evan's notes
cal 3discreteodeenv systems

On this page

  • Walkthrough
  • Remainders
  • Estimating the remainder
  • Integral estimate
  • Alternating-series estimate
  • Power series
  • Interval of convergence
  • Operations on power series
  • Partial sums and remainders
  • Example: N=3N=3N=3
  • Integral remainder bounds
  • Integral remainder estimate
  • Choosing NNN for a target error tolerance
  • Alternating series remainder estimate
  • Example: rounding to two decimal places
  • Power series
  • Radius and interval of convergence
  • General procedure for finding the interval
  • Example: finding the interval of convergence
  • Power series from the geometric series
  • Example: finding a series for 32+x2\frac{3}{2+x^2}2+x23​
  • Differentiating and integrating power series
  • Differentiating the geometric series
  • The exponential series

Intermediate Calculus

§2 Remainders and Power Series

Evan Luo · Sep 4, 2026

Intermediate Calculus

§2 Remainders and Power Series

Evan LuoSep 4, 2026

15 min read

Walkthrough

Remainders

An infinite series represents a sum that never ends:

S=a0+a1+a2+a3+⋯S = a_0 + a_1 + a_2 + a_3 + \cdotsS=a0​+a1​+a2​+a3​+⋯

Because we cannot add terms forever, we must stop at some finite cutoff index NNN. This splits the series into two parts:

S=SN+RNS = S_N + R_NS=SN​+RN​
  1. The partial sum SN=a0+a1+⋯+aNS_N = a_0 + a_1 + \cdots + a_NSN​=a0​+a1​+⋯+aN​, which is our calculated approximation.
  2. The remainder RN=aN+1+aN+2+⋯R_N = a_{N+1} + a_{N+2} + \cdotsRN​=aN+1​+aN+2​+⋯, which is the leftover tail we omitted.

A common point of confusion is what the index NNN represents. The subscript NNN marks the last included index, not the total count of terms. If the series starts at n=0n = 0n=0, the partial sum S3S_3S3​ contains four terms (a0,a1,a2,a3a_0, a_1, a_2, a_3a0​,a1​,a2​,a3​), and the remainder R3R_3R3​ starts at index N+1=4N+1 = 4N+1=4.

To know whether an approximation is reliable, we need to bound the size of this discarded remainder.


Estimating the remainder

How we estimate RNR_NRN​ depends on the behavior of the terms.

Integral estimate

For a convergent series S=∑n=0∞anS=\sum_{n=0}^{\infty}a_nS=∑n=0∞​an​ and an integer N≥0N\ge0N≥0, suppose an=f(n)a_n=f(n)an​=f(n) for n≥Nn\ge Nn≥N and fff is continuous, positive, and nonincreasing on [N,∞)[N,\infty)[N,∞). Then we can trap the omitted tail between areas under y=f(x)y=f(x)y=f(x):

∫N+1∞f(x) dx≤RN≤∫N∞f(x) dx\int_{N+1}^{\infty} f(x)\,dx \le R_N \le \int_N^{\infty} f(x)\,dx∫N+1∞​f(x)dx≤RN​≤∫N∞​f(x)dx
  • Starting the integral at N+1N+1N+1 places the curve beneath the rectangles, giving a lower bound.
  • Starting the integral at NNN shifts the reference frame so the curve stays above the rectangles, giving an upper bound.

If you are asked to guarantee that the error remains below a chosen tolerance ε\varepsilonε, focus on the upper bound: find an index NNN such that ∫N∞f(x) dx<ε\int_N^{\infty} f(x)\,dx < \varepsilon∫N∞​f(x)dx<ε. Because RNR_NRN​ is smaller than this integral, your error is guaranteed to be less than ε\varepsilonε.

Alternating-series estimate

For an alternating series whose magnitudes bn≥0b_n\ge0bn​≥0 are nonincreasing and approach 000, the Alternating Series Estimation Theorem bounds the truncation error by the first omitted magnitude:

∣S−SN∣≤bN+1|S - S_N| \le b_{N+1}∣S−SN​∣≤bN+1​

To estimate the true sum to a specific precision, calculate SNS_NSN​ and check whether the window [SN−bN+1,SN+bN+1][S_N - b_{N+1}, S_N + b_{N+1}][SN​−bN+1​,SN​+bN+1​] rounds unambiguously to your target decimal place.


