Unit 10 Notes: Taylor & Maclaurin Series (AP Calculus BC)

Taylor Polynomial Approximations

What a Taylor polynomial is

A Taylor polynomial is a polynomial that imitates a function near a specific point. The key idea is: if you match enough derivative information at a point, a polynomial can “hug” the function extremely well in a neighborhood of that point.

Concretely, suppose you care about a function f(x)f(x) near x=ax=a. You build a polynomial Pn(x)P_n(x) of degree nn so that it matches:

  • the function value: Pn(a)=f(a)P_n(a)=f(a)
  • the first derivative: Pn(a)=f(a)P_n'(a)=f'(a)
  • the second derivative: Pn(a)=f(a)P_n''(a)=f''(a)
  • and so on, up through the nnth derivative.

This creates a polynomial approximation that is “locally tuned” to the function’s behavior at aa.

Why Taylor polynomials matter

Taylor polynomials matter because they let you:

  • Approximate values of complicated functions using simple arithmetic.
  • Estimate errors (how accurate your approximation is) using rigorous bounds.
  • Set up Taylor series (infinite versions of these polynomials), which power many convergence and representation questions in Unit 10.

A good mental model: a Taylor polynomial is like taking a “snapshot” of the function at x=ax=a, including slope, concavity, and higher-order shape, then reconstructing the nearby curve using a polynomial.

How the Taylor polynomial formula works

The nnth-degree Taylor polynomial for f(x)f(x) about x=ax=a is

Pn(x)=k=0nf(k)(a)k!(xa)kP_n(x)=\sum_{k=0}^{n} \frac{f^{(k)}(a)}{k!}(x-a)^k

Here:

  • f(k)(a)f^{(k)}(a) means the kkth derivative evaluated at aa.
  • k!k! (factorial) normalizes the coefficients.
  • (xa)k(x-a)^k shifts the approximation to be centered at aa.

When a=0a=0, it’s called a Maclaurin polynomial (a special case of Taylor).

Notation you’ll see (and how to translate it)
IdeaCommon notationMeaning
nnth Taylor polynomial about aaPn(x)P_n(x) or Tn(x)T_n(x)Polynomial approximation of degree nn
Taylor series about aan=0cn(xa)n\sum_{n=0}^{\infty} c_n(x-a)^nInfinite power series centered at aa
Maclaurin polynomial/seriesSame but with a=0a=0Centered at 00
Example 1: Build a Maclaurin polynomial for sin(x)\sin(x)

You often know derivative cycles for trig functions, so sin(x)\sin(x) is a classic.

We compute derivatives and evaluate at 00:

  • f(x)=sin(x)f(x)=\sin(x) so f(0)=0f(0)=0
  • f(x)=cos(x)f'(x)=\cos(x) so f(0)=1f'(0)=1
  • f(x)=sin(x)f''(x)=-\sin(x) so f(0)=0f''(0)=0
  • f(x)=cos(x)f'''(x)=-\cos(x) so f(0)=1f'''(0)=-1
  • f(4)(x)=sin(x)f^{(4)}(x)=\sin(x) so f(4)(0)=0f^{(4)}(0)=0
  • f(5)(x)=cos(x)f^{(5)}(x)=\cos(x) so f(5)(0)=1f^{(5)}(0)=1

The degree-5 Maclaurin polynomial is

P5(x)=k=05f(k)(0)k!xkP_5(x)=\sum_{k=0}^{5} \frac{f^{(k)}(0)}{k!}x^k

Only the nonzero derivative values contribute:

P5(x)=xx33!+x55!P_5(x)=x-\frac{x^3}{3!}+\frac{x^5}{5!}

So near 00,

sin(x)xx36+x5120\sin(x)\approx x-\frac{x^3}{6}+\frac{x^5}{120}

A common mistake here is forgetting factorials (for example, writing xx33x-\frac{x^3}{3} instead of xx36x-\frac{x^3}{6}).

Example 2: Use a Taylor polynomial to approximate a value

Approximate e0.1e^{0.1} using the degree-3 Maclaurin polynomial for exe^x.

