GEOMETRIC INTERPRETATIONS of CURVATURE Contents 1. Notation and Summation Conventions 1 2. Affine Connections 1 3. Parallel Tran
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GEOMETRIC INTERPRETATIONS OF CURVATURE ZHENGQU WAN Abstract. This is an expository paper on geometric meaning of various kinds of curvature on a Riemann manifold. Contents 1. Notation and Summation Conventions 1 2. Affine Connections 1 3. Parallel Transport 3 4. Geodesics and the Exponential Map 4 5. Riemannian Curvature Tensor 5 6. Taylor Expansion of the Metric in Normal Coordinates and the Geometric Interpretation of Ricci and Scalar Curvature 9 Acknowledgments 13 References 13 1. Notation and Summation Conventions We assume knowledge of the basic theory of smooth manifolds, vector fields and tensors. We will assume all manifolds are smooth, i.e. C1, second countable and Hausdorff. All functions, curves and vector fields will also be smooth unless otherwise stated. Einstein summation convention will be adopted in this paper. In some cases, the index types on either side of an equation will not match and @ so a summation will be needed. The tangent vector field @xi induced by local i coordinates (x ) will be denoted as @i. 2. Affine Connections Riemann curvature is a measure of the noncommutativity of parallel transporta- tion of tangent vectors. To define parallel transport, we need the notion of affine connections. Definition 2.1. Let M be an n-dimensional manifold. An affine connection, or connection, is a map r : X(M) × X(M) ! X(M), where X(M) denotes the space of smooth vector fields, such that for vector fields V1;V2; V; W1;W2 2 X(M) and function f : M! R, (1) r(fV1 + V2;W ) = fr(V1;W ) + r(V2;W ), (2) r(V; aW1 + W2) = ar(V; W1) + r(V; W2), for all a 2 R. (3) r(V; fW ) = V (f)W + fr(V; W ). We write r(V; W ) = rV W . 1 2 ZHENGQU WAN Theorem 2.2. For fixed W , (rV W )jp only depends on V jp. Proof. It suffices to show if V jp = 0 then (rU W )jp = 0. The proof relies on the following lemma: if V jp = 0 then there exists smooth scalar fields fk and vector ~ P ~ fields Vk such that fk(p) = 0 and V = k fkVk. This fact is easily proven using P ~ partitions of unity. Using this lemma, we then write V = k fkVk where fk(p) = 0. Then X (rP ~ W )jp = fk(p)(r ~ W )jp = 0: k fkVk Vk k Remark 2.3. Since rV W depends on V pointwise, we may write rvW := rV W jp where v = Vp 2 TpM. We also note that rV W jp depends on the local values of W , that is, if W1 = W2 in some neighborhood of p, then rvW1jp = rvW2jp for all v 2 TpM. We now give an expression for the connection r in local coordinates (xi) on an j i open set U. Suppose we have two vector fields W = w @j and V = v @i on U. Then @vi r V = wj @ + wjvir @ : W @xj i @j i k We define functions Γij : U ! R, for 1 ≤ i; j; k ≤ n, by k r@j @i = Γij@k: These functions are called the Christoffel symbols and depend on the coordinate system used to define them. Since covariant differentiation takes values in X(M), we see immediately that the Christoffel symbols are smooth. We now show existence of a global affine connection on a manifold M. Theorem 2.4. For any manifold M, there exists an affine connection on M. Proof. Let fUαgα be an atlas of M and let fραgα be the associated partition of unity. On each open set Uα, we have a connection rα given in the coordinates on k P Uα by Γij = 0. We define r by rV W = α(rα)ρα·V (ρα · W ). Note that at each point p, rjp is a finite sum. Some straightforward computations will show that r satisfies the three properties in Theorem 2.1 and rV W is smooth when V; W are smooth. Remark 2.5. The affine connection r on a manifold need not be unique. If we k vary the Christoffel symbols Γij in each of the charts Uα of the proof, we may get different affine connections. Remark 2.6. We know that rwV depends on W locally, however we can further show that if η is a smooth curve such that η(0) = p and η0(0) = w, then the value of rwV only depends on behavior of V on