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Differential Geometry by Will Merry Lecture notes based on the Differential Geometry course lectured by Prof. P.M.H. Wilson in Michaelmas term 2007 for Part III of the Cambridge Mathematical Tripos. Contents 1 Smooth manifolds............................. 1 2 Vector fields................................ 9 3 Submanifolds................................ 14 4 Lie groups................................. 18 5 Vector bundles and sheaves........................ 24 6 Differential forms and cohomology..................... 35 7 Integration on manifolds and Lie derivatives................ 44 8 Connections on vector bundles....................... 49 9 Koszul connections............................. 57 10 Elementary Riemannian geometry..................... 66 Please let me know on w.merry@dpmms.cam.ac.uk if you find any errors - I m sure there are many! 1 Smooth manifolds 1.1 Definitions A topological manifold M of dimension n is a second countable Hausdorff topological space that is locally homeomorphic to R n ; that is, for any p M there exists an open neighborhood U of p and a homeomorphism h : U O R n, where O is open in R n. We call the homeomorphism h : U O a chart, and we call U a coordinate neighborhood of p. We write M n to signify that the dimension of M is n. 1.2 Charts Let r i : R n R denote projection onto the ith coordinate, and given a chart h : U O, let x i = r i h : U R. The functions x i are the coordinates of h on U. Given two charts h : U O and k : V Ω on a topological manifold M such that U V, the function k h 1 : hu V ku V is a homeomorphism between open sets of R n. We call k h 1 the transition function between the charts h and k. 1.3 Definitions An atlas A on a topological manifold M n is a collection {U α, h α α A} of charts on M such that: 1. {U α α A} is an open cover of M, 2. For any α, β A such that U α U β, the transition function h αβ := h α h 1 β is smooth posesses continuous partial deriviatives of all orders. 1

1 Smooth manifolds 2 In general, we say two charts satisfying the conditions of 2 above are compatible. Note that this implies that the transition function between the two charts is a diffeomorphism. A smooth structure on M is an atlas A that is maximal with respect to property 2 above. 1.4 Lemma Any atlas determines a unique smooth structure. Let A ={U α, h α α A} be an atlas on M, and consider the collection of charts A consisting of all charts on M that are compatible with all the charts in A. Clearly A A. We now check A is an atlas. Indeed, property 1 is immediate, and to check property 2, let h : U O and k : V Ω be two charts in A such that U V. We must show that k h 1 is smooth, and it is enough to check this locally. Given p U V, choose a chart h α : U α O α in A such that p U α. Then W = U V U α is an open neighborhood of p and k h 1 hw = k h 1 φw = k h 1 α h α h 1 : hw kw is smooth by assumption. Thus A is an atlas, and clearly A is maximal amongst atlases containing A. Therefore it is enough to specify an atlas when defining a smooth structure on a topological manifold, and we will do this without further comment. 1.5 Definition A smooth manifold of dimension n is an n-dimensional topological manifold M equipped with a smooth structure. 1.6 Examples 1. Any open subset V of a smooth manifold M n is itself a smooth manifold; second countability, the Hausdorff condition and the locally Euclidean property are inherited by subsets, and if {U α, h α α A} is an atlas on M, then {U α V, h α Uα V α A} forms an atlas on V. 2. R n is Hausdorff and second countable for a countable base, take all balls of rational radii with rational centres, and certainly locally Euclidean. The identity map determines an atlas on R n there are no transition functions to worry about and smooth structure determined by this atlas makes R n into a smooth n-manifold. We call this the standard smooth structure on R n. 3. The n-dimensional sphere S n R n+1 is a n-dimensional smooth manifold. Indeed, for i = 1... n + 1, let U + i := {y S n y i > 0} and similarly let U i denote the set of points in S n whose ith coordinate is negative. Note that {U ± i } is an open cover of Sn. Now define h i : U ± i R n to be the map that forgets the ith coordinate; h i y 1,..., y n+1 = y 1,..., ŷi,..., y n+1. Suppose i < j; then the transition function h ij : u 1,..., u n u 1,..., ûi,..., ± 1 u 2,..., u n, which is smooth note u 1. A similar formula holds for i > j, and for i = j the transition function is just the identity map. Thus all the transition functions are diffeomorphisms in particular homeomorphisms, and we have a smooth structure on S n. 4. RP n := S n /{±1} is a smooth manifold of dimension n. Let U + i := {x S n x i > 0} and similarly define U i ; note that {U ± i i = 1,..., n + 1} define an open cover of S n. Let π : S n S n /{±1} =: RP n denote the canonical projection. Observe that πu + i = πu i, and that π restricted to U ± i is a homeomorphism RP n is given the quotient topology induced by π. Hence the composition πu + i π 1 U + i h i R n

1 Smooth manifolds 3 is a well defined homeomorphism, call it k i. Moreover we have k j k 1 i = h j π 1 h i π 1 1 = h j h 1 i which is smooth. It follows that πu + i, k i defines an atlas on RP n. 5. The two-dimensional torus T. Define an equivalence relation on R 2 by x y if and only if x i y i Z for i = 1, 2. Let T denote R 2 /. Any unit square Q R 2 with vertices a, b, a+1, b, a, b+1 and a+1, b+1 determines a homeomorphism intq UQ T, where UQ is an open subset of T in fact, UQ is all of T apart from two circles. The inverse map h Q : UQ intq then is a homeomorphism from an open set of T into an open set of R 2. Clearly the {UQ} cover T, and if Q 1 and Q 2 are two squares with a non-empty intersection then one easily sees that the coordinate transformation h Q2 h 1 Q 1 is given locally by translations; that is, each component of h Q1 Q 1 Q 2 of which in general there will be seven - draw a picture! is mapped by a translation onto a corresponding component of h Q2 Q 1 Q 2 by h Q2 h 1 Q 1. Thus we have a smooth structure, and T is a smooth 2-manifold. 1.7 Definition Let M m and N n be smooth manifolds. A continuous map Φ : M N is called smooth if for each p M for some and hence all charts h : U O R m and k : V Ω R n on M and N respectively with p U and Φp V such that the map the composite map called the local expression of Φ k Φ h 1 : hu Φ 1 V kφu V is smooth. If Φ is a homeomorphism and its inverse Φ 1 : N M is also smooth then we say Φ is a diffeomorphism. We say that Φ is a local diffeomorphism if given any p M we can find a neighborhood U of p such that Φ U : U ΦU is a diffeomorphism. A smooth function on an open subset U M is a smooth map f : U R where R is given the standard smooth structure cf. Example 1.6.2. Observe that when we give R n the standard smooth structure, the charts on manifolds become diffeomorphisms their local expression is the identity. 1.8 Germs Let M be a manifold and p M. Functions f, g defined on open subsets U, V respectively containing p are said to have the same germ at p if there exists a neighborhood W of p contained in U V such that f W g W. More precisely, define an equivalence relation on the space of smooth functions defined in a neighborhood of p, by U, f V, g if and only if there exists a neighborhood W of p contained in U V such that f W g W. A germ is an equivalence class under this relation. Notationally, we will not differentiate between a germ f at p and a representative U, f of f. This will hopefully not be confusing. Let Cp denote the set of germs of smooth functions at p occasionally we write CM,p when there is more than one manifold under consideration. Observe that Cp is a ring; given germs f and g with representatives U, f and V, g respectively we define f + g to be germ containing U V, f + g and f g to be the germ containing U V, f g where f gp := fp gp. Moreover we have a natural inclusion of the constant germs into Cp, which induces a natural map R Cp making Cp into an R-algebra. A germ f has a well defined value at p although nowhere else though, and this defines a surjective ring homomorphism eval : Cp R sending f fp. If we let F p denote the kernel of eval, then F p is an ideal of Cp. In fact, since eval is surjective, F p is a maximal ideal, and in fact is the unique maximal ideal, since if fp 0 then if U, f is any representative there exists a neighborhood V U of p such that f is never zero on V. Then the germ containing V, 1 /f is an inverse for f. Hence any germ in Cp \F p is invertible; equivalently F p is the unique maximal ideal and Cp is thus a local ring.

