Mathematics · Glossary

What is holomorphic function?

Definition 16.1 University Mathematics — Year 3 · Chapter 16 — Holomorphic Functions

f ⁣:ΩCf \colon \Omega \to \C is holomorphic on Ω\Omega if for every z0Ωz_0 \in \Omega

f(z0)=limh0f(z0+h)f(z0)hf'(z_0) = \lim_{h\to0}\frac{f(z_0 + h) - f(z_0)}{h}

exists (hCh \in \C^*). Sums, products, quotients (nonvanishing denominators), compositions of holomorphic functions are holomorphic, with the usual formulas (the Year 1–2 proofs are verbatim: they only use field operations and limits). H(Ω)\mathcal H(\Omega) denotes the set of holomorphic functions on Ω\Omega.

Examples

Example 16.3

Polynomials in zz, rational functions off their poles, and — by Year 2’s term-by-term differentiation theorem for power series, whose proof works identically over C\C — every sum of a power series an(za)n\sum a_n(z - a)^n inside its disc of convergence: holomorphic, with derivative nan(za)n1\sum na_n(z - a)^{n-1} (same radius). In particular expz=zn/n!\exp z = \sum z^n/n! is entire (holomorphic on C\C) with exp=exp\exp' = \exp. On the other hand zzˉz \mapsto \bar z, z\abs z, Rez\operatorname{Re}z are nowhere holomorphic (Cauchy–Riemann fails everywhere): holomorphy is orientation-and-angle-preserving rigidity, not smoothness.

Example 16.11 (Singularities dictate radii)

Why does the innocent real function 11+x2\frac1{1 + x^2} have a Taylor series at x=3x = 3 converging only for x3<10\abs{x - 3} < \sqrt{10}, when nothing goes wrong on the real line? Because the theorem above makes the radius of convergence at aa equal to the distance from aa to the nearest point where holomorphy fails. Here f(z)=11+z2f(z) = \frac1{1 + z^2} is holomorphic exactly on C{±i}\C\setminus\{\pm\iu\}, so the expansion at a=3a = 3 converges on the largest disc avoiding ±i\pm\iu, of radius 3i=10\abs{3 - \iu} = \sqrt{10} — and cannot converge on a larger one, since the sum would extend ff holomorphically to a neighborhood of ±i\pm\iu, where f\abs f \to \infty. The real theory sees the mysterious radius 10\sqrt{10}; the complex plane sees two poles. This is the practical rule: to find a radius of convergence, locate the singularities — e.g. the Taylor series of tan\tan at 00 has radius π2\frac\pi2 (nearest zeros of cos\cos), and the Bernoulli generating function zez1\frac z{\eu^z - 1} (Problem 16.1, Part VI) has radius 2π2\pi (nearest nonzero zeros of ez1\eu^z - 1: ±2iπ\pm2\iu\pi).

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