- What Is a Power Series?
- Radius of Convergence
- Finding the Radius via the Ratio Test
- The Interval of Convergence, Endpoints
- Interactive Convergence Visualiser
- Functions Represented by Power Series
- Differentiation of Power Series
- Integration of Power Series
- Worked Examples
- Common Mistakes
- 10-Question Quiz
- Continue in Series & Sequences
§ 01What Is a Power Series?
A power series is an infinite polynomial: a sum of terms of the form cₙ(x − a)ⁿ. Unlike a finite polynomial, it may only converge for certain values of x, making the domain itself an object of study.
Every function you have encountered in calculus, eˣ, sin x, cos x, ln(1+x), can be expressed as a power series around an appropriate centre. Power series are the bridge between the world of sequences and the world of functions, and they underpin everything from Taylor approximations to the solutions of differential equations.
Here a is the centre of the series, and {cn} is the sequence of coefficients. When a = 0, the series is a Maclaurin series (or simply a "power series in x"). For general a, it is a Taylor series centred at a.
The key question for any power series is: for which values of x does the series converge? The answer is always an interval (possibly a single point, possibly all of ℝ) centred at a, the interval of convergence.
§ 02Radius of Convergence
For every power series Σ cₙ(x−a)ⁿ, there exists a number R ∈ [0, ∞] called the radius of convergence such that:
The three special cases for R are:
- R = 0: the series converges only at x = a (a single point).
- R = ∞: the series converges for all x ∈ ℝ (the entire number line).
- 0 < R < ∞: the series converges on the open interval (a−R, a+R) and diverges outside it.
The radius of convergence is a property of the coefficients {cₙ} alone: it does not depend on what happens at the endpoints. This is why it is called the radius: it describes the half-width of the interval of convergence before endpoint behaviour is decided.
Hadamard's formula gives the exact radius, but it requires computing a limsup, which can be difficult. In practice, we use the Ratio Test or Root Test on the series directly: this is almost always more tractable.
§ 03Finding the Radius via the Ratio Test
The most common method. Apply the Ratio Test to the power series treated as a series in x:
Step-by-step procedure
- Step 1. Write out the ratio |an+1/an| where an = cₙ(x−a)ⁿ.
- Step 2. Factor out |x−a| from the ratio.
- Step 3. Compute the limit of the remaining coefficient ratio.
- Step 4. Set the result < 1 and solve for |x−a| to find R.
- Step 5. Test the two endpoints x = a ± R separately.
§ 04The Interval of Convergence — Checking Endpoints
Once R is found, the interval of convergence is one of four possibilities depending on what happens at x = a − R and x = a + R:
| Left endpoint x = a−R | Right endpoint x = a+R | Interval of Convergence |
|---|---|---|
| Diverges | Diverges | (a−R, a+R) |
| Converges | Diverges | [a−R, a+R) |
| Diverges | Converges | (a−R, a+R] |
| Converges | Converges | [a−R, a+R] |
To test an endpoint x = a ± R, substitute that x-value into the series. The result is a constant-term series (x is now a specific number), which you test with any standard test, p-series, alternating series test, divergence test, etc.
§ 05Interactive Convergence Visualiser
The chart below plots the partial sum approximation SN(x) of the power series against the true function f(x). Use the slider to increase N and observe how the approximation improves inside the radius of convergence: and breaks down outside it.
Partial sums of selected power series vs. true function
Notice that for series with finite R = 1 (the geometric series and ln(1+x)), the approximation visibly diverges for |x| > 1, no matter how many terms you use. For R = ∞ (eˣ, sin x, cos x), the partial sums eventually converge everywhere, though you need more terms further from the centre.
§ 06Functions Represented by Power Series
The following power series centred at 0 (Maclaurin series) are the most important in all of calculus. Memorising them unlocks fast computation of limits, integrals, and differential equations.
| Function | Power Series | Radius R |
|---|---|---|
| eˣ | Σ xⁿ/n! = 1 + x + x²/2! + x³/3! + ··· | ∞ |
| sin x | Σ (−1)ⁿx²ⁿ⁺¹/(2n+1)! = x − x³/6 + x⁵/120 − ··· | ∞ |
| cos x | Σ (−1)ⁿx²ⁿ/(2n)! = 1 − x²/2 + x⁴/24 − ··· | ∞ |
| 1/(1−x) | Σ xⁿ = 1 + x + x² + x³ + ··· | 1 |
| ln(1+x) | Σ (−1)ⁿ⁺¹xⁿ/n = x − x²/2 + x³/3 − ··· | 1 |
| arctan x | Σ (−1)ⁿx²ⁿ⁺¹/(2n+1) = x − x³/3 + x⁵/5 − ··· | 1 |
| (1+x)ᵏ | Σ C(k,n)xⁿ = 1 + kx + k(k−1)x²/2! + ··· | 1 (k∉ℕ) |
These series can be combined, composed, multiplied, and transformed to produce power series for more complex functions. The key operations (differentiation and integration) are covered in the next two sections.
§ 07Differentiation of Power Series
Inside the open interval of convergence (a−R, a+R), a power series can be differentiated term by term, and the resulting series has the same radius of convergence R:
Note the sum starts at n = 1 because the n = 0 term (the constant c₀) differentiates to zero. The differentiated series has the same radius R, though the interval of convergence may change at endpoints (endpoints that converged may now diverge, or vice versa).