1 Smooth manifolds 4 1.9 Definitions A tangent vector v at p M is a linear derivation of the R-algebra Cp, that is, a linear map Cp R such that vf g = fpvg + vfgp. The tangent vectors form a real vector space in the obvious way; this space is denoted T p M and is called the tangent space to M at p. Note that if c is the constant germ cp = c R then if v is any tangent vector we have vc = 0. Indeed, vc = cv1 and v1 = v1 1 = v1 + v1 implies v1 = 0. 1.10 Charts and tangent vectors Let C0 denote CR n,0 and let M be a smooth n-manifold, p M and h : U O Rn a chart on M about p such that hp = 0 in general we say such a chart is centred about p. Then h defines an isomorphism h of R-algebras h defined by, for f C0, h f = f h. h is an isomorphism precisely because φ is a diffeomorphism. Then given v T p M we can associate a tangent vector h v T 0 R n where h v is the derivation of C0 defined by h vf = vh h. As h is an isomorphism, so is h and thus we have defined an isomorphism h : T p M T 0 R n. 1.11 A basis for the tangent space Let r 1,..., r n denote the standard coordinates on R n. Consider the operator 0 r defined by i 0 r f = f i r 0. Then 0 i r is an linear derviation of C i 0 and hence an element of T 0 R n. Observe that 0 r r j = δ j i i. In fact, we claim that { 0 r i = 1,..., n } forms a basis for T i 0 R n. To prove this we need the following result from calculus. 1.12 Calculus lemma Let f : U R be smooth, where U R n is open and convex. Then there exist smooth functions g ij : U R i, j = 1,..., n such that for any y U we have fy = f0 + f r i 0ri y + r i yr j yg ij y, 1 where as in the rest of these notes we use the summation convention that we sum over indices in an expression that appear in the top and the bottom - we note that the index in 0 r is considered i to be on the bottom it s on the bottom of a fraction. 1.13 Proposition { r i 0 i = 1,..., n } is a basis of T 0 R n. Suppose v = a i i 0 is the zero derivation here and elsewhere, where possible we will abbreviate an expression of the form 0 x to i i 0 - this of course won t work if we are working with several different coordinate systems at once. Then vr i = a i = 0, and so v = 0. Now let v T 0 R n, and set a i := vr i. Consider v 0 := a i i 0 T 0 R n. Given a germ f C0, pick a representative U, f, where we may assume U is convex. Write f as in 1 and compute: vf = vf0 + f r i 0vri + vr i r j g ij. Now the first term disappears, as v is zero on constants, and since r i 0 = 0, the derivation property kills the last term. Thus vf = f r i 0vri = a i i 0 f = v 0 f. Thus v = v 0 and the we have a basis.

1 Smooth manifolds 5 1.14 Observation Observe we can canonically identify T 0 R n with R n via a i i 0 a i e i, where {e i } is the standard basis of R n so r i e j = δ i j. In fact, given any p Rn, the same proof shows { i p } forms a basis of T p R n and thus the identification a i i p a i e i allows us to identify T p R n with R n for any p R n. 1.15 A basis for T p M Now let M n be a smooth manifold and p M. Pick a chart h : U O R n centered about p. Let x 1,..., x n be the coordinates of h. Recall we have a map h 1 : T 0 R n T p M that is an isomorphism. Define the tangent vector p x by, i p x i f := h 1 0 r i f = r i f h 1 0. Since h 1 is an isomorphism, we have the following immediate corollary. 1.16 Corollary Let M n be a smooth manifold and p in M. If U, h is a chart centred at { p with coordinates } x 1,..., x n then T p M is a n-dimensional real vector space with basis p x i = 1,..., n. i Moreover if v T p M then v = a i p x where a i := vx i. i 1.17 Jacobians Suppose now U, h and V, k are both charts centred at p. Write x 1,..., x n for the coordinates of h and y 1,..., y n for the coordinates of k. Let r 1,... r n denote the coordinates on hu and s 1,..., s n the coordinates on kv. Observe by the previous Corollary we have Let F be the coordinate transformation h k 1. F i = r i F. Now note and hence y j p = xi y j p x i p. 2 x i y j p = y j p x i = = = s j xi k 1 0 s j ri h k 1 0 s j ri F 0 = F i s j 0, where JF 0 is the Jacobian of F at 0. Thus we have We can write F = F 1,..., F n where x i p = JF 0, 3 yj p = JF 0 i p j y j x i.

1 Smooth manifolds 6 1.18 General charts More generally, given any chart U, h on M n with coordinates x 1,..., x n, we can define for any p U by the formula p x i f := f h 1 r i hp, x i p where r 1,..., r n are the coordinates on hu. If, hp = c = c 1,..., c n, say if we consider the linear coordinate transformation k = y 1,..., y n where y i := x i c i, then if s 1,..., s n denote the coordinates on ku we have p y i f = s i f k 1 0 = f h 1 r i c = p x i f. { } Hence for any p U, p x is a basis of T i p M. 1.19 Changing coordinates If v T p M and U, h and V, k are charts about p with coordinates x 1,..., x n and y 1,..., y n respectively then writing a i p x i = v = b j p y j and using 2we see that 1.20 Definition a i = vx i = b j p y j x j = b j xi p. 4 yj Let Φ : M N be a smooth map between smooth manifolds. Let p M. We have a map Φ : C N,Φp C M,p defined by Φ f = f Φ. Now define the derivative of Φ at p to be the map dφp : T p M T Φp N defined by dφpvf = vφ f. Thus dφp is a linear map between the tangent spaces. Where possible we will omit the p from the notation and just write dφ. The chain rule is tautologous: if Ψ : N P is a smooth map of smooth manifolds such that Ψ Φ : M P is defined then dψ Φ = dψ dφ. Indeed, if v T p M and f A P,ΨΦp then d Ψ Φ vf = vψ Φ f = vψ Φ f = vφ f Ψ dφvf Ψ dφvψ f dψdφvf.

