What is Summation?
A series is the sum of the terms of a sequence. In 9231 Paper 2, you are expected to find closed-form expressions for sums like:
The Cambridge 9231 syllabus tests three distinct techniques. You must recognise which applies — sometimes two are needed in combination.
Memorise the formulae for Σr, Σr², Σr³ and use them directly or in combination.
Express f(r) = g(r) − g(r−1). The sum telescopes and nearly all terms cancel.
Split a rational f(r) into partial fractions first, then apply Method of Differences.
Sigma Notation — a Quick Reminder
Make sure you are fluent with the following sigma algebra before attempting series questions:
Cambridge often asks for Σ from r = 3 to n, or r = 2 to 2n. Always subtract the missing initial terms. Writing the full formula and subtracting is safer than guessing at a new formula.
- A typical question first asks you to show a partial fraction or difference form — this is the setup for part (ii).
- Part (ii) then asks you to sum to n terms using the result in part (i).
- Part (iii) often asks for the sum from r = k to n, or for the sum to infinity (only if the series converges).
- Always simplify your final answer — Cambridge mark schemes expect a neat closed form.
The Standard Results
These four results must be memorised. They are not provided in the Cambridge formula booklet for P2.
| Series | Closed Form | Degree in n | Memory Hint |
|---|---|---|---|
| Σ 1 (r=1 to n) | n | Linear | Trivial — n ones |
| Σ r | ½n(n+1) | Quadratic | "Triangular numbers" — Gauss's formula |
| Σ r² | ⅙n(n+1)(2n+1) | Cubic | Three factors: n, n+1, 2n+1 divided by 6 |
| Σ r³ | [½n(n+1)]² | Quartic | (Σr)² — beautiful symmetry |
This is one of the most elegant results in elementary number theory. The sum of the first n cubes equals the square of the sum of the first n integers. Verify: 1³+2³+3³ = 36 = 6² = (1+2+3)². It holds for all n — try proving it by induction (Lesson 2.2)!
Using Standard Results in Combination
Most exam questions require you to expand f(r) as a polynomial, then apply the results term-by-term.
= 2 · ⅙n(n+1)(2n+1) − ½n(n+1)
= ⅓n(n+1)(2n+1) − ½n(n+1)
= n(n+1) · [⅓(2n+1) − ½]
= n(n+1) · [(4n+2 − 3)/6]
Partial Sums — Lower Limit Not 1
Method of Differences
This is the most important technique in the P2 series topic. It works whenever you can write:
Why It Works — The Telescoping Argument
Write out the sum term by term. With f(r) = g(r) − g(r−1):
- If f(r) = g(r) − g(r−1), then Σ(r=1 to n) f(r) = g(n) − g(0)
- If f(r) = g(r+1) − g(r), then Σ(r=1 to n) f(r) = g(n+1) − g(1)
- For a partial sum Σ(r=m to n), the result is g(n) − g(m−1)
- Always substitute a few values to confirm which terms survive before writing the final answer.
Finding the Difference Form — Partial Fractions Route
When f(r) is a rational function, use partial fractions to write it as a telescoping difference. The standard pattern is:
Sum to Infinity
If the series converges (each term → 0 as r → ∞), take the limit of your finite sum:
Only quote a sum to infinity if you can confirm the terms tend to zero. For example, Σ 1/r (harmonic series) diverges even though each term → 0. Always check the form of your closed-form sum as n → ∞.
Worked Examples
(ii) Hence find Σ 2/[r(r+2)] for r = 1 to n, and deduce the sum to infinity.
Multiply through: 2 = A(r+2) + Br
r = 0: 2 = 2A → A = 1
r = −2: 2 = −2B → B = −1
Write out first three and last three terms:
= 3/2 − (2n+3)/[(n+1)(n+2)]
Hence find Σ r(r+1) for r = 1 to n.
Let g(r) = r(r+1)(r+2). Then r(r+1) = ⅓[g(r) − g(r−1)].
g(n) = n(n+1)(n+2), g(0) = 0.
Σ(r=1 to 2n) r² = ⅙·(2n)(2n+1)(4n+1) = ⅓n(2n+1)(4n+1)
Practice Questions
All questions are at Cambridge 9231 examination level. Try each before revealing the hint or solution.
= ½n(n+1)(2n+1) + n(n+1)
= n(n+1)[½(2n+1) + 1]
= n(n+1)·½(2n+3)
Check n=2: 1·5 + 2·8 = 5+16 = 21. Formula: ½·2·3·7 = 21. ✓
(ii) Hence find Σ 4/[(2r−1)(2r+3)] for r = 1 to n.
4/[(2r−1)(2r+3)] = A/(2r−1) + B/(2r+3)
4 = A(2r+3) + B(2r−1)
r = ½: 4 = 4A → A = 1
r = −3/2: 4 = −4B → B = −1
Surviving terms (gap 4 = step of 2 in odd numbers, so 2 survive at each end):
r=1 gives 1/1; r=2 gives 1/3 — these survive at the start.
At the end: −1/(2n+1) and −1/(2n+3) survive.
S = 1 + 1/3 − 1/(2n+1) − 1/(2n+3)
(ii) By summing from r = 1 to n, use this result to derive the standard formula for Σr³.
Part (ii):
Sum both sides from r=1 to n:
LHS telescopes: (n+1)⁴ − 1⁴ = (n+1)⁴ − 1
RHS: 4Σr³ + 6Σr² + 4Σr + Σ1
= 4Σr³ + 6·⅙n(n+1)(2n+1) + 4·½n(n+1) + n
= 4Σr³ + n(n+1)(2n+1) + 2n(n+1) + n
Rearrange:
4Σr³ = (n+1)⁴ − 1 − n(n+1)(2n+1) − 2n(n+1) − n
After careful expansion and factorisation:
4Σr³ = n²(n+1)²
Interactive Series Calculator
Select a series type, set the upper limit n, and explore the partial sums and their closed-form values side by side.
Formula Sheet — P2 Series
Quick reference for use during revision. These results are not provided in the Cambridge formula booklet — you must know them.
- Read the question structure: A "show that" part (i) always sets up part (ii). Use the given result exactly — don't re-derive.
- Standard results: Expand f(r) as a polynomial first, then apply Σr², Σr, Σ1 individually.
- Method of Differences: Always write out at least 3 terms from each end to identify surviving terms — one error here loses all subsequent marks.
- Partial fractions route: Solve for A and B by substituting roots of the denominators (cover-up method is fastest).
- Partial sums (r = k to n): Always subtract Σ(r=1 to k−1). Never guess at a new formula.
- Sum to infinity: State what happens to each remaining term as n → ∞ before quoting the limit.