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§14.5.1 Deficiency Relation

14.5.1 Deficiency Relation

One of the reformulations of the Second Fundamental Theorem is characterized in a way so that it comprises the statements of Picard-like theorems in a compact manner (of course, the conclusions are substantially more far-reaching than just the Picard theorems themselves). We first introduce the relevant terminology.

Definition 14.5.1.1.

Let 𝑎∈ℂ̂, 𝑓:𝐷(0,𝑅)→ℂ̂ be meromorphic. For 𝑘∈ℕ, 𝑟<𝑅, define 𝑛(𝑘)(𝑟,𝑎,𝑓) be the number of zeros of 𝑓−𝑎 or 1/𝑓 (if 𝑎=∞) within 𝐷(0,𝑟), where a repeated zero is counted at most 𝑘 times.

Then define the truncated Nevanlinna counting function (of order 𝑘) by

𝑁(𝑘)(𝑟,𝑎,𝑓)=∫0𝑟𝑛(𝑘)(𝑥,𝑎,𝑓)−𝑛(𝑘)(0,𝑎,𝑓)𝑥d𝑥+𝑛(𝑘)(0,𝑎,𝑓)log𝑟.

Denote the functions for when 𝑘=1 by 𝑁‾(𝑟,𝑎,𝑓)=𝑁(1)(𝑟,𝑎,𝑓) and 𝑛‾(𝑟,𝑎,𝑓)=𝑛(1)(𝑟,𝑎,𝑓).

Definition 14.5.1.2.

For any 𝑎∈ℂ̂ and a meromorphic function 𝑓:𝐷(0,𝑅)→ℂ̂, define the deficiency (or defect) 𝑎 in 𝑓 by

𝛿(𝑎,𝑓)=lim inf𝑟→𝑅−𝑚(𝑟,𝑎,𝑓)𝑇(𝑟,𝑓)=1−lim sup𝑟→𝑅−𝑁(𝑟,𝑎,𝑓)𝑇(𝑟,𝑓).
Then 𝑎 is said to be a deficient value of 𝑓 if its deficiency is nonzero.

Remark.

Because 𝑁(𝑟,𝑎,𝑓)≤𝑇(𝑟,𝑓)+𝒪︀(1) holds by the First Fundamental Theorem, the deficiency will always be a nonnegative real value.

The deficiency is the primary value we are interested in. We also observe the use of the Verzweigungsindex (ramification index) 𝜃 and the truncated deficiency Θ (of order 1):

𝜃(𝑎,𝑓)=lim inf𝑟→𝑅−𝑁(𝑟,𝑎,𝑓)−𝑁‾(𝑟,𝑎,𝑓)𝑇(𝑟,𝑓),Θ(𝑎,𝑓)=1−lim sup𝑟→𝑅−𝑁‾(𝑟,𝑎,𝑓)𝑇(𝑟,𝑓).

Using these formulations, we now have

Theorem 14.5.1.3 (Deficiency Relation).

Suppose 𝑓:𝐷(0,𝑅0)→ℂ̂ (0<𝑅0≤∞) is meromorphic and admissible. Then 𝑆={𝑎∈ℂ̂:Θ(𝑎,𝑓)>0} is a countable set and

∑𝑎∈𝑆[𝛿(𝑎,𝑓)+𝜃(𝑎,𝑓)]≤∑𝑎∈𝑆Θ(𝑎,𝑓)≤2.
Proof.

For any 𝑞 numbers {𝑎𝜈}𝜈=1𝑞⊂ℂ,

𝑚(𝑟,𝑓)𝑇(𝑟,𝑓)+∑𝜈=1𝑞𝑚(𝑟,𝑎𝜈,𝑓)𝑇(𝑟,𝑓)+𝑁1(𝑟,𝑓)𝑇(𝑟,𝑓)≤2+𝑆(𝑟,𝑓)𝑇(𝑟,𝑓)

as 𝑟→𝑅0− by the Second Fundamental Theorem of Nevanlinna Theory (Theorem 14.4.1Theorem 14.4.1Theorem 14.4.1). Then,

𝑞−1−𝑆(𝑟,𝑓)𝑇(𝑟,𝑓)≤𝑁(𝑟,𝑓′)−𝑁(𝑟,1𝑓′)−2𝑁(𝑟,𝑓)𝑇(𝑟,𝑓)+𝑁(𝑟,𝑓)𝑇(𝑟,𝑓)+∑𝜈=1𝑞𝑁(𝑟,𝑎𝜈,𝑓)𝑇(𝑟,𝑓).

At each pole of 𝑓 with multiplicity 𝑝, 𝑓′ will have a pole of multiplicity 𝑝+1. Then distinct poles can be counted as 𝑁(𝑟,𝑓′)−𝑁(𝑟,𝑓)=𝑁‾(𝑟,𝑓). Then

𝑞−1−𝑆(𝑟,𝑓)𝑇(𝑟,𝑓)≤𝑁‾(𝑟,𝑓)−𝑁(𝑟,0,𝑓′)𝑇(𝑟,𝑓)+∑𝜈=1𝑞𝑁(𝑟,𝑎𝜈,𝑓)𝑇(𝑟,𝑓).

Each zero 𝑧 of multiplicity 𝑚 of 𝑓−𝑎𝜈 gives rise to a zero of multiplicity 𝑚−1 of 𝑓′. Then 𝑛‾(𝑟,𝑎𝜈,𝑓)=𝑛(𝑟,𝑎𝜈,𝑓)−𝑛𝑎𝜈(𝑟,0,𝑓′) where 𝑛𝑎𝜈(𝑟,0,𝑓′) is the zero discrete counting function of 𝑓′ with the proviso that points are counted at points where 𝑓=𝑎𝜈. In effect, 𝑁𝑎𝜈(𝑟,0,𝑓′) counts the solutions to 𝑓=𝑎𝜈, where each solution is under-counted once. Hence, this difference counts these under-counts, or effectively, the number of solutions without consideration of multiplicity.

