
LECTURE9:THERICCI ANDTHE SECTIONALCURVATURE1. THE RICCI AND THE SECTIONAL CURVATUREI The Ricci curvature of a Riemannian manifold.We start with some simple algebra. Let B :V×V→Rbe a symmetric bilinearform defined on a vector space V. Then we can assign to it a quadratic formQ : V→R, Q(u) := B(v,).Conversely we can recover the symmetric bilinear form Bfrom its quadratic formQ via the polarization formula2B(u,u) = Q(u +) - Q(u) - Q(u).There isalsoamore succinctwaytorecoverBfromQisvia2B(u,) = [Q(u+tu)](0)where the'refers to t-derivative.Recall that the Ricci curvature tensor Ric is the contraction of the Riemanncurvature tensor Rm,Rc(X,Y) = c(Rm)(X,Y) = Tr(Z -→#Rm(Z,X, ,Y))It is a symmetric (O,2)-tensor field on M. In local coordinates one hasRcij =g RipjqApplying the previous trick to Rc, we see that to study the (0,2)-tensor Rc, it isenough to study the real-valued function Rc(X, X) defined on TM, which is easierto handle. In view of the fact Rc(AX,AX)= Rc(X,X), we may simplify a bitfurther by studying Rc(X,X) only for unit-length vector fields X eT(SM):Definition 1.1.For any.unit tangent vector X, E SpM CT,M,we callRic(Xp) = Rc(Xp, Xp)the Ricci curvature of M at p in thedirection of Xp.So the Ricci curvature function Ric is not a function on M, but a function onthe unit sphere bundle SM C TM (one can think of the Ricci curvature as a function definedon one-dimensional subspaces of T,M).It encodes all information of the tensor Rc viaRc(Xp,Yp) =Xp +YpllRic(X, +Yp) -XplI?Ric(X,) -Ypll?Ric(p)where Yp + -Xp, and we denoted X = X/llXIl
LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE 1. The Ricci and the sectional curvature ¶ The Ricci curvature of a Riemannian manifold. We start with some simple algebra. Let B : V ×V → R be a symmetric bilinear form defined on a vector space V . Then we can assign to it a quadratic form Q : V → R, Q(v) := B(v, v). Conversely we can recover the symmetric bilinear form B from its quadratic form Q via the polarization formula 2B(u, v) = Q(u + v) − Q(u) − Q(v). There is also a more succinct way to recover B from Q is via 2B(u, v) = [Q(u + tv)]′ (0), where the ′ refers to t-derivative. Recall that the Ricci curvature tensor Ric is the contraction of the Riemann curvature tensor Rm, Rc(X, Y ) = c(Rm)(X, Y ) = Tr(Z 7→ ♯Rm(Z, X, ·, Y )). It is a symmetric (0, 2)-tensor field on M. In local coordinates one has Rcij = g pqRipjq Applying the previous trick to Rc, we see that to study the (0,2)-tensor Rc, it is enough to study the real-valued function Rc(X, X) defined on TM, which is easier to handle. In view of the fact Rc(λX, λX) = λ 2Rc(X, X), we may simplify a bit further by studying Rc(X, X) only for unit-length vector fields X ∈ Γ ∞(SM): Definition 1.1. For any ✿✿✿✿✿ unit tangent vector Xp ∈ SpM ⊂ TpM, we call Ric(Xp) = Rc(Xp, Xp) the Ricci curvature of M at p in the direction of Xp. So the Ricci curvature function Ric is not a function on M, but a function on the unit sphere bundle SM ⊂ TM (one can think of the Ricci curvature as a function defined on one-dimensional subspaces of TpM). It encodes all information of the tensor Rc via Rc(Xp, Yp) = 1 2 h ∥Xp + Yp∥ 2Ric(X\p + Yp) − ∥Xp∥ 2Ric(Xbp) − ∥Yp∥ 2Ric(Ybp) i , where Yp ̸= −Xp, and we denoted Xb = X/∥X∥. 1