For f(x)=exf(x)=e^x, every derivative is exe^x, so f(k)(0)=1f^{(k)}(0)=1 for all kk. Thus

P3(x)=1+x+x22!+x33!P_3(x)=1+x+\frac{x^2}{2!}+\frac{x^3}{3!}

Plug in x=0.1x=0.1:

e0.11+0.1+0.122+0.136e^{0.1}\approx 1+0.1+\frac{0.1^2}{2}+\frac{0.1^3}{6}

Compute:

  • 0.12=0.010.1^2=0.01 so 0.012=0.005\frac{0.01}{2}=0.005
  • 0.13=0.0010.1^3=0.001 so 0.00160.0001667\frac{0.001}{6}\approx 0.0001667

So

e0.11.1051667e^{0.1}\approx 1.1051667

This is the basic move behind many AP questions: “Use a Taylor polynomial of degree nn about aa to approximate f(b)f(b).”

Exam Focus
  • Typical question patterns:
    • “Find the Taylor polynomial of degree nn for f(x)f(x) about x=ax=a.”
    • “Use a Maclaurin polynomial to approximate f(c)f(c) and show work.”
    • “Given values of derivatives at aa, write Pn(x)P_n(x) (no re-differentiation needed).”
  • Common mistakes:
    • Mixing up aa and xx (writing powers of xx when the center is a0a\neq 0; you need (xa)k(x-a)^k).
    • Forgetting factorials in coefficients.
    • Using a polynomial beyond its “safe zone” (approximating far from aa without any error reasoning).

Lagrange Error Bound

What the error term is

A Taylor polynomial is an approximation, so you need a way to quantify the gap:

Rn(x)=f(x)Pn(x)R_n(x)=f(x)-P_n(x)

This difference Rn(x)R_n(x) is called the **remainder** (or error) after using the degree-nn Taylor polynomial.

Why the Lagrange error bound matters

The AP exam often asks for a guaranteed bound on the error: not “what the exact error is” (usually hard), but “how big it could be at most.” The Lagrange Error Bound gives a clean way to do that if you can bound the next derivative.

This is especially important when you approximate numerical values (like sin(0.2)\sin(0.2) or e0.1e^{0.1}) and must justify the number of correct decimal places.

The Lagrange Error Bound formula (how it works)

If you use the degree-nn Taylor polynomial about aa, and if f(n+1)(t)f^{(n+1)}(t) exists on the interval between aa and xx, then

Rn(x)M(n+1)!xan+1|R_n(x)|\le \frac{M}{(n+1)!}|x-a|^{n+1}

where MM is any number such that

f(n+1)(t)M|f^{(n+1)}(t)|\le M

for all tt between aa and xx.

Interpretation:

  • The error depends on the size of the next derivative (captured by MM).
  • The error shrinks quickly when xa|x-a| is small and nn is larger, because factorials grow fast.

A subtle but crucial point: the bound uses the maximum possible size of the n+1n+1 derivative on the interval. If you underestimate MM, your “bound” may be false.

Example 1: Bound the error for approximating e0.1e^{0.1} with P3(x)P_3(x)

We previously used P3(x)P_3(x) about a=0a=0 to approximate e0.1e^{0.1}. Now bound the error.

Here f(x)=exf(x)=e^x and n=3n=3, so we need f(4)(x)=exf^{(4)}(x)=e^x.

On the interval between 00 and 0.10.1, the maximum of ete^t occurs at t=0.1t=0.1 (because ete^t increases). So we can take

M=e0.1M=e^{0.1}

Then

R3(0.1)e0.14!0.14|R_3(0.1)|\le \frac{e^{0.1}}{4!}|0.1|^4

Compute pieces:

  • 4!=244!=24
  • 0.14=0.00010.1^4=0.0001

So

R3(0.1)e0.1240.0001|R_3(0.1)|\le \frac{e^{0.1}}{24}\cdot 0.0001

Since e0.11.1052e^{0.1}\approx 1.1052, the bound is approximately

R3(0.1)1.1052240.00010.0000046|R_3(0.1)|\le \frac{1.1052}{24}\cdot 0.0001\approx 0.0000046

So the approximation is accurate to about the millionths place (and certainly to 4 decimal places).

Example 2: Choosing MM correctly

Suppose you approximate sin(x)\sin(x) near 00 using P5(x)P_5(x) and want an error bound at x=0.3x=0.3.

Here n=5n=5, so we need the 6th derivative. The derivatives of sin(x)\sin(x) cycle, and the 6th derivative is sin(x)-\sin(x). So

f(6)(t)=sin(t)1|f^{(6)}(t)|=|\sin(t)|\le 1

for all real tt. You can safely choose M=1M=1.