Then

∑𝜈𝑁‾(𝑟,𝑎𝜈,𝑓)=∑𝜈𝑁(𝑟,𝑎𝜈,𝑓)−𝑁{𝑎𝜈}𝜈(𝑟,0,𝑓′)

(where 𝑁{𝑎𝜈}𝜈(𝑟,0,𝑓′) is the zero counting function of 𝑓′ with the condition that the points 𝑧 satisfy 𝑓(𝑧)∈{𝑎𝜈}𝜈), and letting 𝑁0(𝑟,0,𝑓′) count the critical points of 𝑓 that satisfy 𝑓∉{𝑎𝜈}𝜈,

𝑁{𝑎𝜈}𝜈(𝑟,0,𝑓′)+𝑁0(𝑟,0,𝑓′)=𝑁(𝑟,0,𝑓′).

Hence,

𝑞−1−𝑆(𝑟,𝑓)𝑇(𝑟,𝑓)≤𝑁‾(𝑟,𝑓)𝑇(𝑟,𝑓)−𝑁0(𝑟,0,𝑓′)𝑇(𝑟,𝑓)+∑𝜈=1𝑞𝑁‾(𝑟,𝑎𝜈,𝑓)𝑇(𝑟,𝑓).(14.5.1.1)

Then taking the superior limits on both side through a sequence {𝑟𝑛} such that lim𝑛→∞𝑆(𝑟𝑛,𝑓)𝑇(𝑟𝑛,𝑓)=0 (whose existence is given by Theorem 14.4.1.8Theorem 14.4.1.8Theorem 14.4.1.8) and loosening the inequality by removing the 𝑁0 term,

𝑞−1≤lim sup𝑛→∞𝑁‾(𝑟𝑛,∞,𝑓)𝑇(𝑟𝑛,𝑓)+∑𝜈=1𝑞lim sup𝑛→∞𝑁‾(𝑟𝑛,𝑎𝜈,𝑓)𝑇(𝑟𝑛,𝑓)≤lim sup𝑟→𝑅0−𝑁‾(𝑟,∞,𝑓)𝑇(𝑟,𝑓)+∑𝜈=1𝑞lim sup𝑟→𝑅0−𝑁‾(𝑟,𝑎𝜈,𝑓)𝑇(𝑟,𝑓)=1−Θ(∞,𝑓)+∑𝜈=1𝑞[1−Θ(𝑎𝜈,𝑓)].

Therefore, ∑𝜈=1𝑞Θ(𝑎𝜈,𝑓)+Θ(∞,𝑓)≤2. The Θ(∞,𝑓) term may or may not be truncated. Without loss of generality, we allow the arbitrary distinct {𝑎𝜈}𝜈𝑞 to comprise ∞, to obtain a more uniformized expression.

Assume some arbitrary 𝑁∈ℕ. If 2𝑁+1 values in the Riemann sphere have truncated deficiencies each exceeding 1/𝑁, then applying the previous to result to these 2𝑁+1 values, their truncated deficiency sum exceeds 2, which is a contradiction. Thus, ∀𝑁∈ℕ, at most 2𝑁 values have truncated deficiencies exceeding 1/𝑁. Let these exceeding values form the finite set 𝑆𝑁. Then

𝑆=⋃𝑁=1∞𝑆𝑁={𝑎∈ℂ̂:Θ(𝑎,𝑓)>0}

is a countable set, and hence can be described with a sequence {𝑎𝜈}𝜈=1𝑞. Then by the inequality,

∑𝜈=1𝑞Θ(𝑎𝜈,𝑓)≤2⟹∑𝜈=1∞Θ(𝑎𝜈,𝑓)≤2.□

Notice that the method we used to prove countability is the exact same as in Corollary 10.2.3.1Corollary 10.2.3.1Corollary 10.2.3.1.

Remark.

Ahlfors’ geometric formulation of the second fundamental theorem suggests that the value 2 in the inequality is connected to the Euler characteristic of the Riemann sphere via triangulation.

Therefore, we have

Corollary 14.5.1.3.1.

A non-constant meromorphic function omits at most two values on the Riemann sphere.
Proof.

Assume there exists three values 𝑎, 𝑏, 𝑐∈ℂ̂ that meromorphic function 𝑓 does not ever attain. Then 𝑁(𝑟,𝑎,𝑓), 𝑁(𝑟,𝑏,𝑓), 𝑁(𝑟,𝑐,𝑓) all vanish identically with respect to radius while 𝑇>0.

Then 𝛿(𝑎,𝑓), 𝛿(𝑏,𝑓), 𝛿(𝑐,𝑓)=1. By the deficiency relation (Theorem 14.5.1.3Theorem 14.5.1.3Theorem 14.5.1.3),

2≥∑𝑧∈𝑆[𝛿(𝑧)+𝜃(𝑧)]≥𝛿(𝑎,𝑓)+𝛿(𝑏,𝑓)+𝛿(𝑐,𝑓)=3,

which is an impossibility. ⁠□

Corollary 14.5.1.3.2 (Picard’s Little Theorem).

Any non-constant entire function omits at most one value.
Proof.Any such function can be regarded as a meromorphic function on the plane that omits ∞. Then the conclusion follows from Corollary 14.5.1.3.1Corollary 14.5.1.3.1Corollary 14.5.1.3.1. ⁠□

The use of spherically normal families in the proof of the Great Picard Theorem for more general domains is unavoidable. For further treatment, refer to [5].