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Topological invariants and Holomorphic Mappings

R. E. Greene, K.-T. Kim and N. V. Shcherbina (Greene) Department of Mathematics, University of California, Los Angeles, CA 90095 U. S. A. greene@math.ucla.edu (Kim) Department of Mathematics, Pohang University of Science and Technology, Pohang City 37673 South Korea. kimkt@postech.ac.kr (Shcherbina) Department of Mathematics, University of Wuppertal, Wuppertal 42119 Germany shcherbina@math.uni-wuppertal.de

Abstract. Invariants for Riemann surfaces covered by the disc and for hyperbolic manifolds in general involving minimizing the measure of the image over the homotopy and homology classes of closed curves and maps of the kk-sphere into the manifold are investigated. The invariants are monotonic under holomorphic mappings and strictly monotonic under certain circumstances. Applications to holomorphic maps of annular regions in \mathbb{C} and tubular neighborhoods of compact totally real submanifolds in general in n\mathbb{C}^{n}, n2n\geq 2, are given. The contractibility of a hyperbolic domain with contracting holomorphic mapping is explained.

1. Introduction

It is an elegant and effective technique in Riemannian geometry to consider the minimum-length curve in each nontrivial free homotopy class of closed curves in a compact Riemannian manifold. Such a minimum-length curve always exists and is a smooth closed geodesic. This idea is, for example, the basic step in proving that a compact, orientable manifold of even dimension with everywhere positive sectional curvature is simply connected (cf. [21] p. 172, Theorem 26). If the Riemannian manifold is not compact, then a minimal length curve may not exist, but it remains of interest to consider the infimum of the lengths of closed curves in the free homotopy class and also the infimum over all nontrivial free homotopy classes as well.

The purpose of this paper is to examine this general idea in the context of complex manifolds and also to consider the corresponding possibilities for the situation of maps of the kk-sphere which are homotopically nontrivial, with length replaced by a suitable idea of kk-dimensional measure.

For Riemann surfaces which are covered by the unit disc Δ\Delta—that is, all Riemann surfaces except ,{0},{}\mathbb{C},\mathbb{C}\setminus\{0\},\mathbb{C}\cup\{\infty\}, and compact surfaces of genus 1—the situation becomes one of Riemannian metrics: If π:ΔM\pi\colon\Delta\to M is a holomorphic covering map of the Riemann surface, then the Poincaré metric on the unit disc Δ\Delta “pushes down” to a smooth Riemannian (Hermitian) metric on MM, i.e., there is a unique metric on MM such that π\pi is a local isometry. This canonical push-down metric on such MM’s has the property that, if F:M1M2F\colon M_{1}\to M_{2} is a holomorphic map, then FF is metric nonincreasing. This property will be exploited early in the paper to recover various classical results on maps of annular regions in \mathbb{C} from the viewpoint of minimization of lengths of curves in free homotopy classes.

Extension of these ideas to higher dimensional complex manifolds and to kk-homotopy classes, k>1k>1, involves new features: The natural metric to consider is of course the “hyperbolic metric” introduced by S. Kobayashi, which defines a natural extension to all dimensions of the canonical metric construction for Riemann surfaces just discussed. But a new aspect arises: the Kobayashi metric on a hyperbolic manifold (in the sense of Kobayashi) need not be a Riemannian metric in dimension 2\geq 2. It is, however, a Finsler metric with an infinitesimal form known as the Kobayashi-Royden metric [23]. But for such an infinitesimal metric, which is only upper semi-continuous and does not satisfy the triangle inequality in general, it is necessary to exercise care in defining kk-dimensional volume measure to the image of a kk-sphere in the manifold. We shall consider primarily the details of this matter only for some subsets of n\mathbb{C}^{n}, n2n\geq 2 (cf. Sections 9 and 10), although in principle greater generality would be possible with other hypotheses. This relevant general idea is kk-dimensional Hausdorff measures. These ideas are applied in the final sections to obtain results for holomorphic mappings of tubular neighborhoods of totally real kk-spheres in n\mathbb{C}^{n}, analogous to the earlier results on maps of annular regions (cf. Section 3). It is also natural to consider the tubular neighborhoods of more general compact totally real submanifolds. For such a general case, the degree of maps, a homology invariant is more appropriate and has been investigated.


Some Notation


  • FUKobF^{\textrm{Kob}}_{U} : the Kobayashi-Royden metric of an open set UU in n\mathbb{C}^{n}

  • μX,dk(A)\mu^{k}_{X,d}(A) : the kk-dimensional Hausdorff measure of the subset AA in the metric space (X,d)(X,d)

  • μEuck(B)\mu^{k}_{\textrm{Euc}}(B) : the kk-dimensional Hausdorff measure of the subset BB in n\mathbb{C}^{n} with respect to the Euclidean norm

  • μKob,Uk(C)\mu^{k}_{\textrm{Kob},U}(C) : the kk-dimensional Hausdorff measure of the subset CC of an open set UU in n\mathbb{C}^{n} with respect to the Kobayashi distance

2. The 1\ell_{1}-invariant

Let (X,ρ)(X,\rho) be a metric space with the metric ρ\rho. For a continuous curve α:[a,b]X\alpha\colon[a,b]\to X, and a partition of the interval [a,b][a,b]

P:={tk:k=0,1,,N, with a=t0<t1<<tN=b}P:=\{t_{k}\colon k=0,1,\cdots,N,\textrm{ with }a=t_{0}<t_{1}<\cdots<t_{N}=b\}

for some positive integer NN, let

s(α,P):=k=1Nρ(α(tk1),α(tk)).s(\alpha,P):=\sum_{k=1}^{N}\rho(\alpha(t_{k-1}),\alpha(t_{k})).

If the set {s(α,P):P a partition of [a,b]}\{s(\alpha,P)\colon P\textrm{ a partition of }[a,b]\} is bounded above, we say that α\alpha is rectifiable and define the length L(α)L(\alpha) of α\alpha by

L(α)=sup{s(α,P):P a partition of [a,b]}.L(\alpha)=\sup\{s(\alpha,P)\colon P\textrm{ a partition of }[a,b]\}.

As usual, reparametrizations of rectifiable curves are rectifiable and the length is independent of parametrization.

Definition 2.1.

A map F:X1X2F\colon X_{1}\to X_{2} from a metric space (X1,ρ1)(X_{1},\rho_{1}) to (X2,ρ2)(X_{2},\rho_{2}) is called distance nonincreasing if ρ2(F(x),F(y))ρ1(x,y)\rho_{2}(F(x),F(y))\leq\rho_{1}(x,y) for all x,yX1x,y\in X_{1}.

Notice that, if a map FF is distance nonincreasing, then the FF-images of rectifiable curves are rectifiable and the FF-images have length \leq the length of the original curve, i.e., length F(γ(t))F(\gamma(t))\leq length γ(t)\gamma(t), for all rectifiable curves γ(t)\gamma(t) in X1X_{1}.

Definition 2.2 (The 1\ell_{1}-invariant).

Consider a metric space (X,ρ)(X,\rho) which is not simply connected. Then the 1\ell_{1}-invariant of the metric space XX is defined to be

1(X):=inf{L(α):αa non-contractible rectifiable loop in X},inf=+.\ell_{1}(X):=\inf\{L(\alpha)\colon\alpha~{}\textrm{a non-contractible rectifiable loop in }X\},~{}\inf\varnothing=+\infty.
Proposition 2.1.

If f:(X1,ρ1)(X2,ρ2)f\colon(X_{1},\rho_{1})\to(X_{2},\rho_{2}) is a distance nonincreasing map, and if the induced homomorphism f:π1(X1)π1(X2)f_{*}\colon\pi_{1}(X_{1})\to\pi_{1}(X_{2}) is injective, then 1(X2)1(X1)\ell_{1}(X_{2})\leq\ell_{1}(X_{1}).

Proof.

For a loop α\alpha in X1X_{1} denote by [α][\alpha] the set of all loops that are free homotopic to α\alpha in X1X_{1}. Set

1([α])=inf{L(β):β[α]}.\ell_{1}([\alpha])=\inf\{L(\beta)\colon\beta\in[\alpha]\}.

Then

1(X1)=inf{1([α]):α non-contractible in X1}.\ell_{1}(X_{1})=\inf\{\ell_{1}([\alpha])\colon\alpha\textrm{ non-contractible in }X_{1}\}.