Then

R5(0.3)16!0.36|R_5(0.3)|\le \frac{1}{6!}|0.3|^6

This is usually enough for AP justification; you don’t need to fully decimal-evaluate unless asked.

Exam Focus
  • Typical question patterns:
    • “Use the Lagrange Error Bound to find an upper bound on the error when approximating f(x)f(x) by Pn(x)P_n(x) at x=bx=b.”
    • “Find the degree nn needed so the approximation error is less than a given tolerance.”
    • “Justify that the approximation is within 0.0010.001 (or has a certain number of correct decimals).”
  • Common mistakes:
    • Using f(n)f^{(n)} instead of f(n+1)f^{(n+1)} in the bound.
    • Picking MM from the wrong interval (you must use the interval between aa and the target xx).
    • Treating the bound as the exact error; it’s only a guaranteed maximum.

Radius and Interval of Convergence of Power Series

What a power series is

A power series is an infinite polynomial-like expression, typically centered at some point aa:

n=0cn(xa)n\sum_{n=0}^{\infty} c_n(x-a)^n

For each fixed xx, this becomes an infinite series of numbers. The big question is: for which xx values does it converge?

Why convergence matters

If a power series converges, it defines a function (you can plug in xx and get a finite value). If it diverges, it doesn’t represent a meaningful value there.

On the AP exam, you’re often asked to:

  • find the radius of convergence (how far from the center it converges)
  • find the interval of convergence (the exact set of xx values, including endpoint checks)
The radius vs. the interval (what’s the difference?)

For many power series centered at aa, there exists a number RR such that:

  • the series converges for xa<R|x-a|<R
  • the series diverges for xa>R|x-a|>R
  • at xa=R|x-a|=R (the endpoints), convergence must be checked separately

That RR is the radius of convergence. The interval of convergence is typically

(aR,a+R)(a-R,a+R)

plus whatever endpoints actually converge.

How to find the radius (Ratio Test is the workhorse)

The most common method is the Ratio Test applied to the general term.

If your series is

n=0un\sum_{n=0}^{\infty} u_n

and

L=limnun+1unL=\lim_{n\to\infty} \left|\frac{u_{n+1}}{u_n}\right|

then:

  • if L<1L<1, the series converges
  • if L>1L>1 (or infinite), the series diverges
  • if L=1L=1, the test is inconclusive

In a power series, unu_n depends on xx, so the Ratio Test usually produces an inequality in xx that gives xa<R|x-a|<R.

Example 1: Find the interval of convergence

Find the interval of convergence of

n=1(x2)nn\sum_{n=1}^{\infty} \frac{(x-2)^n}{n}

Let

un=(x2)nnu_n=\frac{(x-2)^n}{n}

Compute the ratio:

un+1un=(x2)n+1n+1n(x2)n=x2nn+1\left|\frac{u_{n+1}}{u_n}\right|=\left|\frac{(x-2)^{n+1}}{n+1}\cdot \frac{n}{(x-2)^n}\right|=\left|x-2\right|\cdot \frac{n}{n+1}

Take the limit:

L=limnx2nn+1=x2L=\lim_{n\to\infty} \left|x-2\right|\cdot \frac{n}{n+1}=|x-2|

Convergence requires x2<1|x-2|<1, so the radius is R=1R=1 and the “open interval” is 1<x<31<x<3.

Now check endpoints:

  • At x=3x=3: series becomes n=11n\sum_{n=1}^{\infty} \frac{1}{n}, which diverges (harmonic series).
  • At x=1x=1: series becomes n=1(1)nn\sum_{n=1}^{\infty} \frac{(-1)^n}{n}, which converges (alternating harmonic).

So the interval of convergence is

[1,3)[1,3)

Example 2: A power series with factorials

Find the radius of convergence of

n=0n!3n(x+1)n\sum_{n=0}^{\infty} \frac{n!}{3^n}(x+1)^n

Let

un=n!3n(x+1)nu_n=\frac{n!}{3^n}(x+1)^n

Ratio:

un+1un=(n+1)!3n+1(x+1)n+13nn!1(x+1)n=n+13(x+1)\left|\frac{u_{n+1}}{u_n}\right|=\left|\frac{(n+1)!}{3^{n+1}}(x+1)^{n+1}\cdot \frac{3^n}{n!}\cdot \frac{1}{(x+1)^n}\right|=\left|\frac{n+1}{3}(x+1)\right|

As nn\to\infty, this ratio grows without bound unless x=1x=-1 makes the factor (x+1)(x+1) equal to zero. So:

  • If x1x\neq -1, the ratio tends to infinity, so the series diverges.
  • If x=1x=-1, every term after the first is zero, so it converges.

