0 \le (0.8+\xi_C)^2(1+\xi_C)^{-4} \le \frac{0.64}{0.0016} = 400,

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: f(−0.8)=(0.2)−1=5f(-0.8) = (0.2)^{-1} = 5, and P2(−0.8)=1−(−0.8)+(−0.8)2=1+0.8+0.64=2.44P_2(-0.8) = 1 - (-0.8) + (-0.8)^2 = 1+0.8+0.64 = 2.44, so

R2(−0.8)=5−2.44=2.56,R_2(-0.8) = 5 - 2.44 = 2.56,

an exact, finite, moderate number — consistent with both formulas (each merely expresses 2.562.56 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 xx near −1-1, the Cauchy remainder is the one used to prove convergence rigorously, since the Lagrange remainder's bound ∣x1+ξL∣\left|\frac{x}{1+\xi_L}\right|-type expressions blow up while the Cauchy form's ratio (x−ξC1+ξC)n\left(\frac{x-\xi_C}{1+\xi_C}\right)^n can be shown to stay bounded by ∣x∣n|x|^n using ∣ξC∣<∣x∣|\xi_C| < |x|.

CounterexampleWhy continuity of f(n)f^{(n)} on the closed interval is needed

The theorem requires f,f′,…,f(n)f, f', \dots, f^{(n)} continuous on the closed interval II between aa and xx, not merely on the open interval. Weaken this hypothesis and the conclusion can fail. Let n=0n = 0, a=0a = 0, x=1x = 1, and define

f(t)={t0<t≤11t=0.f(t) = \begin{cases} t & 0 < t \le 1 \\ 1 & t = 0.\end{cases}

Here ff is continuous on (0,1](0,1] and differentiable there with f′(t)=1f'(t) = 1, but ff is not continuous at the left endpoint t=0t=0 (since f(0)=1f(0)=1 but lim⁡t→0+f(t)=0\lim_{t\to0^+} f(t) = 0). This violates hypothesis (1) of the theorem (continuity of f=f(0)f = f^{(0)} on the closed interval [0,1][0,1]), while the derivative f′f' exists and is even continuous (constantly 11) on the open interval (0,1)(0,1). The conclusion (the Mean Value Theorem, i.e. n=0n=0 case) asserts the existence of ξ∈(0,1)\xi \in (0,1) with

f(1)−f(0)=f′(ξ)(1−0).f(1) - f(0) = f'(\xi)(1-0).

Compute the left side: f(1)−f(0)=1−1=0f(1) - f(0) = 1 - 1 = 0. But f′(ξ)=1f'(\xi) = 1 for every ξ∈(0,1)\xi \in (0,1), so the right side is 1⋅1=1≠01 \cdot 1 = 1 \ne 0. No such ξ\xi exists — the conclusion genuinely fails. The failure is entirely due to the discontinuity at the endpoint a=0a=0: 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 φ\varphi continuous on [a,x][a,x] to guarantee φ\varphi 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 n=0n=0 (the ordinary Mean Value Theorem) fails without it.

Scope, edge cases & common traps

SituationWhat holdsWhat can go wrong
f∈Cn+1f \in C^{n+1} on all of II (closed)Both Lagrange and Cauchy forms valid, ξ\xi's may differ—
f(n+1)f^{(n+1)} exists only on open interval, f(n)f^{(n)} discontinuous at an endpointNeither form guaranteedSee counterexample above
x<ax < aBoth formulas still hold, with ξ\xi between xx and aaSign of (x−a)n+1(x-a)^{n+1}, (x−ξ)n(x−a)(x-\xi)^n(x-a) must be tracked carefully
Estimating remainder near ∣x−a∣|x-a| large relative to radius of convergenceCauchy form often gives convergence when Lagrange does notApplying Lagrange's crude bound blindly, as in Example 2
ξL\xi_L and ξC\xi_CBoth exist, both lie strictly between aa and xxAssuming ξL=ξC\xi_L = \xi_C — false in general

The mathematician behind it

Origins · 1 minJoseph-Louis Lagrange and how this was discovered
JL
Joseph-Louis Lagrange
1736–1813 · Analysis and the calculus of variations in the era of Euler and Laplace

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 ε\varepsilon–δ\delta-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.