Let ϵ>0\epsilon>0. Take a noncontractible loop β\beta in X1X_{1} with 1([β])<1(X1)+ϵ\ell_{1}([\beta])<\ell_{1}(X_{1})+\epsilon. Then fβf\circ\beta is noncontractible in X2X_{2}, since ff_{*} is injective. Then 1([fβ])1(X2)\ell_{1}([f\circ\beta])\geq\ell_{1}(X_{2}). The distance nonincreasing property of ff implies that

1(X2)1([fβ])1([β])<1(X1)+ϵ.\ell_{1}(X_{2})\leq\ell_{1}([f\circ\beta])\leq\ell_{1}([\beta])<\ell_{1}(X_{1})+\epsilon.

Since this holds for any ϵ>0\epsilon>0, the assertion follows immediately. ∎

Distance nonincreasing/length nonincreasing maps arise naturally in complex analysis. The classical Schwarz Lemma is equivalent to the fact that a holomorphic function ff from the unit disc Δ={z:|z|<1}\Delta=\{z\in\mathbb{C}\colon|z|<1\} into itself with f(0)=0f(0)=0 has the property that d(0,f(z))d(0,z)d(0,f(z))\leq d(0,z), where d=d= the Poincaré distance. Since the action by holomorphic isometries of Δ\Delta to itself relative to the Poincaré metric are transitive on Δ\Delta, what is known as the Schwarz-Pick Lemma follows immediately: If f:ΔΔf\colon\Delta\to\Delta is holomorphic, then d(f(z1),f(z2))d(z1,z2)d(f(z_{1}),f(z_{2}))\leq d(z_{1},z_{2}) for all z1,z2Δz_{1},z_{2}\in\Delta, where dd is the Poincaré distance.

This can be extended to Riemann surfaces as follows: If MM is a Riemann surface that is holomorphically covered by the unit disc Δ\Delta. say π:ΔM\pi\colon\Delta\to M is a holomorphic covering map, then the covering transformation of the covering π\pi are holomorphic isometries for the Poincaré metric. It follows that MM has a unique Riemannian (indeed Hermitian) metric for which π\pi is locally isometric. Let us call this the canonical metric for MM.

If M1M_{1} and M2M_{2} are two such Riemann surfaces, with canonical (Riemannian) metrics g1g_{1} and g2g_{2} respectively, and if F:M1M2F\colon M_{1}\to M_{2} is a holomorphic map, then the pull back Fg2F^{*}g_{2} to M1M_{1} of the metric g2g_{2}, is less than or equal to g1g_{1}, i.e.,

Fg2|pg1|pF^{*}g_{2}|_{p}\leq g_{1}|_{p}

for each pM1p\in M_{1}, where

Fg2|p(v,w)=g2|F(p)(dFp(v),dFp(w)),F^{*}g_{2}|_{p}(v,w)=g_{2}|_{F(p)}(dF_{p}(v),dF_{p}(w)),

for all v,wv,w in the real tangent space of M1M_{1} at pp, so dFp(v)dF_{p}(v) and dFp(w)dF_{p}(w) are in the real tangent space of M2M_{2} at F(p)F(p).

To see this distance nonincreasing property, note that if π1:ΔM1\pi_{1}\colon\Delta\to M_{1} and π2:ΔM2\pi_{2}\colon\Delta\to M_{2} are holomorphic covering maps, then F:M1M2F\colon M_{1}\to M_{2} can be lifted to a holomorphic map F^:ΔΔ\hat{F}\colon\Delta\to\Delta in such a way that the diagram

ΔF^Δπ1π2M1FM2\begin{CD}\Delta @>{\hat{F}}>{}>\Delta\\ @V{\pi_{1}}V{}V@V{}V{\pi_{2}}V\\ M_{1}@>{}>{F}>M_{2}\end{CD}

commutes. The map F^\hat{F} is nonincreasing for the Poincaré metric by the Schwarz-Pick Lemma. (cf. [14])

It follows, since π1\pi_{1} and π2\pi_{2} are (local) isometries, in the sense indicated of the inequality on the pull-back metric, that F:M1M2F\colon M_{1}\to M_{2} is length nonincreasing/distance nonincreasing for the canonical metrics of M1M_{1} and of M2M_{2}, respectively.

3. Holomorphic maps of Riemann surfaces of general type

In the case that M={z:1R<|z|<R}M=\{z\in\mathbb{C}\colon\frac{1}{\sqrt{R}}<|z|<\sqrt{R}\}, R>1R>1, which is covered by the unit disc Δ\Delta, the canonical metric on MM is straightforward to compute. The function F(z)=eizF(z)=e^{iz} defines a covering map of the “strip” {x+iy:lnR<y<lnR}\{x+iy\colon-\ln R<y<\ln R\} onto MM, while the strip is biholomorphic to the upper half plane via the composition of a linear map, exponentiation, and a linear fractional transformation. Tracing through gives the formula

(π/(2lnR)2)r2cos2(πlnr/(2lnR))dr2+(π/(2lnR))2cos2(πlnr/(2lnR))dθ2\frac{\big{(}\pi/(2\ln R)^{2}\big{)}}{r^{2}\cos^{2}\big{(}\pi\ln r/(2\ln R)\big{)}}dr^{2}+\frac{\big{(}\pi/(2\ln R)\big{)}^{2}}{\cos^{2}\big{(}\pi\ln r/(2\ln R)\big{)}}d\theta^{2}

for the canonical metric on MM in (r,θ)(r,\theta) polar coordinates. (Cf. [8], p. 39.)

The free homotopy classes of closed curves in MM are characterized by winding number (around 0) and are nontrivial for all winding numbers except 0. Since winding number is 12π\frac{1}{2\pi} times the total change in polar angle θ\theta around the curve, it follows easily that, for any rectifiable curve γ\gamma in MM, the length of the curve in the canonical metric is π2/lnR\geq\pi^{2}/\ln R. Thus the 1\ell_{1}-invariant of MM in its canonical metric is π2/lnR\geq\pi^{2}/\ln R and indeed

(1) 1(M)=π2lnR,\ell_{1}(M)=\frac{\pi^{2}}{\ln R},

with the infimum realized by once-around the curve r=1r=1 (θ\theta goes from 0 to 2π2\pi), either clockwise or counterclockwise. (Throughout, we are using the Poincaré metric on the unit disc Δ\Delta to be 4(1zz¯)2dzdz¯4(1-z\bar{z})^{-2}dz\ d\bar{z} so that the curvature 1\equiv-1.)

Since {z:A<|z|<B}\{z\in\mathbb{C}\colon A<|z|<B\} is linearly biholomorphic to {z:A/B<|z|<B/A}\{z\colon\sqrt{A/B}<|z|<\sqrt{B/A}\}, the 1\ell_{1}-invariant of {z:A<|z|<B}\{z\in\mathbb{C}\colon A<|z|<B\} is equal to π2/ln(B/A)\pi^{2}/\ln(B/A). The 1\ell_{1}-invariant is preserved by biholomorphic mapping, so the classical result follows:

Theorem 3.1 (Hadamard).

The region {z:A1<|z|<B1}\{z\colon A_{1}<|z|<B_{1}\} is biholomorphic to {z:A2<|z|<B2}\{z\colon A_{2}<|z|<B_{2}\} if, and only if, B1/A1=B2/A2B_{1}/A_{1}=B_{2}/A_{2}.

This result, originally proved by Hadamard (Cf. [17]), is usually proved by non-metric methods, e.g., Schwarz Reflection, [9, 1, 25] et al.

The nonincreasing property of the 1\ell_{1}-invariant gives an extension of this result:

Theorem 3.2.

If 0<A1<B10<A_{1}<B_{1}, 0<A2<B20<A_{2}<B_{2} and B1/A1>B2/A2B_{1}/A_{1}>B_{2}/A_{2}, then every holomorphic mapping f:{z:A1<|z|<B1}{z:A2<|z|<B2}f\colon\{z\colon A_{1}<|z|<B_{1}\}\to\{z\colon A_{2}<|z|<B_{2}\} is homotopically trivial, that is, it is homotopic to a constant map.