2LECTURE 9:THERICCI AND THESECTIONALCURVATUREReduce a curvature-like tensor to its bi-quadratic formNow we move from symmetric (0,2)-tensor to "very symmetric"(o,4)-tensorsthat we studied last time, namely, curvature-like tensors T. We letQ(X,Y) := T(X,Y,X,Y)be the bi-quadratic form associated to T. It turns out that one can recover T fromQin the same spirit above:Lemma 1.2. Let T be a curvature-like tensor, and letfx,y,z,w(t) = Q(X +tz,Y +tW) -t(Q(X, W)+Q(z,Y).Then (fx,y,z.W - fyx,z,w)"(0) = 12T(X, Y,Z, W).Proof. Obviously fx,y,z,w is a polynomial of degree 4 in t, whose quadratic coeffi-cients equalsT(Z, W,X,Y) + T(Z,Y,X, W) +T(X, W,Z,Y) + T(X,Y,Z, W)which, by using the symmetries for curvature-like tensors, equals2T(X,Y,Z,W) +2T(Z,Y,X,W)Similarly the quadratic coefficient of fy,x,z,w equals2T(Y,X, Z,W) + 2T(Z,X, Y,W)So the quadratic coefficient of fx,y,z,w(t) -fy,x,z.w(t) is2T(X,Y,Z,W) + 2T(Z,Y,X,W) - 2T(Y,X,Z,W) - 2T(Z,X, Y,W),口which, after applying the first Bianchi identity, equals 6T(X,Y, Z, W).Remark. One may explicitly write down a “pure algebraic polarization formula" ofT(X,Y, Z, W) in terms of the bi-quadratic form Q, which is quite lengthy.I The sectional curvature.As a result, to study the curvature tensor Rm of a Riemannian manifold (M, g),it is enough to study the associated bi-quadratic form, namely, Rm(X,Y,X,Y).Again, by using some simple algebra, we can simplify a bit further.Lemma 1.3. For any T E (^V*) and any X,Y e V, if we denote X' = aX +bY,Y'- cX +dY, thenT(X',Y', X',Y') = (ad - bc)?T(X,Y,X,Y).Proof.This follows from a very simple computation:T(X',Y',X',Y') = T(aX +bY,cX +dY,aX +bY,cX + dY)= (ad - bc)T(X,Y,aX + bY,cX + dY)= (ad - bc)?T(X,Y,X, Y)口
2 LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE ¶ Reduce a curvature-like tensor to its bi-quadratic form. Now we move from symmetric (0,2)-tensor to “very symmetric” (0,4)-tensors that we studied last time, namely, curvature-like tensors T. We let Q(X, Y ) := T(X, Y, X, Y ) be the bi-quadratic form associated to T. It turns out that one can recover T from Q in the same spirit above: Lemma 1.2. Let T be a curvature-like tensor, and let fX,Y,Z,W (t) = Q(X + tZ, Y + tW) − t 2 (Q(X, W) + Q(Z, Y )). Then (fX,Y,Z,W − fY,X,Z,W ) ′′(0) = 12T(X, Y, Z, W). Proof. Obviously fX,Y,Z,W is a polynomial of degree 4 in t, whose quadratic coefficients equals T(Z, W, X, Y ) + T(Z, Y, X, W) + T(X, W, Z, Y ) + T(X, Y, Z, W). which, by using the symmetries for curvature-like tensors, equals 2T(X, Y, Z, W) + 2T(Z, Y, X, W). Similarly the quadratic coefficient of fY,X,Z,W equals 2T(Y, X, Z, W) + 2T(Z, X, Y, W). So the quadratic coefficient of fX,Y,Z,W (t) − fY,X,Z,W (t) is 2T(X, Y, Z, W) + 2T(Z, Y, X, W) − 2T(Y, X, Z, W) − 2T(Z, X, Y, W), which, after applying the first Bianchi identity, equals 6T(X, Y, Z, W). □ Remark. One may explicitly write down a “pure algebraic polarization formula” of T(X, Y, Z, W) in terms of the bi-quadratic form Q, which is quite lengthy. ¶ The sectional curvature. As a result, to study the curvature tensor Rm of a Riemannian manifold (M, g), it is enough to study the associated bi-quadratic form, namely, Rm(X, Y, X, Y ). Again, by using some simple algebra, we can simplify a bit further. Lemma 1.3. For any T ∈ ⊗2 (∧ 2V ∗ ) and any X, Y ∈ V , if we denote X′ = aX + bY, Y ′ = cX + dY , then T(X ′ , Y ′ , X′ , Y ′ ) = (ad − bc) 2T(X, Y, X, Y ). Proof. This follows from a very simple computation: T(X ′ , Y ′ , X′ , Y ′ ) = T(aX + bY, cX + dY, aX + bY, cX + dY ) = (ad − bc)T(X, Y, aX + bY, cX + dY ) = (ad − bc) 2T(X, Y, X, Y ). □

