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§8.2 Conformal Metrics and Curvature

8.2 Conformal Metrics and Curvature

Let Ω⊆ℂ be a region and let 𝜌∈𝐶(Ω) be a positive function. The conformal metric (in the following chapters when we refer to metric we mean conformal) induced by 𝜌 is given by

d𝑠=𝜌(𝑧)|d𝑧|ord𝑠2=𝜌(𝑧)2|d𝑧|2.

The term “conformality” is explained in the previous section (note that this specific usage has little to do with holomorphy). The distance between two points 𝑧1,𝑧2∈Ω is defined as

𝑑(𝑧1,𝑧2)=inf𝛾⊂Ω∫𝛾𝜌(𝑧)|d𝑧|,

where the infimum is taken over all piecewise smooth curves 𝛾 in Ω joining 𝑧1 and 𝑧2.

A 𝐶2 metric is said to be regular. The (Gaussian) curvature of the regular metric 𝜌 at 𝑧∈Ω is defined as

𝐾𝜌(𝑧)=−∇2(log𝜌(𝑧))𝜌(𝑧)2,(8.2.1)

where ∇2=𝜕2/𝜕𝑥2+𝜕2/𝜕𝑦2=4𝜕2/𝜕𝑧‾𝜕𝑧 is the Laplacian operator. This is the same definition as the Gaussian curvature in (8.1.6)(8.1.6)(8.1.6).

The three following metrics are of particular interest in complex differential geometry:

  1. Perhaps the most trivial metric is the Euclidean metric (also known as the parabolic metric) on ℂ, and is given by

    𝜌=1,d𝑠2=|d𝑧|2.

    The Euclidean distance between two points 𝑧1,𝑧2∈ℂ is

    inf𝛾∫𝛾|d𝑧|=|𝑧2−𝑧1|

    is the length of the straight line segment connecting 𝑧1 and 𝑧2. The group formed by all transformations in the form of 𝑧↦ei𝜃𝑧+𝑎 (where 𝑎∈ℂ and 𝜃∈ℝ) is known as the group of rigid motions, or more abstractly, the special Euclidean group of order 2, denoted by SE(2)<Aut(ℂ), intuitively consists of all rotations and translations and their compositions, while the Euclidean group E(2)>SE(2) consists of reflections in the form of 𝑧↦ei𝜃𝑧‾+𝑎. Obviously, the Euclidean metric is invariant under both groups.

    From (8.2.1)(8.2.1)(8.2.1), we find that Euclidean metric has curvature 𝐾=0.

  2. The Poincaré metric (also referred to as the hyperbolic metric) on 𝔻 is given by

    𝜆(𝑧)=21−|𝑧|2,d𝑠𝜆2=4|d𝑧|2(1−|𝑧|2)2.(8.2.2)

    In Lemma 3.5.4Lemma 3.5.4Lemma 3.5.4, it was shown that the metric is invariant under Aut(𝔻).

    We will now calculate the Poincaré distance between two points 𝑧1,𝑧2∈ℂ. First assume the case where 𝑧1=0 and 𝑧2=𝑅∈(0,1). Consider a piecewise smooth curve 𝛾⊂𝔻 parameterized by 𝑧(𝑡) connecting 𝑧1 and 𝑧2; or in other words

    𝑧(𝑡)=𝑥(𝑡)+i𝑦(𝑡),𝑧(0)=𝑧1=0,𝑧(1)=𝑧2=𝑅,

    where 𝑥∈𝐶1([0,1]) and 𝑦∈𝐶1([0,1]) are real-valued functions. Then

    ∫𝛾d𝑠=∫012𝑥′(𝑡)2+𝑦′(𝑡)21−𝑥(𝑡)2−𝑦(𝑡)2d𝑡≥∫012|𝑥′(𝑡)|1−𝑥(𝑡)2d𝑡≥|∫012𝑥′(𝑡)1−𝑥(𝑡)2d𝑡|=|∫0𝑅2d𝑥1−𝑥2|=log(1+𝑅1−𝑅).

    Assuming that 𝛾 is in the form of 𝑧(𝑡)=𝑅𝑡,𝑧′(𝑡)=𝑅 where 𝑡∈[0,1], we have

    ∫𝛾d𝑠=∫012𝑅d𝑡1−𝑅2𝑡2=log(1+𝑅1−𝑅).