1 Smooth manifolds 7 { } { } If p x is a basis of T i p M and Φp y is a basis of T j Φp N then where Φ i = y i Φ and thus Hence if then and thus 1.21 Example y dφ p i x j = x j yi Φ = Φi x j p, dφ p x j = Φi x j p Φp y i. v = a j p x j, dφv = b i Φp y i dφv = a j dφ p x j = a j Φi x j p Φp y i, b i = a j Φi p. 5 xj As a special case, if Φ : R m R n is smooth and p R m, with r 1,..., r m the standard coordinates on R m and s 1,..., s n the standard coordinates of R n we have dφ p r i = JΦp j Φp i s j. 6 In particular, under the identification of T p R n with R d as in Section 1.14, the derivative dφp is just the linear map determined by the Jacobian JΦp. Given this, one might ask why the chain rule was so easy to prove as it is not so simple to prove in standard multivariate calculus. The answer is in our use of Lemma 1.12, which in turn used the standard chain rule in multivariate calculus. 1.22 Definition A smooth curve on a manifold M is a smooth map c : a, b M, where a, b R is an interval and R is given the standard smooth structure. For t a, b the tangent vector to c at t is d dc dr t T ct M, we write d/dr instead of /r when n = 1, and is denoted ċt. If c : a, b M is a smooth curve, and x 1,..., x n local coordinates about ct 0 then for t close to t 0 we set c i t := x i ct. Then ċt x i d = dc dr t x i = d dr xi c = dci dr t, and hence that is, ċt = dci dr t i ct, 7 ċ = dci dr i c. In particular if M = R n and we use the identification of T ct R n with R n given in Section 1.12 we have ċt = dci dr te i, which recovers the standard definition from multivariate calculus for the derivative of a smooth curve c : a, b R n.

1 Smooth manifolds 8 1.23 An alternative definition of tangent vectors We now focus our attention on smooth curves in M defined on a neighborhood of 0. A smooth curve c : ɛ, ɛ M with c0 = p defines a tangent vector ċ0 T p M. Note that smooth curves c and γ define the same tangent vector if and only if, for some and hence every chart h centred at p we have h c and h γ defining the same tangent vector in T 0 R n. By the previous section, this is if and only if d dr h c 0 = d h γ 0. 8 dr Conversely suppose v T p M is any tangent vector. By making a linear change of coordinates in the vector space T p M we may assume that we have local coordinates h = x 1,..., x n about p such that v = 1 p. Define ct = h 1 t, 0,..., 0. Then for f Cp we have d ċ0f = dc dr 0 f = d f c0 dr = f h 0 r1 = p x 1 f = vf. Thus any tangent vector v T p M can be written as ċ0 for some smooth curve c : ɛ, ɛ M. Thus we can make the following alternative definition of T p M: a tangent vector at p M is an equivalence class of smooth curves c : ɛ, ɛ M such that c0 = p, where c γ if and only if for some chart h centred at p, 8 holds. 1.24 Definition Let M be a smooth manifold. The tangent bundle of M is the disjoint union of the tangent spaces; T M := T p M. p M We have a natural projection π : T M M sending v T p M p. When referring to an element of T M, we will often write p, v to indicate that v T p M. 1.25 Theorem Let M be a smooth n-manifold. Then T M is naturally a smooth 2n-manifold such that π is smooth. Let {U α, h α } be an atlas on M, where h α : U α O α has coordinates x 1 α,..., x n α. Define a local trivialisation t α : T U α := p U α T p M U α R n by If U α U β then the map t α t 1 β t α p, v = p, v x 1 α,..., v x n α. p, a 1,..., a n : U α U β R n U α U β R n sends p, a i x1 β x i p,..., a i xn β α x i p α cf. 4. In particular, the map ψ αβ p := t β t 1 α p, : R n R n is a linear isomorphism, and moreover the map ψ αβ : U α U β GLn, R, p ψ αβ p

2 Vector fields 9 is smooth. Now define h α : T U α O α R n by h α = h α id t α. Then observe for α, β such that U α U β the transition function h α : h β U α U β R n h α U α U β R n sends h 1 β q, a 1,..., a n h αβ q, ψ αβ h 1 β q a 1,..., a n, which is smooth. Moreover the collection { T U α, h α } is a collection of bijections such that T M = α T U α. Now define a topology on T M by declaring the h α to be homeomorphisms. This will make T M into a smooth 2n-dimensional manifold with atlas { T U α, h α } as soon as we know that is Hausdorff and second countable under this topology. If p, v q, w then either p q and we can use the Hausdorff property of M or p = q and v w and we can use the Hausdorff property of R n to separate p, v and q, w. To see second countability, we may assume that {U α } is a countable cover of M; then each U α R n is second countable, and hence so are the T U α and since{t U α } is a countable cover of T M it follows T M is second countable. It is immediate that π is smooth, as its local expression with respect to charts U α, h α and T Uα, h α is the map proj1 : U α R n U α. This completes the proof. In fact this proof actually shows that T M is a smooth vector bundle of rank n over M vector bundles will be defined in Chapter 5. 1.26 Bundle maps between tangent bundles Let Φ : M m N n be smooth. Then Φ induces a bundle morphism dφ : T M T N defined by dφp, v = dφpv. Moreover, dφ is smooth. Indeed, if p, v T M and U, h is a chart about p, and V, k a chart on N about Φp then the local expression k dφ h 1 is the map hp, a 1,..., a m k Φ h 1 hp, a j Φ1 Φn p,..., aj xj x j p, cf. 5 which is smooth. 2 Vector fields 2.1 Definition A vector field on M is a smooth section of π : T M M, that is, a smooth map X : M T M such that π X = id M. Thus if X is a vector field, Xp, which we will often write as X p, lies in T p M for all p M. The assertion that X is smooth is equivalent to the following. Let U, h be a chart on M with coordinates x 1,..., x n. Then for p U we can write X p = X i p i p for some functions X i : U R, and to say X : M T M is smooth is equivalent to saying that the X i are smooth functions on U. Indeed, with respect to the chart T U, h on T M, X has local expression p x 1 p,..., x n p, X 1 p,..., X n p and thus X is smooth if and only if all the X i are smooth. Let X M denote the set of all smooth vector fields on M. For f C M and X X M, we can define a new vector field fx : M T M by fx p = fpx p T p M. Similarly we can also define for f, g C M and X, Y X M a vector field in the obvious way, and so X M becomes a module over the ring C M. We can also define local vector fields to be smooth sections of π defined only on some open set U M. We denote the local vector fields over U M by X U. In particular if x 1,..., x n are local coordinates on U M then i X U.