Proof. The map ff is homotopically trivial if and only if the ff-image of the curve γ(t)=12(A1+B1)(cost,sint),(t[0,2π])\gamma(t)=\frac{1}{2}(A_{1}+B_{1})(\cos t,\sin t),~{}(t\in[0,2\pi]) is homotopic to a constant curve: this is an immediate consequence of covering space theory. If ff is not homotopically trivial, then the free homotopy class of the ff-image indicated is nontrivial. Then Proposition 2.1 gives that

1({z:A2<|z|<B2})1({z:A1<|z|<B1}),\ell_{1}(\{z\colon A_{2}<|z|<B_{2}\})\leq\ell_{1}(\{z\colon A_{1}<|z|<B_{1}\}),

and the result follows from the formula (1) for the 1\ell_{1}-invariant. \Box

This Theorem 3.2 implies in particular the historical result:

Theorem 3.3 (de Possel [3]).

There is a 1-1 holomorphic mapping g:{z:0<A1<|z|<B1}{z:0<A2<|z|<B2}g\colon\{z\colon 0<A_{1}<|z|<B_{1}\}\to\{z\colon 0<A_{2}<|z|<B_{2}\} whose image separates the boundary components of {z:A2<|z|<B2}\{z\colon A_{2}<|z|<B_{2}\} if and only if B1/A1B2/A2B_{1}/A_{1}\leq B_{2}/A_{2}.

Notice that the condition on gg implies that gg is injective on homotopy; For instance the gg-image of the curve γ\gamma in the preceding proof will be a closed curve in {z:A2<|z|<B2}\{z\colon A_{2}<|z|<B_{2}\} that goes around the origin exactly once. Notice also that the “if” part of this theorem is obviously true by a complex linear map. (Cf. [6, 11] for the original proof.)

A conclusion by the same argument holds for multiply connected domains and Riemann surfaces as well.

Theorem 3.4.

Let XX and YY be Riemann surfaces holomorphically covered by the unit disc with 1(X)<1(Y)\ell_{1}(X)<\ell_{1}(Y). If f:XYf\colon X\to Y is a holomorphic map, then it cannot be injective on homotopy. In particular, ff cannot be a homotopy equivalence.

4. Non-Riemannian Kobayashi hyperbolic case

The only properties of the “canonical metric” on Riemann surfaces covered by the disc that were crucial here were that holomorphic maps were distance nonincreasing and that the canonical metric was locally comparable (in both directions) with any metric derived from local coordinates. In this context, it is clear that the whole viewpoint has an immediate extension to complex manifolds which are “hyperbolic” in the sense introduced by S. Kobayashi. In this section, we consider only complex manifolds (or complex spaces) that are hyperbolic in the sense of Kobayashi, namely, those for which the Kobayashi pseudodistance is an actual distance function. [15, 16].

In this setting, one can define again the 1\ell_{1}-invariant 1(M)\ell_{1}(M) of a hyperbolic manifold to be the infimum of the lengths of closed curves that are not freely homotopic to 0 (assuming MM is not simply connected). Then following the pattern of before one gets the results:

Theorem 4.1.

If f:M1M2f\colon M_{1}\to M_{2} is a holomorphic map of hyperbolic manifolds, and if ff is injective on free homotopy classes of closed curves (in the sense that if γ(t)\gamma(t) is a closed curve in M1M_{1} not freely homotopic to a constant, then f(γ(t))f(\gamma(t)) is not freely homotopic to a constant), then

1(M2)1(M1).\ell_{1}(M_{2})\leq\ell_{1}(M_{1}).

Thus the results discussed in the concrete instances of Riemann surfaces covered by the unit disc and of annular regions in \mathbb{C} in particular, can be extended to far more general settings. The idea of the 1\ell_{1}-invariant via free homotopy classes of closed curves can also be extended to higher dimensional homotopy classes of maps of the kk-sphere into complex hyperbolic manifolds, and to some extent, into general length spaces. These methods will be explored in subsequent sections.

5. Holomorphic mappings of tubular domains

The previous discussion of annular regions in \mathbb{C} has a straightforward extension to tubular domains in n\mathbb{C}^{n}, n>1n>1. For this, define, for 0<r<10<r<1,

Tn(r)={z=(z1,,zn)n:|z1|=1,z(z1,0,,0)<r},T^{n}(r)=\{\vec{z}=(z_{1},\ldots,z_{n})\in\mathbb{C}^{n}\colon|z_{1}|=1,\|\vec{z}-(z_{1},0,\ldots,0)\|<r\},

where \|\cdot\| is the Euclidean norm. Set A(r1,r2)={z:r1<|z|<r2}A(r_{1},r_{2})=\{z\in\mathbb{C}\colon r_{1}<|z|<r_{2}\} where 0<r1<r20<r_{1}<r_{2}. The projection map Pn(z1,,zn)=z1P_{n}(z_{1},\ldots,z_{n})=z_{1} takes Tn(r)T^{n}(r) onto A(1r,1+r)A(1-r,1+r) and there is a natural injection Jn(z)=(z,0,,0)J_{n}(z)=(z,0,\ldots,0) mapping A(1r,1+r)A(1-r,1+r) into Tn(r)T^{n}(r). These maps are homotopy equivalences: JnJ_{n} and PnP_{n} are homotopy inverses to each other. This observation together with Theorem 3.2 gives rise to a comparison result on these tubular domains (meaning tubular neighborhoods of a circle, where the dimensions need not be equal):

Theorem 5.1.

If f:Tn(r)Tm(s)f\colon T^{n}(r)\to T^{m}(s) with r,sr,s between 0 and 11, is holomorphic and if s<rs<r, then ff is homotopic to a constant map.

Proof. The map ff is homotopic to a constant map if and only if the ff-image of the closed curve Γ(t)=(eit,0,,0),t[0,2π]\Gamma(t)=(e^{it},0,\ldots,0),~{}t\in[0,2\pi] in Tn(r)T^{n}(r) is homotopic to a constant curve in Tm(s)T^{m}(s). This is again by the standard covering space theory. But, this happens if and only if the holomorphic map F:A(1r,1+r)A(1s,1+s)F\colon A(1-r,1+r)\to A(1-s,1+s) defined by F:=PmfJnF:=P_{m}\circ f\circ J_{n} is homotopic to a constant. This last follows from the homotopy equivalences already noted. Now Theorem 3.2 implies that, if s<rs<r, this map FF is, and consequently ff is also, homotopic to a constant. \Box

6. Higher homotopy invariants

It is natural to consider extending the previous introduced ideas about curve lengths in free homotopy classes of closed curves to higher dimensional homotopy classes. In particular, if (X,d)(X,d) is a metric space (which we assume arc-wise connected for convenience), then consider continuous maps f:SkXf\colon S^{k}\to X, k>1k>1, Sk={(x0,,xk)k+1:x02++xk2=1}S^{k}=\{(x_{0},\cdots,x_{k})\in\mathbb{R}^{k+1}\colon x_{0}^{2}+\ldots+x_{k}^{2}=1\} and define two such f0,f1:SkXf_{0},f_{1}\colon S^{k}\to X to be free-homotopic if there is a continuous function H:Sk×[0,1]XH\colon S^{k}\times[0,1]\to X such that, for all pp, H(p,0)=f0(p)H(p,0)=f_{0}(p) and H(p,1)=f1(p)H(p,1)=f_{1}(p). If one has a situation where, for suitably restricted ff, one can define the measure of (the image of) such f:SkXf\colon S^{k}\to X, then one could imitate the definition of the 1\ell_{1}-invariant corresponding to the k=1k=1 case. But certain difficulties arise: One needs an idea of such a measure and one would want to know that each free homotopy class of continuous maps SkXS^{k}\to X would contain at least one map ff with the associated measure of the image of ff being finite. This would correspond to rectifiable curves and their lengths, and free-homotopy classes of curves, as in earlier sections.

In the case where (X,d)(X,d) is a Riemannian manifold and dd its Riemannian metric distance, the right idea of measure is, for smooth maps f:SkXf\colon S^{k}\to X, the measure of f|Af|_{A}, ASkA\subset S^{k}, A=A= the set of points of SkS^{k} where the differential dfdf has rank kk, and the measure of f|Af|_{A} is the usual Riemann-metric induced measure on kk-dimensional submanifolds. This measure is

μ(f)=Sk|volume form|\mu(f)=\int_{S^{k}}|\textsl{volume form}|

where the |volume form||\textsl{volume form}| on (v1,,vk)(v_{1},\ldots,v_{k}), where v1,,vkTpSkv_{1},\ldots,v_{k}\in T_{p}S^{k}, is equal to the absolute value of the kk-dimensional Riemannian volume at f(p)f(p) of f(v1)f(vk)f_{*}(v_{1})\wedge\cdots\wedge f_{*}(v_{k}). It is easy to show (and well-known) that every free homotopy class of continuous maps SkXS^{k}\to X in this case (XX is a Riemannian manifold) contains a smooth (not necessarily everywhere nonsingular) map: If ff is a continuous map in the free homotopy class then a sufficiently good smooth approximation of ff will be in the same free homotopy class (by deformation along minimal geodesics). So every free homotopy class contains finite kk-measure maps and hence one can define the infimum of measures over finite-measure (smooth, e.g.) maps in the class and also an k\ell_{k} invariant (= infimum over all nontrivial free homotopy classes).

