The Casorati–Weierstrass Theorem: Dense Image Near an Essential Singularity
Let be holomorphic on the punctured disk , with an essential singularity at .
Prove that for every and every , the image intersects the disk for all .
In other words: the image of any punctured neighborhood of an essential singularity is dense in .
As a warm-up sanity check: verify this is consistent with the behaviors near .
Answer: Casorati–Weierstrass: Dense Image Near Essential Singularity
Key Idea / Intuition
If the image of avoided a whole disk around some value , then would be bounded near — forcing to be either a removable singularity or a pole of , contradicting the assumption that it's essential. So the image can never dodge an open set: it must be dense.
Formal Proof / Solution
Theorem (Casorati–Weierstrass): If has an essential singularity at , then for every punctured neighborhood , the image is dense in .
Proof by contradiction:
Suppose is not dense in . Then there exists and such that
Define
Since , we have holomorphic on and
So is bounded on the punctured disk. By Riemann's removable singularity theorem, extends to a holomorphic function on the full disk .
Case 1: .
Then extends holomorphically to . So is a removable singularity of — contradiction.
Case 2: .
Then near , where and . Thus
which has a pole of order at — also a contradiction.
In both cases, we contradict the assumption that is an essential singularity.
Sanity check with :
Write . Then , so
- The modulus ranges over as vary.
- The argument ranges over all of (mod ).
So takes all nonzero values and its image is indeed dense in (actually all of , by Picard's great theorem — a much stronger result).
Remark: Picard's Great Theorem strengthens this dramatically: near an essential singularity, takes every complex value with at most one exception, infinitely often. Casorati–Weierstrass is the elegant, accessible version of this idea.
Source: Stein & Shakarchi, Complex Analysis, Chapter 3; classical theorem