    Hence, the Poincaré distance between 0 and 𝑅 is given by

    𝑑(0,𝑅)=log(1+𝑅1−𝑅)

    and the straight line segment connecting the two points is a geodesic (path of least length under a metric or other criteria). For fixed 𝜃∈ℝ since 𝑧↦𝑧ei𝜃∈Aut(𝔻), by the Schwarz–Pick Lemma (Lemma 3.5.4Lemma 3.5.4Lemma 3.5.4), we have

    𝑑(0,𝑅)=𝑑(0,𝑅ei𝜃)=log(1+𝑅1−𝑅)

    by the invariance under Aut(𝔻). Now let 𝑧1 and 𝑧2 be arbitrary points in 𝔻. The Möbius transformation

    𝜑𝑧1(𝑧)=𝑧−𝑧11−𝑧1‾𝑧

    maps 𝑧1 to 0 and maps 𝑧2 to 𝑧2−𝑧11−𝑧1‾𝑧2. Hence, we have

    𝑑(𝑧1,𝑧2)=𝑑(0,𝑧2−𝑧11−𝑧1‾𝑧2)=log[1+|𝑧2−𝑧11−𝑧1‾𝑧2|1−|𝑧2−𝑧11−𝑧1‾𝑧2|]=inf𝛾∫𝛾d𝑠,

    which is the Poincaré distance (or hyperbolic distance) between 𝑧1 and 𝑧2. The infimum is attained along the geodesic curve 𝛾 parameterized by

    𝑧(𝑡)=𝜑𝑧1−1(𝑧2−𝑧11−𝑧1‾𝑧2𝑡)

    for 𝑡∈[0,1]. By Theorem 5.1.8Theorem 5.1.8Theorem 5.1.8, the geodesic is either an arc or a straight line segment passing through 𝑧1 and 𝑧2. Since 𝜕𝔻 is orthogonal to the straight line passing through 0 and 𝑧2−𝑧11−𝑧1‾𝑧2, by the conformality of 𝜑𝑧1−1, 𝜑𝑧1−1(𝜕𝔻)=𝜕𝔻 is orthogonal to the circular (or straight line) extension of the geodesic curve.

    As a consequence of the Schwarz–Pick Lemma (Lemma 3.5.4Lemma 3.5.4Lemma 3.5.4), for any 𝑓:𝔻→𝔻 is holomorphic, we have

    𝑑(𝑓(𝑧1),𝑓(𝑧2))≤𝑑(𝑧1,𝑧2),

    where equality is attained iff 𝑓∈Aut(𝔻). The Poincaré metric has constant negative curvature −1 since

    𝐾𝜆=−4𝜆2𝜕2log∘𝜆𝜕𝑧‾𝜕𝑧=−4𝜆2𝜕𝜕𝑧‾(𝜆𝑧′𝜆)=−2𝜆2𝜕𝜕𝑧‾(2𝑧‾1−|𝑧|2)=−2𝜆2(𝜆+𝑧‾𝜆𝑧‾′)=−(1−|𝑧|2)22(𝜆+𝑧‾2𝑧(1−|𝑧|2)2)=−(1−|𝑧|2)−|𝑧|2=−1,

    where 𝜆𝑧′=𝜕𝜆/𝜕𝑧 and 𝜆𝑧‾′=𝜕𝜆/𝜕𝑧‾.

  3. The spherical metric (also referred to as the elliptic metric) on ℂ̂ is given by

    𝜎(𝑧)=21+|𝑧|2,d𝑠𝜎2=4|d𝑧|2(1+|𝑧|2)2.(8.2.3)

    Under the inverse stereographic projection of 𝑆2→ℂ̂, for a given 𝑧∈ℂ̂, the corresponding point in 𝑆2 is

    (𝑥1,𝑥2,𝑥3)=(𝑧+𝑧‾|𝑧|2+1,𝑧−𝑧‾i|𝑧|2+i,|𝑧|2−1|𝑧|2+1).