2 Vector fields 10 2.2 Proposition Let M n be a smooth manifold on which there exist n independent vector fields X 1,..., X n, that is, for all p M, {X 1 p,..., X n p} is a basis of T p M. Then T M is isomorphic as a vector bundle to M R n. By this we mean this will be explained in more detail in Chapter 5 - see Section 5.4 in particular that there exists a diffeomorphism F : T M M R n such that F T p M {p} R n and the restriction of F to T p M, F p : T p M {p} R n is a linear isomorphism. Define F : T M M R n by F p, v = p, c 1,..., c n where v = c i X i p in the basis {X i p} of T p M. Then F is a bijection by assumption, and restricts as required. We thus need only show F and F 1 are smooth. Given a chart U, h with local coordinates x 1,..., x n on M, the local expression of F in the charts T U, ĥ and U Rn, h id is p, a 1,..., a n p, c 1,..., c n where a i i p = v = c i X i p. Now we can write X i p = b j i p j p for some smooth functions b j i : U R. Then a j j p = v = c i X i p = c i b j i p j p, and thus a j = c i b j i p. This shows that F 1 is smooth, as the b j i are smooth. Moreover, since matrix inversion is smooth, and p [ b j i p] is smooth, if [ d i j p] denotes the inverse matrix to [ b j i p] then p [ d i j p] is also smooth. Then as c i = d i j paj, we see that F is also smooth. 2.3 Definition Given a smooth vector field X and f C M, we can define a function Xf : M R by Xfp = X p f. If U, h is a chart about p with coordinates x 1,..., x n, then we can locally write X p = X i p i p, and thus Xfp = X i p f x i p. In particular, Xf is smooth. Hence we may also view X as a derivation of C M; since X p is a derivation of Cp we immediately have In fact, more is true. 2.4 Proposition Xfgp = Xfp gp + fp Xgp. A map X : C M C M is a deriviation if and only if there exists X X M such that for all f C M, Xf = Xf. We have just shown given X X M, defining X : C M C M by Xf = Xf does indeed define a derivation. Conversely, suppose X is a derivation of C M, p M and define a tangent vector X p T p M by, for f C p, X p f := X f p, where f is any smooth function defined on all of M such that the image of f in C p is f. There are three things to check in order to conclude this is well defined. Firstly we need to know that there exists a smooth extension f of f to a function defined on all of M a priori, we only know that f defines a function on a neighborhood of p. Secondly we need to know that if f and f are two such extensions then X fp = X f p. Then we need to check X p is indeed a derivation of C p, and thus does indeed define an element of T p M.

2 Vector fields 11 The key fact we need is the following: given any p M and any neighborhoods U V of p there exists a smooth function ψ : M R such that ψ U 1 and ψ M\V 0. Such a function is called a bump function. That such functions exist is not obvious, and depends on the existence of partitions of unity. We will define these in Chapter 5, Theorem 5.17, and prove the existence of bump functions in Corollary 5.18. For now however we will just accept such functions ψ exist. It is then immediate that such an extension f exists. In order to check X p f is independent of the choice of extension, it is enough to observe that if f C M vanishes in a neighborhood of p then X fp = 0. If f V 0 for some neighborhood of p, then choose a neighborhood U V of p, pick a bump function ψ such that ψ U 1 and ψ M\V 0, and then consider the smooth function ψ : M R, ψ := 1 ψ. Then ψ U 0 and ψ M\V 1, and so as functions on M, f = fψ. The derivation property of X ensures X fψ p = 0, and so also X fp = 0 as required. It is clear now that X p is a derivation of C p, since X acts as a derivation on the chosen extensions. To complete the proof, we show that p X p is smooth, and thus this construction defines us a vector field X on M. For this it is enough to check that if x 1,..., x n are any local coordinates on a neighborhood U of p then Xx i C U, regarding x i : U R as smooth functions on U. But this is clear, since if f C U is any function then using a bump function we extend f to f C M, and then observe that X f C M. 2.5 XY is not a derivation Given X, Y X M and f C M, we can define XY f = XY f. However this does not define a vector field, as this is not a derivation of C M. Indeed, XY fg = X {Y fg + fy g} = XY f g+y f Xg+Xf Y g+f XY g XY f g+f XY g. However, this shows that [X, Y ] := XY Y X is a derivation of C M. It thus follows that [X, Y ] := XY Y X defines a vector field on M. We call [X, Y ] the Lie bracket of X and Y. 2.6 Properties of the Lie bracket 1. The map [, ] : X M X M X M is bilinear over R and skew-symmetric. 2. If f, g C M and X, Y X M then [fx, gy ] = fg[x, Y ] + fxgy gy fx. 3. If U, h is a chart on M with coordinates x 1,..., x n and in this chart Xp = X i p i p and Y p = Y i p i p then [X, Y ]p = X i p Y j p Y i p Xj p j p. 9 x i x i 4. The coordinate local vector fields i, j always satisfy [ i, j ] = 0. 5. The Jacobi identity: for X, Y, Z X M, [X, [Y, Z]] + [Y, [Z, X]] + [Z, [X, Y ]] = 0. 1 is clear. To prove 2, we first compute XgY. Let l C M. Then and hence XgY = Xg Y + g XY. Then Next, to prove 3 we compute XgY l = Xg Y l = Xg Y l + g XY l, [fx, gy ] = fxgy gy fx XY f = X f Xg Y + fgxy g Y f X + gfy X fg[x, Y ] + f Xg Y g Y f X. Y j f x j = X i Y j f x i x j + Xi Y j 2 f x i x j. Symmetry of the mixed partial derivatives then proves 3. Finally both 4 and 5 follow from 3.