3LECTURE 9:THERICCI AND THESECTIONALCURVATURENow suppose (M,g)is a Riemannian manifold.Recall thatgg is a curvature-like tensor, such that129g(Xp,Yp,Xp,) = (Xp, X)(Yp, Yp) - (Xp,y)2,which is nothing else but the square of the area of the parallelogram with sidesX,,Yp.Applying theprevious lemma to Rm and gg,we immediatelygetProposition 1.4.The quantityRm(Xp,Yp, Xp,Yp)K(Xp, Yp) :=(Xp, Xp)(Yp, Yp) - (Xp, Yp)2depends only on the two dimensional plane II, = span(X,, Yp) C T,M, i.e. it isindependent of the choices of basis [Xp,Yp] of IIp.Definition1.5.We will callK(IIp) = K(Xp,Y)the sectional curvature of (M, g) at p with respect to the plane IlpNote that the Ricci curvature that we studied above are closely related to thesectional curvatures: If X, is a unit vector in T,M, we may extend X, to an or-thonormal basis [ei =Xp,e2,".",em] of T,M. As a result,(1)Ric(X,)- Rm(ei,ei,ei,ei)- K(ei,ei),i>2i>2In other words, the Ricci curvature Ric(X,)is“the sum of sectional curvatures"fora specially chosen set of m -1 pairwise orthogonal planes containing Xp.Erample.Here are three basic examples:(1)For theEuclidean space (Rm,go),onehasRm=0, soK(II,)=0 and Ric(Xp) =0.(2) For the unit sphere (Sm, ground), one has Rm = gg, soK(Ip)=1 and Ric(Xp)=m -1.Onemay also prove theconclusion by calculating the Christoffel symbols.(3) For the hyperbolic space (Hm, ghyperbolic), one can prove (exercise)K(II,)=-1 and Ric(X,)=-(m -1).Remark. One may give a conceptional proof of the fact that these three spaces haveconstant sectional curvature: For (Rm,go),the isometry group E(m)=O(m) × IRmacts transitively on the set Gr2(TIRm) = [IIp I p E Rm,II, C T,M is a plane]Since the sectional curvature is invariant under the action of the isometric group,we must have K(1l,) = K(II'), i.e. the sectional curvature is a constant. The samephenomena occurs for (Sm, ground) (with isometry group O(m+1) and for (Hm, ghyperbolic)(with isometry group O+(m, 1)
LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE 3 Now suppose (M, g) is a Riemannian manifold. Recall that 1 2 g○∧ g is a curvaturelike tensor, such that 1 2 g○∧ g(Xp, Yp, Xp, Yp) = ⟨Xp, Xp⟩⟨Yp, Yp⟩ − ⟨Xp, Yp⟩ 2 , which is nothing else but the square of the area of the parallelogram with sides Xp, Yp. Applying the previous lemma to Rm and 1 2 g○∧ g, we immediately get Proposition 1.4. The quantity K(Xp, Yp) := Rm(Xp, Yp, Xp, Yp) ⟨Xp, Xp⟩⟨Yp, Yp⟩ − ⟨Xp, Yp⟩ 2 depends only on the two dimensional plane Πp = span(Xp, Yp) ⊂ TpM, i.e. it is independent of the choices of basis {Xp, Yp} of Πp. Definition 1.5. We will call K(Πp) = K(Xp, Yp) the sectional curvature of (M, g) at p with respect to the plane Πp. Note that the Ricci curvature that we studied above are closely related to the sectional curvatures: If Xp is a unit vector in TpM, we may extend Xp to an orthonormal basis {e1 = Xp, e2, · · · , em} of TpM. As a result, (1) Ric(Xp)=X i≥2 Rm(ei , e1, ei , e1)=X i≥2 K(ei , e1). In other words, the Ricci curvature Ric(Xp) is “the sum of sectional curvatures” for a specially chosen set of m − 1 pairwise orthogonal planes