In the case of more general metric spaces, it is not in general clear that any useful concept of kk-dimensional measure exists. But in the case of metrics which are locally equivalent to Riemannian metrics, the familiar general idea of Hausdorff kk-dimensional measure, can be used.

Definition 6.1 (Cf. [16], p. 343).

Given a metric space (X,d)(X,d), for a nonnegative real number kk and a subset AA, the kk-dimensional Hausdorff measure μX,dk(A)\mu^{k}_{X,d}(A) is defined as

μX,dk(A)=supϵ>0inf{i=1(δ(Ai))k:A=i=1Ai,δ(Ai)<ϵ},\mu^{k}_{X,d}(A)=\sup_{\epsilon>0}\inf\Big{\{}\sum_{i=1}^{\infty}\big{(}\delta(A_{i})\big{)}^{k}\colon A=\bigcup_{i=1}^{\infty}A_{i},\delta(A_{i})<\epsilon\Big{\}},

where δ(Ai)\delta(A_{i}) is the diameter of AiA_{i} defined by

δ(Ai)=supp,qAid(p,q).\delta(A_{i})=\sup_{p,q\in A_{i}}d(p,q).

For a smooth map f:SkMf\colon S^{k}\to M of the kk-sphere SkS^{k} into a Riemannian manifold MM, this μMk(f(Sk))\mu^{k}_{M}(f(S^{k})) gives essentially the same concept of the kk-dimensional measure as the Riemannian measure already defined. But this new notion of measure has the advantage that smoothness is not involved.

Rather than exploring these matters further in generality, we restrict our attention now to the specific situation of the Kobayashi metric for a bounded connected open set UU in n\mathbb{C}^{n}. The open set UU has its Kobayashi metric in the infinitesimal form, the Kobayashi-Royden metric, as it is usually defined by

FUKob(p,v)=inf{r>0:f𝒪(Δ,U),f(0)=p,df(0)=vr}F^{\textrm{Kob}}_{U}(p,v)=\inf\Big{\{}r>0\colon f\in\mathcal{O}(\Delta,U),f(0)=p,df(0)=\frac{v}{r}\Big{\}}

where Δ={z:|z|<1}\Delta=\{z\in\mathbb{C}\colon|z|<1\} and where 𝒪(Δ,U)\mathcal{O}(\Delta,U) denotes the set of holomorphic maps from Δ\Delta to UU. As is well-known [24, 23], the Kobayashi distance from pp to qq for p,qUp,q\in U is the infimum of the length of the C1C^{1} curves from pp to qq in UU where the length is taken to be the integral γFUKob(z,dz)\int_{\gamma}F^{Kob}_{U}(z,dz). (The existence of this integral was also shown in [Op. cit.]). Moreover, it was shown in [2] that FUKob(p,v)F^{Kob}_{U}(p,v) is locally comparable to the standard Euclidean norm of vv in n\mathbb{C}^{n}. This leads easily to the fact that for every free homotopy class of maps SkUS^{k}\to U, there is a smooth map f:SkUf\colon S^{k}\to U (as already noted) and the smooth map will have finite Hausdorff kk-measure relative to the Kobayashi metric, denoted by μKob,Uk(f(Sk))\mu^{k}_{\textrm{Kob},U}(f(S^{k})). We call such a map kk-rectifiable (meaning: Hausdorff kk-measure is finite), and the kk-measure just constructed will be called, in this paper, the Hausdorff-Kobayashi kk-measure.

Thus, one can define an invariant

k(U)=\displaystyle\ell_{k}(U)= infimum of the Hausdorff-Kobayashi kk-measures
over all the Hausdorff-Kobayashi kk-rectifiable
representatives of the nontrivial free homotopy
classes in UU
Lemma 6.1.

If F:UVF\colon U\to V is a holomorphic mapping from a bounded domain in n\mathbb{C}^{n} to a bounded domain in m\mathbb{C}^{m} and if it is injective on free homotopy in the sense that the FF-image of every nontrivial kk-class in UU is nontrivial in VV, then k(V)k(U)\ell_{k}(V)\leq\ell_{k}(U).

Proof. This follows immediately from the fact that FF is distance nonincreasing and hence diameter nonincreasing with respect to the Kobayashi metrics of UU and VV, so the Hausdorff sums are not increased by composition with FF. \Box

7. Illustration of the kk-homotopy invariant

The most natural way to find a bounded connected open set in n\mathbb{C}^{n} which has a nontrivial kk-homotopy class is to take a tubular neighborhood of an embedded kk-sphere. This is particularly interesting from the viewpoint of complex analysis if one takes the kk-sphere to be totally real as a submanifold. In particular, the unit kk-sphere in k+1\mathbb{R}^{k+1} is totally real in k+1\mathbb{C}^{k+1}. Let TrT_{r} be the radius r>0r>0 tubular neighborhood

Tr={(x0,,xk)+λu:\displaystyle T_{r}=\{(x_{0},\ldots,x_{k})+\lambda\vec{u}\colon x02++xk2=1,\displaystyle x_{0}^{2}+\ldots+x_{k}^{2}=1,
uk+1,u=1,0λ<r}.\displaystyle\vec{u}\in\mathbb{C}^{k+1},~{}\|u\|=1,~{}0\leq\lambda<r\}.

For small values of rr, this is a strongly pseudoconvex domain with CC^{\infty} boundary (actually 0<r<120<r<\frac{1}{2} suffices). According to [7], the Kobayashi-Royden metric goes to ++\infty near the boundary relative to the Euclidean metric. Note that there is a natural smooth projection, say P:TrSkP\colon T_{r}\to S^{k}, defined by P(z)=P(z)= the closest point to zz in the Euclidean sense in the set SkS^{k}. The injection SkTrS_{k}\hookrightarrow T_{r} is a homotopy equivalence with PP its homotopy inverse. And the identity (injection) map SkTrS_{k}\to T_{r} is homotopically nontrivial. There may be other smooth maps, say Γ:SkTr\Gamma\colon S^{k}\to T_{r}, homotopic to the injection which have the associated Hausdorff-Kobayashi kk-measure assigned to them being less than the measure assigned to the injection. But the infimum will be realized among the family of maps with image lying in some set of the form

{x+λu:xSk,uk+1,u=1,0λr1}\{\vec{x}+\lambda\vec{u}\colon\vec{x}\in S_{k},\vec{u}\in\mathbb{C}^{k+1},~{}\|u\|=1,~{}0\leq\lambda\leq r_{1}\}

for some r1<rr_{1}<r: this follows easily from the estimates on the growth of the Kobayashi metric near the boundary of TrT_{r} compared to the Euclidean metric. This will yield a conclusion similar to Theorem 3.1, once a technical point about the Kobayashi/Royden infinitesimal metric is established. This will be discussed further in the following sections.

8. Monotonicity of the Kobayashi metric

To find some analogue in this situation of Theorems 3.1, one needs to have an idea of strict monotonicity of the Kobayashi distance for the domains (open connected subsets) in n\mathbb{C}^{n}. Specifically, if two domains Ω1\Omega_{1} and Ω2\Omega_{2} satisfy Ω1Ω2\Omega_{1}\subset\Omega_{2}, then of course their respective Kobayashi-Royden metrics FΩ1Kob,FΩ2KobF^{\textrm{Kob}}_{\Omega_{1}},F^{\textrm{Kob}}_{\Omega_{2}} satisfy FΩ2Kob(p,v)FΩ1Kob(p,v)F^{\textrm{Kob}}_{\Omega_{2}}(p,v)\leq F^{\textrm{Kob}}_{\Omega_{1}}(p,v) for all pΩ1p\in\Omega_{1} and vnv\in\mathbb{C}^{n}. But we would like to obtain a strict comparison between them.

Lemma 8.1.