    If we let 𝑃=(𝑥1,𝑥2,𝑥3) and 𝑄=(𝑥1̃,𝑥2̃,𝑥3̃) be two points in 𝑆2, the distance between the two points is the length of the shortest arc 𝑥⏜ (a subset of great circle passing the two points). By considering 𝑃 and 𝑄 as vectors from (0,0,0), this distance is equal to

    arccos(𝑃⋅𝑄)=2arctan1−𝑥1𝑥1̃−𝑥2𝑥2̃−𝑥3𝑥3̃1+𝑥1𝑥1̃+𝑥2𝑥2̃+𝑥3𝑥3̃=2arctan1−(𝑧+𝑧‾)(𝑧̃+𝑧̃‾)(|𝑧|2+1)(|𝑧̃|2+1)+(𝑧−𝑧‾)(𝑧̃−𝑧̃‾)(|𝑧|2+1)(|𝑧̃|2+1)−(|𝑧|2−1)(|𝑧̃|2−1)(|𝑧|2+1)(|𝑧̃|2+1)1+(𝑧+𝑧‾)(𝑧̃+𝑧̃‾)(|𝑧|2+1)(|𝑧̃|2+1)−(𝑧−𝑧‾)(𝑧̃−𝑧̃‾)(|𝑧|2+1)(|𝑧̃|2+1)+(|𝑧|2−1)(|𝑧̃|2−1)(|𝑧|2+1)(|𝑧̃|2+1)=2arctan−𝑧𝑧̃‾−𝑧‾𝑧̃+|𝑧|2+|𝑧̃|2𝑧𝑧̃‾+𝑧‾𝑧̃+|𝑧|2|𝑧̃|2+1=2arctan(𝑧−𝑧̃)(𝑧‾−𝑧̃‾)(𝑧𝑧̃‾+1)(𝑧‾𝑧̃+1).

    Notice that the fraction within the square root is a product between a complex number and its conjugate. Thus, this distance is equal to

    𝑑(𝑧,𝑧̃)=2arctan|𝑧−𝑧̃𝑧𝑧̃‾+1|

    in the extended complex plane. Let 𝑧̃=𝑧+Δ𝑧. It follows that

    𝑑(𝑧,𝑧+Δ𝑧)=2arctan|Δ𝑧|𝑧|2+𝑧Δ𝑧‾+1|=2arctan|Δ𝑧|𝑧|2+111+𝑧Δ𝑧‾|𝑧|2+1|=2arctan|Δ𝑧|𝑧|2+1(1+𝒪︀(Δ𝑧))|=2arctan|Δ𝑧|𝑧|2+1+𝒪︀(Δ𝑧2)|=2[|Δ𝑧|𝑧|2+1+𝒪︀(Δ𝑧2)|+𝒪︀(Δ𝑧3[1|𝑧|2+1+𝒪︀(Δ𝑧)]3)]=2[|Δ𝑧|𝑧|2+1+ℴ︀(Δ𝑧2)|],

    where we have taken the liberty to coalesce orders for simplification. Since

    limΔ𝑧→0|𝑑(𝑧,𝑧+Δ𝑧)Δ𝑧|=2|𝑧|2+1,

    the metric as defined in (8.2.3)(8.2.3)(8.2.3) has a clear geometric meaning: the distance between two points 𝑧 and 𝑧̃ under the metric in (8.2.3)(8.2.3)(8.2.3) is the shortest distance between the corresponding points in 𝑆2, or their spherical distance.

    Thus, if curve 𝛾 joins 𝑧 and 𝑧̃, we have

    𝑑(𝑧,𝑧̃)=inf𝛾∫𝛾𝜎(𝑧)|d𝑧|,

    which attains its infimum when the inverse stereographic projection of 𝛾 is a great circle of 𝑆2. Thus, 𝜎 is known as the spherical metric.

    The corresponding curvature is given by

    𝐾𝜎=−4𝜎2𝜕2𝜕𝑧‾𝜕𝑧(log𝜎(𝑧))=−4𝜎2𝜕𝜕𝑧‾(𝜎𝑧′𝜎)=2𝜎2𝜕𝜕𝑧‾(2𝑧‾1+|𝑧|2)=2𝜎2(𝜎+𝑧‾𝜎𝑧‾′)=(1+|𝑧|2)22(21+|𝑧|2−2|𝑧|2(1+|𝑧|2)2)=(1+|𝑧|2)−|𝑧|2=1,

    where 𝜎𝑧′=𝜕𝜎/𝜕𝑧 and 𝜎𝑧‾′=𝜕𝜎/𝜕𝑧‾. This can also be verified by computing the principal curvatures of the unit sphere, which are both one.