containing Xp. Example. Here are three basic examples: (1) For the Euclidean space (R m, g0), one has Rm = 0, so K(Πp) ≡ 0 and Ric(Xp) ≡ 0. (2) For the unit sphere (S m, ground), one has Rm = 1 2 g○∧ g, so K(Πp) ≡ 1 and Ric(Xp) ≡ m − 1. One may also prove the conclusion by calculating the Christoffel symbols. (3) For the hyperbolic space (Hm, ghyperbolic), one can prove (exercise) K(Πp) ≡ −1 and Ric(Xp) ≡ −(m − 1). Remark. One may give a conceptional proof of the fact that these three spaces have constant sectional curvature: For (R m, g0), the isometry group E(m) = O(m) ⋉ Rm acts transitively on the set Gr2(TR m) = {Πp | p ∈ R m, Πp ⊂ TpM is a plane}. Since the sectional curvature is invariant under the action of the isometric group, we must have K(Πp) = K(Π′ q ), i.e. the sectional curvature is a constant. The same phenomena occurs for (S m, ground) (with isometry group O(m+1)) and for (Hm, ghyperbolic) (with isometry group O+(m, 1))

4LECTURE9:THERICCIAND THESECTIONALCURVATURERemark. We may compare the sectional curvature K with the curvature operatorR : A2(T,M) → A2(T,M). By definition we have(Rp(Xp ^ Yp), Xp^Yp)K(Xp,Yp) :(Xp, Xp)(Yp, Yp) - (Xp, Yp)2As a consequence, the curvature operator R determines the sectional curvature K.2.BASICPROPERTIESOFSECTIONALCURVATURESI Sectional curvature for low dimensional manifolds.Let (M,g) be a Riemannian manifold. By definition, the sectional curvature Kis NOT a function on M,but instead a function on the Grassmannian bundleGr2(TM) = [(p, II,) I p E M, II, C T,M is 2-dimensional)(1) If M has dimension m = 1, obviously R = 0 and it makes no sense to talkabout sectional curvature (so again as we have seen in Lecture 3, essentially there isnoRiemanniangeometryindimensionalone)(2) If M has dimension m = 2, i.e. is a surface, then one can regard the sectionalcurvature K as a function defined on M in the natural way. Moreover, inview of the equation (1), for any direction X, we have Ric(X,) = K(p). Inother words, for surfaces the sectional curvature, the Ricci curvature and thescalar curvature are all the same.One can show that in this case K is reallythe Gauss curvature in undergraduate differential geometry course.(3) If M has dimension m ≥ 3, by using the exponential map that we willlearn later, for each 2-dimensional plane IIp E T,M, locally one gets a 2-dimensional submanifold Spnear p in M whose tangent space atp is Ip,and the sectional curvature K(II,) is nothing else but the Gauss curvatureof S, (endowed with the subspace Riemannian metric) at p. Thus the sec-tional curvature is a natural generalization of the Gauss curvature to higherdimensional Riemannian manifolds.(4) In general the sectional curvatures encodes more information than the Riccicurvatures.However,ifMhasdimensionm=3,thenaccordingtotheequation (1), for an orthonormal basis e1, e2, e3,Ric(ei) = K(e1,e2) + K(e1,e3),Ric(e2) = K(ei, e2) + K(e2, e3),Ric(e3) = K(e1, e3) +K(e2, e3).As a result, in this case the Ricci curvatures determine the sectional curva-tures: For each plane IIp, one just start with an orthonormal basis [ei,e2]of Ip, extend it to an orthonormal basis [ei, e2, es) of T,M and then solvethe above system of equations to get2K(Ilp) = Ric(e1) + Ric(e2) -Ric(e3)