This means the radius of convergence is R=0R=0 (only converges at the center).

That’s a good reminder: not every power series converges on an interval; sometimes it collapses to a single point.

Exam Focus
  • Typical question patterns:
    • “Find the radius of convergence and interval of convergence of a power series.”
    • “Use the Ratio Test (or Root Test) to determine convergence.”
    • “Check endpoints separately and classify convergence (absolute vs conditional).”
  • Common mistakes:
    • Forgetting to check endpoints after finding xa<R|x-a|<R.
    • Algebra errors when simplifying the ratio—especially with factorials and powers.
    • Assuming endpoints behave the same; they often differ (one converges, the other diverges).

Finding Taylor and Maclaurin Series

What a Taylor series is

A Taylor series is what you get if you keep increasing the Taylor polynomial degree forever. Formally, the Taylor series of f(x)f(x) about x=ax=a is

n=0f(n)(a)n!(xa)n\sum_{n=0}^{\infty} \frac{f^{(n)}(a)}{n!}(x-a)^n

The corresponding Maclaurin series is the special case a=0a=0:

n=0f(n)(0)n!xn\sum_{n=0}^{\infty} \frac{f^{(n)}(0)}{n!}x^n

Important nuance: Writing down the Taylor series is one step; asserting it actually equals f(x)f(x) is another. On the AP exam, you often use known expansions or are implicitly working where equality is valid.

Why learning to find series matters

You’re building a toolkit to:

  • generate power series representations for functions,
  • approximate values efficiently,
  • analyze limits and integrals using series,
  • and solve differential equation–style modeling problems (in broader calculus contexts).
Two main methods for finding series
  1. Derivative method (from the definition): compute f(n)(a)f^{(n)}(a) patterns.
  2. Known series + algebra: start from a “library” of standard series (like geometric) and transform.

The second method is usually faster and more common in AP problems, but the derivative method is essential when a function isn’t easily linked to a known series.

A small “library” of standard Maclaurin series

These are commonly used in AP Calculus BC:

  1. Geometric series

11x=n=0xn\frac{1}{1-x}=\sum_{n=0}^{\infty} x^n

(valid for x<1|x|<1)

  1. Exponential

ex=n=0xnn!e^x=\sum_{n=0}^{\infty} \frac{x^n}{n!}

(converges for all real xx)

  1. Sine

sin(x)=n=0(1)nx2n+1(2n+1)!\sin(x)=\sum_{n=0}^{\infty} (-1)^n\frac{x^{2n+1}}{(2n+1)!}

(converges for all real xx)

  1. Cosine

cos(x)=n=0(1)nx2n(2n)!\cos(x)=\sum_{n=0}^{\infty} (-1)^n\frac{x^{2n}}{(2n)!}

(converges for all real xx)

  1. Natural log (often derived via integration)

ln(1+x)=n=1(1)n+1xnn\ln(1+x)=\sum_{n=1}^{\infty} (-1)^{n+1}\frac{x^n}{n}

(valid for 1<x1-1<x\le 1)

  1. Arctangent (often derived from geometric)

arctan(x)=n=0(1)nx2n+12n+1\arctan(x)=\sum_{n=0}^{\infty} (-1)^n\frac{x^{2n+1}}{2n+1}

(valid for x1|x|\le 1)

A frequent mistake is memorizing these without the conditions (intervals) where they converge.

Example 1: Find the Taylor series for ln(x)\ln(x) about a=1a=1

This is a classic BC skill because it produces a power series centered at 11.

Let f(x)=ln(x)f(x)=\ln(x). Compute derivatives:

  • f(1)=ln(1)=0f(1)=\ln(1)=0
  • f(x)=1xf'(x)=\frac{1}{x} so f(1)=1f'(1)=1
  • f(x)=1x2f''(x)=-\frac{1}{x^2} so f(1)=1f''(1)=-1
  • f(x)=2x3f'''(x)=\frac{2}{x^3} so f(1)=2f'''(1)=2
  • f(4)(x)=6x4f^{(4)}(x)=-\frac{6}{x^4} so f(4)(1)=6f^{(4)}(1)=-6

A pattern emerges: for n1n\ge 1,

f(n)(1)=(1)n1(n1)!f^{(n)}(1)=(-1)^{n-1}(n-1)!