Power series

A power series extends a polynomial to infinitely many terms and is centered at a constant aaa:

∑n=0∞cn(x−a)n=c0+c1(x−a)+c2(x−a)2+⋯\sum_{n=0}^{\infty} c_n(x-a)^n = c_0 + c_1(x-a) + c_2(x-a)^2 + \cdots∑n=0∞​cn​(x−a)n=c0​+c1​(x−a)+c2​(x−a)2+⋯

At the center x=ax = ax=a, every term with n≥1n \ge 1n≥1 becomes zero, leaving only c0c_0c0​. Therefore, every power series converges at its center.

For other values of xxx, convergence depends on how far xxx is from the center. This behavior is captured by the radius of convergence, RRR:

  • The series converges absolutely when ∣x−a∣<R|x - a| < R∣x−a∣<R.
  • The series diverges when ∣x−a∣>R|x - a| > R∣x−a∣>R.

Interval of convergence

To find the complete set of xxx-values where the series converges:

  1. Use the Ratio Test—or the Root Test when it fits better—to determine the interior condition ∣x−a∣<R|x-a|<R∣x−a∣<R.
  2. Rewrite that condition as the open interval (a−R,a+R)(a-R,a+R)(a−R,a+R).
  3. When RRR is finite, test each endpoint individually by substituting x=a−Rx=a-Rx=a−R and x=a+Rx=a+Rx=a+R into the original series. The test used to find the radius is generally inconclusive at the boundary, so a different numerical-series test decides whether each endpoint is included.

Operations on power series

Inside the open interval of convergence, power series can be treated like polynomials:

  • Algebraic substitutions: A rational function can often be reshaped into A1−u\frac{A}{1-u}1−uA​ to use the geometric series formula 11−u=∑n=0∞un\frac{1}{1-u} = \sum_{n=0}^{\infty} u^n1−u1​=∑n=0∞​un for ∣u∣<1|u| < 1∣u∣<1.
  • Calculus term by term: You can differentiate and integrate a power series term by term. The radius of convergence RRR remains unchanged, though endpoint behavior must be re-evaluated.

For example, differentiating ∑n=0∞xnn!\sum_{n=0}^{\infty} \frac{x^n}{n!}∑n=0∞​n!xn​ term by term returns the same series, and its value at x=0x=0x=0 is 111. These are the defining properties behind the familiar Maclaurin series for exe^xex.

Partial sums and remainders

A series contains infinitely many terms, but in practice we can only add finitely many. That limitation raises two practical questions:

  1. If we truncate a series, how large can the omitted part be?
  2. If the terms depend on an input variable xxx, for which values of xxx does the series converge?

While some series evaluate to a known closed form, such as

∑n=1∞1n2=π26,\sum_{n=1}^{\infty}\frac{1}{n^2}=\frac{\pi^2}{6}, n=1∑∞​n21​=6π2​,

other closely related series have no simple exact formula:

∑n=1∞1n3=?\sum_{n=1}^{\infty}\frac{1}{n^3}=? n=1∑∞​n31​=?

Error estimates allow us to quantify how closely a finite computation approximates the true infinite sum.

Example: N=3N=3N=3

Consider an infinite series written term by term from an initial index n=0n=0n=0:

S=a0+a1+a2+a3+a4+a5+⋯ .S=a_0+a_1+a_2+a_3+a_4+a_5+\cdots. S=a0​+a1​+a2​+a3​+a4​+a5​+⋯.

If we stop after the term with index 333, we obtain the partial sum

S3=a0+a1+a2+a3.S_3=a_0+a_1+a_2+a_3. S3​=a0​+a1​+a2​+a3​.

The difference between the total sum SSS and this finite approximation is the remainder R3R_3R3​:

R3=S−S3=a4+a5+a6+⋯ .R_3=S-S_3=a_4+a_5+a_6+\cdots. R3​=S−S3​=a4​+a5​+a6​+⋯.

Because a3a_3a3​ is already included inside S3S_3S3​, the first missing term in the remainder is a4a_4a4​.

Because this series begins at n=0n=0n=0, the partial sum S3S_3S3​ contains four terms. The subscript NNN denotes the last included index, not the total number of terms added.

