Laurent series, classification of singularities, Casorati–Weierstrass
Why this is asked: Classify a singularity from the Laurent tail or from the behaviour of |f| nearby: bounded ⇒ removable, → ∞ ⇒ pole, neither ⇒ essential (and then the image of every punctured neighbourhood is dense).
In one sentence
Count the negative powers in the Laurent series: none means removable, finitely many means a pole, infinitely many means essential — and each of those is equivalent to a statement about that you can check without expanding anything.
Why the exam asks it
Because "essential" gets read as "a very bad pole", and it is the opposite: a pole is the case where , and essential is the case where does not settle down at all. And because the same function has different Laurent series on different annuli, so a question can hand you the wrong one and let you classify from it.
The idea
On an annulus where is holomorphic,
converging there. The principal part is the sum over .
The classification
is an isolated singularity if is holomorphic on some punctured disc around it. Then, from the Laurent series on that punctured disc:
- Removable — no negative powers. Equivalently is bounded near (Riemann's theorem), equivalently exists. at : the series has no negative terms at all.
- Pole of order — finitely many negative powers, the lowest being . Equivalently . Equivalently has a removable singularity with nonzero limit.
- Essential — infinitely many negative powers. Equivalently has no limit, finite or infinite. at : the series never terminates.
Each of these is an equivalence, which is what makes them usable. You almost never expand a Laurent series in an exam; you take a limit and read the row.
For : along the positive reals , along the negative reals . Two different limits along two approaches, so neither "bounded" nor "" holds, and the singularity is essential without expanding anything.
Zeros and poles are reciprocal
If has a zero of order at then has a pole of order there, and conversely. So has simple poles exactly at , because has simple zeros there. Orders add under multiplication and subtract under division, and counting them settles most questions of the form "what kind of singularity does this have".
The annulus matters
.
On , expand , giving
— one negative power, so a simple pole at , which is correct.
On , expand , giving
— infinitely many negative powers, and it would be a mistake to call the singularity essential. That series does not describe behaviour near at all; it describes behaviour near infinity. Only the expansion on the punctured disc closest to the point classifies the singularity there.
Casorati–Weierstrass and Picard
Near an essential singularity, the image of every punctured neighbourhood is dense in .
So comes arbitrarily close to every complex number, arbitrarily near . Picard's great theorem sharpens this enormously: actually attains every complex value infinitely often, with at most one exception. For the exception is , which it never takes.
Both are stated for essential singularities specifically, and both are false at poles, where and the image eventually avoids every bounded set.
Not every singularity is isolated
has poles wherever , that is at . These accumulate at , so no punctured disc around is free of singularities, and is not an isolated singularity at all. It has no Laurent series there and the classification simply does not apply.
Branch points are the other non-isolated case: and at are not isolated singularities either, because no single-valued branch exists on a punctured disc.
Where intuition breaks
"Essential means faster." That describes a pole. Essential means has no limit — tends to one way and the other. This is the topic's central confusion.
" is unbounded near , so there is a pole." Unbounded is not the same as tending to infinity. is unbounded near and has an essential singularity. The pole condition is , meaning every approach.
"The Laurent series has infinitely many negative powers, so the singularity is essential." Only if it is the expansion on a punctured disc around the point. The expansion of has infinitely many and the singularity at is a simple pole.
"Every singularity is isolated." at . Options quietly assume isolation so that the classification applies; it does not always.
" is bounded near , so we cannot say much." Riemann's theorem says the singularity is removable — extends holomorphically. Bounded is a very strong hypothesis here, and recognising it as sufficient is often the whole question.
"An essential singularity means misses lots of values." The reverse. By Picard it takes every value infinitely often, with at most one exception.
" has a pole at ." It has a branch point, which is not an isolated singularity. No Laurent series exists.
The exam's angle
- Take a limit before expanding. Finite limit means removable; means a pole; neither means essential. That is the whole classification and it needs no series.
- For pole order, multiply and check. having a finite nonzero limit pins exactly.
- Count zeros of the denominator. Order of pole equals order of zero, so has simple poles and double ones.
- Check isolation before classifying. If the singularities accumulate — anything with inside a periodic function — the question is about non-isolation.
- Read which annulus a given series belongs to. A series with infinitely many negative powers proves nothing until you know where it converges.
The night before
- No negative powers: removable bounded near the limit exists. .
- Finitely many, lowest : pole of order . .
- Infinitely many: essential no limit at all. .
- Zero of order for pole of order for .
- One function, many annuli, many Laurent series. Only the innermost punctured disc classifies. has a simple pole at and an infinite principal part on .
- Casorati–Weierstrass: image of every punctured neighbourhood is dense. Picard: every value infinitely often, at most one exception — omits .
- at : poles accumulate, so not isolated, so unclassifiable.
- Branch points (, ) are not isolated singularities.
See it move
Check yourself
Let ∖{0}. The residue of f at z = 0 is
More in Singularities and Residues
Take it further
- The mistake this prevents: execution slip → real wrong options, and why each one tempts
- The mistake this prevents: standard counterexample → real wrong options, and why each one tempts
- Previous-year questions set on this — every option and the answer, free:December 2025 · Part BDecember 2024 · Part BJune 2024 · Part CDecember 2024 · Part CJune 2023 · Part B
Last revised . Found a mistake? Tell us — corrections are the fastest thing we act on.
Next: Residue theorem and standard contour integrals
Create a free account to keep your place and have this feed your study plan.
Open this in the full syllabus view · Unit 2