4 LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE Remark. We may compare the sectional curvature K with the curvature operator Rp : Λ2 (TpM) → Λ 2 (TpM). By definition we have K(Xp, Yp) = ⟨Rp(Xp ∧ Yp), Xp ∧ Yp⟩ ⟨Xp, Xp⟩⟨Yp, Yp⟩ − ⟨Xp, Yp⟩ 2 . As a consequence, the curvature operator R determines the sectional curvature K. 2. Basic properties of sectional curvatures ¶ Sectional curvature for low dimensional manifolds. Let (M, g) be a Riemannian manifold. By definition, the sectional curvature K is NOT a function on M, but instead a function on the Grassmannian bundle Gr2(TM) = {(p, Πp) | p ∈ M, Πp ⊂ TpM is 2-dimensional}. (1) If M has dimension m = 1, obviously R ≡ 0 and it makes no sense to talk about sectional curvature (so again as we have seen in Lecture 3, essentially there is no Riemannian geometry in dimensional one). (2) If M has dimension m = 2, i.e. is a surface, then one can regard the sectional curvature K as a function defined on M in the natural way. Moreover, in view of the equation (1), for any direction Xp we have Ric(Xp) = K(p). In other words, for surfaces the sectional curvature, the Ricci curvature and the scalar curvature are all the same. One can show that in this case K is really the Gauss curvature in undergraduate differential geometry course. (3) If M has dimension m ≥ 3, by using the exponential map that we will learn later, for each 2-dimensional plane Πp ∈ TpM, ✿✿✿✿✿✿✿ locally one gets a 2- dimensional submanifold Sp near p in M whose tangent space at p is Πp, and the sectional curvature K(Πp) is nothing else but the Gauss curvature of Sp (endowed with the subspace Riemannian metric) at p. Thus the sectional curvature is a natural generalization of the Gauss curvature to higher dimensional Riemannian manifolds. (4) In general the sectional curvatures encodes more information than the Ricci curvatures. However, if M has dimension m = 3, then according to the equation (1), for an orthonormal basis e1, e2, e3, Ric(e1) = K(e1, e2) + K(e1, e3), Ric(e2) = K(e1, e2) + K(e2, e3), Ric(e3) = K(e1, e3) + K(e2, e3). As a result, in this case the Ricci curvatures determine the sectional curvatures: For each plane Πp, one just start with an orthonormal basis {e1, e2} of Πp, extend it to an orthonormal basis {e1, e2, e3} of TpM and then solve the above system of equations to get 2K(Πp) = Ric(e1) + Ric(e2) − Ric(e3)

LECTURE 9:THERICCI AND THESECTIONALCURVATURE5I Riemannian manifolds with curvature bounds.Unlikealgebraicquantitieslikecurvaturetensors,thesectional/Ricci/scalarcur-vatures are real-valued functions. Since we may compare real nubmers, we can defineDefinition 2.1. Let (M,g) be a Riemannian manifold. We say (M, g) has(1)constant sectional curvaturecifK(1,)=cforall pand all planes ,CT,M.(2) constant Ricci curvature c if Ric(X,) = c for all p and all vectors X, E SpM.(3) positive sectional curvature if K(IIp) >0 for all p and all planes II, C T,M.Similarly wemay define.(M,g)has negative/nonpositive/nonnegative sectional curvature if K(1I,)isnegative/nonpositive/nonnegative for all p and all planes II, C T,M.. (M, g) has positive/negative/nonpositive/nonnegative Ricci curvature if Ric(Xp)ispositive/negative/nonpositive/nonnegativeforallpandall XnESnM..(M,g) has sectional curvatureK≥c or K≤ c if K(1Ip)≥ c or K(1lp)≤cfor all p and all planes IIp T,M..