More generally, stopping at index NNN produces

SN=a0+a1+⋯+aNS_N=a_0+a_1+\cdots+a_N SN​=a0​+a1​+⋯+aN​

and leaves the remainder

RN=S−SN=aN+1+aN+2+⋯=∑n=N+1∞an.\boxed{ R_N=S-S_N=a_{N+1}+a_{N+2}+\cdots =\sum_{n=N+1}^{\infty}a_n }. RN​=S−SN​=aN+1​+aN+2​+⋯=n=N+1∑∞​an​​.

The remainder RNR_NRN​ is the signed leftover between the true sum and the approximation. The error size is its absolute value, ∣RN∣|R_N|∣RN​∣. When every term ana_nan​ is positive, RN>0R_N>0RN​>0, so the remainder and the error size coincide. For alternating series, RNR_NRN​ can be positive or negative, requiring us to bound ∣RN∣|R_N|∣RN​∣.

Integral remainder bounds

Integral remainder estimate

When the terms of a series are generated by a continuous function,

an=f(n),a_n=f(n), an​=f(n),

we can bound the remainder geometrically using areas under the curve. For this comparison to hold, fff must satisfy three conditions:

  • continuous, ensuring the graph has no jumps or breaks;
  • positive, ensuring the area lies entirely above the xxx-axis;
  • decreasing, ensuring successive terms shrink in size.

The following diagram illustrates these comparisons for N=3N=3N=3, starting from n=0n=0n=0:

Lower bound for R3R_3R3​

With N=3N=3N=3, the first four rectangles are already included in S3S_3S3​. The remainder starts at N+1=4N+1=4N+1=4.

The series split at N equals 3A decreasing curve and rectangles a zero through a six. The rectangles a zero through a three are included in S three. The tail starts with a four at x equals four, which is N plus one.a0a_0a0​a1a_1a1​a2a_2a2​a3a_3a3​a4a_4a4​a5a_5a5​a6a_6a6​01234567N=3N=3N=3N+1=4N+1=4N+1=4
S3=a0+a1+a2+a3S_3=a_0+a_1+a_2+a_3S3​=a0​+a1​+a2​+a3​: already included
R3=a4+a5+a6+⋯R_3=a_4+a_5+a_6+\cdotsR3​=a4​+a5​+a6​+⋯: first omitted term onward
∫4∞f(x) dx≤R3\displaystyle \int_4^\infty f(x)\,dx\le R_3∫4∞​f(x)dx≤R3​

From x=4x=4x=4 onward, the curve lies below the tail rectangles. Its area is therefore a lower estimate of the tail.

Upper bound for R3R_3R3​

The gray rectangles stay in place for context. The first tail rectangle is still a4a_4a4​, but placing it over [3,4][3,4][3,4] makes the curve sit above it.

a0a_0a0​a1a_1a1​a2a_2a2​a3a_3a3​a4a_4a4​a5a_5a5​a6a_6a6​a7a_7a7​01234567N=3N=3N=3N+1=4N+1=4N+1=4
R3≤∫3∞f(x) dx\displaystyle R_3\le \int_3^\infty f(x)\,dxR3​≤∫3∞​f(x)dx

Starting the area at x=3x=3x=3 puts the curve above the same tail rectangles, so this area is an upper estimate.

The integral from 444 is the lower bound. The integral from 333 is the upper bound.

To see where the bounds come from, compare an individual term an=f(n)a_n=f(n)an​=f(n)—represented by a rectangle of width 111 and height f(n)f(n)f(n)—with the area under f(x)f(x)f(x) over unit intervals:

  • Comparing to the unit interval to the right gives

    ∫nn+1f(x) dx≤an.\int_n^{n+1}f(x)\,dx\le a_n. ∫nn+1​f(x)dx≤an​.
  • Comparing to the unit interval to the left gives

    an≤∫n−1nf(x) dx.a_n\le\int_{n-1}^{n}f(x)\,dx. an​≤∫n−1n​f(x)dx.

Returning to the N=3N=3N=3 diagram, the remainder tail starts at n=4n=4n=4:

R3=a4+a5+a6+⋯ .R_3=a_4+a_5+a_6+\cdots. R3​=a4​+a5​+a6​+⋯.

