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Let \(\gamma:[0, l] \rightarrow S\) be a geodesic on a complete surface \(S\), and assume that \(\gamma(l)\) is not conjugate to \(\gamma(0)\). Let \(w_{0} \in T_{\gamma(0)}(S)\) and \(w_{1} \in T_{\gamma(l)}(S)\). Prove that there exists a unique Jacobi field \(J(s)\) along \(\gamma\) with \(J(0)=w_{0}\), \(J(l)=w_{1} .\)

Short Answer

Expert verified
The non-conjugacy of \(\gamma(l)\) to \(\gamma(0)\) ensures a unique Jacobi field \(J(s)\).

Step by step solution

01

Understanding the Problem

A geodesic \(\gamma:[0, l] \rightarrow S\) is given on a complete surface \(S\), and \(w_{0} \in T_{\gamma(0)}(S)\) and \(w_{1} \in T_{\gamma(l)}(S)\) are tangent vectors at the endpoints of the geodesic. We need to prove the existence and uniqueness of a Jacobi field \(J(s)\) along \(\gamma\) such that \(J(0)=w_{0}\) and \(J(l)=w_{1}\).
02

Define the Jacobi Field

A Jacobi field \(J(s)\) along the geodesic \(\gamma(s)\) is a vector field that satisfies the Jacobi equation \(J''(s) + R(J(s), \gamma'(s)) \gamma'(s) = 0\), where \(R\) is the Riemann curvature tensor.
03

Utilize Initial and Boundary Conditions

We need to ensure that \(J(0) = w_{0}\) and \(J(l) = w_{1}\). Since \(J(s)\) satisfies the Jacobi equation, it is determined by its values and derivatives at two points, provided those values uniquely specify solutions of a second-order linear differential equation.
04

Varifying Non-conjugacy Condition

Given that \(\gamma(l)\) is not conjugate to \(\gamma(0)\), this implies that the differential of the exponential map at \(\gamma(0)\) is an isomorphism between the tangent spaces \(T_{\gamma(0)}(S)\) and \(T_{\gamma(l)}(S)\).
05

Formulate and Solve the Linear System

Given the initial condition \(J(0) = w_0\) and the boundary condition \(J(l) = w_1\), we can set up a linear system. The non-conjugacy guarantees that this system has a unique solution.
06

Conclusion

By solving the linear system, we find that there exists a unique Jacobi field \(J(s)\) that satisfies the given conditions. Hence, the existence and uniqueness of the Jacobi field \(J(s)\) with \(J(0) = w_{0}\) and \(J(l) = w_{1}\) is proven.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Geodesics
A geodesic is the shortest path between two points on a curved surface. Think of it like the generalization of a straight line, but for curved spaces. On Earth, the geodesics are the great circles, like the equator or the segments connecting the North and South Poles along the surface.

For a mathematical description, consider a surface \(S\), and let \(\gamma(s)\) be a curve on this surface parameterized by \(s\). The curve \(\gamma(s)\) is a geodesic if the acceleration vector of the curve is always perpendicular to the surface. This can be formulated using the geodesic equation:

\[ \frac{D \dot{\gamma}}{ds} = 0 \] where \(\frac{D}{ds}\) denotes the covariant derivative along the curve.
  • Geodesics take the shortest path between two points in a curved space.
  • The concept generalizes straight lines to curved surfaces.
  • Geodesics satisfy a special differential equation known as the geodesic equation.
Understanding geodesics helps in studying distances and shortest paths in differential geometry.
Riemann Curvature Tensor
The Riemann curvature tensor, often just called the curvature tensor, is a mathematical object that measures the curvature of a Riemannian manifold. It's like the DNA of the space's curvature.

Mathematically, if you have a manifold \(M\) with a metric \(g\), the Riemann curvature tensor \(R\) is a multi-dimensional array of numbers that capture how much \(M\) deviates from being flat. It appears in the equation used to describe the Jacobi field:

\[ J''(s) + R(J(s), \gamma'(s)) \gamma'(s) = 0 \] Here \(R(J(s), \gamma'(s)) \gamma'(s)\) represents how the curvature of the space affects the vector field \(J(s)\).

Key points to understand about the Riemann curvature tensor:
  • It describes how vectors change as they move around in a curved space.
  • In simple terms, it measures the failure of parallel transport to preserve the angle or length of vectors.
  • It's crucial in studying the intrinsic properties of the space, independent of any embedding.
By understanding the curvature tensor, we can gain insights into the fundamental nature of the space we are studying.
Conjugate Points
Conjugate points are special points on a geodesic where infinitesimally close geodesics intersect. Imagine two points on Earth's surface where multiple shortest paths (great circles) converge.