(M,g) has Ricci curvature Ric≥ c orRic≤ cif Ric(X,)≥c or Ric(X,)≤ cforallpand all vectorsX,S,M.More generally, given two Riemannian metrics g1 and g2 on any smooth manifoldM, with sectional curvature functions Kgr, Kg, and Ricci curvature functions Ricgn,Ricga, we may compare Kg, and Kg, as functions on Gr2(TM), and compare Ricgiand Ricga as functions on SM.Erample.We can write down the change of sectional curvature under scaling of themetric: if we scale a Riemannian metric g to Ag, where A is a positive constant, then(1)by the Koszul formula, the Levi-Civita connection xY remains unchanged.(2) it follows that the (1,3)-curvature tensor R remains unchanged,(3) as a result, the Riemann curvature tensor is changed to Rmxg = ARmg,(4) and thus the Ricci curvature tensor remains unchanged: Rcag = Rcg,(5)but the two sectional curvatures are related by Kxg =^-1Kg,(6) and it follows that Ricag =^-1Ricg (no conflict with (4) since unit vectors changed)(7) and thus Sxg = >-1Sg.In particular, for each c one gets a Riemannian manifold with constant sectionalcurvature c, namely the space (sm, Iground) if c > 0, and (Hm, ghuperbolic) if c < 0.Manifolds with curvature bounds will be one of the major themes of this course.Remark.Since the curvature operator R,is a symmetric operator on a real vectorspace, it has real eigenvalues.Definition 2.2. We say (M, g) is a Riemannian manifold with posi-tive curvature operator if all eigenvalues of Rp are positive
LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE 5 ¶ Riemannian manifolds with curvature bounds. Unlike algebraic quantities like curvature tensors, the sectional/Ricci/scalar curvatures are ✿✿✿✿✿✿✿✿✿✿✿ real-valued functions. Since we may compare real nubmers, we can define Definition 2.1. Let (M, g) be a Riemannian manifold. We say (M, g) has (1) constant sectional curvature c if K(Πp) = c for all p and all planes Πp ⊂ TpM. (2) constant Ricci curvature c if Ric(Xp) = c for all p and all vectors Xp ∈ SpM. (3) positive sectional curvature if K(Πp) > 0 for all p and all planes Πp ⊂ TpM. Similarly we may define • (M, g) has negative/nonpositive/nonnegative sectional curvature if K(Πp) is negative/nonpositive/nonnegative for all p and all planes Πp ⊂ TpM. • (M, g) has positive/negative/nonpositive/nonnegative Ricci curvature if Ric(Xp) is positive/negative/nonpositive/nonnegative for all p and all Xp ∈ SpM. • (M, g) has sectional curvature K ≥ c or K ≤ c if K(Πp) ≥ c or K(Πp) ≤ c for all p and all planes Πp ⊂ TpM. • (M, g) has Ricci curvature Ric ≥ c or Ric ≤ c if Ric(Xp) ≥ c or Ric(Xp) ≤ c for all p and all vectors Xp ∈ SpM. More generally, given two Riemannian metrics g1 and g2 on any smooth manifold M, with sectional curvature functions Kg1 , Kg2 and Ricci curvature functions Ricg1 , Ricg2 , we may compare Kg1 and Kg2 as functions on Gr2(TM), and compare Ricg1 and Ricg2 as functions on SM. Example. We can write down the change of sectional curvature under scaling of the metric: if we scale a Riemannian metric g to λg, where λ is a positive constant, then (1) by the Koszul formula, the Levi-Civita connection ∇XY remains unchanged, (2) it follows that the (1,3)-curvature tensor R remains unchanged, (3) as a result, the Riemann curvature tensor is changed to Rmλg = λRmg, (4) and thus the Ricci curvature tensor remains