2 Vector fields 12 2.7 Corollary X M is an infinite dimensional Lie algebra under [, ]. 2.8 Definition Let Φ : M N be a diffeomorphism and X X M. We can define the pushforward of X to N under Φ to be Φ X defined by Φ X q = dφ X Φ 1 q Tq N. 10 Thus if f C N we have so Φ X f = Xf Φ Φ 1, 11 dφ X = Φ X Φ. 2.9 Lemma Let Φ : M N be a diffeomorphism and X, Y X M. Then Φ [X, Y ] = [Φ X, Φ Y ]. In other words, Φ defines a Lie algebra isomorphism Φ : X M X N. Let q N and set p = Φ 1 q. Suppose f C N. Then we compute: Φ [X, Y ] q f = dφ [X, Y ] p f = [X, Y ] p f Φ = X p Y f Φ Y p Xf Φ = X p dφ Y f Y p dφ Xf = X p Φ Y f Φ Y p Φ Xf Φ = dφ X p Φ Y f dφ Y p Φ Xf = Φ X q Φ Y f Φ Y q Φ Xf = [Φ X, Φ Y ] q f. An unpleasant calculation. Note that we used both characterisations 10 and 11 at different stages in the proof. 2.10 Definition Let X X M and p M. A smooth curve c : a, b M with a < 0 and b > 0 is called an integral curve of X at p if c0 = p, Xct = ċt for all t a, b. 2.11 Theorem existence and uniqueness of integral curves Let M be a smooth manifold, p M and X X M. Then there exists an open interval I p containing 0 and an integral curve c p : I p M of X such that c p 0 = p. Moreover, if γ : J M is another integral curve of X such that γ0 = p, with J an open interval containing 0 then J I p and c p J γ. If c : a, b M is a smooth curve, and x 1,..., x n local coordinates about ct 0 then for t close to t 0, recall by 7we have ċt = dci dr t i ct,

2 Vector fields 13 where c i = x i c. Suppose in this chart Xq = X i q i q. Then the assertion that c is an integral curve becomes dc i dr t i ct = X i ct i ct, and thus the assertion comes down to solving the system of ODE s dc i dr t = Xi ct, c i 0 = X i p. 12 So choose a chart U, φ about p. Let I p denote the union of all the open intervals containing the origin which are the domains of integral curves of X satisfying the initial condition that the origin maps to p. Applying the standard theorem on existence to solutions of ODE s to the system of equations 12 we see that I p. Suppose now c and γ are integral curves of X defined on open intervals A, B respectively with A B. Then if there exists t 0 A B such that ct 0 = γt 0, then by the standard theorem on uniqueness to solutions of ODE s, the subset of A B on which c and γ is open and non-empty. By continuity it is also closed, and hence by connectedness it is equal to A B. It follows there exists an integral curve c p of X defined on all of I p, which completes the proof. 2.12 Definitions Let M be a smooth manifold, and X X M. In the notation of the proof above, for t R define U t := {p M t I p } and define φ t : M M by φ t p = c p t. 2.13 Theorem flow theorem For each t it holds that: 1. U t is open, and M = t>0 U t. 2. If t I p then I φtp = {s t s I p }. 3. φ t : U t U t is a diffeomorphism with inverse φ t. 4. If s, t R then the domain of φ s φ t is contained in but not generally equal to U s+t. If s, t have the same sign however then we have equality. In any case, on the domain of φ s φ t we have φ s φ t = φ s+t. 5. Given p M there exists a maximal open neighborhood V of p and maximal ɛ > 0 such that the map φ : ɛ, ɛ V, t, q φ t q = γ q t is a well defined smooth map. Note by 3 we have for s, t R such that all of s, t and s + t < ɛ this implies φs + t, p = φs, φ t p. We say that φ is the local flow of X at p. We won t prove the Flow Theorem; it essentially follows from the ODE theorem on smooth the dependance on initial conditions. 2.14 Definitions A smooth vector field X is called complete if U t = M for all t R, in other words, for all p M,the domain of c p is all of R. In this case the transformations {φ t } t R form a group of transformations of M parametrized by the real numbers. It is called the one-parameter group of X. The associated map φ is then a global flow. Note that if X is not complete, {φ t } t R do not form a group, since their domains depend on t. In this case we refer to {φ t } t R as the local one-parameter group of X.

3 Submanifolds 14 2.15 Proposition Let X be a smooth vector field on a smooth manifold M. If c is an integral curve of M whose maximal domain is not all of R, then the image of c cannot lie in any compact subset of M. Let a, b denote the maximal domain of c, and p := c0. Suppose b < but that the image of c lies in a compact set K of M the case a > is similar. If {t i } is any sequence of times approaching b from below, then {ct i } is a sequence of points in K, and thus passing to a subsequence if necessary we may assume ct i q K. Choose a neighborhood U of q and ɛ > 0 such that that the local flow φ of X is defined on ɛ, ɛ U so for t a, b ɛ, ɛ, φt, p = ct. Pick i large enough such that ct i U and t i +ɛ > b, and define γ : a, t i +ɛ M by { ct a < t < b γt = φt t i, ct i t i ɛ < t < t i + ɛ. By assumption these definitions agree on the overlap, since φt t i, ct i = ϕt t i, φ ti p = ϕt t i + t i, p = ct. and hence γ is an integral curve of X satisfying γ0 = p and defined on a larger interval then a, b. Contradiction. 2.16 Corollary If M is a compact smooth manifold then every smooth vector field on M is complete. 3 Submanifolds 3.1 Definition Let Φ : M N be a smooth map between manifolds. We say that Φ is an immersion if dφp is injective for each p M. 3.2 Definitions Let Φ : M N an injective immersion. Then the pair M, Φ is an immersed submanifold of N. If in addition Φ is a topological embedding, that is, Φ is a homeomorphism onto its image with the subspace topology then the pair M, Φ is an embedded submanifold. In this case we often suppress Φ and identify M with its image ΦM N and thus regard Φ as the inclusion M N. Let Φ : M N be an embedding. Then for p M, the map dφp : T p M T Φp N identifies the tangent space T p M with a subspace of T Φp N. Then dφ : T M T N is a smooth embedding, so T M is an embedded submanifold of T N. 3.3 Definitions Let Φ : M m N n be smooth. A point p M is called a regular point of Φ if dφp is surjective. If p M is not a regular point then it is a critical point. A point q N is a regular value of Φ if for any p Φ 1 q, p is a regular point. Note that if Φ 1 q = then this condition is vacuously true. If q N is not a regular value then it is a critical value. Note that if m < n then any point q N such that f 1 q is non-empty is a critical value. 3.4 Theorem implicit function theorem Let U be a neighborhood of 0 in R m and Φ : U R n a smooth map such that Φ0 = 0. Then: 1. If m n, let i : R m R n denote the canonical inclusion. If Φ has maximal rank m at 0 then there exists a chart h on R n and a neighborhood W of 0 R m such that h Φ W = i W.