In the context of Jacobi fields, if \(\gamma(0)\) and \(\gamma(l)\) are conjugate points along a geodesic \(\gamma\), there will be a non-trivial solution to the Jacobi equation that vanishes at both points. This means:

\[\gamma(0)\] and \[\gamma(l)\] are conjugate points if there exist non-zero Jacobi fields [\[J(s)\] such that \[J(0) = 0\] and \[J(l) = 0\].

Important notes:
  • Conjugate points indicate the failure for geodesics from being globally shortest paths.
  • If \[\gamma(l)\] is not conjugate to \[\gamma(0)\], then the exponential map from \[\gamma(0)\] to \[\gamma(l)\] is an isomorphism.
  • This concept helps in understanding the stability and behavior of geodesics in a manifold.
Recognizing conjugate points is essential in analyzing the uniqueness and multiplicity of geodesics between points in a manifold.
Differential Geometry
Differential geometry is the field of mathematics dealing with geometric properties and structures using calculus. It's like the toolkit for bending and deforming objects in a smooth way.

It is fundamental in understanding concepts like geodesics, curvature, and manifold properties. The primary objects of study in differential geometry are differentiable manifolds, which are spaces that locally resemble Euclidean space and allow for the application of calculus.

Key concepts include:
  • Geodesics: Curves that represent the shortest path between points in a curved space.
  • Curvature: Quantified by tensors like the Riemann curvature tensor, describing how a space bends.
  • Jacobi fields: Solutions to a differential equation that describe how geodesics spread apart or come together.
Understanding differential geometry is crucial for fields like general relativity and string theory, where the shape and curvature of space affect physical phenomena.

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Most popular questions from this chapter

(Kazdan-Warner's Remark.) Let \(S \subset R^{3}\) be an extended compact surface of revolution (cf. Remark 4, Sec. 2-3) obtained by rotating the curve $$ \alpha(s)=(0, \varphi(s), \psi(s)) $$ parametrized by arc length \(s \in[0, l]\), about the \(z\) axis. Here \(\varphi(0)=\varphi(l)=0\) and \(\varphi(s)>0\) for all \(s \in[0, l]\). The regularity of \(S\) at the poles implies further that \(\varphi^{\prime}(0)=1, \varphi^{\prime}(l)=-1\) (cf. Exercise 10, Sec. 2-3). We also know that the Gaussian curvature of \(S\) is given by \(K=-\varphi^{\prime \prime}(s) / \varphi(s)\) (cf. Example 4, Sec. 3-3). a. Prove that $$ \int_{0}^{t} K^{\prime} \varphi^{2} d s=0, \quad K^{\prime}=\frac{d K}{d s} $$ b. Conclude from part a that there exists no compact (extended) surface of revolution in \(R^{3}\) with monotonic increasing curvature. The following exercise outlines a proof of Hopf's theorem: A regular surface with constant mean curvature which is homeomorphic to a sphere is a sphere (cf. Remark 2). Hopf's main idea has been used over and over again in recent work. The exercise requires some elementary facts on functions of complex variables.

Let \(J(s)\) be a Jacobi field along a geodesic \(\gamma:[0, l] \rightarrow S\) such that \(\left\langle J(0), \gamma^{\prime}(0)\right\rangle=0\) and \(J^{\prime}(0)=0\). Prove that \(\left\langle J(s), \gamma^{\prime}(s)\right\rangle=0\) for all \(s \in[0, l]\).

Let \(S\) and \(\bar{S}\) be regular surfaces and let \(\varphi: S \rightarrow \bar{S}\) be a diffeomorphism. Assume that \(\bar{S}\) is complete and that a constant \(c>0\) exists such that $$ I_{p}(v) \geq c \bar{I}_{\psi(p)}\left(d \varphi_{p}(v)\right) $$ for all \(p \in S\) and all \(v \in T_{p}(S)\), where \(I\) and \(\bar{I}\) denote the first fundamental forms of \(S\) and \(\bar{S}\), respectively. Prove that \(S\) is complete.