unchanged: Rcλg = Rcg, (5) but the two sectional curvatures are related by Kλg = λ −1Kg, (6) and it follows that Ricλg = λ −1Ricg (no conflict with (4) since unit vectors changed) (7) and thus Sλg = λ −1Sg. In particular, for each c one gets a Riemannian manifold with constant sectional curvature c, namely the space (S m, 1 c ground) if c > 0, and (Hm, 1 −c ghyperbolic) if c < 0. Manifolds with curvature bounds will be one of the major themes of this course. Remark. Since the curvature operator Rp is a symmetric operator on a real vector space, it has real eigenvalues. Definition 2.2. We say (M, g) is a Riemannian manifold with positive curvature operator if all eigenvalues of Rp are positive

6LECTURE 9:THERICCI AND THESECTIONALCURVATUREObviously if (M,g)has positive curvature operator, then it has positive sectionalcurvature.However, the converse is not true:.ItwasprovenbyC.BohmandB.Wilkingin2008thatmanifoldswithpositive curvature operators are space forms, i.e. are complete Riemannianmanifolds with constant sectional curvature.: On the other hands, there exist Riemannian manifolds with positive sectionalcurvature which are not constant (e.g. the complex projective space Cpmendowed with the Fubini-Study metric)Sofor such Riemannian manifolds the curvature operator is not positive. The secretis: the space A2(T,M) is a vector space that contains elements of the form ui Aui+ua A v2 which do not correspond to any 2-dimensional plane in T,M. After all, theGrassmannian Gr2(T,M) is a smooth manifold of dimension 2(m - 2), while thespace of bi-vectors A(T,M) has dimension (㎡).I Riemannian manifolds with isotropic sectional curvature at a point.Finally study the following question: At a given point, when will the sectionalcurvature be independent of the choice of II, C T,M?Proposition 2.3. Let (M, g) be a Riemannian manifold and p e M. The followingare equivalent:(1) K(IIp) = c for all II, CT,M.(2)Rmp=gpgp:(3) Rp(Xp, Yp)Zp = c(Yp, Zp)Xp (Xp, Zp)Yp) for any Xp, Yp, Zp E T,M(4) R,= cld on AT,M.(5) The Weyl curvature tensor Wp = 0 and Ricci curvature tensor Rcp = (m - 1)cgpProof. (1) (2)According to Lemma 1.2, if T is a curvature-like tensor, thenT=0 T(X,Y,X,Y) =0,VX,YApply this to the curvature-like tensor T=Rmp-gpgp,we seeRmp= 29p K(Il) =c,VII, C T,M.(2)(3)and/(4)→(1)areobvious(2) (4) Take an orthonormal basis (ei) of T,M, then [ei Aej i< j) is abasis of A'T,M.On this basis,(Rp(e ej),ek Net) =Rmp(ei,ej,ek,e) =couxdjtwhere in the last step we used the fact i < j, k < l. As a result, we seeRp(eiNe,) = ceiej,Vi<j.In other words, Rp = cld for all e Aej. Since Rp is linear, Rp = cld on A’TpM
6 LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE Obviously if (M, g) has positive curvature operator, then it has positive sectional curvature. However, the converse is not true: • It was proven by C. Bohm and B. Wilking in 2008 that manifolds with positive curvature operators are space forms, i.e. are complete Riemannian manifolds with constant sectional curvature. • On the other hands, there exist Riemannian manifolds with positive sectional curvature which are not constant (e.g. the complex projective space CPm endowed with the Fubini-Study metric). So for such Riemannian manifolds the curvature operator is not positive. The secret is: the space Λ2 (TpM) is