Summing the single-rectangle inequalities from n=N+1n=N+1n=N+1 to ∞\infty∞ yields the integral remainder estimate:

∫N+1∞f(x) dx≤RN≤∫N∞f(x) dx.\boxed{ \int_{N+1}^{\infty}f(x)\,dx \le R_N \le \int_N^{\infty}f(x)\,dx }. ∫N+1∞​f(x)dx≤RN​≤∫N∞​f(x)dx​.

The difference in limits reflects the boundary between the included and omitted terms:

SN ends at aN,RN begins at aN+1.S_N\text{ ends at }a_N, \qquad R_N\text{ begins at }a_{N+1}. SN​ ends at aN​,RN​ begins at aN+1​.
  • Integrating from x=4x=4x=4 places the curve below the tail rectangles, producing an area strictly smaller than the remainder:

    ∫4∞f(x) dx≤R3.\int_4^{\infty}f(x)\,dx\le R_3. ∫4∞​f(x)dx≤R3​.
  • Integrating from x=3x=3x=3 shifts the reference frame so the curve stays above those same rectangles, producing an area larger than the remainder:

    R3≤∫3∞f(x) dx.R_3\le\int_3^{\infty}f(x)\,dx. R3​≤∫3∞​f(x)dx.

Here, lower bound denotes a value smaller than R3R_3R3​. The integral starting farther right covers less total area, which is why ∫N+1∞f(x) dx\int_{N+1}^\infty f(x)\,dx∫N+1∞​f(x)dx forms the lower bound and ∫N∞f(x) dx\int_N^\infty f(x)\,dx∫N∞​f(x)dx forms the upper bound.

Choosing NNN for a target error tolerance

Let ε\varepsilonε (epsilon) be the largest error we are willing to allow. We do not need to compute RNR_NRN​ directly; it suffices to choose an index NNN that forces the upper bound below ε\varepsilonε:

∫N∞f(x) dx<ε.\int_N^{\infty}f(x)\,dx<\varepsilon. ∫N∞​f(x)dx<ε.

Because RNR_NRN​ is bounded above by this integral, satisfying this inequality guarantees

0<RN<ε.0<R_N<\varepsilon. 0<RN​<ε.

Evaluating the improper integral and solving the inequality for NNN gives a sufficient cutoff that guarantees the requested error tolerance.

Alternating series remainder estimate

An alternating series has terms that alternate in sign:

S=b0−b1+b2−b3+⋯=∑n=0∞(−1)nbn.S=b_0-b_1+b_2-b_3+\cdots =\sum_{n=0}^{\infty}(-1)^n b_n. S=b0​−b1​+b2​−b3​+⋯=n=0∑∞​(−1)nbn​.

If the positive magnitudes bnb_nbn​ decrease monotonically toward zero,

bn≥0,bn+1≤bn,lim⁡n→∞bn=0,b_n\ge0, \qquad b_{n+1}\le b_n, \qquad \lim_{n\to\infty}b_n=0, bn​≥0,bn+1​≤bn​,n→∞lim​bn​=0,

the series converges by the Alternating Series Test. Successive partial sums oscillate around the true sum SSS, each step bringing the approximation closer. Consequently, the truncation error is bounded by the magnitude of the first omitted term:

∣S−SN∣≤bN+1.\boxed{|S-S_N|\le b_{N+1}}. ∣S−SN​∣≤bN+1​​.

This result is the Alternating Series Estimation Theorem.

Example: rounding to two decimal places

Consider the alternating series

S=∑n=0∞(−1)n4n(n+1)=1−18+148−1256+⋯ .S=\sum_{n=0}^{\infty}\frac{(-1)^n}{4^n(n+1)} =1-\frac18+\frac1{48}-\frac1{256}+\cdots. S=n=0∑∞​4n(n+1)(−1)n​=1−81​+481​−2561​+⋯.

Evaluating the partial sum through index N=3N=3N=3 gives

S3=1−18+148−1256=0.891927083….\begin{aligned} S_3 &=1-\frac18+\frac1{48}-\frac1{256}\\ &=0.891927083\ldots. \end{aligned} S3​​=1−81​+481​−2561​=0.891927083….​

The first omitted term corresponds to n=4n=4n=4:

b4=144(5)=11280=0.00078125.b_4=\frac{1}{4^4(5)}=\frac1{1280}=0.00078125. b4​=44(5)1​=12801​=0.00078125.