3 Submanifolds 15 2. If m n, let π : R m R n denote projection onto the first n coordinates. If Φ has maximal rank n at 0 then there exists a chart k on R m and a neighborhood V of 0 R m such that Φ k V = π V. ] First we prove 1. The hypotheses imply that the m n matrix x 0 j has rank m. Hence by rearranging the component functions Φ i of Φ if necessary which amounts to composing Φ with an invertible [ transformation ] of R m, which is a diffeomorphism we may assume that the m m minor Φ i x 0 j is invertible. Define F : U R n m R n by 1 i,j m [ Φ i F x 1,..., x m, x m+1,..., x n := Φx 1,..., x m + 0,..., 0, x m+1,..., x n. Then F i = Φ, and the Jacobian matrix of F at 0 is [ ] [ Φ i x 0 j ] 1 i m Φ i x 0 j m+1 i n 0 I n m Thus by the inverse function theorem F has a local inverse h, and h Φ = h F i = i. This proves 1. [ ] Φ Similarly in 2, we may assume that the n n minor i x 0 is invertible, and hence j 1 i,j n defining G : U R m n R m by Gx 1,..., x m := Φx 1,..., x m, x n+1,..., x m. Then Φ = π G, and the Jacobian matrix of G at 0 is [ [ ] [ ] Φ i Φ x 0 i j x 0 j 1 j n 0 I m n n+1 j m ] Thus by the inverse function theorem G has a local inverse k, and Φ k = π G k = π. 3.5 Definition Let M m be a submanifold of N n. A chart U, h on N with local coordinates x 1,..., x n is called a slice chart for M in N if M U = {p U x m+1 p = = x n p = 0}. 3.6 Proposition submanifold criterion Let Φ : M m N n be an immersion. Then for any p M, there exists a neighborhood U of p and a coordinate map V, k defined on some neighborhood V of Φp, with local coordinates y 1,..., y n such that: 1. A point q belongs to ΦU V if and only if y m+1 q = = y n q = 0, so 2. Φ U is an embedding. k ΦU V = R m {0} kv. If Φ was an embedding, then we may take U = M, and hence ΦM V = {q V y m+1 q = = y n q = 0}. In other words, an immersed submanifold M m N n is one such that every point p M has a chart V, k about Φp and a neighborhood U such that k is a slice chart for U in N, and an embedded submanifold is one such that every point p M has a chart V, k about Φp such that

3 Submanifolds 16 k is a slice chart for M in N. Let i : R m R n denote the inclusion. Let h be a chart centred about p, and l a chart centred about Φp. Since l Φ h 1 has maximal rank m at 0, by the implicit function theorem there exists a chart l of R n and a neighborhood W of 0 R m such that l l Φ h 1 W = i W. Then set U = h 1 W and k = l l. Then by restricting the domain of l if necessary, 1 clearly holds. Furthermore, since Φ U = k 1 i h is the composition of embeddings, so is Φ U. Finally, if Φ was an embedding then ΦU = ΦM V for some open set V N, and hence ΦU V = ΦM V V, and so replacing V by V V, the last statement follows. 3.7 Proposition Every regular level set of a smooth map is an embedded submanifold. Suppose Φ : M m N n is smooth. Suppose initially that Φ is a submersion. If q N, and p P := Φ 1 q, then by the Theorem 3.4 there are charts U, h of M about centred about p and V, k on N centered about q such that Φ has local expression y 1,..., y m y 1,..., y n, 0,..., 0 in these two charts. Thus P U is the slice {x 1,..., x m U x n+1 = = x m = 0}, and so P is an embedded submanifold of M. Now we consider the general case, and drop the assumption that Φ is a submersion. If q is any regular value of of Φ such that P := Φ 1 q, then for each p P, dφp has rank n. Let U := {p M dφp has rank n}. Then P U, and we will show that U is open. Given this, Φ U : U N is a submersion, and we can apply the above to conclude that P is an embedded submanifold of U, and hence also an embedded submanifold of M. If p U, then the determinant of some n n minor of the n m matrix representing dφp in some smooth local coordinates is non-zero. Since the determinant is continuous, there is a neighborhood V of p such that this minor has non-zero determinant, and thus V U and U is open. 3.8 Theorem Sard If Φ : M N is smooth then the set of critical values of Φ has measure zero in N. We will not prove this theorem in this course. 3.9 Theorem Let Φ : M m N n be a smooth map, with m nis smooth. If q N is a regular value of Φ such that P := Φ 1 q, then P is a topological manifold of dimension m n. Moreover there exists a unique smooth for which P, i where i : P M is inclusion becomes an embedded submanifold of M. Let k : V R n be a chart on N centred about q; given p P, let h : U R m be a chart on M centred about p. Decompose R m = R n R m n, and let π 1 : R m R n and π 2 : R m R n m denote the projections onto the two factors. Let i 2 : R m n R n denote the inclusion a 1,..., a m n 0,..., 0, a 1,..., a m n. Since k Φ h 1 has maximum rank at 0 R m by Theorem 3.4 there exists a chart W, l around 0 R m such that k Φ h 1 l = π 1 W. Let W := π 2 W, so W is open in R m n and k Φ h 1 l i 2 W = π 1 i 2 W = 0. Thus if j := h 1 l i 2 W then jw P. In fact, we claim that jw = P h 1 l W,

3 Submanifolds 17 so that j maps W homeomorphically onto a neighborhood of p P in the subspace topology. Indeed, clearly jw P h 1 l W, since jw = h 1 l i 2 W = h 1 l W 0 R m n. Conversely, if p P h 1 l W, then p = h 1 lu for some unique u W, and since we have 0 = k Φp = k Φ h 1 l u = π 1 u, u = 0, a 0 W for some a W, and thus p = ja jw. It follows that the inclusion i : P M is a topological embedding. Finally, we endow P with the smooth structure induced by the charts { jw, j 1} as p ranges over P. Then i : P M is smooth, since h i j 1 1 = l i2. 3.10 Corollary Let Φ : M m N n be smooth, q N a regular value and P = Φ 1 q. Then for p P, we have di T p P = ker dφp. Since both subspaces have common dimension m n, it suffices to check that dit p P ker dφp. Let v T p P. Then for f CN,q we have dφdivf = dφ ivf = vf Φ i. But Φ i q, and hence f Φ i is a constant function, and thus vf Φ i = 0. 3.11 Example GLn, R is an open subset of Matn, R = R n2. The set Symn, R of symmetric matrices may be identified with R nn+1 2. Now define Φ : GLn, R Symn, R by ΦA = AA t. Observe that Φ 1 I = On, the real orthogonal n n matrices. We claim that I is a regular value of Φ. First for A GLn, R we can define a diffeomorphism R A : GLn, R GLn, R by right multiplication: R A X = XA. Now observe that if A On then Φ R A = Φ. Thus by the chain rule, we have dφa dr A I = dφi. Since R A is a diffeomorphism this shows that rankdφa = rankdφi. It is therefore enough to check that dφi is surjective. Now observe that T I GLn, R = T I Matn, R = Matn, R. Specifically, if we take global coordinates x i j on GLn, R, where we send x i ja = a i j, A = [ a i j], a i j x i j I [ a i j] Matn, R. We can represent an arbitary element A T I GLn, R by the curve c A : t I + ta note that ct GLn, R for small enough t. Now since ΦI + ta = I + ta + A t + t 2 AA t we have dφia = d dt t=0 ΦI + ta = A + A t. Now finally let S by an arbitrary symmetric matrix, then if A = S /2 we have A + A t = S. Thus dφi is surjective, and thus On is an embedded submanifold of GLn, R of dimension nn 1 2.