Let \(U \subset R^{3}\) be an open connected subset of \(R^{2}\) and let \(\mathbf{x}: U \rightarrow S\) be an isothermal parametrization (i.e., \(E=G, F=0\); cf. Sec. 4-2) of a regular surface \(S\). We identify \(R^{2}\) with the complex plane \(\mathbb{C}\) by setting \(u+i v=\zeta\), \((u, v) \in R^{2}, \zeta \in \mathbb{C}\). \(\zeta\) is called the complex parameter corresponding to \(\mathbf{x}\). Let \(\phi: \mathbf{x}(U) \rightarrow \mathbb{C}\) be the complex- valued function given by $$ \phi(\zeta)=\phi(u, v)=\frac{e-g}{2}-i f=\phi_{1}+i \phi_{2} $$ where \(e, f, g\) are the coefficients of the second fundamental form of \(S\). a. Show that the Mainardi-Codazzi equations (cf. Sec. 4-3) can be written, in the isothermal parametrization \(\mathrm{x}\), as $$ \left(\frac{e-g}{2}\right)_{a}+f_{*}=E H_{a} \quad\left(\frac{e-g}{2}\right)_{*}-f_{*}=-E H_{*} $$ and conclude that the mean curvature \(H\) of \(\mathbf{x}(U) \subset S\) is constant if and only if \(\phi\) is an analytic function of \(\zeta\) (i.e., \(\left(\phi_{1}\right)_{a}=\left(\phi_{2}\right)_{2},\left(\phi_{1}\right)_{\nu}=\) \(\left.-\left(\phi_{2}\right)_{2}\right) .\) h. Define the "complex derivative" $$ \frac{\partial}{\partial \bar{\zeta}}=\frac{1}{2}\left(\frac{a}{\partial x}-i \frac{\partial}{\partial x}\right) \text {. } $$ and prove that \(\phi(\zeta)=-2\left\langle\mathbf{x}_{\gamma}, N_{\zeta}\right\rangle\), where by \(\mathbf{x}_{c}\), for instance, we mean the vector with complex coordinates $$ \mathbf{x}_{p}=\left(\frac{\partial x}{\partial \zeta}, \frac{\partial y}{\partial \zeta}, \frac{\partial z}{\partial \zeta}\right) $$ c. Let \(f: U \subset C \rightarrow V \subset C\) be a one-to-one complex function given by \(f(u+i v)=x+i y=\eta\). Show that \((x, y)\) are isothermal parameters on \(S\) (i.e., \(\eta\) is a complex parameter on \(S\) ) if and only if \(f\) is analytic and \(f^{\prime}(\zeta) \neq 0, \zeta\) \& \(U\). Let \(\mathbf{y}=\mathbf{x} \circ f^{-1}\) be the correspond ing parametrization and define \(\phi(\eta)=-2\left\\{\mathbf{y}_{4}, N_{4}\right\\}\). Show that on \(x(U) \cap y(V) .\) $$ \phi(\zeta)=\psi(\eta)\left(\frac{3 \eta}{\partial \zeta}\right)^{2} $$ d. Let \(S^{2}\) be the unit sphere of \(R^{3}\). Use the stereographic projection (cf. Exercise 16, Sec. 2.2) from the poles \(N=(0,0,1)\) and \(S=(0,0,-1)\) to cover \(S^{2}\) by the coordinate neighborhoods of two (isothermal) complex parameters, \(\zeta\) and \(\eta\), with \(\zeta(S)=0\) and \(n(N)=0\), in such a way that in the intersection \(W\) of these coordinate neighborhoods (the sphere minus the two poles) \(\eta=\zeta^{-1}\). Assume that there exists on each coontinate neighborhood analytic functicns \(\psi(\zeta), \psi(n)\) such that \((+)\) holds in W. Use Liouville's theorem to prove that \(\varphi(\zeta)=0\) (hence, \(\psi(\eta)=0\) ). c. Let \(S \subset R^{3}\) be a regular surface with constant mean curvature homeomorphic to a sphere. Assume that there exists a conformal diffeomorphism \(\varphi: S \rightarrow S^{2}\) of \(S\) onto the unit sphere \(S^{2}\) (this is a consequence of the uniformization theorem for Riemann surfaces and will be assumed here). Let \(\bar{\zeta}\) and \(\bar{\eta}\) be the complex parameters corresponding ander \(\varphi\) to the parameters \(\zeta\) and \(\eta\) of \(S^{2}\) given in part \(\mathrm{d}\). By part a, the function \(\phi(\bar{\zeta})=((e-g) / 2)-\) if is analytic. The similar function \(\psi(\bar{p})\) is also 5.3. Complete Surfaces. Theorem of Hopf.Aioow \(93 t\) analytic, and by part c they are related by \((+)\). Use part d to show that \(\phi(\bar{\zeta})=0\) (hence, \(\psi(\bar{i})=0\) ). Conclude that \(S\) is made up of umbilical points and hence is a sphere. This proves Hopf's theorem.

Let \(\alpha:[0, l] \rightarrow R^{3}\) be a regular closed curve parametrized by arc length. Assume that \(0 \neq|k(s)| \leq 1\) for all \(s \in[0, l]\). Prove that \(l \geq 2 \pi\) and that \(l=2 \pi\) if and only if \(\alpha\) is a plane convex curve.

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