History
- 1772 — Lagrange proposes founding the calculus on Taylor series expansions, seeking an algebraic (not infinitesimal) remainder formula.
- 1797 — Lagrange's Théorie des fonctions analytiques develops the Lagrange remainder in the context of his program to avoid infinitesimals.
- 1821 — Cauchy's Cours d'Analyse rigorizes limits and continuity, laying groundwork for a fully rigorous mean value theorem.
- 1823 — Cauchy's lectures on the differential calculus present the Cauchy Mean Value Theorem and the alternative remainder form later named for him.
- Late 19th century — Both remainder forms become standard textbook tools once real analysis is fully axiomatized following Weierstrass and Dedekind.
Do the Lagrange and Cauchy remainder formulas always give the same numerical value for Rn(x)R_n(x)?

Yes — both are exact formulas for the same number Rn(x)=f(x)−Pn(x)R_n(x) = f(x) - P_n(x); they must agree numerically once you plug in the actual value of ξL\xi_L or ξC\xi_C that makes each formula true. What differs is the intermediate point: the ξL\xi_L that makes the Lagrange formula correct is generally not the same real number as the ξC\xi_C 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, φ(t)\varphi(t) (the residual) and a "ruler" function such as (x−t)n+1(x-t)^{n+1} or (x−t)(x-t), 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 ξ\xi. Using Rolle's theorem alone on φ\varphi would only give a point where φ′(ξ)=0\varphi'(\xi)=0, which is not what we want (indeed φ′\varphi' is generally never zero here); we need the ratio of φ\varphi'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 xx close to −1-1 requires bounding (1+ξL)−(n+1)(1+\xi_L)^{-(n+1)} where ξL\xi_L could be arbitrarily close to −1-1, giving no useful bound. The Cauchy form's extra factor (x−ξC)n(x-\xi_C)^n vanishes exactly where the derivative term blows up, and a short computation shows the ratio ∣x−ξC1+ξC∣<∣x∣\left|\frac{x-\xi_C}{1+\xi_C}\right| < |x| stays below 11, giving a genuine geometric decay bound. This is the standard textbook route to proving the binomial series converges on all of (−1,1)(-1,1) for every real exponent.

Does the theorem require f(n+1)f^{(n+1)} to be continuous?

No — only that f(n+1)f^{(n+1)} exists at every point of the open interval between aa and xx; continuity of f(n+1)f^{(n+1)} is not assumed or used in the proof. What is required is that f,f′,…,f(n)f, f', \dots, f^{(n)} be continuous on the closed interval, since the proof applies the Cauchy Mean Value Theorem to φ\varphi, 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, Rn(x)=∫axf(n+1)(t)n!(x−t)n dtR_n(x) = \int_a^x \frac{f^{(n+1)}(t)}{n!}(x-t)^n\,dt, requires f(n+1)f^{(n+1)} 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 f(n+1)f^{(n+1)} 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 φ(t)\varphi(t) using the moving-center Taylor polynomial rather than working directly with Rn(x)R_n(x)?

Because Rn(x)=f(x)−Pn(x)R_n(x) = f(x) - P_n(x) is a fixed number once a,x,na, x, n are fixed — it has no "tt" to differentiate with respect to. The trick is to replace the fixed center aa by a variable center tt, forming φ(t)=f(x)−(Taylor polynomial of f centered at t, evaluated at x)\varphi(t) = f(x) - (\text{Taylor polynomial of } f \text{ centered at } t, \text{ evaluated at } x), which is a genuine function of tt satisfying φ(x)=0\varphi(x) = 0 and φ(a)=Rn(x)\varphi(a) = R_n(x). Differentiating this function in tt is what produces the telescoping sum collapsing to the single clean expression φ′(t)=−f(n+1)(t)n!(x−t)n\varphi'(t) = -\frac{f^{(n+1)}(t)}{n!}(x-t)^n, which is the engine driving both remainder formulas.

Before this

Where this leads