the curve η. Thus, rwV is well-defined even if V is only defined along a curve through p and tangent to w. Definition 2.7. Let η : I !M be a smooth curve. A vector field V along η is a smooth map V : I ! T M such that for each t 2 I, V (t) 2 Tη(t)M. Remark 2.6 above says that for a vector v, the map W 7! rvW is defined on vector fields W along curves η such that η(0) = p and η0(0) = w. Definition 2.8. A vector field V along a curve η is parallel if rη_(t)V = 0 for all t. GEOMETRIC INTERPRETATIONS OF CURVATURE 3 Theorem 2.9. Let η : [0; 1] !M be a smooth curve and let v 2 Tη(0)M. Then, there exists a unique parallel vector field V along η such that V (0) = v. Proof. First, we consider the case when η is contained in a local coordinate chart. k In local coordinates, V (t) = V (t)@k satisfies the system of ODEs dV k + V iη_jΓk = 0 for k = 1; : : : ; n dt ij with initial conditions V k(0) = vk. Observe that the map k k j j (V ; t) 7! −Γij(η(t))V η_ (t) k k j j is continuous; for fixed t, the map (V ) 7! −ΓijV η_ is linear and thus globally Lipchitz continuous in V k. Picard-Lindelof theorem tells us that this equation has a unique solution V (t). For general η, we let 0 = t0 < ··· < tN = 1 be a partition of [0; 1] such that, for each i, ηj[ti−1;ti] is contained in a coordinate chart Ui. The previous paragraph implies that there is a parallel vector field V along ηj[0;t1] such that V (0) = v. If ~ we have a parallel vector field V along ηj[0;ti], we obtain a vector field V along ~ ηj[ti;ti+1] such that V (ti) = V (ti), again using the previous paragraph. Then, V ~ extends to a vector field along ηj[0;ti+1] by defining V (t) = V (t) for t 2 [ti; ti+1]. By induction, we get a vector field V which is parallel along all of η. 3. Parallel Transport One problem on general manifolds is, unlike Euclidean spaces, if p; q 2 M are dis- tinct points, then there is no natural identification TpM = TqM. In this section, we illustrate how we may construct such an isomorphism, called parallel trans- portation, using the notion of parallel vector fields. However, this isomorphism will depend on a choice of path between p and q. Definition 3.1. Let η : [0; 1] !M be a curve connecting two points p; q 2 M, i.e. η(0) = p and η(1) = q. Let v 2 TpM and let V denote the parallel vector field along η ensured by Theorem 2.9. The vector V (1) is called the parallel transport of v along η and the map v 7! V (1) is denoted Tη(0)!η(1) or Tp!q or by T if the path η is clear from the context. Remark 3.2. Since the equation defining parallel transportation is a linear ODE, for any path η from p to q, we have Tp!q(av + w) = aTp!qv + Tp!qw. From the definition of parallel transport we see that Tp!q is the inverse of Tq!p. Thus Tp!q is an isomorphism from TpM to TqM. Remark 3.3. Let η be a curve and p = η(0). If fv1;:::; vng is a basis of TpM, then we can extend vi to parallel vector fields Ei(t) along η. Since parallel transportation is invertible, fE1(t);:::;En(t)g forms a basis of Tη(t)M at each t. We have defined parallel transport in terms of the affine connection. The fol- lowing theorem shows that we may define the affine connection in terms of parallel transport. Theorem 3.4. Suppose we have a smooth vector field V and a smooth curve η 1 such that η_(0) = v. Then lim!0+ Tη()!η(0)V () − V (0) = rη_ (0)V . 4 ZHENGQU WAN Proof. Let E1;:::;En be parallel vector fields along η forming a basis at each point. k k Write V (t) = V (t)Ek(t). Then, Tη()!η(0)V () = V ()Ek(0), since Tη()!η(0) is a linear map. Then, 1 1 (T V () − V (0)) = (V k() − V k(0))E (0): η()!η(0) k d k Taking the limit ! 0 gives us dt jt=0(V )(t)Ek(0). Since Ek is parallel, we also have that 0 k k 0 k rη0(0)V (t)jt=0 = η (0)(V (t))Ek(0) + V (0)rη0(0)Ek(t) = η (0)(V (t))Ek(0): d k This is, by definition dt jt=0(V )(t)Ek(0), so the two quantities are the same. Remark 3.5. Note that this theorem states that the affine connection is equal to to the limit of a difference quotient.