Plug into the Taylor series formula:

ln(x)=n=1(1)n1(n1)!n!(x1)n\ln(x)=\sum_{n=1}^{\infty} \frac{(-1)^{n-1}(n-1)!}{n!}(x-1)^n

Since (n1)!n!=1n\frac{(n-1)!}{n!}=\frac{1}{n}, this simplifies to

ln(x)=n=1(1)n1(x1)nn\ln(x)=\sum_{n=1}^{\infty} (-1)^{n-1}\frac{(x-1)^n}{n}

This is equivalent to the well-known series for ln(1+u)\ln(1+u) if you set u=x1u=x-1.

Example 2: Find a Maclaurin series using known series (no derivatives)

Find a power series for

11+3x\frac{1}{1+3x}

Start from the geometric series:

11r=n=0rn\frac{1}{1-r}=\sum_{n=0}^{\infty} r^n

Here you want 1+3x1+3x in the denominator, so rewrite:

11+3x=11(3x)\frac{1}{1+3x}=\frac{1}{1-(-3x)}

So r=3xr=-3x. Substitute:

11+3x=n=0(3x)n=n=0(1)n3nxn\frac{1}{1+3x}=\sum_{n=0}^{\infty} (-3x)^n=\sum_{n=0}^{\infty} (-1)^n 3^n x^n

Convergence requires 3x<1|-3x|<1, so x<13|x|<\frac{1}{3}.

Exam Focus
  • Typical question patterns:
    • “Find the Maclaurin series for f(x)f(x)” (often trig, exponential, log).
    • “Find the Taylor series centered at aa and state its interval of convergence.”
    • “Use a known series (often geometric) to produce a new one by substitution.”
  • Common mistakes:
    • Dropping the center shift: writing powers of xx instead of (xa)(x-a).
    • Not simplifying factorial patterns correctly (like turning (n1)!n!\frac{(n-1)!}{n!} into 1n\frac{1}{n}).
    • Forgetting to transform the convergence condition when substituting (for example, r<1|r|<1 becomes a condition on xx).

Representing Functions as Power Series

What “represent as a power series” means

To represent a function as a power series means to rewrite it in the form

f(x)=n=0cn(xa)nf(x)=\sum_{n=0}^{\infty} c_n(x-a)^n

on some interval of convergence.

This is more than an algebra trick: once you have a power series, you can often differentiate, integrate, and approximate in ways that are difficult with the original function.

Why this is powerful (big ideas)

Power series are like “function LEGO bricks.” Once you know a few standard series, you can build many others by:

  • Substitution (replace xx with another expression)
  • Multiplying by a power (shift indices)
  • Differentiating/integrating term-by-term (within the interval of convergence)

On the AP exam, this shows up in problems that ask for a series for a new function, and often also ask for the radius/interval of convergence after the transformation.

Core tools for transforming series

Suppose

f(x)=n=0cnxnf(x)=\sum_{n=0}^{\infty} c_n x^n

Then (within the interval of convergence):

  1. Multiply by xmx^m:

xmf(x)=n=0cnxn+mx^m f(x)=\sum_{n=0}^{\infty} c_n x^{n+m}

  1. Differentiate:

f(x)=n=1ncnxn1f'(x)=\sum_{n=1}^{\infty} n c_n x^{n-1}

  1. Integrate:

f(x)dx=C+n=0cnn+1xn+1\int f(x)\,dx=C+\sum_{n=0}^{\infty} \frac{c_n}{n+1}x^{n+1}

A common misconception is that you can always differentiate/integrate any series anywhere. For AP purposes, the safe statement is: you can do these operations on the interval of convergence, and the resulting series has the same radius of convergence.

Example 1: Derive the series for ln(1+x)\ln(1+x) by integrating a geometric series

Start with

11x=n=0xn\frac{1}{1-x}=\sum_{n=0}^{\infty} x^n

Replace xx with x-x:

11+x=n=0(1)nxn\frac{1}{1+x}=\sum_{n=0}^{\infty} (-1)^n x^n

This holds for x<1|x|<1.