4 Lie groups 18 3.12 Distributions Let M be a smooth manifold. A r-dimensional distribution D on M is a choice of an r-dimensional subspace Dp T p M for each p M. A distribution D is smooth if D M := p M Dp is a smooth subbundle of T M see Chapter 6 for the precise definition of subbundles. Equivalently, D is smooth if every p M has a neighborhood U and smooth vector fields X 1,..., X r X U such that {X 1 q,..., X r q} is a basis for Dq for each q U. We say a smooth vector field X X U where U M is an open subset belongs to D if X p Dp for all p U. A distribution D is called involutive if given X, Y X U belonging to D we also have [X, Y ] ΘU belonging to D. Note that a one-dimensional distribution is just a vector field. If M, f is an immersed submanifold of N and D is a distribution on N, we call M, f an integral submanifold of D if dφt p M = DΦp for all p M. A distribution D on N is called completely integrable if each point is contained in an integral submanifold of N. A locally integrable distribution is one such that every point p N is contained in an integral submanifold of an open subset U N. Note that an integral manifold of a one-dimensional distribution is just the image of a curve. 3.13 Theorem Frobenius A distribution is involutive if and only if it is completely integrable. 3.14 Theorem Whitney Any smooth manifold M n may be embedded in R 2n. We will not prove either of these theorems in this course. The version of Theorem 3.14 stated is a truly difficult result. An earlier and much easier result also due to Whitney states that we can embed M n in R 2n+1. 4 Lie groups 4.1 Definitions A Lie group G is a smooth manifold endowed with a group structure such that the multiplication map m : G G G, p, q pq and the inversion map i : G G, p p 1 are smooth maps. A Lie subgroup H of G is the image of an immersed submanifold H, Φ of G such that H is a Lie group, and Φ : H G is a homomorphism of the abstract groups H and G. Thus if H G is a Lie subgroup then the inclusion i : H G is an immersion. It is a non-trivial fact that a closed subgroup H G is a Lie group with respect to the subspace topology. 4.2 Examples 1. From the previous lecture, GLn, R, On and SOn are all Lie groups. 2. The n-torus T n = R n /Z is an abelian Lie group the group structure is induced by addition on R n. In fact, any compact abelian Lie group is a torus. 3. A given manifold can carry multiple Lie group structures. In addition to the standard one, we can make R 3 into a Lie group by defining ma, b = a 1 + b 1, a 2 + b 2 + a 1 b 3, a 3 b 3 where a = a 1, a 2, a 3, b = b 1, b 2, b 3. This corresponds to identifying R 3 with the subgroup H of GL3, R consisting of matrices of the form 1 a 1 a 2 0 1 a 3 0 0 1 The fact that this is a subgroup confirms that m does indeed endow R 3 with a group structure..

4 Lie groups 19 4.3 Definition Let G be a Lie group. Set g := T e G where e is the identity element of G. g is called the Lie algebra of G. Our initial aim is to show that g is indeed a Lie algebra and thus the definition is not completely inane. 4.4 Computing the Lie algebra o n of On. Recall from Example 3.11 that On is an embedded submanifold of GLn, R of dimension nn 1 2. Thus o n := T I On is naturally a subspace of gl n := T I GLn, R = Matn, R. We can no longer represent a element of o n by a curve of the form ct = I + ta for some A Matn, R, as even for small t, I + ta has no reason to lie in On. However by elementary calculus, we can write Then if we require ct On then we need ct = I + ta + Ot 2. I + ta + Ot 2 I + ta + Ot 2 t = I, or equivalently A + A t = 0. This gives o n {A gl n A + A t = 0} and then counting dimensions gives equality. Alternatively one could proceed as in Example 3.11, with the map dφ : T I GLn, R T I Symn, R, and then use Corollary 3.10 to conclude that T I On was the kernel of dφi. Since dφia = A + A t, we recover the same result. 4.5 Definition Let G be a Lie group. Let l p : G G denote the diffeomorphism q pq. Let X X G. We say that X is a left-invariant vector field if l p X = X for all p G. We let X l G denote the set of left-invariant vector fields on G. In more detail, this means that for any q G we require for f C pq, X pq f = l p X pq f = dl p X q f = X q f l p. Suppose X X l G, and let ξ = X e. Let f C p. Then X p f = X e f l p = dl p X e f = dl p ξf. It follows that if we define a section X ξ : G T G by, for p G and f C p, X ξ pf = dl p ξf, then X ξ = X and thus X ξ is a left-invariant vector field. Hence a left-invariant vector field X is determined by ξ = X e. In fact, if ξ is an arbitrary element of g, then defining X ξ as above yields a left-invariant vector field. 4.6 Proposition Let G be a Lie group, and ξ g = T e G. Define a section X ξ : G T G by Then X ξ is a vector field on G; moreover X ξ is left-invariant. X ξ p = dl p ξ T p G. 13 We need only verify that X ξ is a smooth section of π : T G G and left-invariant. Let h e : U e O be a chart centred about e, with coordinates x 1,..., x n n = dim G. Fix a point p G. Observe that if U p := l p U e and h p := h e l p 1 then h p : U p O is a chart centered about p. Let y 1,..., y n denote the coordinates of this chart. Now choose U e U e such that if U p = l p U e then mu p U e U p. We then have the following commutative diagram U p U e m U p O O F O