If Ω1\Omega_{1} and Ω2\Omega_{2} are bounded domains in n\mathbb{C}^{n} satisfying Ω1Ω2\Omega_{1}\subset\subset\Omega_{2} (relatively compact), then for any compact subset KK of Ω1\Omega_{1} there exists a constant cKc_{K} with 0<cK<10<c_{K}<1 such that

FΩ2Kob(p,v)<cKFΩ1Kob(p,v),F^{\textrm{Kob}}_{\Omega_{2}}(p,v)<c_{K}F^{\textrm{Kob}}_{\Omega_{1}}(p,v),

for any pKp\in K and any vnv\in\mathbb{C}^{n}.

Proof. Let the bounded domains Ω1\Omega_{1} and Ω2\Omega_{2} in n\mathbb{C}^{n} satisfy Ω1Ω2\Omega_{1}\subset\subset\Omega_{2}, i.e., Ω1\Omega_{1} is a relatively compact subdomain of Ω2\Omega_{2}.

Then there exists δ>0\delta>0 such that the Euclidean distance between Ω1\Omega_{1} and nΩ2\mathbb{C}^{n}\setminus\Omega_{2} is at least δ\delta.

Let pΩ1p\in\Omega_{1}. Notice that there exist positive numbers bb and BB such that

bFΩ1Kob(p,v)B,vn with v=1,b\leq F^{\textrm{Kob}}_{\Omega_{1}}(p,v)\leq B,~{}\forall v\in\mathbb{C}^{n}\textrm{ with }\|v\|=1,

where \|~{}\| denotes the standard Euclidean norm. Fix pΩ1p\in\Omega_{1} and vnv\in\mathbb{C}^{n} with v=1\|v\|=1. Let ϵ>0\epsilon>0 be given arbitrarily, and then choose h𝒪(Δ,Ω1)h\in\mathcal{O}(\Delta,\Omega_{1}) satisfying h(0)=ph(0)=p, h(0)=v/rh^{\prime}(0)=v/r for some r>0r>0 and

FΩ1Kob(p,v)r<FΩ1Kob(p,v)+ϵ.F^{\textrm{Kob}}_{\Omega_{1}}(p,v)\leq r<F^{\textrm{Kob}}_{\Omega_{1}}(p,v)+\epsilon.

Take

h~(z)=h(z)+δzv.\tilde{h}(z)=h(z)+\delta zv.

Then

h~(0)=h(0)=p,h~(0)=h(0)+δv=(1r+δ)v\tilde{h}(0)=h(0)=p,~{}\tilde{h}^{\prime}(0)=h^{\prime}(0)+\delta v=\Big{(}\frac{1}{r}+\delta\Big{)}v

and

h~(z)Ω2,zΔ,\tilde{h}(z)\subset\Omega_{2},\ \forall z\in\Delta,

since h~(z)h(z)=δzv<δ\|\tilde{h}(z)-h(z)\|=\|\delta zv\|<\delta for every zΔz\in\Delta. So h~𝒪(Δ,Ω2)\tilde{h}\in\mathcal{O}(\Delta,\Omega_{2}).

This implies

FΩ2Kob(p,v)\displaystyle F^{\textrm{Kob}}_{\Omega_{2}}(p,v) 11/r+δ\displaystyle\leq\frac{1}{1/r+\delta}
=r1+rδ\displaystyle=\frac{r}{1+r\delta}
FΩ1Kob(p,v)+ϵ1+δFΩ1Kob(p,v)\displaystyle\leq\frac{F^{\textrm{Kob}}_{\Omega_{1}}(p,v)+\epsilon}{1+\delta F^{\textrm{Kob}}_{\Omega_{1}}(p,v)}
11+δb(FΩ1Kob(p,v)+ϵ).\displaystyle\leq\frac{1}{1+\delta b}(F^{\textrm{Kob}}_{\Omega_{1}}(p,v)+\epsilon).

Since ϵ>0\epsilon>0 is arbitrary, we obtain that

FΩ2Kob(p,v)11+δbFΩ1Kob(p,v)F^{\textrm{Kob}}_{\Omega_{2}}(p,v)\leq\frac{1}{1+\delta b}F^{\textrm{Kob}}_{\Omega_{1}}(p,v)

for any vnv\in\mathbb{C}^{n}, due to the homogeneity of the Kobayashi-Royden metric.

Note that bb depends on the location of pp. But on a compact set it stays bounded away from zero, and the desired conclusion follows immediately. \Box

The restriction in Lemma 8.1 to a compact set KK can be removed.

Lemma 8.2.

If UU is a bounded open set in n\mathbb{C}^{n} with its closure contained in another bounded open set VV, then there is a constant c(0,1)c\in(0,1) such that

FVKob(p,v)cFUKob(p,v)(p,v)U×n,F^{\textrm{Kob}}_{V}(p,v)\leq cF^{\textrm{Kob}}_{U}(p,v)\quad\forall(p,v)\in U\times\mathbb{C}^{n},

where FUKobF^{\textrm{Kob}}_{U} and FVKobF^{\textrm{Kob}}_{V} are the infinitesimal Kobayashi-Royden metrics of UU and VV, respectively.

Proof. Denote by cl(A)\textrm{cl}(A) the closure in n\mathbb{C}^{n} of the subset AA of n\mathbb{C}^{n}. There is a bounded open set WW satisfying

cl(U)Wcl(W)V.\textrm{cl}(U)\subset W\subset\textrm{cl}(W)\subset V.

With WW so chosen, we have:

FWKob(q,v)FUKob(q,v)(q,v)U×n,F^{\textrm{Kob}}_{W}(q,v)\leq F^{\textrm{Kob}}_{U}(q,v)\quad\forall(q,v)\in U\times\mathbb{C}^{n},

and

FVKob(p,v)FWKob(p,v)(p,v)W×n.F^{\textrm{Kob}}_{V}(p,v)\leq F^{\textrm{Kob}}_{W}(p,v)\quad\forall(p,v)\in W\times\mathbb{C}^{n}.

Lemma 8.1 gives that there is a constant cc with 0<c<10<c<1 such that

FVKob(q,v)cFWKob(q,v)(q,v)cl(U)×n.F^{\textrm{Kob}}_{V}(q,v)\leq cF^{\textrm{Kob}}_{W}(q,v)\quad\forall(q,v)\in\textrm{cl}(U)\times\mathbb{C}^{n}.

In particular, this yields that

FVKob(p,v)cFWKob(p,v)cFUKob(p,v)(p,v)U×n,F^{\textrm{Kob}}_{V}(p,v)\leq cF^{\textrm{Kob}}_{W}(p,v)\leq cF^{\textrm{Kob}}_{U}(p,v)\quad\forall(p,v)\in U\times\mathbb{C}^{n},

as desired. \Box

9. The example from Section 7 concluded

The results of Section 6 and Section 7 together with the growth of the Kobayashi-Royden metric established in [7] can be combined to establish the results about the domains TrT_{r} defined in Section 6:

First we note that the k\ell_{k}-invariants are nonzero in this case. As before, we assume that all rr-values are small enough that TrT_{r} is strongly pseudoconvex.

Lemma 9.1.

With TrT_{r} as defined in Section 6, and k\ell_{k} defined as before,

k(Tr)>0.\ell_{k}(T_{r})>0.

Proof. Since TrT_{r} has smooth strictly pseudoconvex boundary, Graham [7] gives that there is a compact subset KK of TrT_{r} such that for each pTrKp\in T_{r}\setminus K and all vv,

FTrKob(p,v)v,F^{\textrm{Kob}}_{T_{r}}(p,v)\geq\|v\|,

where \|~{}\| represents the usual Euclidean norm. For such a fixed compact set KK, there is a constant c>0c>0 such that

FTrKob(p,v)cvF^{\textrm{Kob}}_{T_{r}}(p,v)\geq c\|v\|

for all pKp\in K and all vnv\in\mathbb{C}^{n}.

Replace cc by min{c,1}\min\{c,1\}. It follows that k(Tr)ckL(Tr)\ell_{k}(T_{r})\geq c^{k}\ L(T_{r}), where L(Tr)L(T_{r}) represents the infimum of the Euclidean Hausdorff kk-measure of the image of SkS^{k} in TrT_{r} not homotopic to a constant. This latter infimum is positive by elementary considerations. \Box

Theorem 9.1.

If 0<r<s0<r<s, then k(Tr)>k(Ts)\ell_{k}(T_{r})>\ell_{k}(T_{s}). In particular, TrT_{r} is not biholomorphic to TsT_{s}.

Proof. Consider the inclusion map TrTsT_{r}\hookrightarrow T_{s}. By Graham [7], given any C>0C>0, there is a compact subset KK of TrT_{r} such that FTrKobC(Euclidean metric)F^{\textrm{Kob}}_{T_{r}}\geq C\cdot\textrm{(Euclidean metric)} at every point pTrKp\in T_{r}\setminus K, since FTrKobF^{\textrm{Kob}}_{T_{r}} goes to infinity at the boundary of TrT_{r} and hence, choosing CC sufficiently large, FTrKob2FTsKobF^{\textrm{Kob}}_{T_{r}}\geq 2F^{\textrm{Kob}}_{T_{s}}. This follows since FTsKobF^{\textrm{Kob}}_{T_{s}} is bounded by some multiple of Euclidean metric on TrT_{r} since TrTsT_{r}\subset\subset T_{s}. By Lemma 8.1 (and its proof) there is an ϵ\epsilon with 0<ϵ<10<\epsilon<1 such that FTrKob(1+ϵ)FTsKobF^{\textrm{Kob}}_{T_{r}}\geq(1+\epsilon)F^{\textrm{Kob}}_{T_{s}} at every point of KK. Then

FTrKob(1+ϵ)FTsKobF^{\textrm{Kob}}_{T_{r}}\geq(1+\epsilon)F^{\textrm{Kob}}_{T_{s}}

at every point of TrT_{r}. It follows that k(Tr)(1+ϵ)kk(Ts)\ell_{k}(T_{r})\geq(1+\epsilon)^{k}\ell_{k}(T_{s}) and, since k(Ts)>0\ell_{k}(T_{s})>0,

k(Tr)>k(Ts).\ell_{k}(T_{r})>\ell_{k}(T_{s}).

This completes the proof. \Box

The arguments used to prove Theorem 3.2 can be extended in a straightforward way to prove a corresponding result for the domains of TrT_{r} type:

Theorem 9.2.

If r1>r2r_{1}>r_{2}, then every holomorphic mapping f:Tr1Tr2f\colon T_{r_{1}}\to T_{r_{2}} is homotopic to a constant map.

10. Tubular neighborhoods in general

The analysis of tubular neighborhoods of totally real embeddings of spheres in the previous section can be extended to more general circumstances. But this extension involves what amounts to a shift from homotopy to homology: the role of being homotopically nontrivial is taken over by having degree not equal to 0.

The first step is to define the relevant concept of degree: Suppose that MM is a smooth (C2C^{2} suffices) compact connected submanifold without boundary of a Euclidean space N\mathbb{R}^{N} and let

Tr=wM{vN:vw<r},T_{r}=\bigcup_{w\in M}\{v\in\mathbb{R}^{N}\colon\|v-w\|<r\},

where \|~{}\| is the usual Euclidean norm. Notice that there exists R>0R>0 such that TrT_{r}, for any rr with 0<r<R0<r<R, there exists a natural projection π:TrM\pi\colon T_{r}\to M onto MM, defined by

π(v)=infpMpv\pi(v)=\inf_{p\in M}\|p-v\|

so that π(v)\pi(v) is the closest point to vv among points of MM, with respect to the Euclidean distance. If g:MTrg\colon M\to T_{r} is a continuous map of MM into TrT_{r}, then it is natural to define the degree of gg, denoted by degg\deg g, to be the degree of πg:MM\pi\circ g\colon M\to M. (If MM is orientable, this is to be the usual \mathbb{Z}-valued degree. If MM is nonorientable, we take degree to be 2\mathbb{Z}_{2}-valued.) If G:Tr1Tr2G\colon T_{r_{1}}\to T_{r_{2}} is a continuous map, with r1,r2(0,R)r_{1},r_{2}\in(0,R), we define

degG:=the degree of Gi:MTr2,\deg G:=\textrm{the degree of }G\circ i\colon M\to T_{r_{2}},

where i:MTr1i\colon M\to T_{r_{1}} is an injection. As well known, these concepts of degree are multiplicative: the degree of a composition is equal to the product of the degrees.

With these definitions in sight, the analogue of Theorem 9.2 is the following:

Theorem 10.1.

Let MM be a smooth compact connected totally real submanifold of n\mathbb{C}^{n}. Then there is a constant R>0R>0 such that, if 0<r<s<R0<r<s<R and if F:TsTrF\colon T_{s}\to T_{r} is holomorphic then, FF has degree zero.

The conditions on RR here are such that

  • TrT_{r} has smooth strongly pseudoconvex boundary and

  • the projection map π:TrM\pi\colon T_{r}\to M is well defined (and continuous in particular),

whenever 0<r<R0<r<R.

Note that this result is in fact an extension of Theorem 9.2 since, in the case that MM is a sphere, FF being homotopic to a constant is equivalent to degF=0\deg F=0. But in general, of course, degF=0\deg F=0 does not imply that FF is homotopic to a constant. The most obvious example may be the map of Sp×SpS^{p}\times S^{p} to itself, p1p\geq 1, identity on the first factor and constant on the second.

Proof of Theorem 10.1 follows the general pattern of the proofs of previous theorems, but requires some preparation.

First, we need

Definition 10.1.

Let k=dimMk=\dim M. For r(0,R)r\in(0,R) as above, let

Vrk:=inf{μKob,Trk(g(M))g:\displaystyle V_{r}^{k}:=\inf\{\mu^{k}_{\textrm{Kob},T_{r}}(g(M))\mid g\colon MTr continuous\displaystyle M\to T_{r}\textrm{ continuous}
and rectifiable with degg0}.\displaystyle\textrm{and rectifiable with }\deg g\neq 0\}.

Now we need

Lemma 10.1.

Vrk>0V^{k}_{r}>0 for any r(0,R)r\in(0,R).

Proof; With g:MTrg\colon M\to T_{r}, degg0\deg g\neq 0, the composition g^:=πg:MM\hat{g}:=\pi\circ g\colon M\to M has nonzero degree and is hence surjective.

The projection π:TRM\pi\colon T_{R}\to M admits a constant C>0C>0 such that π(x)π(y)Cxy\|\pi(x)-\pi(y)\|\leq C\|x-y\| with respect to the standard Euclidean norm. Thus the Euclidean Hausdorff kk-volume of πg(M)\pi\circ g(M) is at least as large as that of MM, bounded away from 0.

On the other hand, for 0<r<R0<r<R, TrT_{r} is bounded strongly pseudoconvex. So, by [7], the Kobayashi-Royden metric FTrKobF^{\textrm{Kob}}_{T_{r}} of TrT_{r} goes to infinity compared to the Euclidean metric as the base point approaches the boundary of TrT_{r}. Hence there is a constant c>0c>0 such that FTrKob(q,w)cwF^{\textrm{Kob}}_{T_{r}}(q,w)\geq c\|w\| for any qTr,wnq\in T_{r},w\in\mathbb{C}^{n}. Hence we obtain that

μKob,Trk(g(M))ckμEuck(g(M)).\mu^{k}_{\textrm{Kob},T_{r}}(g(M))\geq c^{k}\mu^{k}_{Euc}(g(M)).

Since

μEuck(g(M))CkμEuck(π(g(M)))CkμEuck(M),\mu^{k}_{Euc}(g(M))\geq C^{-k}\mu^{k}_{Euc}(\pi(g(M)))\geq C^{-k}\mu^{k}_{Euc}(M),

it follows that infgμKob,Trk(g(M))(c/C)kμEuck(M)>0\inf_{g}\mu_{\textrm{Kob},T_{r}}^{k}(g(M))\geq(c/C)^{k}\mu^{k}_{Euc}(M)>0, as desired. \Box

Lemma 10.2.

Vsk<VrkV^{k}_{s}<V^{k}_{r} if 0<r<s<R0<r<s<R.

Proof: By Lemma 8.2, the strict inclusion of the closure of TrT_{r} into TsT_{s} implies that there is a constant cc with 0<c<10<c<1 such that FTsKob(z,v)cFTrKob(z,v)F^{\textrm{Kob}}_{T_{s}}(z,v)\leq cF^{\textrm{Kob}}_{T_{r}}(z,v) for any zTrz\in T_{r} and vnv\in\mathbb{C}^{n}. Hence for each g:MTrg\colon M\to T_{r} of nonzero degree,

μKob,Tsk(g(M))ckμKob,Trk(g(M)).\mu^{k}_{\textrm{Kob},T_{s}}(g(M))\leq c^{k}\mu^{k}_{\textrm{Kob},T_{r}}(g(M)).

So VskckVrkV^{k}_{s}\leq c^{k}V^{k}_{r}. Since Vs>0V_{s}>0 by Lemma 10.1, it follows that Vsk<VrkV^{k}_{s}<V^{k}_{r}. \Box.

Proof of Theorem 10.1. Let 0<r<s<R0<r<s<R as in the hypothesis. Suppose that F:TsTrF\colon T_{s}\to T_{r} is holomorphic. And suppose, for a proof by contradiction that degF0\deg F\neq 0. If a continuous map g:MTsg\colon M\to T_{s} has a nonzero degree, then

deg(Fg)=(degF)(degg)0.\deg(F\circ g)=(\deg F)(\deg g)\neq 0.

Thus

VrkμKob,Trk(Fg(M)),V^{k}_{r}\leq\mu^{k}_{\textit{Kob},T_{r}}(F\circ g(M)),

since Fg:MTrF\circ g\colon M\to T_{r} is a continuous map with nonzero degree. But μKob,Trk(Fg(M))μKob,Tsk(g(M))\mu^{k}_{\textit{Kob},T_{r}}(F\circ g(M))\leq\mu^{k}_{\textit{Kob},T_{s}}(g(M)), since FF is Kobayashi-metric nonincreasing. Thus

VrkμKob,Tsk(g(M)),V^{k}_{r}\leq\mu^{k}_{\textit{Kob},T_{s}}(g(M)),

which implies that

VrkVsk.V^{k}_{r}\leq V^{k}_{s}.

This contradicts Lemma 10.2, and the proof is complete. \Box

11. Contraction Mapping and Homotopy

The situation of a map f:UVf\colon U\to V with VUV\subset U with ff distance nonincreasing for some metric dUd_{U} on UU is a natural condition for considering the ideas associated to iterations of contraction mappings. It is a familiar and long-standing principle of analysis that in the case where ff is distance nonincreasing by a factor 0α<10\leq\alpha<1, then ff must have a fixed point if UU is complete with respect to the metric dUd_{U}. This is a natural way to prove the existence of a short-term solution of ordinary differential equations, the local surjectivity in the Inverse Function Theorem via Newton’s Method, and many other basic results (Cf. e.g. [5]). Such contraction mapping ideas were used in [4] to prove a fixed point theorem for holomorphic maps in Banach spaces, now known as the Earle-Hamilton Fixed Point Theorem. The finite dimensional version was proved earlier in [22]. In both papers, the Carathéodory metric rather than the Kobayashi metric was used. We point out also that the finite dimensional version was proved even earlier in [13] p. 83 (p. 92, in the 2nd ed.), using the fact that any compact analytic set in the complex Euclidean space consists of finitely many points. On the other hand, the following theorem shows that the Kobayashi metric can also be used in the contraction mapping context in a way similar to [22] and [4].

Theorem 11.1.

If UU is a bounded domain in n\mathbb{C}^{n} and f:UUf\colon U\to U is a holomorphic mapping such that f(U)f(U) is contained in a compact subset of UU, then there is a unique point z0Uz_{0}\in U such that f(z0)=z0f(z_{0})=z_{0}. Moreover, this z0z_{0} is exactly the only point such that the iterates fn(z)=ff(z)f^{n}(z)=f\circ\ldots\circ f(z), nn-times, of ff converge uniformly on UU to the constant map at z0z_{0} on UU.

Proof. Choose an open set VV in n\mathbb{C}^{n} with its compact closure V¯\overline{V} in n\mathbb{C}^{n} satisfying

f(U)VV¯U.f(U)\subset V\subset\overline{V}\subset U.

Let dUd_{U} be the Kobayashi distance on UU. Lemma 8.2 shows that there exists 0c<10\leq c<1 such that

FUKob(f(p),df|p(v))cFVKob(f(p),df|p(v)),(p,v)U×n,F^{\textrm{Kob}}_{U}(f(p),df|_{p}(v))\leq c\cdot F^{\textrm{Kob}}_{V}(f(p),df|_{p}(v)),~{}\forall(p,v)\in U\times\mathbb{C}^{n},

which in turn implies that

FUKob(fγ(t)),(fγ)(t))\displaystyle F^{\textrm{Kob}}_{U}(f\circ\gamma(t)),(f\circ\gamma)^{\prime}(t)) cFVKob(fγ(t)),(fγ)(t))\displaystyle\leq c\cdot F^{\textrm{Kob}}_{V}(f\circ\gamma(t)),(f\circ\gamma)^{\prime}(t))
cFUKob(γ(t),γ(t))\displaystyle\leq c\cdot F^{\textrm{Kob}}_{U}(\gamma(t),\gamma^{\prime}(t))

for any C1C^{1} curve γ:[0,1]U\gamma\colon[0,1]\to U. So we have

FUKob(fγ(t)),(fγ)(t))cFKobU(γ(t),γ(t))F^{\textrm{Kob}}_{U}(f\circ\gamma(t)),(f\circ\gamma)^{\prime}(t))\leq c\cdot F^{\textrm{Kob}}_{U}(\gamma(t),\gamma^{\prime}(t))

for any C1C^{1} curve γ:[0,1]U\gamma\colon[0,1]\to U, and consequently

dU(f(p),f(q))cdU(p,q),p,qU.d_{U}(f(p),f(q))\leq c\cdot d_{U}(p,q),~{}\forall p,q\in U.

Namely, ff is a strict contraction with the contraction factor cc.

Now denote by fnf^{n} the nn-th iterate of ff defined inductively by

f1=f,fn+1=ffn(n=1,2,).f^{1}=f,~{}f^{n+1}=f\circ f^{n}\quad(n=1,2,\cdots).

If pUp\in U, then it follows that the sequence fn(p)f^{n}(p) is a Cauchy sequence with respect to dUd_{U}. Even if UU were not necessarily dUd_{U}-complete, this Cauchy sequence still converges because, for n1n\geq 1, fn(p)f^{n}(p) belongs to V¯\overline{V}, a compact set with V¯U\overline{V}\subset U. Thus z0:=limnfn(p)z_{0}:=\lim\limits_{n\to\infty}f^{n}(p) exists in V¯\overline{V}, and consequently in UU. And f(z0)=z0f(z_{0})=z_{0}. Of course this is the unique fixed point: if f(z1)=z1f(z_{1})=z_{1} then

dU(z0,z1)=dU(f(z0),f(z1))cdU(z0,z1),d_{U}(z_{0},z_{1})=d_{U}(f(z_{0}),f(z_{1}))\leq c\cdot d_{U}(z_{0},z_{1}),

which implies dU(z0,z1)=0d_{U}(z_{0},z_{1})=0 and z0=z1z_{0}=z_{1}.

The uniform convergence of fnf^{n} on UU follows by

dU(z0,fk+1(p))\displaystyle d_{U}(z_{0},f^{k+1}(p)) =dU(fk+1(z0),fk+1(p))\displaystyle=d_{U}(f^{k+1}(z_{0}),f^{k+1}(p))
ckdU(f(z0),f(p))\displaystyle\leq c^{k}d_{U}(f(z_{0}),f(p))
ckdU(z0,f(p)),\displaystyle\leq c^{k}d_{U}(z_{0},f(p)),

which implies

suppUdU(z0,fk+1(p))cksupf(p)VdU(z0,f(p)).\sup_{p\in U}d_{U}(z_{0},f^{k+1}(p))\leq c^{k}\sup_{f(p)\in V}d_{U}(z_{0},f(p)).

Note that supf(p)VdU(z0,fm(p))\sup_{f(p)\in V}d_{U}(z_{0},f^{m}(p)) is bounded, since the Kobayashi distance is a continuous function by [2]. Moreover, there exists a positive integer mm such that for some constant C>0C>0 it holds that

1CdU(z0,fn(p))z0fn(p)CdU(z0,fn(p))\frac{1}{C}\ d_{U}(z_{0},f^{n}(p))\leq\|z_{0}-f^{n}(p)\|\leq C\ d_{U}(z_{0},f^{n}(p))

for any n>mn>m. Altogether, we see that the convergence of fkf^{k} to the constant function at z0z_{0} is uniform on UU, \Box

This recovers Theorem 9.2: With the notation therein, if f:Tr1Tr2f\colon T_{r_{1}}\to T_{r_{2}} with r1>r2r_{1}>r_{2} is holomorphic then, since Tr2T_{r_{2}} is relatively compact in Tr1T_{r_{1}}, there is a point z0Tr1z_{0}\in T_{r_{1}} with f(z0)=z0f(z_{0})=z_{0}. Consider fnf^{n} with nn large. Then as mentioned before

deg(fn)=(degf)n.\deg(f^{n})=\big{(}\deg f\big{)}^{n}.