By the estimation theorem, the true sum SSS lies within b4b_4b4​ of S3S_3S3​:

0.891145833…≤S≤0.892708333….0.891145833\ldots \le S \le 0.892708333\ldots. 0.891145833…≤S≤0.892708333….

Because both the upper and lower bounds round to 0.890.890.89, the estimate

S≈0.89\boxed{S\approx0.89} S≈0.89​

is guaranteed correct to two decimal places.

Stopping one term earlier at N=2N=2N=2 would not provide enough precision:

S2=0.895833333…,∣S−S2∣≤1256=0.00390625.S_2=0.895833333\ldots, \qquad |S-S_2|\le\frac1{256}=0.00390625. S2​=0.895833333…,∣S−S2​∣≤2561​=0.00390625.

This error interval spans from roughly 0.89190.89190.8919 to 0.89970.89970.8997, which contains values rounding to 0.890.890.89 as well as values rounding to 0.900.900.90. Thus, N=3N=3N=3 is necessary to determine the second decimal place unambiguously.

Power series

A polynomial terminates after a finite degree:

c0+c1x+c2x2+⋯+ckxk.c_0+c_1x+c_2x^2+\cdots+c_kx^k. c0​+c1​x+c2​x2+⋯+ck​xk.

A power series extends this concept to infinitely many terms:

c0+c1x+c2x2+⋯=∑n=0∞cnxn.c_0+c_1x+c_2x^2+\cdots =\sum_{n=0}^{\infty}c_nx^n. c0​+c1​x+c2​x2+⋯=n=0∑∞​cn​xn.

More generally, a power series can be centered at any real number aaa:

∑n=0∞cn(x−a)n=c0+c1(x−a)+c2(x−a)2+⋯.\boxed{ \sum_{n=0}^{\infty}c_n(x-a)^n =c_0+c_1(x-a)+c_2(x-a)^2+\cdots }. n=0∑∞​cn​(x−a)n=c0​+c1​(x−a)+c2​(x−a)2+⋯​.

In this expression:

  • xxx is the independent variable;
  • aaa is a constant called the center;
  • cnc_ncn​ is the coefficient of the nnnth power.

At the center x=ax=ax=a, every term with n≥1n\ge1n≥1 vanishes, leaving only c0c_0c0​. Therefore, every power series converges at its center.

Radius and interval of convergence

For values of x≠ax\ne ax=a, convergence depends on the distance ∣x−a∣|x-a|∣x−a∣ from the center. For any power series, exactly one of three cases occurs:

  1. The series converges only at the center x=ax=ax=a.
  2. The series converges for all real numbers xxx.
  3. There exists a real number R>0R>0R>0, called the radius of convergence, such that the series converges absolutely when ∣x−a∣<R|x-a|<R∣x−a∣<R and diverges when ∣x−a∣>R|x-a|>R∣x−a∣>R:
∣x−a∣<R⟺a−R<x<a+R.|x-a|<R \quad\Longleftrightarrow\quad a-R<x<a+R. ∣x−a∣<R⟺a−R<x<a+R.

When RRR is finite, the condition ∣x−a∣<R|x-a|<R∣x−a∣<R does not specify whether convergence holds at the boundary points x=a−Rx=a-Rx=a−R and x=a+Rx=a+Rx=a+R. Testing these endpoints individually determines the complete interval of convergence.

General procedure for finding the interval

To find the full set of values where a power series converges:

  1. Identify the center aaa.
  2. Apply the ratio test (or root test) to find the condition ∣x−a∣<R|x-a|<R∣x−a∣<R that ensures absolute convergence.
  3. Rewrite ∣x−a∣<R|x-a|<R∣x−a∣<R as the open interval (a−R,a+R)(a-R, a+R)(a−R,a+R).
  4. Substitute each endpoint, x=a−Rx=a-Rx=a−R and x=a+Rx=a+Rx=a+R, into the original series to obtain numerical series.
  5. Test each endpoint series separately, including an endpoint in the interval if and only if its series converges.

Example: finding the interval of convergence

Find the interval of convergence for

∑n=1∞(x−3)nn.\sum_{n=1}^{\infty}\frac{(x-3)^n}{n}. n=1∑∞​n(x−3)n​.

The center is a=3a=3a=3. At x=3x=3x=3, every term equals 000, so the series converges.

To determine convergence for x≠3x\ne3x=3, use the Ratio Test. Recall that for a series ∑an\sum a_n∑an​, the Ratio Test evaluates the limit of consecutive term ratios:

  • if the limit is strictly less than 111, the series converges absolutely;
  • if the limit is strictly greater than 111, the series diverges;
  • if the limit is equal to 111, the test is inconclusive and another test must be used.

Applying this to the terms

an=(x−3)nn.a_n=\frac{(x-3)^n}{n}. an​=n(x−3)n​.

the ratio becomes

∣an+1an∣=∣(x−3)nn+1∣⟶∣x−3∣.\begin{aligned} \left|\frac{a_{n+1}}{a_n}\right| &=\left|(x-3)\frac{n}{n+1}\right|\\ &\longrightarrow |x-3|. \end{aligned} ​an​an+1​​​​=​(x−3)n+1n​​⟶∣x−3∣.​

The series converges absolutely when this limit is strictly less than 111:

∣x−3∣<1,|x-3|<1, ∣x−3∣<1,

which simplifies to

2<x<4.2<x<4. 2<x<4.

The radius of convergence is R=1R=1R=1. Now test the boundary points x=2x=2x=2 and x=4x=4x=4:

  • At x=2x=2x=2, the series becomes

    ∑n=1∞(−1)nn,\sum_{n=1}^{\infty}\frac{(-1)^n}{n}, n=1∑∞​n(−1)n​,

    which converges by the Alternating Series Test. Because the corresponding series of absolute values ∑1n\sum \frac{1}{n}∑n1​ diverges, this convergence is conditionally convergent. The point x=2x=2x=2 is included in the interval.

  • At x=4x=4x=4, the series becomes

    ∑n=1∞1n,\sum_{n=1}^{\infty}\frac1n, n=1∑∞​n1​,

    which is the divergent harmonic series. The point x=4x=4x=4 is excluded.

Combining the interior and the valid endpoint gives the interval of convergence:

[2,4).\boxed{[2,4)}. [2,4)​.

The bracket at 222 denotes inclusion, while the parenthesis at 444 denotes exclusion.

Power series from the geometric series

Many power series can be constructed directly from the geometric series formula without applying the ratio test from scratch:

11−u=∑n=0∞un,∣u∣<1.\frac{1}{1-u}=\sum_{n=0}^{\infty}u^n, \qquad |u|<1. 1−u1​=n=0∑∞​un,∣u∣<1.

To find a power series for a rational function, rearrange the algebraic expression into the form A1−u\frac{A}{1-u}1−uA​, identify the expression acting as uuu, and substitute it into the summation.

Example: finding a series for 32+x2\frac{3}{2+x^2}2+x23​

Find a power series representation for

f(x)=32+x2.f(x)=\frac{3}{2+x^2}. f(x)=2+x23​.

First, factor the denominator to match the geometric template 1−u1-u1−u:

32+x2=3211+x2/2=3211−(−x2/2).\frac{3}{2+x^2} =\frac32\frac{1}{1+x^2/2} =\frac32\frac{1}{1-(-x^2/2)}. 2+x23​=23​1+x2/21​=23​1−(−x2/2)1​.

Here, the variable expression is

u=−x22.u=-\frac{x^2}{2}. u=−2x2​.

Substituting uuu into the geometric expansion:

32+x2=32∑n=0∞(−x22)n=∑n=0∞3(−1)n2n+1x2n.\begin{aligned} \frac{3}{2+x^2} &=\frac32\sum_{n=0}^{\infty} \left(-\frac{x^2}{2}\right)^n\\ &=\boxed{ \sum_{n=0}^{\infty} \frac{3(-1)^n}{2^{n+1}}x^{2n} }. \end{aligned} 2+x23​​=23​n=0∑∞​(−2x2​)n=n=0∑∞​2n+13(−1)n​x2n​.​

This geometric representation is valid whenever ∣u∣<1|u|<1∣u∣<1:

∣−x22∣<1⟺∣x∣<2.\left|-\frac{x^2}{2}\right|<1 \quad\Longleftrightarrow\quad |x|<\sqrt2. ​−2x2​​<1⟺∣x∣<2​.