4 Lie groups 20 where F is defined to be the smooth composite at the bottom. Given q U p, wee can restrict this to {q} U e l q U p {h p q} O F hpq, O Then the map dl q : T e G T q G is given, with respect to the bases { } e x of i Te G and { } q y of T j q G by dl e q x i = JF h p q, 0 j q i y j, where JF h p q, 0 is the Jacobian matrix of F at the point h p q, 0 O O cf. 6. Since the entries of JF h p q, 0 are smooth functions of q U g, we have shown that for any fixed ξ T e G, the images dl q ξ depend smoothly on q. Thus X ξ is smooth. Finally, we check X ξ is left-invariant. Indeed, This completes the proof. 4.7 Corollary l p X ξ pq = dl p X ξ q = dl p dl q ξ = dl pq ξ = X ξ pq. We have a linear isomorphism between g and X l G given by ξ X ξ. 4.8 Corollary Let G n be a Lie group, and g its Lie algebra. Then g is a n-dimensional Lie algebra! under the bracket induced g from the bracket on X l G inherited from X G. We need only show that if X ξ and X η are left invariant then so is [X ξ, X η ]. But by Lemma 2.9, for any p G, since l p is a diffeomorphism we have l p [X ξ, X η ] = [l p X ξ, l p X η ] = [X ξ, X η ], so [X ξ, X η ] is left-invariant. Thus we can define a Lie bracket on g by setting [ξ, η] = ζ where [X ξ, X η ] = X ζ. 4.9 The commutator bracket Suppose now that G is a matrix Lie group, that is, G is a Lie group and a closed subgroup of GLn, R. Then as we have seen, T e G can be identified with a subspace of Matn, R. We already have a bracket on Matn, R, namely the commutator [A, B] := AB BA. In fact, these two brackets coincide. In this section we ll prove the case when G = GLn, R. Using the matrix entries x i j as global coordinates on GLn, R, the natural isomorphism T I GLn, R gl n takes the form a i j x i j I a i j. Any matrix A = aj i defines a left-invariant vector field XA, defined by for P GLn, R X A P = dl P a i j I. Under the above identification the map dl P I is just left multiplication by P = pj i, and thus in coordinates X A P = p i ja j k P. 14 x i j x i k

4 Lie groups 21 Given two matrices A, B, using 9, the Lie bracket of the corresponding left-invariant vector fields is given by { [X A, X B ] P = p i ja j k p l m b m h p i j b j k p l m a m } h P x i k x i k { p i ja j k δl i δ k mb m h p i jb j k δl i δ k ma m h { } p i ja j k bk h p i jb j k ak h In particular, if P = I then we obtain [X A, X B ] I = { a i kb k h b i ka k } h x i h x i h P. P = [A, B] i h } x i h x l h P x l h I = X [A,B] I. Since a left-invariant vector field is determined by its value at the identity, this shows that [X A, X B ] = X [A,B], which is precisely what we wanted to show. To deal with the case when G is merely a subgroup of GLn, R we consider the following more general situation. 4.10 Restriction to subgroups Let H G be a Lie subgroup and let i : H G denote inclusion. Then i is an immersion, and so di T e H = dih is a subspace of g. If ξ h then letting ξ = diξ dih we have left-invariant vector fields X ξ X l H and X ξ X l G. If l G,p and l H,p denote the respective left multiplication diffeomorphisms for p H then l G,p i = i l H,p and thus di X ξ p = di dl H,p ξ = dl G,p diξ = dl G,p ξ = X ξp. We have previously only defined Φ X for Φ a diffeomorphism: if Φ : M N is smooth and X X M then it may still be the case that there exists a well defined vector field Y X N satisfying Y q = dφ X Φ 1 q - in this case we write Y = Φ X and say X and Y are Φ -related.the difference is that if Φ is not a diffeomorphism there is no guarantee that such a vector field exists. However if it does, the proofs of our previous results eg. Lemma 2.9 still go through. Thus the computation above shows that i X ξ = X ξ, and hence by Lemma 2.9 we conclude that di h is a Lie subalgebra of g, and di : h g is a Lie algebra homomorphism, that is [X ξ, X η ] H = [ X ξ, X η ]G. In particular the bracket on H is induced from that of G. Applying to this to H GLn, R we conclude that the bracket is again given by matrix commutation, as required. 4.11 Lemma Let G be a Lie group, and X ξ X l G be a left-invariant vector field associated to some ξ g. Let θ : ɛ, ɛ G be the integral curve for X ξ such that θ0 = e. Then for s, t < ɛ/2 we have θs + t = θs θt, where denotes group multiplication in G, that is θs + t = l θs θt. For fixed s, we show that the curves t θs + t and t θs θt are both integral curves of X ξ defined on ɛ /2, ɛ /2 though e. Uniqueness of integral curves then forces equality. Define ct : ɛ/2, ɛ/2 G by ct = θs + t. Then certainly c0 = θs. Moreover d ċt = dc dr t d = dθ dr s+t. = θs + t = X ξ θs + t = X ξ ct.

4 Lie groups 22 Suppose now p = θs G. Define γt = l p θt. Then γ0 = p e = p = θs and d γt = d l p θ dr t d = dl p dθ dr t = dl p θt = dl p X ξ θt = X ξ l p θt = X ξ γt, where for the last but one equality we used left-invariance of X ξ. Thus both c and γ are indeed integral curves of X ξ through e defined on the same interval as claimed. 4.12 Corollary Any left-invariant vector field on a Lie group G is complete. Let X ξ be an arbitrary left-invariant vector field on G, corresponding to ξ g.let θ : ɛ, ɛ G be the integral curve through e for X ξ. Define c : R G as follows. Given t R, choose N N such that t /N ɛ /2, ɛ /2. Define ct = θ t /N N. First, let use check θ is well defined. Suppose N was another such integer. Then since θ t /NN NN = θ t /NN by Corollary 4.11, we have θ t /N N = θ t /NN NN = θ t /N N. Certainly c0 = e, and given t R, letting p = θ t /N N 1 as before we have d ċt = d l p θ dr t d = dl p dθ dr t = dl p θt = dl p X ξ θt = X ξ l p θt = X ξ ct. Thus c is an integral curve of X ξ at e defined on all of R. By maximality, θ must also be defined on all of R. To complete the proof, we must show that for any p G, if c p t is the integral curve for X ξ with c p 0 = p, then c p is also defined on all of R. But given p G, define γ : R G by t p θt = l p θt. Then certainly γ0 = p, and an identical calculation to the above shows that γ is an integral curve of X ξ. Maximality then implies that c p is defined on all of R. 4.13 Definition A one-parameter subgroup of a Lie group G is a homomorphism of Lie groups θ : R G where R is given the additive group structure. If ξ g, the one-parameter subgroup generated by ξ is the one-parameter subgroup θt that is the integral curve through e of X ξ. 4.14 Proposition There is a one-to-one correspondence between one-parameter subgroups of G and left-invariant vector fields and hence also with g. We already know that a left-invariant vector field gives rise to a one-parameter subgroup. Conversely, suppose θ : R G is a one-parameter subgroup. Define ξ = dθ d 0 Te G. Then dr