4.3.5 · D5Calculus III — Sequences & Series

Question bank — Telescoping series

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Before we start, one shared vocabulary reminder so every symbol below is earned:


True or false — justify

A series telescopes only if it can be written using partial fractions.
False — partial fractions is just the most common tool to manufacture ; logs, trig differences, and factorial ratios telescope too. The defining property is the difference form, not the method that reveals it.
If every interior term cancels, the sum must equal .
False — cancellation leaves , and the sum is . Only when does the leftover vanish and the sum reduce to .
A telescoping series always converges.
False — it converges iff exists (is finite); if diverges or grows, so does . Telescoping guarantees a closed form for , not convergence.
If then exactly two terms survive at each end.
True — with a gap of , the cancellation only matches every second helper value, so two leading () and two trailing terms remain. General rule: gap leaves leading and trailing survivors.
Writing (helper increasing) breaks telescoping.
False — it still telescopes; you just get , a sign flip of the standard result. The direction of the difference only swaps which boundary is positive.
For , changing the starting index from to changes the answer.
True — the surviving lead term becomes , not , so the sum is . The first two terms you dropped were real contributions, not cancelled ones.
If the telescoping sum is guaranteed to be positive.
False — the sum is , whose sign is just the sign of . Nothing forces ; e.g. a helper with gives a negative sum.
Two different helper sequences can produce the same series .
True — adding any constant to every leaves unchanged, so is only determined up to a constant. The sum is unaffected because cancels.

Spot the error

", and since interior terms cancel, too."
The error is assuming identical cancellation. The gap here is , so two terms survive at each end and the sum is , not .
" telescopes with , so the sum is ."
The leftover limit was ignored. Here , so the sum is .
"I found , both plus, so it can't telescope."
The partial fraction sign is wrong: it is . A telescoping difference requires opposite signs on the two pieces; a plus–plus split is an algebra slip.
"The series starts at and , so I plug as the lead — done, no need to write terms."
The verdict is only correct for a gap-1 telescope. If the gap is larger you must write out 4–5 terms first, or you will miss extra survivors.
" has each term , so the sum must be ."
Terms is only the necessary condition for convergence, never the value. Telescoping gives .
"Since is exact for every finite , the infinite sum is just ."
You cannot leave in an infinite sum — you must take . The correct object is , a number, not an -dependent expression.

Why questions

Why does partial fraction decomposition so often unlock telescoping?
It splits one fraction into simpler pieces whose denominators differ by a shift (like and ), which is exactly the pattern that cancels neighbour-to-neighbour. See Partial Fraction Decomposition.
Why do only the boundary terms survive, not any interior ones?
Each interior helper value appears once with (from term ) and once with (from term ), so they annihilate in pairs. Only (no earlier partner) and (no later partner) are unpaired.
Why is telescoping considered "rare and precious" among series methods?
Most tools (see Convergence Tests for Series) only decide whether a series converges; telescoping actually delivers the exact value, because the sum reduces to a finite boundary expression.
Why does the whole infinite sum depend only on and , ignoring the middle?
Because every middle contribution is cancelled by construction, the total is entirely a "boundary" quantity — like a definite integral depending only on its endpoints. The interior is genuinely irrelevant to the value.
Why must we compute and not just ?
is required for convergence but tells you nothing about the sum. The value lives in , so it is the helper's limit — via Limits of Sequences — that fixes the answer.
Why is telescoping the discrete cousin of the fundamental idea behind integration?
Summing a difference collapses to endpoints, mirroring how integrating a derivative collapses to . This is the Method of Differences, the finite/discrete analogue.

Edge cases

A series where (nonzero limit): does it still telescope, and what is the sum?
Yes, it still telescopes — telescoping is about the difference form, not the limit. The sum is ; the machinery is unchanged, only the surviving limit is nonzero.
oscillates, e.g. : is the series convergent?
No — keeps flipping between two values, so does not exist. The series diverges by oscillation even though it "telescopes" algebraically.
A single-term "series" : what happens?
It is simply with nothing to cancel — telescoping degenerates gracefully to the one difference. The formula still holds with .
The gap equals the whole length, e.g. : how much cancels?
Nothing cancels — with gap over only terms, no meets a matching within range. All six pieces survive: .
(helper grows without bound): what is the sum?
The series diverges — . Telescoping still gives the exact partial sum, but the limit fails to exist finitely, so there is no sum.
The two pieces are equal, : is this a telescoping series?
Trivially yes, with sum — every term is zero. It is the degenerate boundary case where "first minus last" gives once you note makes everything collapse to nothing.

Recall One-line self-test

Sum of ? ::: , because .


Connections

  • Telescoping series (Hinglish) — the parent topic these traps drill.
  • Partial Fraction Decomposition — the engine most traps abuse.
  • Sequence of Partial Sums — where the collapse is defined.
  • Limits of Sequences — the limit that decides every edge case.
  • Convergence Tests for Series — why "converges" ≠ "has this value".
  • Method of Differences — the discrete-analogue lens.
  • Geometric Series — the other exact-sum family, for contrast.