At the endpoints x=±2x=\pm\sqrt2x=±2​, the terms (−1)n32(-1)^n\frac{3}{2}(−1)n23​ do not approach zero, so the series diverges there. The interval of convergence is

(−2,2).\boxed{(-\sqrt2,\sqrt2)}. (−2​,2​)​.

Because the variable appears as x2nx^{2n}x2n, every odd power has coefficient zero. For instance, the term involving x6x^6x6 corresponds to 2n=62n=62n=6, which is n=3n=3n=3.

Differentiating and integrating power series

Inside its open interval of convergence, a power series can be differentiated or integrated term by term, just like a polynomial.

If

f(x)=∑n=0∞cn(x−a)n,f(x)=\sum_{n=0}^{\infty}c_n(x-a)^n, f(x)=n=0∑∞​cn​(x−a)n,

differentiating each term gives

f′(x)=∑n=1∞ncn(x−a)n−1.\boxed{ f'(x)=\sum_{n=1}^{\infty}n c_n(x-a)^{n-1} }. f′(x)=n=1∑∞​ncn​(x−a)n−1​.

Reindexing the sum so that the exponent begins at 000 yields the equivalent form:

f′(x)=∑n=0∞(n+1)cn+1(x−a)n.f'(x)=\sum_{n=0}^{\infty}(n+1)c_{n+1}(x-a)^n. f′(x)=n=0∑∞​(n+1)cn+1​(x−a)n.

Similarly, integrating term by term introduces an arbitrary constant CCC:

∫f(x) dx=C+∑n=0∞cnn+1(x−a)n+1.\boxed{ \int f(x)\,dx =C+\sum_{n=0}^{\infty} \frac{c_n}{n+1}(x-a)^{n+1} }. ∫f(x)dx=C+n=0∑∞​n+1cn​​(x−a)n+1​.

Term-by-term differentiation and integration preserve the original radius of convergence RRR. However, behavior at the endpoints a±Ra\pm Ra±R can change, so endpoints must be re-evaluated after differentiating or integrating.

Differentiating the geometric series

Starting from the standard geometric series,

11−x=∑n=0∞xn,∣x∣<1,\frac{1}{1-x}=\sum_{n=0}^{\infty}x^n, \qquad |x|<1, 1−x1​=n=0∑∞​xn,∣x∣<1,

differentiating both sides with respect to xxx gives:

1(1−x)2=∑n=1∞nxn−1=∑n=0∞(n+1)xn,∣x∣<1.\boxed{ \frac{1}{(1-x)^2} =\sum_{n=1}^{\infty}n x^{n-1} =\sum_{n=0}^{\infty}(n+1)x^n }, \qquad |x|<1. (1−x)21​=n=1∑∞​nxn−1=n=0∑∞​(n+1)xn​,∣x∣<1.

The exponential series

Consider the series

f(x)=∑n=0∞xnn!.f(x)=\sum_{n=0}^{\infty}\frac{x^n}{n!}. f(x)=n=0∑∞​n!xn​.

Differentiating term by term:

f′(x)=∑n=1∞nxn−1n!=∑n=1∞xn−1(n−1)!=∑n=0∞xnn!=f(x).\begin{aligned} f'(x) &=\sum_{n=1}^{\infty}n\frac{x^{n-1}}{n!}\\ &=\sum_{n=1}^{\infty}\frac{x^{n-1}}{(n-1)!}\\ &=\sum_{n=0}^{\infty}\frac{x^n}{n!}\\ &=f(x). \end{aligned} f′(x)​=n=1∑∞​nn!xn−1​=n=1∑∞​(n−1)!xn−1​=n=0∑∞​n!xn​=f(x).​

The function satisfies the differential equation f′(x)=f(x)f'(x)=f(x)f′(x)=f(x) with initial condition f(0)=1f(0)=1f(0)=1. The unique function satisfying these conditions is the natural exponential function, establishing the identity

ex=∑n=0∞xnn!\boxed{e^x=\sum_{n=0}^{\infty}\frac{x^n}{n!}} ex=n=0∑∞​n!xn​​

for all real numbers xxx.

Source: https://notes.ohevan.com/notes/intermediate-calculus/02-remainders-and-power-series

© 2026 Evan Luo. All rights reserved.

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·Last edited Sep 20, 2026
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© 2026 Evan Luo. All rights reserved.