But fn(Tr1)f^{n}(T_{r_{1}}) is contained in a small ball around z0z_{0}. So the composition Pr2fniP_{r_{2}}\circ f^{n}\circ i must have degree 0, and the rest of necessary arguments follows immediately.

A variant of this idea also produces this result about connected open subsets in n\mathbb{C}^{n} and their images under holomorphic maps to themselves where the image is contained in a relatively compact subset.

Theorem 11.2.

If UU is a bounded connected open set with smooth boundary in n\mathbb{C}^{n}, and if there is a holomorphic map f:UUf\colon U\to U such that f(U)f(U) is contained in a compact subset of UU and that, for some zUz\in U and for all k=1,2,k=1,2,\ldots, the induced map f:πk(U,z)πk(U,f(z))f_{*}\colon\pi_{k}(U,z)\to\pi_{k}(U,f(z)) is an isomorphism, then UU is contractible.

The theorem is illustrated by a bounded open sets UU with smooth boundary that are star-shaped around the origin with f(z)=rzf(z)=rz for a constant rr with 0<r<10<r<1.

The proof involves two lemmas:

Lemma 11.1.

Every bounded open set UU in N\mathbb{R}^{N} with smooth boundary has the homotopy type of a finite CW complex.

Lemma 11.2.

With UU and ff as in the hypotheses of Theorem 11.2, and with z0z_{0} the fixed point of ff (which has already been shown to exist), the kk-th homotopy group πk(U)=0\pi_{k}(U)=0 for any k=1,2,k=1,2,\cdots.

The proof of Theorem 11.2 follows from these two lemmas and the Whitehead theorem ([26]. See also [12], Theorem 4.5 in page 346), since ff and the constant map z0z_{0} have the same action on the homotopy groups of UU at z0z_{0}. [The general result of Whitehead is that, if both XX and YY have the homotopy type of connected finite CW complexes and if two continuous maps f,g:XYf,g\colon X\to Y, where ff is a homotopy equivalence, satisfy the properties that f(x0)=g(x0)f(x_{0})=g(x_{0}) for some x0Xx_{0}\in X and g,f:πk(X,x0)πk(Y,f(x0))g_{*},f_{*}:\pi_{k}(X,x_{0})\to\pi_{k}(Y,f(x_{0})) are identical for every k=1,2,k=1,2,\cdots, then ff is homotopic to gg.] In our case, f=0f_{*}=0 and gg is to be the constant map at z0z_{0}, so both ff_{*} and gg_{*} coincide as the trivial map of πk\pi_{k} for every kk. \Box

Remark 11.1.

The open set UU is homotopically equivalent to a finite CW complex, but not homeomorphic to. Note for instance that any finite CW complex is compact. On the other hand, the fact that UU is of the same homotopy type with a finite CW complex is sufficient for the preceding proof.

Proof of Lemma 11.1: Let d(z)=dist (z,U)d(z)=\textrm{dist }(z,\mathbb{C}\setminus U), where dist (z,A)=inf{zw:wA}\textrm{dist }(z,A)=\inf\{\|z-w\|\colon w\in A\}. Here of course \|~{}\| is the Euclidean norm of n\mathbb{C}^{n}. Since UU is open, d(z)>0d(z)>0 for every zUz\in U and the map zd(z)z\to d(z) is Lipschitz continous. Also, since UU has smooth boundary, d(z)d(z) is of class C1C^{1} at least (CC^{\infty} if UU has CC^{\infty} boundary) on 𝒩ϵ:={zU:d(z)<ϵ}\mathcal{N}_{\epsilon}:=\{z\in U\colon d(z)<\epsilon\} for sufficiently small a constant ϵ>0\epsilon>0, and grad d=1\|\textsl{grad }d\|=1 at every zUz\in U with d(z)<ϵd(z)<\epsilon, where grad d\textsl{grad }d is the real Euclidean gradient.

Now set δ(z)=lnd(z)\delta(z)=-\ln d(z). Then δ\delta is smooth on 𝒩ϵ\mathcal{N}_{\epsilon}, and grad δ(z)1/ϵ\|\textsl{grad }\delta(z)\|\geq 1/\epsilon for every z𝒩ϵz\in\mathcal{N}_{\epsilon}. (In fact, the inequality is ==, but we do not need it here.) Now, for notational convenience, let

K1={zU:d(z)ϵ},Km={zU:d(z)ϵ/m}K_{1}=\{z\in U\colon d(z)\geq\epsilon\},\quad K_{m}=\{z\in U\colon d(z)\geq\epsilon/m\}

for m=1,2,m=1,2,\cdots. (We shall need only the first few of these). The sets KmK_{m} defined as such are compact in n\mathbb{C}^{n}.

Now dd may not be smooth on UU; indeed, dd cannot be smooth since dd has a maximum in UU but grad d=1\|\textsl{grad }d\|=1 at every point at which dd is of class C1C^{1}. So δ\delta is also nonsmooth at some points. However, by standard convolution smoothing arguments, there is a smooth function, say Δ\Delta, such that Δ\Delta is uniformly close to δ\delta on K4K_{4} but (uniformly) C1C^{1}-close to δ\delta on K4K1K_{4}\setminus K_{1}. By usual Morse theoretic considerations ([19]. Cf. Section I.6 of [18]. See also [10].) there is a function Δ1\Delta_{1} which is uniformly C1C^{1}-close to Δ\Delta on K3K_{3} and has only nondegenerate critical points. Since Δ\Delta and δ\delta are C1C^{1}-close on K4K1K_{4}\setminus K_{1} and grad δ1/ϵ\|\textsl{grad }\delta\|\geq 1/\epsilon on K4K1K_{4}\setminus K_{1}, it follows by the usual partition of unity argument that Δ\Delta on the interior of K3K_{3}, and δ\delta on UU can be patched together to yield a function Δ2\Delta_{2}, say, such that

Δ2(z)=Δ(z),zK3\Delta_{2}(z)=\Delta(z),\forall z\in K_{3}

with grad Δ21/(2ϵ)\|\textsl{grad }\Delta_{2}\|\geq 1/(2\epsilon) on UK1U\setminus K_{1}, and such that

Δ2(z)=δ(z),zUK1.\Delta_{2}(z)=\delta(z),\forall z\in U\setminus K_{1}.

Then Δ2\Delta_{2} is an exhaustion function for UU with only nondegenerate critical points, since Δ2\Delta_{2} has no critical points in UK1U\setminus K_{1} and hence only nondegenerate critical points in UU, which necessarily lie in the set where Δ=Δ1\Delta=\Delta_{1}.

The standard Morse theory gives now that UU has the homotopy type of a finite CW complex, with cells given by the finite number of nondegenerate critical points of Δ2\Delta_{2}. \Box

Proof of Lemma 11.2: Let z0z_{0} be the fixed point of ff. Suppose that Γ:SkU\Gamma\colon S^{k}\to U is a representation of a kk-homotopy class in πk(U,z0)\pi_{k}(U,z_{0}). By Theorem 11.1, the iterates fnΓf^{n}\circ\Gamma converge uniformly on SkS^{k} to the constant map at z0z_{0}. In particular, if a positive constant rr is such that Bn(z0,r)={z:zz0<r}UB^{n}(z_{0},r)=\{z\colon\|z-z_{0}\|<r\}\subset U and fnΓ(Sk)Bn(z0,r)f^{n}\Gamma(S^{k})\subset B^{n}(z_{0},r), then [fnΓ]=0[f^{n}\circ\Gamma]=0 in πk(U,z0)\pi_{k}(U,z_{0}). But by hypothesis, fn:πk(U,z0)πk(U,z0)f^{n}_{*}\colon\pi_{k}(U,z_{0})\to\pi_{k}(U,z_{0}) is an isomorphism. So [Γ]=0[\Gamma]=0 in πk(U,z0)\pi_{k}(U,z_{0}). \Box

Acknowledgements

After this article was written and posted in arXiv.org, T. Pacini kindly informed us the relevance of [20]. We express our gratitude for this.

Research of the second named author (Kim) is partially supported by the NRF Grant 4.0021348 of The Republic of Korea.

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