a vector space that contains elements of the form u1 ∧v1 + u2 ∧ v2 which do not correspond to any 2-dimensional plane in TpM. After all, the Grassmannian Gr2(TpM) is a smooth manifold of dimension 2(m − 2), while the space of bi-vectors Λ2 (TpM) has dimension m 2 . ¶ Riemannian manifolds with isotropic sectional curvature at a point. Finally study the following question: At a given point, when will the sectional curvature be independent of the choice of Πp ⊂ TpM? Proposition 2.3. Let (M, g) be a Riemannian manifold and p ∈ M. The following are equivalent: (1) K(Πp) = c for all Πp ⊂ TpM. (2) Rmp = c 2 gp○∧ gp. (3) Rp(Xp, Yp)Zp = c(⟨Yp, Zp⟩Xp − ⟨Xp, Zp⟩Yp) for any Xp, Yp, Zp ∈ TpM. (4) Rp = cId on Λ 2TpM. (5) The Weyl curvature tensor Wp = 0 and Ricci curvature tensor Rcp = (m − 1)cgp. Proof. (1) ⇐⇒ (2) According to Lemma 1.2, if T is a curvature-like tensor, then T ≡ 0 ⇐⇒ T(X, Y, X, Y ) = 0, ∀X, Y. Apply this to the curvature-like tensor T = Rmp − c 2 gp○∧ gp, we see Rmp = c 2 gp○∧ gp ⇐⇒ K(Πp) = c, ∀ Πp ⊂ TpM. (2) ⇐⇒ (3) and (4) =⇒ (1) are obvious. (2) =⇒ (4) Take an orthonormal basis {ei} of TpM, then {ei ∧ ej | i < j} is a basis of Λ2TpM. On this basis, ⟨Rp(ei ∧ ej ), ek ∧ el⟩ = Rmp(ei , ej , ek, el) = cδikδjl, where in the last step we used the fact i < j, k < l. As a result, we see Rp(ei ∧ ej ) = cei ∧ ej , ∀i < j. In other words, Rp = cId for all ei ∧ ej . Since Rp is linear, Rp = cId on Λ2TpM

7LECTURE 9:THE RICCI AND THE SECTIONAL CURVATURE(2)→ (5)We start with the unique orthogonal decompositionS(p)1Rmp=Wp++m-,E@sp + 2m(m-1,9@p:where E, = Rcp - SlPgp is the traceless Rici tensor. If (2) holds, then by theuniqueness of the decomposition,Wp=0, Ep=0 and S(p)=m(m-1)c.As a result,Rcp=(m-1)cgp(5) → (2)Conversely if Wp = 0 and Rcp = (m - 1)cgp, thenS(p) = Tr(Rcp) = m(m- 1)cSo E,=0 and thusRmp=299p.口This completes the proofRecall from Lecture 7 that a Riemannian manifold is flat if the (1,3)-curvaturetensor R=0. As a consequence,Corollary 2.4. A Riemannian manifold (M,g) is a flat manifold if and only if itssectional curvatures are identically zero.Similarly by using the polarization formula for Ricci curvature tensor, we mayalso easily get a Ricci curvature version:Proposition 2.5. Let (M, g) be a Riemannian manifold and p E M. Then Ric(X,) =cforallXpESpMifandonlyifRcp=cgp
LECTURE 9: THE RICCI AND THE SECTIONAL CURVATURE 7 (2) =⇒ (5) We start with the unique orthogonal decomposition Rmp = Wp + 1 m − 2 Ep○∧ gp + S(p) 2m(m − 1)gp○∧ gp, where Ep = Rcp − S(p) m gp is the traceless Ricci tensor. If (2) holds, then by the uniqueness of the decomposition, Wp = 0, Ep = 0 and S(p) = m(m − 1)c. As a result, Rcp = (m − 1)cgp. (5) =⇒ (2) Conversely if Wp = 0 and Rcp = (m − 1)cgp, then S(p) = Tr(Rcp) = m(m − 1)c. So Ep = 0 and thus Rmp = c 2 gp○∧ gp. This completes the proof. □ Recall from Lecture 7 that a Riemannian manifold is flat if the (1,3)-curvature tensor R = 0. As a consequence, Corollary 2.4. A Riemannian manifold (M, g) is a flat manifold if and only if its sectional curvatures are identically zero. Similarly by using the polarization formula for Ricci curvature tensor, we may also easily get a Ricci curvature version: Proposition 2.5. Let (M, g) be a Riemannian manifold and p ∈ M. Then Ric(Xp) = c for all Xp ∈ SpM if and only if Rcp = cgp