This means that if f(x) = Σ cₙ(x−a)ⁿ within its interval, then f is infinitely differentiable there, and every coefficient is determined by the derivatives: cₙ = f⁽ⁿ⁾(a)/n!, which is precisely the Taylor series formula.
§ 08Integration of Power Series
Similarly, a power series can be integrated term by term inside its open interval of convergence. The resulting series also has radius R:
This is extraordinarily useful for integrating functions that have no elementary antiderivative. For example, ∫ sin(x²) dx, ∫ e−x² dx, and ∫ sin(x)/x dx all lack closed forms, but their power series can be integrated term by term to produce a series representation of the antiderivative.
§ 09Worked Examples
Twelve worked examples covering radius and interval of convergence, endpoint testing, and operations on power series.
- Apply the Ratio Test: |an+1/an| = |xn+1/(n+1)| / |xⁿ/n| = |x|·n/(n+1).
- Limit: lim n/(n+1) = 1, so L = |x|. Converges when |x| < 1. ∴ R = 1.
- Check x = 1: Σ 1/n, diverges (harmonic series).
- Check x = −1: Σ (−1)ⁿ/n, converges by AST.
- Ratio: |xn+1/(n+1)!| / |xⁿ/n!| = |x|/(n+1).
- Limit: lim |x|/(n+1) = 0 for all x.
- L = 0 < 1 for all x ∈ ℝ. ∴ R = ∞.
- Interval of convergence: (−∞, ∞): this is the Maclaurin series for eˣ.
- Ratio: |(x−3)n+1/4n+1| / |(x−3)ⁿ/4ⁿ| = |x−3|/4.
- Converges when |x−3|/4 < 1, i.e. |x−3| < 4. ∴ R = 4, centre a = 3.
- Check x = 7 (x−3 = 4): Σ 1, diverges.
- Check x = −1 (x−3 = −4): Σ (−1)ⁿ, diverges (terms don't → 0).
- Ratio: |(n+1)²xn+1| / |n²xⁿ| = |x| · (n+1)²/n².
- lim (n+1)²/n² = 1. So L = |x|.
- Converges when |x| < 1. ∴ R = 1.
- Endpoints: at x = ±1, terms n²(±1)ⁿ → ∞, so both endpoints diverge.
- Root Test: lim |2ⁿxⁿ|1/n = lim 2|x| = 2|x|.
- Converges when 2|x| < 1, i.e. |x| < 1/2. ∴ R = 1/2.
- This is the geometric series 1/(1−2x), valid for |x| < 1/2.
- Note d/dx[1/(1−x)] = 1/(1−x)².
- Differentiate Σxⁿ term by term: d/dx[Σ xⁿ] = Σ nxⁿ⁻¹ = Σn=1∞ nxⁿ⁻¹.
- Re-index: Σn=0∞ (n+1)xⁿ.
- Since d/dx[ln(1+x)] = 1/(1+x) = Σ(−1)ⁿxⁿ, integrate both sides:
- ln(1+x) = ∫Σ(−1)ⁿxⁿ dx = Σ(−1)ⁿ xn+1/(n+1) + C
- At x = 0: ln(1) = 0 = 0 + C, so C = 0.
- ln(1+x) = Σn=0∞(−1)ⁿxn+1/(n+1) = x − x²/2 + x³/3 − ···
- d/dx[arctan x] = 1/(1+x²) = Σ(−1)ⁿx²ⁿ for |x| < 1.
- Integrate: arctan x = Σ(−1)ⁿ x2n+1/(2n+1) + C.
- At x = 0: arctan(0) = 0 = C. So C = 0.
- arctan x = x − x³/3 + x⁵/5 − x⁷/7 + ···, valid for −1 ≤ x ≤ 1.
- At x = 1: arctan 1 = π/4 = 1 − 1/3 + 1/5 − ···: Leibniz's formula!
- sin u = Σ(−1)ⁿu2n+1/(2n+1)!. Substitute u = x²:
- sin(x²) = Σ(−1)ⁿx4n+2/(2n+1)!
- Integrate term by term from 0 to 1:
∫₀¹ sin(x²)dx = Σ(−1)ⁿ/(2n+1)! · 1/(4n+3) - Terms: 1/3 − 1/(7·6) + 1/(11·120) − ···
- = 0.33333 − 0.02381 + 0.00076 − 0.00001 + ··· ≈ 0.3103
- Ratio: |(n+1)!xn+1/(n!xⁿ)| = (n+1)|x|.
- lim(n+1)|x| = ∞ for any x ≠ 0. So L = ∞ > 1 for all x ≠ 0.
- Series diverges for every x ≠ 0. At x = 0, the series trivially = 1.
- Write x/(1−x²) = x · 1/(1−x²).
- Use 1/(1−u) = Σuⁿ with u = x²: 1/(1−x²) = Σ x2n.
- Multiply by x: x/(1−x²) = Σ x2n+1 = x + x³ + x⁵ + x⁷ + ···
- Valid for |x²| < 1, i.e. |x| < 1.
- Ratio: |xn+1/(n+1)3/2| / |xⁿ/n3/2| = |x|·(n/(n+1))3/2 → |x|.
- R = 1.
- x = 1: Σ 1/n3/2: p-series with p = 3/2 > 1. Converges. ✓
- x = −1: Σ (−1)ⁿ/n3/2, alternating, bn = 1/n3/2 → 0, decreasing. Converges by AST. ✓
§ 10Common Mistakes
§ 1110-Question Quiz
Select one answer per question then click Check All Answers.