The importance of the selected regions lies in the uniformization to be mentioned in Section 13Section 13Section 13.

Let Ω1 and Ω2 be two open regions in ℂ such that 𝑓:Ω1→Ω2 is univalent (implying that 𝑓′≠0 by Lemma 5.1.2Lemma 5.1.2Lemma 5.1.2). If 𝜌 is a metric on Ω2, then

𝑓∗𝜌=(𝜌∘𝑓)|𝑓′|(8.2.4)

defines a metric on Ω1, referred to as the metric pullback of 𝜌 by 𝑓.

Curvature as defined in (8.2.1)(8.2.1)(8.2.1) is invariant under pullbacks of conformal mappings, or in the case above, we now aim to show that (under assumptions of regularity)

𝐾𝜌(𝑓(𝑧))=𝐾𝑓∗𝜌(𝑧).(8.2.5)

By explicit definition,

𝐾𝑓∗𝜌(𝑧)=−∇2(log∘𝑓∗𝜌(𝑧))(𝑓∗𝜌)(𝑧)2=−∇2(log∘𝜌∘𝑓)(𝑧)+∇2(log|𝑓′(𝑧)|)(𝑓∗𝜌)(𝑧)2.

Since 𝑓′(𝑧)≠0, log∘|𝑓′|=ℜ𝔢log(𝑓′) is harmonic on Ω1 with a vanishing Laplacian. Hence,

𝐾𝑓∗𝜌(𝑧)=−∇2(log∘𝜌∘𝑓(𝑧))(𝜌∘𝑓)2|𝑓′|2=−4(𝜌∘𝑓)2|𝑓′|2𝜕𝜕𝑧‾(𝜕𝜕𝑧(log∘𝜌∘𝑓(𝑧)))=−4(𝜌∘𝑓)2|𝑓′|2𝜕𝜕𝑧‾(𝜕𝜕𝑓(log∘𝜌∘𝑓)𝜕𝑓𝜕𝑧+𝜕𝜕𝑓‾(log∘𝜌∘𝑓)𝜕𝑓‾𝜕𝑧)=−4(𝜌∘𝑓)2|𝑓′|2𝜕𝜕𝑧‾(𝜕log∘𝜌∘𝑓𝜕𝑓𝜕𝑓𝜕𝑧+𝜕log∘𝜌∘𝑓𝜕𝑓‾(𝜕𝑓𝜕𝑧‾)‾)=−4(𝜌∘𝑓)2|𝑓′|2𝜕𝑓𝜕𝑧𝜕𝜕𝑧‾(𝜕log∘𝜌∘𝑓𝜕𝑓)=−4(𝜌∘𝑓)2|𝑓′|2𝜕𝑓𝜕𝑧(𝜕2log∘𝜌∘𝑓𝜕𝑓2𝜕𝑓𝜕𝑧‾+𝜕2log∘𝜌∘𝑓𝜕𝑓‾𝜕𝑓(𝜕𝑓𝜕𝑧)‾)=−4(𝜌∘𝑓)2𝜕2log∘𝜌∘𝑓𝜕𝑓‾𝜕𝑓=−∇𝑓2(log∘𝜌∘𝑓)(𝜌∘𝑓)2=𝐾𝜌(𝑓(𝑧)).

For a given metric d𝑠=𝜆(𝑧)|d𝑧|, if there is some other parameterization such that d𝑠=𝜆′(𝑧′)|d𝑧′|, 𝑧′=𝑓(𝑧) is conformal, then the relation is given by 𝜆=𝑓∗𝜆′. Under differing parameterizations of a metric d𝑠, we once again have the invariance of curvature.

Remark.

In the work of Ahlfors and others, there is no 2⋅ term in front of the hyperbolic and spherical metrics, in which cases the curvatures are −4 and 4 respectively.