Now integrate both sides from 00 to xx. The left side:

0x11+tdt=ln(1+x)\int_0^x \frac{1}{1+t}\,dt=\ln(1+x)

The right side integrates term-by-term:

0xn=0(1)ntndt=n=0(1)nxn+1n+1\int_0^x \sum_{n=0}^{\infty} (-1)^n t^n\,dt=\sum_{n=0}^{\infty} (-1)^n\frac{x^{n+1}}{n+1}

Rewrite the index with k=n+1k=n+1:

ln(1+x)=k=1(1)k1xkk\ln(1+x)=\sum_{k=1}^{\infty} (-1)^{k-1}\frac{x^k}{k}

This is the standard Maclaurin series for ln(1+x)\ln(1+x).

Convergence: the original geometric series required x<1|x|<1. At endpoints, you check separately; this series converges at x=1x=1 (alternating harmonic) and diverges at x=1x=-1 (harmonic-like), giving 1<x1-1<x\le 1.

Example 2: Create a power series for arctan(x)\arctan(x)

A common route is to start from

11+x2\frac{1}{1+x^2}

Use geometric series with r=x2r=-x^2:

11(x2)=n=0(x2)n=n=0(1)nx2n\frac{1}{1-(-x^2)}=\sum_{n=0}^{\infty} (-x^2)^n=\sum_{n=0}^{\infty} (-1)^n x^{2n}

(valid for x<1|x|<1).

Now integrate term-by-term:

0x11+t2dt=arctan(x)\int_0^x \frac{1}{1+t^2}\,dt=\arctan(x)

and

0xn=0(1)nt2ndt=n=0(1)nx2n+12n+1\int_0^x \sum_{n=0}^{\infty} (-1)^n t^{2n}\,dt=\sum_{n=0}^{\infty} (-1)^n\frac{x^{2n+1}}{2n+1}

So

arctan(x)=n=0(1)nx2n+12n+1\arctan(x)=\sum_{n=0}^{\infty} (-1)^n\frac{x^{2n+1}}{2n+1}

This representation is useful for approximating arctan(1)\arctan(1) (which relates to π\pi) and for many series-based approximation questions.

Example 3: Represent a nonstandard function by substitution and scaling

Find a power series for

x24x\frac{x^2}{4-x}

First rewrite it to match geometric form. Factor the denominator:

x24x=x24(1x4)=x2411x4\frac{x^2}{4-x}=\frac{x^2}{4\left(1-\frac{x}{4}\right)}=\frac{x^2}{4}\cdot \frac{1}{1-\frac{x}{4}}

Now apply geometric series with r=x4r=\frac{x}{4}:

11x4=n=0(x4)n\frac{1}{1-\frac{x}{4}}=\sum_{n=0}^{\infty} \left(\frac{x}{4}\right)^n

So

x24x=x24n=0(x4)n=n=0xn+24n+1\frac{x^2}{4-x}=\frac{x^2}{4}\sum_{n=0}^{\infty} \left(\frac{x}{4}\right)^n=\sum_{n=0}^{\infty} \frac{x^{n+2}}{4^{n+1}}

Convergence comes from x4<1\left|\frac{x}{4}\right|<1, so x<4|x|<4.

Common pitfall: forgetting to carry the prefactor x24\frac{x^2}{4} into the series.

How these representations connect back to Taylor polynomials

Once you have a power series, a Taylor polynomial is just a truncation (cutting off after finitely many terms). For example, if

f(x)=n=0cnxnf(x)=\sum_{n=0}^{\infty} c_n x^n

then a degree-NN Maclaurin polynomial is

PN(x)=n=0NcnxnP_N(x)=\sum_{n=0}^{N} c_n x^n

That’s why “represent as a power series” and “approximate with a polynomial” are two sides of the same idea.

Exam Focus
  • Typical question patterns:
    • “Find a power series representation for g(x)g(x) using a known series for f(x)f(x).”
    • “Differentiate/integrate a power series to obtain a series for a related function, and state the interval of convergence.”
    • “Use a power series to approximate a definite integral or function value.”
  • Common mistakes:
    • Not updating the convergence condition after substitution (for example, r<1|r|<1 becomes an inequality in xx).
    • Differentiating/integrating incorrectly (especially index shifts and new starting indices).
    • Forgetting the constant of integration when integrating an indefinite series (when appropriate); using a definite integral from 00 often avoids this.