Method of Differences
The method of differences (also called telescoping) is a technique for summing series where most terms cancel. It is used when the general term can be written as a difference f(r)−f(r+1) (or similar), causing consecutive terms to cancel in the sum.
The Key Idea
If we can write the general term as:
ur=f(r)−f(r+1)
then:
∑r=1nur=[f(1)−f(2)]+[f(2)−f(3)]+⋯+[f(n)−f(n+1)]=f(1)−f(n+1)
Most intermediate terms cancel — this is called telescoping.
Using Partial Fractions
The most common application is to decompose a fraction using partial fractions, then telescope.
Worked Example 1: Find ∑r=1nr(r+1)1.
Partial fractions: r(r+1)1=r1−r+11.
∑r=1n(r1−r+11)=(1−21)+(21−31)+⋯+(n1−n+11)
=1−n+11=n+1n
Worked Example 2: Find ∑r=1nr(r+2)1.
r(r+2)1=21(r1−r+21) (cover-up rule).
∑r=1n21(r1−r+21)
Write out the first few and last few terms:
=21[(1−31)+(21−41)+(31−51)+⋯+(n1−n+21)]
After cancellation, the surviving terms are:
=21(1+21−n+11−n+21)=21(23−n+11−n+21)
General Technique
- Decompose the general term ur into partial fractions (or another telescoping form).
- Write out the first 2-3 and last 2-3 terms.
- Cancel all intermediate terms.
- Simplify the remaining terms.
Non-Fraction Examples
The method of differences also works for non-fraction terms. If ur=f(r+1)−f(r):
Example 3: Given ur=(r+1)!−r!, find ∑r=1nur.
∑r=1n[(r+1)!−r!]=(n+1)!−1!=(n+1)!−1
Example 4: ∑r=1n[r⋅r!]=∑r=1n[(r+1)!−r!]=(n+1)!−1 since r⋅r!=(r+1−1)⋅r!=(r+1)!−r!.
Practice Problems
- Find ∑r=1n(2r−1)(2r+1)1.
- Find ∑r=1nr(r+1)(r+2)2.
- Show that ∑r=1nr(r+1)1=n+1n and deduce the value as n→∞.
- Find ∑r=120r(r+1)1.
Solutions: