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Differentiable Manifolds: Charts and Atlases That Bring Calculus to Curved Spaces

Prerequisite:Topological Spaces: What Remains of Nearness When the Metric Is Discarded、Vector Spaces and Linear Maps: From the Eight Axioms to the Rank-Nullity Theorem、Limits and Continuity: Reading ε-δ as a Contract on Error

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  • The definition of a manifold comes in two layers. First, as a topological space it must be locally homeomorphic to Rn\mathbb{R}^n; second, the maps that glue local coordinates to one another (the transition maps) must be of class CkC^k. The first layer carries the shape, the second carries the possibility of differentiating.
  • There is exactly one reason for demanding that the transition maps be CkC^k: so that the notion of differentiation defined through coordinates does not depend on the choice of coordinates. Everything in the definition follows from this single requirement.
  • The definition adds the Hausdorff condition and second countability. Neither is a consequence of the local data. Dropping them lets pathologies such as the line with two origins appear.
  • For SnS^n (stereographic projection), RPn\mathbb{RP}^n (homogeneous coordinates) and Tn=Rn/ZnT^n = \mathbb{R}^n/\mathbb{Z}^n (integer translations), the atlases can be written out completely. The transition maps are, respectively, the inversion u↦u/∣u∣2u \mapsto u/|u|^2, rational expressions, and translations.
  • The CkC^k property of functions and maps on a manifold is defined through coordinate representations, and compatibility makes it independent of the chart chosen. That composites are again CkC^k also follows from this.
  • One topological space can carry different differentiable structures (the chart t↦t3t \mapsto t^3 on R\mathbb{R}). Yet such structures may still be diffeomorphic, so “different structure” and “different manifold” are two distinct assertions.

1. Motivation: differentiating on a curved space

Section titled “1. Motivation: differentiating on a curved space”

Differentiation is local in nature. The derivative of a function ff at a point aa is determined by the behaviour of ff on arbitrarily small neighbourhoods of aa alone. Yet the differentiation taught in calculus is defined only on open subsets of Rn\mathbb{R}^n. We may wish to differentiate a temperature distribution on a sphere, or an electromagnetic field on spacetime; neither the sphere nor spacetime is an open subset of Rn\mathbb{R}^n, so the definition does not apply as it stands.

Historically, Gauss took the decisive step in his 1827 theory of surfaces. He showed that the quantity measuring how a surface curves (the Gaussian curvature) is determined by lengths measured within the surface, independently of how the surface sits inside R3\mathbb{R}^3 (the Theorema Egregium). This is a declaration that geometry can be developed from the internal data of a surface, without looking at it from outside. In 1854, in his inaugural lecture at Göttingen, Riemann extended this standpoint to arbitrary dimensions. The word he used, Mannigfaltigkeit, is our “manifold”.

Once we adopt the intrinsic standpoint, the only tool left to us is coordinates. Expressing points of a surface by longitude and latitude turns a function on the surface into a function of two variables, which we can differentiate. But longitude and latitude are only one choice. A different coordinate system yields a different function of two variables. Here the decisive question arises.

Is the property of “being differentiable”, defined through coordinates, independent of the choice of coordinates?

For it to be independent, the map linking two coordinate systems — the transition map — must itself be differentiable. Indeed, writing f∘φ−1f \circ \varphi^{-1} for the expression of ff in the coordinates φ\varphi and f∘ψ−1f \circ \psi^{-1} for its expression in the coordinates ψ\psi, the two are related by

f∘ψ−1=(f∘φ−1)∘(φ∘ψ−1).f \circ \psi^{-1} = (f \circ \varphi^{-1}) \circ (\varphi \circ \psi^{-1}).

If φ∘ψ−1\varphi \circ \psi^{-1} on the right is of class CkC^k, then the chain rule carries ”f∘φ−1f \circ \varphi^{-1} is CkC^k” over to ”f∘ψ−1f \circ \psi^{-1} is CkC^k”. The definition of a manifold is nothing but a staging of this one line. The sections below translate this intuition into definitions and verify it on representative spaces.

Spaces requiring such preparation are by no means artificial.

  • Solution sets of equations: Sn={x∈Rn+1:∣x∣=1}S^n = \{x \in \mathbb{R}^{n+1} : |x| = 1\} is not an open subset of Rn+1\mathbb{R}^{n+1}, yet near each of its points it can be described by nn coordinates.
  • Configuration spaces: the state of a double pendulum is determined by two angles, and the totality of such states is the torus T2T^2. The set of attitudes of a rigid body is identified with RP3\mathbb{RP}^3. To write equations of motion on these spaces, we must first fix the meaning of differentiation.
  • General relativity: spacetime has no preferred coordinate system (no inertial frame). Physical laws must therefore be written in a form invariant under changes of coordinates. The Jacobian matrix ∂x′μ/∂xν\partial x'^{\mu}/\partial x^{\nu} appearing in the transformation law of tensors is precisely the derivative of a transition map. The requirement that transition maps be CkC^k is the minimal premise for speaking of general covariance.

In this article we define CkC^k manifolds as a stage satisfying the requirements above, and go as far as the CkC^k property of functions and maps on them. Tangent vectors, vector fields and differential forms — the tools with which one actually differentiates on a manifold — are treated in Tangent spaces and the tangent bundle and Vector fields and differential forms.

2. Preliminaries: what we use from topology and multivariable calculus

Section titled “2. Preliminaries: what we use from topology and multivariable calculus”

Let us fix notation and hypotheses. We write N={1,2,…}\mathbb{N} = \{1, 2, \ldots\}, and points of Rn\mathbb{R}^n as u=(u1,…,un)u = (u^1, \ldots, u^n) with upper indices (the convention in manifold theory, chosen to agree with the tensor notation of later articles). Here ∣u∣|u| is the Euclidean norm.

The language of topological spaces is taken from Topological spaces: definition and basic notions and Continuous maps and homeomorphisms. In particular we use the following.

For details on the separation axioms see Separation axioms and metrizability.

For differentiation in several variables we assume Differentiation of functions of several variables and partial derivatives and use the following definition. Let Ω⊂Rn\Omega \subset \mathbb{R}^n be open and F ⁣:Ω→RmF \colon \Omega \to \mathbb{R}^m. We say FF is of class CkC^k (k∈Nk \in \mathbb{N}) when every component of FF has all partial derivatives up to order kk (partial derivatives(Definition 3.1)[多変数関数の微分と偏微分]) and all of them are continuous on Ω\Omega. Class C0C^0 means continuous, and class C∞C^\infty means of class CkC^k for every kk. When FF is C1C^1, we write DF(a)∈Rm×nDF(a) \in \mathbb{R}^{m \times n} for its derivative (Jacobian matrix) at a∈Ωa \in \Omega.

Only two properties are used in an essential way in this article.

Proposition 2.1(Locality and composition for CkC^k maps)

Let k∈N∪{∞}k \in \mathbb{N} \cup \{\infty\}.

  1. (Locality) Let Ω⊂Rn\Omega \subset \mathbb{R}^n be open and F ⁣:Ω→RmF \colon \Omega \to \mathbb{R}^m. If for every a∈Ωa \in \Omega there is an open neighbourhood Wa⊂ΩW_a \subset \Omega of aa such that F∣WaF|_{W_a} is CkC^k, then FF is CkC^k on Ω\Omega.
  2. (Composition) Let Ω⊂Rn\Omega \subset \mathbb{R}^n and Ω′⊂Rm\Omega' \subset \mathbb{R}^m be open, let F ⁣:Ω→RmF \colon \Omega \to \mathbb{R}^m be CkC^k with F(Ω)⊂Ω′F(\Omega) \subset \Omega', and let G ⁣:Ω′→RlG \colon \Omega' \to \mathbb{R}^l be CkC^k. Then G∘F ⁣:Ω→RlG \circ F \colon \Omega \to \mathbb{R}^l is CkC^k, and for k≥1k \ge 1 the chain rule D(G∘F)(a)=DG(F(a)) DF(a)D(G \circ F)(a) = DG(F(a)) \, DF(a) holds at every a∈Ωa \in \Omega.

Remark 2.2

Part 1 is immediate from the fact that partial derivatives are determined on a neighbourhood of each point. Part 2 follows from the chain rule (the chain rule(Theorem 6.1)[多変数関数の微分と偏微分]) applied inductively: higher partial derivatives can be written using products and composites of the entries of DFDF and DGDG, hence remain continuous up to order kk. For detailed proofs see Differentiation of functions of several variables and partial derivatives.

Definition 3.1(Chart (coordinate neighbourhood))

Let MM be a topological space and nn an integer with n≥0n \ge 0. A pair (U,φ)(U, \varphi) is an nn-dimensional chart (coordinate neighbourhood) of MM when

  1. UU is an open subset of MM, and
  2. φ ⁣:U→φ(U)\varphi \colon U \to \varphi(U) is a homeomorphism onto some open subset φ(U)\varphi(U) of Rn\mathbb{R}^n.

Writing the ii-th component of φ\varphi as xi ⁣:U→Rx^i \colon U \to \mathbb{R}, we call φ=(x1,…,xn)\varphi = (x^1, \ldots, x^n) a local coordinate system on UU and each xix^i a coordinate function. For p∈Up \in U, the tuple φ(p)=(x1(p),…,xn(p))\varphi(p) = (x^1(p), \ldots, x^n(p)) is called the coordinates of pp.

When every point of MM lies in the domain of some nn-dimensional chart, MM is called an nn-dimensional locally Euclidean space.

A chart is a device that identifies part of MM with an open subset of Rn\mathbb{R}^n. It corresponds to transferring a portion of the globe onto a flat map, whence the name chart. Just as no single map covers the whole Earth, a single chart cannot in general cover all of MM. So we provide several of them and require consistency on the overlaps.

When the domains of two charts overlap, the overlap carries two sets of coordinates. The map linking them is the transition map.

Definition 3.2(CkC^k compatibility)

Let k∈N∪{∞}k \in \mathbb{N} \cup \{\infty\}. Two nn-dimensional charts (U,φ)(U, \varphi) and (V,ψ)(V, \psi) of MM are CkC^k compatible when either U∩V=∅U \cap V = \emptyset, or both

ψ∘φ−1 ⁣:φ(U∩V)⟶ψ(U∩V),φ∘ψ−1 ⁣:ψ(U∩V)⟶φ(U∩V)\psi \circ \varphi^{-1} \colon \varphi(U \cap V) \longrightarrow \psi(U \cap V), \qquad \varphi \circ \psi^{-1} \colon \psi(U \cap V) \longrightarrow \varphi(U \cap V)

are of class CkC^k. These maps are called transition maps (change of coordinates).

Let us check that this definition makes sense. The set U∩VU \cap V is open in MM, and φ\varphi is a homeomorphism from UU onto φ(U)\varphi(U), so φ(U∩V)\varphi(U \cap V) is open in φ(U)\varphi(U). Since φ(U)\varphi(U) is itself open in Rn\mathbb{R}^n, the set φ(U∩V)\varphi(U \cap V) is open in Rn\mathbb{R}^n; similarly for ψ(U∩V)\psi(U \cap V). Hence ψ∘φ−1\psi \circ \varphi^{-1} is a map from an open subset of Rn\mathbb{R}^n to an open subset of Rn\mathbb{R}^n, and asking whether it is CkC^k makes sense. Note also that ψ∘φ−1\psi \circ \varphi^{-1} and φ∘ψ−1\varphi \circ \psi^{-1} are mutually inverse, so both are homeomorphisms.

MUVU ∩ Vφ(U) ⊂ ℝⁿψ(V) ⊂ ℝⁿφψψ ∘ φ⁻¹transition map
Two charts and the transition map. Viewing the same region of the manifold in two coordinate systems, the map linking them is a map between open subsets of Euclidean space, whose differentiability we can ask about.

Definition 3.3(CkC^k atlas and CkC^k structure)

Let MM be a topological space and k∈N∪{∞}k \in \mathbb{N} \cup \{\infty\}.

  1. A family A={(Uα,φα)}α∈A\mathcal{A} = \{(U_\alpha, \varphi_\alpha)\}_{\alpha \in A} of nn-dimensional charts of MM is an nn-dimensional CkC^k atlas when ⋃α∈AUα=M\bigcup_{\alpha \in A} U_\alpha = M and, for all α,β∈A\alpha, \beta \in A, the charts (Uα,φα)(U_\alpha, \varphi_\alpha) and (Uβ,φβ)(U_\beta, \varphi_\beta) are CkC^k compatible.
  2. A CkC^k atlas A\mathcal{A} is maximal when every nn-dimensional chart of MM that is CkC^k compatible with all charts of A\mathcal{A} already belongs to A\mathcal{A}.
  3. A maximal nn-dimensional CkC^k atlas is called an nn-dimensional differentiable structure of class CkC^k (CkC^k structure) on MM.

Maximality is required in order to identify different atlases that determine the same differentiable structure. For instance, as we shall see, the sphere SnS^n carries an atlas of two charts given by stereographic projection and an atlas of 2n+22n+2 charts given by graph representations over hemispheres, and these give the same notion of differentiation. Passing to maximal atlases, the two become literally the same set.

3.3. Existence and uniqueness of the maximal atlas

Section titled “3.3. Existence and uniqueness of the maximal atlas”

Writing down a maximal atlas directly is impossible in practice. The next proposition guarantees that it suffices to give one small atlas. The heart of the proof is the following lemma.

Lemma 3.4(Propagation of compatibility through an atlas)

Let A\mathcal{A} be an nn-dimensional CkC^k atlas of a topological space MM. If two nn-dimensional charts (U,φ)(U, \varphi) and (V,ψ)(V, \psi) of MM are both CkC^k compatible with every chart of A\mathcal{A}, then (U,φ)(U, \varphi) and (V,ψ)(V, \psi) are CkC^k compatible with each other.

Proof(Lemma 3.4)

If U∩V=∅U \cap V = \emptyset the claim holds by definition, so assume U∩V≠∅U \cap V \ne \emptyset. It suffices to show that ψ∘φ−1\psi \circ \varphi^{-1} is CkC^k on φ(U∩V)\varphi(U \cap V); the other direction follows by exchanging the roles of φ\varphi and ψ\psi.

By part 1 (locality) of Proposition 2.1, it is enough to prove that the map is CkC^k on a neighbourhood of each point of φ(U∩V)\varphi(U \cap V). So take an arbitrary a∈φ(U∩V)a \in \varphi(U \cap V) and put p=φ−1(a)∈U∩Vp = \varphi^{-1}(a) \in U \cap V.

Since A\mathcal{A} covers MM, there is a chart (W,χ)∈A(W, \chi) \in \mathcal{A} with p∈Wp \in W. The set U∩V∩WU \cap V \cap W is open in MM and contains pp, and φ\varphi is a homeomorphism, so φ(U∩V∩W)\varphi(U \cap V \cap W) is an open subset of Rn\mathbb{R}^n containing aa.

On this open set we have

ψ∘φ−1=(ψ∘χ−1)∘(χ∘φ−1).\psi \circ \varphi^{-1} = (\psi \circ \chi^{-1}) \circ (\chi \circ \varphi^{-1}).

Indeed, for s∈φ(U∩V∩W)s \in \varphi(U \cap V \cap W) we have q=φ−1(s)∈U∩V∩Wq = \varphi^{-1}(s) \in U \cap V \cap W and χ∘φ−1(s)=χ(q)∈χ(U∩V∩W)⊂χ(V∩W)\chi \circ \varphi^{-1}(s) = \chi(q) \in \chi(U \cap V \cap W) \subset \chi(V \cap W), so the right-hand side is defined, and its value is ψ(q)=ψ∘φ−1(s)\psi(q) = \psi \circ \varphi^{-1}(s).

Now χ∘φ−1\chi \circ \varphi^{-1} is CkC^k on φ(U∩W)\varphi(U \cap W), because by hypothesis (U,φ)(U, \varphi) is CkC^k compatible with (W,χ)∈A(W, \chi) \in \mathcal{A}. Likewise ψ∘χ−1\psi \circ \chi^{-1} is CkC^k on χ(V∩W)\chi(V \cap W), because (V,ψ)(V, \psi) is CkC^k compatible with (W,χ)(W, \chi). Hence by part 2 (composition) of Proposition 2.1, the map ψ∘φ−1\psi \circ \varphi^{-1} is CkC^k on φ(U∩V∩W)\varphi(U \cap V \cap W).

Since aa was arbitrary, locality gives that ψ∘φ−1\psi \circ \varphi^{-1} is CkC^k on all of φ(U∩V)\varphi(U \cap V).

Proposition 3.5(Existence and uniqueness of the maximal atlas)

Let MM be a topological space and A\mathcal{A} an nn-dimensional CkC^k atlas of MM. Then there is exactly one maximal nn-dimensional CkC^k atlas containing A\mathcal{A}, namely

A∗={(U,φ):(U,φ) is an n-dimensional chart of M that is Ck compatible with every chart of A}.\mathcal{A}^{*} = \{ (U, \varphi) : (U,\varphi) \text{ is an } n \text{-dimensional chart of } M \text{ that is } C^k \text{ compatible with every chart of } \mathcal{A} \}.
Proof(Proposition 3.5)

(1) A⊂A∗\mathcal{A} \subset \mathcal{A}^{*}. Since A\mathcal{A} is an atlas, any two of its charts are CkC^k compatible. Hence every chart of A\mathcal{A} satisfies the defining condition of A∗\mathcal{A}^{*}. In particular the domains of the charts of A∗\mathcal{A}^{*} cover MM.

(2) A∗\mathcal{A}^{*} is an atlas. Covering was shown in (1). If (U,φ),(V,ψ)∈A∗(U, \varphi), (V, \psi) \in \mathcal{A}^{*}, then both are CkC^k compatible with every chart of A\mathcal{A}, so by Lemma 3.4 they are CkC^k compatible with each other.

(3) A∗\mathcal{A}^{*} is maximal. Suppose an nn-dimensional chart (U,φ)(U, \varphi) is CkC^k compatible with every chart of A∗\mathcal{A}^{*}. By (1) we have A⊂A∗\mathcal{A} \subset \mathcal{A}^{*}, so in particular (U,φ)(U,\varphi) is CkC^k compatible with every chart of A\mathcal{A}. This means (U,φ)∈A∗(U, \varphi) \in \mathcal{A}^{*}.

(4) Uniqueness. Let B\mathcal{B} be a maximal CkC^k atlas with A⊂B\mathcal{A} \subset \mathcal{B}. Each chart of B\mathcal{B} is CkC^k compatible with all other charts of B\mathcal{B}, in particular with all charts of A⊂B\mathcal{A} \subset \mathcal{B}, so B⊂A∗\mathcal{B} \subset \mathcal{A}^{*}. Conversely, let (U,φ)∈A∗(U, \varphi) \in \mathcal{A}^{*} and take an arbitrary (V,ψ)∈B(V, \psi) \in \mathcal{B}. Since (V,ψ)∈B⊂A∗(V,\psi) \in \mathcal{B} \subset \mathcal{A}^{*}, both (U,φ)(U,\varphi) and (V,ψ)(V,\psi) are CkC^k compatible with every chart of A\mathcal{A}, so by Lemma 3.4 they are CkC^k compatible with each other. As (V,ψ)(V,\psi) was arbitrary, maximality of B\mathcal{B} gives (U,φ)∈B(U, \varphi) \in \mathcal{B}. Hence A∗⊂B\mathcal{A}^{*} \subset \mathcal{B}, and therefore B=A∗\mathcal{B} = \mathcal{A}^{*}.

Remark 3.6

Two practical consequences are worth recording.

First, to construct a manifold it suffices to write down one atlas. By Proposition 3.5, the CkC^k structure it determines is unique. All the examples below follow this practice.

Second, if (U,φ)(U, \varphi) belongs to a maximal atlas A\mathcal{A} and ∅≠U′⊂U\emptyset \ne U' \subset U is open, then (U′,φ∣U′)(U', \varphi|_{U'}) also belongs to A\mathcal{A}. The reason is as follows. The pair (U′,φ∣U′)(U', \varphi|_{U'}) is a chart, and its transition map with any (V,ψ)∈A(V, \psi) \in \mathcal{A} is the restriction to the open set φ(U′∩V)\varphi(U' \cap V) of the transition map between (U,φ)(U,\varphi) and (V,ψ)(V,\psi), hence is CkC^k. Maximality then puts it in A\mathcal{A}. In other words, the domain of a chart may always be shrunk, a fact we use in §6 when dealing with the CkC^k property of maps.

Note finally that if the definition is extended to k=0k = 0, then any two charts of the same dimension are automatically C0C^0 compatible (transition maps are homeomorphisms, hence continuous). So a C0C^0 structure is determined by the topology and carries no new information. Differentiable structures acquire content only for k≥1k \ge 1.

In Definition 3.3 we fixed nn from the outset by speaking of a family of nn-dimensional charts. Let us verify that this is not an unnatural restriction.

Proposition 3.7(Uniqueness of the dimension)

Let MM be a topological space, (U,φ)(U, \varphi) an nn-dimensional chart of MM and (V,ψ)(V, \psi) an mm-dimensional chart of MM, with U∩V≠∅U \cap V \ne \emptyset. Assume further that the transition maps ψ∘φ−1 ⁣:φ(U∩V)→ψ(U∩V)\psi \circ \varphi^{-1} \colon \varphi(U \cap V) \to \psi(U \cap V) and φ∘ψ−1 ⁣:ψ(U∩V)→φ(U∩V)\varphi \circ \psi^{-1} \colon \psi(U \cap V) \to \varphi(U \cap V) are both of class C1C^1. Then n=mn = m.

Proof(Proposition 3.7)

Take p∈U∩Vp \in U \cap V and put a=φ(p)∈Rna = \varphi(p) \in \mathbb{R}^n and b=ψ(p)∈Rmb = \psi(p) \in \mathbb{R}^m. As observed in §3.2, the set φ(U∩V)\varphi(U \cap V) is open in Rn\mathbb{R}^n and ψ(U∩V)\psi(U \cap V) is open in Rm\mathbb{R}^m. Put F=ψ∘φ−1F = \psi \circ \varphi^{-1} and G=φ∘ψ−1G = \varphi \circ \psi^{-1}. These are mutually inverse, so

G∘F=idφ(U∩V),F∘G=idψ(U∩V).G \circ F = \mathrm{id}_{\varphi(U \cap V)}, \qquad F \circ G = \mathrm{id}_{\psi(U \cap V)}.

By hypothesis FF and GG are both C1C^1, so applying part 2 of Proposition 2.1 (the chain rule) to the first identity at the point aa gives

DG(F(a)) DF(a)=DG(b) DF(a)=InDG(F(a)) \, DF(a) = DG(b) \, DF(a) = I_n

(we used F(a)=ψ(φ−1(a))=ψ(p)=bF(a) = \psi(\varphi^{-1}(a)) = \psi(p) = b). Similarly, applying it to the second identity at bb gives DF(G(b)) DG(b)=DF(a) DG(b)=ImDF(G(b)) \, DG(b) = DF(a)\, DG(b) = I_m.

Hence the linear maps DF(a) ⁣:Rn→RmDF(a) \colon \mathbb{R}^n \to \mathbb{R}^m and DG(b) ⁣:Rm→RnDG(b) \colon \mathbb{R}^m \to \mathbb{R}^n are mutually inverse linear isomorphisms. Isomorphic vector spaces have equal dimension (see Vector spaces and linear transformations, in particular uniqueness of the dimension(Theorem 5.5)[Vector Spaces and Linear Maps]), so n=mn = m.

Remark 3.8

Thanks to Proposition 3.7, on a space carrying an atlas of class C1C^1 or better, the dimension of a chart around each point is uniquely determined. The dimension is locally constant on MM, so if MM is connected it is constant on all of MM. For disconnected spaces some authors allow different dimensions on different components; in this article we fix nn from the start.

Note that if no differentiability of the transition maps is assumed (the C0C^0 case), the same conclusion still holds, but its proof requires Brouwer’s invariance of domain theorem, a deep result of topology. The gap between that and the C1C^1 case, which needs nothing beyond the chain rule, is wide: here we see the power of assuming a differentiable structure.

4. The definition of a differentiable manifold

Section titled “4. The definition of a differentiable manifold”

Definition 4.1(CkC^k manifold)

Let k∈N∪{∞}k \in \mathbb{N} \cup \{\infty\} and let nn be an integer with n≥0n \ge 0. A pair (M,A)(M, \mathcal{A}) is an nn-dimensional CkC^k manifold when

  1. MM is a Hausdorff topological space,
  2. MM is second countable, and
  3. A\mathcal{A} is an nn-dimensional differentiable structure of class CkC^k on MM (that is, a maximal nn-dimensional CkC^k atlas).

We call nn the dimension of MM and write dim⁡M=n\dim M = n. When k=∞k = \infty we call MM a smooth manifold (C∞C^\infty manifold). When A\mathcal{A} is clear from the context we write simply MM.

How the definition of a manifold is assembled. The topological layer and the differentiable layer are separate, and what joins them is the C^k property of the transition maps.

Condition 3 was prepared in §3. By Proposition 3.5, it is in fact enough to give a single nn-dimensional CkC^k atlas to satisfy it. The issue is with conditions 1 and 2. These do not follow from the local condition (local Euclidean-ness), as the next example shows.

Example 4.2(The line with two origins: a non-Hausdorff locally Euclidean space)

Let LL be the quotient space obtained from the disjoint union of two lines R×{0}\mathbb{R} \times \{0\} and R×{1}\mathbb{R} \times \{1\} by identifying (t,0)∼(t,1)(t, 0) \sim (t, 1) for t≠0t \ne 0. We write [t,i][t, i] for equivalence classes. Thus LL is “a line with two origins”.

Put Ui={[t,i]:t∈R}U_i = \{[t, i] : t \in \mathbb{R}\} (i=0,1)(i = 0, 1) and define φi([t,i])=t\varphi_i([t,i]) = t. Each UiU_i is open (indeed π−1(Ui)\pi^{-1}(U_i) is the union of R×{i}\mathbb{R} \times \{i\} and (R∖{0})×{1−i}(\mathbb{R}\setminus\{0\}) \times \{1-i\}, which is open), and φi\varphi_i is a homeomorphism. Since U0∪U1=LU_0 \cup U_1 = L, the family {(U0,φ0),(U1,φ1)}\{(U_0, \varphi_0), (U_1, \varphi_1)\} is a 11-dimensional atlas. The transition map is

φ1∘φ0−1 ⁣:R∖{0}→R∖{0},t↦t,\varphi_1 \circ \varphi_0^{-1} \colon \mathbb{R} \setminus \{0\} \to \mathbb{R} \setminus \{0\}, \qquad t \mapsto t,

that is, the identity, which is C∞C^\infty. So LL carries a 11-dimensional C∞C^\infty atlas, and it is second countable as well (the images of countably many open intervals form a basis).

However, LL is not Hausdorff. Consider the two points 00=[0,0]0_0 = [0,0] and 01=[0,1]0_1 = [0,1]. Every open neighbourhood of 000_0 contains φ0−1((−ε,ε))\varphi_0^{-1}((-\varepsilon, \varepsilon)) for some ε>0\varepsilon > 0, and likewise every open neighbourhood of 010_1 contains φ1−1((−δ,δ))\varphi_1^{-1}((-\delta, \delta)) for some δ>0\delta > 0. Setting ρ=min⁡(ε,δ)/2>0\rho = \min(\varepsilon, \delta)/2 > 0, the point [ρ,0]=[ρ,1][\rho, 0] = [\rho, 1] belongs to both. So 000_0 and 010_1 cannot be separated by disjoint open sets.

As a consequence, the sequence [1/j,0][1/j, 0] (j∈N)(j \in \mathbb{N}), for instance, converges both to 000_0 and to 010_1. Once limits fail to be unique, basic arguments such as uniqueness of solutions of differential equations all collapse. This is why the Hausdorff condition is built into the definition.

Remark 4.3

The reason for imposing second countability lies less in a pathology one can see immediately than in the tools one loses without it. A locally Euclidean space that is Hausdorff and second countable is paracompact, and therefore admits partitions of unity. Partitions of unity are the standard device for gluing locally defined objects (Riemannian metrics, volume elements, connections) into global ones, and they are also used to define integration on manifolds. Whitney’s embedding theorem (an nn-dimensional manifold embeds into R2n+1\mathbb{R}^{2n+1}) likewise presupposes second countability.

What happens without second countability is visible in a simple example. Take an uncountable set AA and give X=⨆α∈ARX = \bigsqcup_{\alpha \in A} \mathbb{R} (disjoint union) the disjoint union topology; then XX is Hausdorff and carries a 11-dimensional C∞C^\infty atlas, but is not second countable (see Exercise 7.1). This example is disconnected; a connected counterexample is provided by the long line, which is Hausdorff and locally Euclidean but neither second countable nor metrizable.

Some authors assume paracompactness in place of second countability. The only difference is that manifolds with uncountably many connected components are then allowed.

Example 4.4(Euclidean space and its open subsets)

(a) Rn\mathbb{R}^n itself. The single-chart family A0={(Rn,id)}\mathcal{A}_0 = \{(\mathbb{R}^n, \mathrm{id})\} is a C∞C^\infty atlas (compatibility need only be checked for (U,φ)(U,\varphi) against itself, and the transition map is the identity, hence C∞C^\infty). Since Rn\mathbb{R}^n is Hausdorff and second countable, the maximal atlas generated by A0\mathcal{A}_0 makes Rn\mathbb{R}^n an nn-dimensional C∞C^\infty manifold. This is called the standard differentiable structure on Rn\mathbb{R}^n.

(b) Open subsets of a manifold. Let (M,A)(M, \mathcal{A}) be an nn-dimensional CkC^k manifold and W⊂MW \subset M a non-empty open subset. Give WW the subspace topology; the Hausdorff condition and second countability are inherited by subspaces. Moreover A∣W={(U∩W,φ∣U∩W):(U,φ)∈A, U∩W≠∅}\mathcal{A}|_W = \{(U \cap W, \varphi|_{U \cap W}) : (U, \varphi) \in \mathcal{A},\ U \cap W \ne \emptyset\} is an nn-dimensional CkC^k atlas of WW. Indeed, U∩WU \cap W is open in WW and φ∣U∩W\varphi|_{U\cap W} is a homeomorphism onto φ(U∩W)\varphi(U \cap W); these sets cover WW; and the transition maps are restrictions to open sets of the transition maps of A\mathcal{A}, hence CkC^k. So by Proposition 3.5, WW is an nn-dimensional CkC^k manifold. It is called an open submanifold.

(c) The general linear group. The set Mn(R)M_n(\mathbb{R}) of all real n×nn \times n matrices is identified with Rn2\mathbb{R}^{n^2} by listing the entries, and is an n2n^2-dimensional C∞C^\infty manifold. The determinant det⁡ ⁣:Mn(R)→R\det \colon M_n(\mathbb{R}) \to \mathbb{R} is a polynomial in the entries, hence continuous (see Determinants and their properties), so

GL(n,R)={A∈Mn(R):det⁡A≠0}=det⁡−1(R∖{0})GL(n, \mathbb{R}) = \{A \in M_n(\mathbb{R}) : \det A \ne 0\} = {\det}^{-1}(\mathbb{R} \setminus \{0\})

is open. By (b), therefore, GL(n,R)GL(n,\mathbb{R}) is an n2n^2-dimensional C∞C^\infty manifold. This is the starting example for Lie groups and Lie algebras (the general linear group GL(n,R)(Example 3.3)[リー群とリー環]).

5. Examples: the sphere, real projective space and the torus

Section titled “5. Examples: the sphere, real projective space and the torus”

From here on we construct explicit atlases on spaces that are not open subsets of Rn\mathbb{R}^n. Throughout we take k=∞k = \infty, but the arguments are the same for any kk. We begin with an operation that builds new manifolds from old.

Proposition 5.1(Product manifolds)

Let (M,A)(M, \mathcal{A}) be an mm-dimensional CkC^k manifold and (N,B)(N, \mathcal{B}) an nn-dimensional CkC^k manifold. With the product topology, M×NM \times N becomes an (m+n)(m+n)-dimensional CkC^k manifold with the CkC^k structure generated by the atlas

A×B={(U×V, φ×ψ):(U,φ)∈A, (V,ψ)∈B},(φ×ψ)(p,q)=(φ(p),ψ(q)).\mathcal{A} \times \mathcal{B} = \{ (U \times V,\ \varphi \times \psi) : (U, \varphi) \in \mathcal{A},\ (V, \psi) \in \mathcal{B} \}, \qquad (\varphi \times \psi)(p, q) = (\varphi(p), \psi(q)).
Proof(Proposition 5.1)

The topological conditions. A product of Hausdorff spaces is Hausdorff (if (p,q)≠(p′,q′)(p,q) \ne (p',q') then the two differ in one factor, and we take the preimages of open sets separating that factor). A product of second countable spaces is second countable (if U\mathcal{U} and V\mathcal{V} are countable bases, then {B×B′:B∈U,B′∈V}\{B \times B' : B \in \mathcal{U}, B' \in \mathcal{V}\} is a countable basis).

These are charts. The set U×VU \times V is open in the product topology, and φ×ψ\varphi \times \psi is a bijection onto φ(U)×ψ(V)⊂Rm×Rn=Rm+n\varphi(U) \times \psi(V) \subset \mathbb{R}^{m} \times \mathbb{R}^{n} = \mathbb{R}^{m+n}; since φ\varphi and ψ\psi are homeomorphisms, so is φ×ψ\varphi \times \psi. The set φ(U)×ψ(V)\varphi(U) \times \psi(V) is a product of open sets, hence open in Rm+n\mathbb{R}^{m+n}. These domains cover M×NM \times N.

Compatibility. Taking (U′,φ′)∈A(U', \varphi') \in \mathcal{A} and (V′,ψ′)∈B(V', \psi') \in \mathcal{B}, we have (U×V)∩(U′×V′)=(U∩U′)×(V∩V′)(U \times V) \cap (U' \times V') = (U \cap U') \times (V \cap V'), and the transition map is

(φ′×ψ′)∘(φ×ψ)−1(u,v)=((φ′∘φ−1)(u), (ψ′∘ψ−1)(v)).(\varphi' \times \psi') \circ (\varphi \times \psi)^{-1}(u, v) = \big( (\varphi' \circ \varphi^{-1})(u),\ (\psi' \circ \psi^{-1})(v) \big).

The first component on the right is a CkC^k function of uu alone and the second a CkC^k function of vv alone, so as a function of (u,v)(u,v) all partial derivatives up to order kk exist and are continuous. Hence the map is CkC^k.

Iterating this construction, a finite product of manifolds is a manifold. In particular, once we know that the circle S1S^1 is a manifold (next subsection), the nn-dimensional torus (S1)n(S^1)^n is one too.

Example 5.2(An atlas on the sphere by stereographic projection)

Give Sn={x=(x1,…,xn+1)∈Rn+1:∣x∣=1}S^n = \{x = (x^1, \ldots, x^{n+1}) \in \mathbb{R}^{n+1} : |x| = 1\} the subspace topology from Rn+1\mathbb{R}^{n+1}. Since Rn+1\mathbb{R}^{n+1} is Hausdorff and second countable, so is SnS^n. Let N=(0,…,0,1)N = (0, \ldots, 0, 1) be the north pole and S=(0,…,0,−1)S = (0, \ldots, 0, -1) the south pole, and set

UN=Sn∖{N},φN(x)=(x1,…,xn)1−xn+1,US=Sn∖{S},φS(x)=(x1,…,xn)1+xn+1.U_N = S^n \setminus \{N\}, \quad \varphi_N(x) = \frac{(x^1, \ldots, x^n)}{1 - x^{n+1}}, \qquad U_S = S^n \setminus \{S\}, \quad \varphi_S(x) = \frac{(x^1, \ldots, x^n)}{1 + x^{n+1}}.

Geometrically φN\varphi_N takes the intersection of the line through NN and xx with the hyperplane xn+1=0x^{n+1} = 0 (stereographic projection).

φN\varphi_N is a homeomorphism. For x∈UNx \in U_N we have xn+1≠1x^{n+1} \ne 1, so the denominator never vanishes and φN\varphi_N is continuous. As a candidate for the inverse take

Φ(u)=(2u1,…,2un, ∣u∣2−1)∣u∣2+1(u∈Rn).\Phi(u) = \frac{(2u^1, \ldots, 2u^n,\ |u|^2 - 1)}{|u|^2 + 1} \qquad (u \in \mathbb{R}^n).

First, Φ(u)∈Sn\Phi(u) \in S^n. Indeed

4∣u∣2+(∣u∣2−1)2=∣u∣4+2∣u∣2+1=(∣u∣2+1)2,4|u|^2 + (|u|^2 - 1)^2 = |u|^4 + 2|u|^2 + 1 = (|u|^2+1)^2,

so ∣Φ(u)∣2=1|\Phi(u)|^2 = 1. Also the (n+1)(n+1)-st component is (∣u∣2−1)/(∣u∣2+1)≠1(|u|^2-1)/(|u|^2+1) \ne 1, so Φ(u)∈UN\Phi(u) \in U_N. Next we check φN(Φ(u))=u\varphi_N(\Phi(u)) = u. Writing ξ\xi for the (n+1)(n+1)-st component of Φ(u)\Phi(u), we have 1−ξ=2/(∣u∣2+1)1 - \xi = 2/(|u|^2+1), hence

φN(Φ(u))=2u/(∣u∣2+1)2/(∣u∣2+1)=u.\varphi_N(\Phi(u)) = \frac{2u/(|u|^2+1)}{2/(|u|^2+1)} = u .

Conversely, for x∈UNx \in U_N put u=φN(x)u = \varphi_N(x). From ∣x∣=1|x|=1,

∣u∣2=1−(xn+1)2(1−xn+1)2=1+xn+11−xn+1,∣u∣2+1=21−xn+1,∣u∣2−1=2xn+11−xn+1,|u|^2 = \frac{1 - (x^{n+1})^2}{(1 - x^{n+1})^2} = \frac{1 + x^{n+1}}{1 - x^{n+1}}, \qquad |u|^2 + 1 = \frac{2}{1 - x^{n+1}}, \qquad |u|^2 - 1 = \frac{2 x^{n+1}}{1 - x^{n+1}},

so the first nn components of Φ(u)\Phi(u) are 2u⋅(1−xn+1)/2=(x1,…,xn)2u \cdot (1-x^{n+1})/2 = (x^1, \ldots, x^n) and the (n+1)(n+1)-st is xn+1x^{n+1}; that is, Φ(u)=x\Phi(u) = x. Since Φ\Phi is a rational expression whose denominator is at least 11, it is continuous. Therefore φN ⁣:UN→Rn\varphi_N \colon U_N \to \mathbb{R}^n is a homeomorphism and (UN,φN)(U_N, \varphi_N) is an nn-dimensional chart. The same computation works for φS\varphi_S upon replacing xn+1x^{n+1} by −xn+1-x^{n+1}.

This is an atlas. Since N≠SN \ne S, we have UN∪US=SnU_N \cup U_S = S^n.

The transition map. We have UN∩US=Sn∖{N,S}U_N \cap U_S = S^n \setminus \{N, S\} and φN(UN∩US)=Rn∖{0}\varphi_N(U_N \cap U_S) = \mathbb{R}^n \setminus \{0\} (the equality φN(x)=0\varphi_N(x) = 0 holds only for x=Sx = S). For u≠0u \ne 0, using the (n+1)(n+1)-st component of Φ(u)\Phi(u) we get 1+ξ=2∣u∣2/(∣u∣2+1)1 + \xi = 2|u|^2/(|u|^2+1), hence

φS∘φN−1(u)=2u/(∣u∣2+1)2∣u∣2/(∣u∣2+1)=u∣u∣2.\varphi_S \circ \varphi_N^{-1}(u) = \frac{2u/(|u|^2+1)}{2|u|^2/(|u|^2+1)} = \frac{u}{|u|^2}.

This is a C∞C^\infty map on Rn∖{0}\mathbb{R}^n \setminus \{0\} (each component is a rational function whose denominator ∣u∣2|u|^2 does not vanish). Moreover this map is its own inverse, so φN∘φS−1\varphi_N \circ \varphi_S^{-1} is given by the same formula and is C∞C^\infty as well. Hence the two charts are C∞C^\infty compatible and SnS^n is an nn-dimensional C∞C^\infty manifold.

An atlas by graphs. Another atlas can be built. For i=1,…,n+1i = 1, \ldots, n+1 and a sign ϵ∈{+1,−1}\epsilon \in \{+1, -1\}, set

Viϵ={x∈Sn:ϵxi>0},ψiϵ(x)=(x1,…,xi^,…,xn+1)V_i^{\epsilon} = \{x \in S^n : \epsilon x^i > 0\}, \qquad \psi_i^{\epsilon}(x) = (x^1, \ldots, \widehat{x^i}, \ldots, x^{n+1})

(the hat indicates that the component is omitted). Then ψiϵ\psi_i^{\epsilon} is a homeomorphism from ViϵV_i^{\epsilon} onto the open ball Bn={u∈Rn:∣u∣<1}B^n = \{u \in \mathbb{R}^n : |u| < 1\}, with inverse the map that inserts ϵ1−∣u∣2\epsilon\sqrt{1 - |u|^2} in the ii-th slot of uu. Since some component of x∈Snx \in S^n is non-zero, these 2(n+1)2(n+1) charts cover SnS^n. A transition map inserts ϵ1−∣u∣2\epsilon\sqrt{1-|u|^2} and deletes another component; as 1−∣u∣2\sqrt{1 - |u|^2} is C∞C^\infty on BnB^n (the radicand is positive), the transition maps are C∞C^\infty.

Furthermore this atlas is C∞C^\infty compatible with the stereographic one. The map ψiϵ∘φN−1\psi_i^{\epsilon} \circ \varphi_N^{-1} is Φ\Phi with its ii-th component deleted, hence C∞C^\infty. Conversely, φN∘(ψiϵ)−1(u)\varphi_N \circ (\psi_i^{\epsilon})^{-1}(u) forms (x1,…,xn)/(1−xn+1)(x^1,\ldots,x^n)/(1 - x^{n+1}) from the point x=(ψiϵ)−1(u)x = (\psi_i^\epsilon)^{-1}(u), whose components are C∞C^\infty, and on the domain xn+1≠1x^{n+1} \ne 1; so it is C∞C^\infty. Hence by Proposition 3.5 both atlases generate the same maximal atlas. That is, either atlas yields the same differentiable structure.

5.3. Real projective space RPn\mathbb{RP}^n

Section titled “5.3. Real projective space RPn\mathbb{RP}^nRPn”

Example 5.3(An atlas on real projective space by homogeneous coordinates)

On Rn+1∖{0}\mathbb{R}^{n+1} \setminus \{0\} introduce the equivalence relation x∼y  ⟺  ∃λ∈R∖{0}, y=λxx \sim y \iff \exists \lambda \in \mathbb{R} \setminus \{0\},\ y = \lambda x, and consider the quotient space RPn=(Rn+1∖{0})/ ⁣∼\mathbb{RP}^n = (\mathbb{R}^{n+1}\setminus\{0\})/\!\sim. Write π\pi for the quotient map and π(x)=[x0:x1:⋯:xn]\pi(x) = [x^0 : x^1 : \cdots : x^n] (homogeneous coordinates; indices run from 00 to nn). We identify RPn\mathbb{RP}^n with the set of all lines through the origin of Rn+1\mathbb{R}^{n+1}.

π\pi is an open map. For an open set V⊂Rn+1∖{0}V \subset \mathbb{R}^{n+1}\setminus\{0\} we have π−1(π(V))=⋃λ≠0λV\pi^{-1}(\pi(V)) = \bigcup_{\lambda \ne 0} \lambda V. For each λ≠0\lambda \ne 0 the map x↦λxx \mapsto \lambda x is a homeomorphism, so λV\lambda V is open, hence so is the union. By the definition of the quotient topology, π(V)\pi(V) is open.

Second countability. Let U\mathcal{U} be a countable basis of Rn+1∖{0}\mathbb{R}^{n+1}\setminus\{0\}. Then {π(B):B∈U}\{\pi(B) : B \in \mathcal{U}\} is a countable family of open sets. Let us see that it is a basis. Let W⊂RPnW \subset \mathbb{RP}^n be open with [x]∈W[x] \in W; then π−1(W)\pi^{-1}(W) is an open set containing xx, so there is B∈UB \in \mathcal{U} with x∈B⊂π−1(W)x \in B \subset \pi^{-1}(W). Then [x]∈π(B)⊂π(π−1(W))=W[x] \in \pi(B) \subset \pi(\pi^{-1}(W)) = W (the last equality holds because π\pi is surjective).

The Hausdorff condition. Put R={(x,y)∈(Rn+1∖{0})2:x∼y}R = \{(x,y) \in (\mathbb{R}^{n+1}\setminus\{0\})^2 : x \sim y\}. For x,yx, y both non-zero, x∼yx \sim y is equivalent to linear dependence of xx and yy, which in turn is the vanishing of all 2×22 \times 2 minors, that is,

xiyj−xjyi=0(0≤i<j≤n).x^i y^j - x^j y^i = 0 \qquad (0 \le i < j \le n).

The left-hand sides are continuous, so RR is an intersection of finitely many closed sets, hence closed. Here we invoke a general fact: if π\pi is open and RR is closed, then the quotient space is Hausdorff. Indeed, if [x]≠[y][x] \ne [y] then (x,y)∉R(x,y) \notin R, and since RR is closed there are open sets with x∈Ax \in A, y∈By \in B and (A×B)∩R=∅(A \times B) \cap R = \emptyset. As π\pi is open, π(A)\pi(A) and π(B)\pi(B) are open sets containing [x][x] and [y][y] respectively. If π(A)∩π(B)≠∅\pi(A) \cap \pi(B) \ne \emptyset, there would be a∈Aa \in A and b∈Bb \in B with [a]=[b][a] = [b], so (a,b)∈(A×B)∩R(a, b) \in (A\times B) \cap R, a contradiction. Hence π(A)∩π(B)=∅\pi(A) \cap \pi(B) = \emptyset.

Charts. For i=0,…,ni = 0, \ldots, n set

Ui={[x]∈RPn:xi≠0},φi([x])=(x0xi,…,xi−1xi,xi+1xi,…,xnxi)∈Rn.U_i = \{[x] \in \mathbb{RP}^n : x^i \ne 0\}, \qquad \varphi_i([x]) = \left( \frac{x^0}{x^i}, \ldots, \frac{x^{i-1}}{x^i}, \frac{x^{i+1}}{x^i}, \ldots, \frac{x^n}{x^i} \right) \in \mathbb{R}^n.

Both the condition xi≠0x^i \ne 0 and the value of φi\varphi_i are invariant under rescaling x↦λxx \mapsto \lambda x, so neither depends on the representative. Since π\pi is open, Ui=π({x:xi≠0})U_i = \pi(\{x : x^i \ne 0\}) is open.

Let us write down the inverse of φi\varphi_i. For u=(u1,…,un)∈Rnu = (u^1, \ldots, u^n) \in \mathbb{R}^n, define the point of Rn+1\mathbb{R}^{n+1}

ιi(u)=(u1,…,ui, 1, ui+1,…,un)\iota_i(u) = (u^1, \ldots, u^i,\ 1,\ u^{i+1}, \ldots, u^n)

so that its ii-th component (counting from 00) equals 11. Then φi−1(u)=[ιi(u)]\varphi_i^{-1}(u) = [\iota_i(u)]. Indeed, φi([ιi(u)])\varphi_i([\iota_i(u)]) divides by the ii-th component 11 of ιi(u)\iota_i(u) and deletes that component, returning uu; conversely if xi≠0x^i \ne 0 then [x]=[x/xi]=[ιi(φi([x]))][x] = [x/x^i] = [\iota_i(\varphi_i([x]))].

The map φi\varphi_i is continuous: φi∘π\varphi_i \circ \pi is a rational map on {xi≠0}\{x^i \ne 0\}, hence continuous, and the restriction of π\pi to {xi≠0}\{x^i \ne 0\} is a quotient map onto UiU_i. And φi−1=π∘ιi\varphi_i^{-1} = \pi \circ \iota_i is continuous as a composite of continuous maps. Hence (Ui,φi)(U_i, \varphi_i) is a chart, and since every [x][x] has some xi≠0x^i \ne 0, the family {(Ui,φi)}i=0n\{(U_i, \varphi_i)\}_{i=0}^{n} covers RPn\mathbb{RP}^n.

Transition maps. The set φi(Ui∩Uj)={u∈Rn:ιi(u)j≠0}\varphi_i(U_i \cap U_j) = \{u \in \mathbb{R}^n : \iota_i(u)^j \ne 0\} is open, and on it

φj∘φi−1(u)=(ιi(u)0ιi(u)j,…, ⋅ ^,…,ιi(u)nιi(u)j)\varphi_j \circ \varphi_i^{-1}(u) = \left( \frac{\iota_i(u)^0}{\iota_i(u)^j}, \ldots, \widehat{\ \cdot\ }, \ldots, \frac{\iota_i(u)^n}{\iota_i(u)^j} \right)

(with the jj-th component omitted). Each component is a quotient of affine functions of uu whose denominator does not vanish on the domain, hence is C∞C^\infty. Therefore RPn\mathbb{RP}^n is an nn-dimensional C∞C^\infty manifold.

A concrete case (RP2\mathbb{RP}^2). Since φ0([1:u1:u2])=(u1,u2)\varphi_0([1 : u^1 : u^2]) = (u^1, u^2) and φ1([x0:x1:x2])=(x0/x1, x2/x1)\varphi_1([x^0:x^1:x^2]) = (x^0/x^1,\ x^2/x^1), on the region u1≠0u^1 \ne 0 we get

φ1∘φ0−1(u1,u2)=φ1([1:u1:u2])=(1u1, u2u1).\varphi_1 \circ \varphi_0^{-1}(u^1, u^2) = \varphi_1([1 : u^1 : u^2]) = \left( \frac{1}{u^1},\ \frac{u^2}{u^1} \right).

In the other direction φ0∘φ1−1(s,t)=φ0([s:1:t])=(1/s, t/s)\varphi_0 \circ \varphi_1^{-1}(s, t) = \varphi_0([s : 1 : t]) = (1/s,\ t/s) for s≠0s \ne 0, again C∞C^\infty.

The space RPn\mathbb{RP}^n is also identified with the sphere SnS^n with antipodal points identified. In physics it is important that RP3\mathbb{RP}^3 is identified with the space of attitudes of a rigid body (the rotation group SO(3)SO(3)).

Example 5.4(An atlas on the torus by translations)

Let Zn⊂Rn\mathbb{Z}^n \subset \mathbb{R}^n be the integer lattice, Tn=Rn/ZnT^n = \mathbb{R}^n / \mathbb{Z}^n the quotient space and π ⁣:Rn→Tn\pi \colon \mathbb{R}^n \to T^n the quotient map (π(x)=x+Zn\pi(x) = x + \mathbb{Z}^n).

π\pi is an open map. If VV is open then π−1(π(V))=⋃m∈Zn(V+m)\pi^{-1}(\pi(V)) = \bigcup_{m \in \mathbb{Z}^n}(V + m) is a union of open sets, hence open, so π(V)\pi(V) is open. Second countability follows by the same argument as in Example 5.3.

The Hausdorff condition. The map d ⁣:Rn×Rn→Rnd \colon \mathbb{R}^n \times \mathbb{R}^n \to \mathbb{R}^n, d(x,y)=y−xd(x,y) = y - x, is continuous, and Zn\mathbb{Z}^n is closed in Rn\mathbb{R}^n (its points are isolated and it has no accumulation points). Hence the relation set R=d−1(Zn)R = d^{-1}(\mathbb{Z}^n) is closed. As π\pi is open, the same argument used in Example 5.3 shows that TnT^n is Hausdorff.

Charts. Let V⊂RnV \subset \mathbb{R}^n be an open set satisfying “if x,y∈Vx, y \in V and x−y∈Znx - y \in \mathbb{Z}^n then x=yx = y” (for example, any open cube of edge length less than 11). Then π∣V ⁣:V→π(V)\pi|_V \colon V \to \pi(V) is a bijection which is continuous and open, hence a homeomorphism. So putting

ψV=(π∣V)−1 ⁣:π(V)⟶V⊂Rn,\psi_V = (\pi|_V)^{-1} \colon \pi(V) \longrightarrow V \subset \mathbb{R}^n,

the pair (π(V),ψV)(\pi(V), \psi_V) is an nn-dimensional chart. For any point π(x)\pi(x) we may take the open cube of edge 1/21/2 centred at xx, so these charts cover TnT^n.

Transition maps. Take two such sets V,WV, W and put Ω=ψV(π(V)∩π(W))⊂V\Omega = \psi_V(\pi(V) \cap \pi(W)) \subset V. Then Ω\Omega is open and the transition map is τ=ψW∘ψV−1=(π∣W)−1∘π∣Ω\tau = \psi_W \circ \psi_V^{-1} = (\pi|_W)^{-1} \circ \pi|_{\Omega}. For x∈Ωx \in \Omega we have π(τ(x))=π(x)\pi(\tau(x)) = \pi(x), hence τ(x)−x∈Zn\tau(x) - x \in \mathbb{Z}^n. The map x↦τ(x)−xx \mapsto \tau(x) - x is continuous with values in the discrete set Zn\mathbb{Z}^n, so the preimage of each m∈Znm \in \mathbb{Z}^n is an open and closed subset of Ω\Omega; therefore this map is locally constant. That is, on each connected component of Ω\Omega,

τ(x)=x+m(m∈Zn constant).\tau(x) = x + m \qquad (m \in \mathbb{Z}^n \text{ constant}).

Translations are C∞C^\infty, so the transition maps are C∞C^\infty. Hence TnT^n is an nn-dimensional C∞C^\infty manifold.

The torus TnT^n is compact, since π([0,1]n)=Tn\pi([0,1]^n) = T^n (see Compactness, in particular the continuous image of a compact set is compact(Theorem 6.1)[コンパクト性]). Moreover TnT^n is diffeomorphic to (S1)n(S^1)^n (that (S1)n(S^1)^n is a manifold follows from S1=T1S^1 = T^1 and Proposition 5.1), and the configuration space T2T^2 of the double pendulum is this space.

6. CkC^k functions and maps on a manifold

Section titled “6. CkC^kCk functions and maps on a manifold”

The purpose of defining manifolds was to speak of differentiation on them. We begin with real-valued functions.

Definition 6.1(CkC^k functions on a manifold)

Let (M,A)(M, \mathcal{A}) be an nn-dimensional CkC^k manifold and f ⁣:M→Rf \colon M \to \mathbb{R}. We say ff is of class CkC^k when for every p∈Mp \in M there is a chart (U,φ)∈A(U, \varphi) \in \mathcal{A} with p∈Up \in U whose coordinate representation

f^=f∘φ−1 ⁣:φ(U)⟶R\hat{f} = f \circ \varphi^{-1} \colon \varphi(U) \longrightarrow \mathbb{R}

is of class CkC^k. We write Ck(M)C^k(M) for the set of all CkC^k functions on MM.

The definition has the form “there exists a chart”, but in fact it is equivalent to “for every chart”. This is the return on requiring compatibility.

Lemma 6.2(Change of coordinate representation)

Let (M,A)(M, \mathcal{A}) be an nn-dimensional CkC^k manifold and f ⁣:M→Rf \colon M \to \mathbb{R}. The following are equivalent.

  1. ff is CkC^k in the sense of Definition 6.1.
  2. For every chart (V,ψ)∈A(V, \psi) \in \mathcal{A}, the map f∘ψ−1f \circ \psi^{-1} is CkC^k on ψ(V)\psi(V).
Proof(Lemma 6.2)

That 2 implies 1 is clear (for each point take any chart containing it).

We show 1 implies 2. Take an arbitrary (V,ψ)∈A(V, \psi) \in \mathcal{A}. By part 1 (locality) of Proposition 2.1, it suffices to show that f∘ψ−1f \circ \psi^{-1} is CkC^k on a neighbourhood of each point of ψ(V)\psi(V). Take s∈ψ(V)s \in \psi(V) and put p=ψ−1(s)∈Vp = \psi^{-1}(s) \in V. By hypothesis 1 there is a chart (U,φ)∈A(U, \varphi) \in \mathcal{A} with p∈Up \in U such that f∘φ−1f \circ \varphi^{-1} is CkC^k on φ(U)\varphi(U).

The set ψ(U∩V)\psi(U \cap V) is an open subset of Rn\mathbb{R}^n containing ss, and on it

f∘ψ−1=(f∘φ−1)∘(φ∘ψ−1).f \circ \psi^{-1} = (f \circ \varphi^{-1}) \circ (\varphi \circ \psi^{-1}).

Indeed, for t∈ψ(U∩V)t \in \psi(U\cap V) we have ψ−1(t)∈U∩V\psi^{-1}(t) \in U \cap V, so φ∘ψ−1(t)∈φ(U∩V)⊂φ(U)\varphi \circ \psi^{-1}(t) \in \varphi(U \cap V) \subset \varphi(U), and the value of the right-hand side is f(ψ−1(t))f(\psi^{-1}(t)).

Since (U,φ)(U,\varphi) and (V,ψ)(V,\psi) both belong to the maximal atlas A\mathcal{A}, they are CkC^k compatible, so φ∘ψ−1\varphi \circ \psi^{-1} is CkC^k on ψ(U∩V)\psi(U \cap V). By hypothesis f∘φ−1f \circ \varphi^{-1} is CkC^k on φ(U)⊃φ(U∩V)\varphi(U) \supset \varphi(U \cap V). Hence part 2 (composition) of Proposition 2.1 gives that f∘ψ−1f \circ \psi^{-1} is CkC^k on ψ(U∩V)\psi(U \cap V). As ss was arbitrary, locality gives that f∘ψ−1f\circ\psi^{-1} is CkC^k on ψ(V)\psi(V).

Definition 6.3(CkC^k maps between manifolds and diffeomorphisms)

Let (M,A)(M, \mathcal{A}) be an mm-dimensional CkC^k manifold, (N,B)(N, \mathcal{B}) an nn-dimensional CkC^k manifold, and F ⁣:M→NF \colon M \to N.

  1. FF is of class CkC^k when for every p∈Mp \in M there are charts (U,φ)∈A(U, \varphi) \in \mathcal{A} with p∈Up \in U and (V,ψ)∈B(V, \psi) \in \mathcal{B} with F(p)∈VF(p) \in V satisfying F(U)⊂VF(U) \subset V, such that the coordinate representation

    ψ∘F∘φ−1 ⁣:φ(U)⟶ψ(V)⊂Rn\psi \circ F \circ \varphi^{-1} \colon \varphi(U) \longrightarrow \psi(V) \subset \mathbb{R}^n

    is of class CkC^k.

  2. FF is a CkC^k diffeomorphism when FF is a bijection and both FF and F−1F^{-1} are CkC^k. When a CkC^k diffeomorphism from MM to NN exists, MM and NN are called diffeomorphic.

Taking N=RN = \mathbb{R} with the chart (R,id)(\mathbb{R}, \mathrm{id}), this definition agrees with Definition 6.1. Note that continuity is not assumed in the definition; it follows automatically.

Proposition 6.4(Continuity of CkC^k maps)

If F ⁣:M→NF \colon M \to N is CkC^k in the sense of Definition 6.3, then FF is continuous.

Proof(Proposition 6.4)

Take p∈Mp \in M and the charts (U,φ)(U, \varphi), (V,ψ)(V, \psi) appearing in the definition. On UU we have

F∣U=ψ−1∘(ψ∘F∘φ−1)∘φF|_U = \psi^{-1} \circ (\psi \circ F \circ \varphi^{-1}) \circ \varphi

(for q∈Uq \in U the right-hand side is ψ−1(ψ(F(q)))=F(q)\psi^{-1}(\psi(F(q))) = F(q)). Now φ\varphi is a homeomorphism, hence continuous; the middle map is CkC^k, hence continuous; and ψ−1\psi^{-1} is a homeomorphism, hence continuous. So F∣UF|_U is continuous.

Let O⊂NO \subset N be open. For the set UU associated with each pp as above, (F∣U)−1(O)=F−1(O)∩U(F|_U)^{-1}(O) = F^{-1}(O) \cap U is open in UU, hence open in MM. As pp varies these sets UU cover MM, so

F−1(O)=⋃p∈M(F−1(O)∩Up)F^{-1}(O) = \bigcup_{p \in M} \big( F^{-1}(O) \cap U_p \big)

is open, being a union of open sets. Therefore FF is continuous.

Proposition 6.5(Basic properties of CkC^k maps)

Let MM, NN, PP be CkC^k manifolds of dimensions mm, nn, ll, with differentiable structures A\mathcal{A}, B\mathcal{B}, C\mathcal{C} respectively.

  1. (Independence of charts) If F ⁣:M→NF \colon M \to N is CkC^k, then for any charts (U,φ)∈A(U, \varphi) \in \mathcal{A} and (V,ψ)∈B(V, \psi) \in \mathcal{B} with F(U)⊂VF(U) \subset V, the map ψ∘F∘φ−1\psi \circ F \circ \varphi^{-1} is CkC^k on φ(U)\varphi(U).
  2. (Composition) If F ⁣:M→NF \colon M \to N and G ⁣:N→PG \colon N \to P are both CkC^k, then G∘F ⁣:M→PG \circ F \colon M \to P is CkC^k.
Proof(Proposition 6.5)

Proof of 1. Take (U,φ)∈A(U,\varphi) \in \mathcal{A} and (V,ψ)∈B(V,\psi) \in \mathcal{B} with F(U)⊂VF(U) \subset V, take an arbitrary a∈φ(U)a \in \varphi(U) and put p=φ−1(a)p = \varphi^{-1}(a). By part 1 of Proposition 2.1, it suffices to prove that the map is CkC^k on a neighbourhood of aa.

Since FF is CkC^k, there are charts (U′,φ′)∈A(U', \varphi') \in \mathcal{A} and (V′,ψ′)∈B(V', \psi') \in \mathcal{B} with p∈U′p \in U', F(p)∈V′F(p) \in V', F(U′)⊂V′F(U') \subset V', such that ψ′∘F∘φ′−1\psi' \circ F \circ \varphi'^{-1} is CkC^k. The set W=U∩U′W = U \cap U' is open and contains pp, and for q∈Wq \in W we have F(q)∈VF(q) \in V and F(q)∈V′F(q) \in V', that is, F(W)⊂V∩V′F(W) \subset V \cap V'. The set φ(W)\varphi(W) is open and contains aa, and on it

ψ∘F∘φ−1=(ψ∘ψ′−1)∘(ψ′∘F∘φ′−1)∘(φ′∘φ−1).\psi \circ F \circ \varphi^{-1} = (\psi \circ \psi'^{-1}) \circ (\psi' \circ F \circ \varphi'^{-1}) \circ (\varphi' \circ \varphi^{-1}).

Indeed, for s∈φ(W)s \in \varphi(W) put q=φ−1(s)∈Wq = \varphi^{-1}(s) \in W; the rightmost map sends ss to φ′(q)∈φ′(W)⊂φ′(U′)\varphi'(q) \in \varphi'(W) \subset \varphi'(U'), the middle one sends this to ψ′(F(q))∈ψ′(V∩V′)\psi'(F(q)) \in \psi'(V \cap V'), and the leftmost one sends that to ψ(F(q))\psi(F(q)).

All three maps are CkC^k: the map φ′∘φ−1\varphi' \circ \varphi^{-1} because (U,φ)(U,\varphi) and (U′,φ′)(U',\varphi') both belong to the maximal atlas A\mathcal{A}, the map ψ∘ψ′−1\psi \circ \psi'^{-1} likewise by compatibility within B\mathcal{B}, and the middle one by hypothesis. Hence part 2 of Proposition 2.1 makes the composite CkC^k on φ(W)\varphi(W). As aa was arbitrary, the claim follows.

Proof of 2. Take p∈Mp \in M. Since GG is CkC^k, there are charts (V0,ψ0)∈B(V_0, \psi_0) \in \mathcal{B} and (W0,χ)∈C(W_0, \chi) \in \mathcal{C} with F(p)∈V0F(p) \in V_0, G(F(p))∈W0G(F(p)) \in W_0 and G(V0)⊂W0G(V_0) \subset W_0 such that χ∘G∘ψ0−1\chi \circ G \circ \psi_0^{-1} is CkC^k.

Next we choose a chart on the MM side. By Proposition 6.4 the map FF is continuous, so F−1(V0)F^{-1}(V_0) is an open set containing pp. Take any chart (U1,φ1)∈A(U_1, \varphi_1) \in \mathcal{A} containing pp and put U=U1∩F−1(V0)U = U_1 \cap F^{-1}(V_0), φ=φ1∣U\varphi = \varphi_1|_U; by Remark 3.6 we have (U,φ)∈A(U, \varphi) \in \mathcal{A}, and F(U)⊂V0F(U) \subset V_0.

Applying part 1 to (U,φ)(U,\varphi) and (V0,ψ0)(V_0, \psi_0), the map ψ0∘F∘φ−1\psi_0 \circ F \circ \varphi^{-1} is CkC^k on φ(U)\varphi(U). This map sends φ(U)\varphi(U) into ψ0(V0)\psi_0(V_0), and χ∘G∘ψ0−1\chi \circ G \circ \psi_0^{-1} is CkC^k on ψ0(V0)\psi_0(V_0), so by part 2 of Proposition 2.1 the map

χ∘(G∘F)∘φ−1=(χ∘G∘ψ0−1)∘(ψ0∘F∘φ−1)\chi \circ (G \circ F) \circ \varphi^{-1} = (\chi \circ G \circ \psi_0^{-1}) \circ (\psi_0 \circ F \circ \varphi^{-1})

is CkC^k on φ(U)\varphi(U). Also (G∘F)(U)⊂G(V0)⊂W0(G\circ F)(U) \subset G(V_0) \subset W_0, so (U,φ)(U,\varphi) and (W0,χ)(W_0, \chi) satisfy the condition in Definition 6.3. As pp was arbitrary, G∘FG \circ F is CkC^k.

Example 6.6(Smoothness of maps around the sphere)

(a) The inclusion ι ⁣:Sn↪Rn+1\iota \colon S^n \hookrightarrow \mathbb{R}^{n+1}. Take (Rn+1,id)(\mathbb{R}^{n+1}, \mathrm{id}) as a chart of Rn+1\mathbb{R}^{n+1} and the stereographic chart (UN,φN)(U_N, \varphi_N) of SnS^n. The condition ι(UN)⊂Rn+1\iota(U_N) \subset \mathbb{R}^{n+1} holds trivially, and the coordinate representation is exactly the map Φ\Phi of Example 5.2, namely

id∘ι∘φN−1(u)=(2u1,…,2un, ∣u∣2−1)∣u∣2+1.\mathrm{id} \circ \iota \circ \varphi_N^{-1}(u) = \frac{(2u^1, \ldots, 2u^n,\ |u|^2-1)}{|u|^2+1}.

The denominator is at least 11, so each component is a C∞C^\infty rational function on Rn\mathbb{R}^n. The same holds for (US,φS)(U_S, \varphi_S), so ι\iota is C∞C^\infty.

(b) The double cover ρ ⁣:Sn→RPn\rho \colon S^n \to \mathbb{RP}^n. Define ρ(x)=[x]\rho(x) = [x] (this makes sense since x≠0x \ne 0). For a point x∈Snx \in S^n choose ii with xi≠0x^i \ne 0, and take the graph chart (Viϵ,ψiϵ)(V_i^{\epsilon}, \psi_i^{\epsilon}) of SnS^n (with ϵ\epsilon the sign of xix^i; here indices run from 00 to nn) together with the chart (Ui,φi)(U_i, \varphi_i) of RPn\mathbb{RP}^n. If y∈Viϵy \in V_i^\epsilon then yi≠0y^i \ne 0, so ρ(Viϵ)⊂Ui\rho(V_i^\epsilon) \subset U_i. For u∈Bnu \in B^n, the ii-th component of y=(ψiϵ)−1(u)y = (\psi_i^\epsilon)^{-1}(u) is ϵ1−∣u∣2\epsilon\sqrt{1-|u|^2} and the remaining components are those of uu, so

φi∘ρ∘(ψiϵ)−1(u)=uϵ1−∣u∣2.\varphi_i \circ \rho \circ (\psi_i^{\epsilon})^{-1}(u) = \frac{u}{\epsilon\sqrt{1 - |u|^2}}.

The denominator does not vanish on BnB^n and is C∞C^\infty there, so this map is C∞C^\infty. Hence ρ\rho is C∞C^\infty.

(c) The quotient map π ⁣:Rn→Tn\pi \colon \mathbb{R}^n \to T^n. Taking the chart (π(V),ψV)(\pi(V), \psi_V) of Example 5.4, we have π(V)⊂π(V)\pi(V) \subset \pi(V) and

ψV∘π∘id−1∣V=(π∣V)−1∘π∣V=idV,\psi_V \circ \pi \circ \mathrm{id}^{-1}|_V = (\pi|_V)^{-1} \circ \pi|_V = \mathrm{id}_V,

so the coordinate representation is the identity, which is C∞C^\infty. Every point of Rn\mathbb{R}^n lies in such a VV, so π\pi is C∞C^\infty. Moreover, since the coordinate representation is the identity, π\pi maps a neighbourhood of each point C∞C^\infty-diffeomorphically onto a neighbourhood of its image (it is a local diffeomorphism).

Remark 6.7

One topological space can carry different differentiable structures. On R\mathbb{R} put h(t)=t3h(t) = t^3; since hh is a homeomorphism, both A1={(R,id)}\mathcal{A}_1 = \{(\mathbb{R}, \mathrm{id})\} and A2={(R,h)}\mathcal{A}_2 = \{(\mathbb{R}, h)\} are 11-dimensional C∞C^\infty atlases. Yet they are not C1C^1 compatible: one transition map h∘id−1=hh \circ \mathrm{id}^{-1} = h is C∞C^\infty, but the other, id∘h−1(s)=s1/3\mathrm{id} \circ h^{-1}(s) = s^{1/3}, is not differentiable at s=0s = 0. So the maximal atlases generated by A1\mathcal{A}_1 and A2\mathcal{A}_2 are different.

Even so, the two manifolds are diffeomorphic. Define F ⁣:(R,A2∗)→(R,A1∗)F \colon (\mathbb{R}, \mathcal{A}_2^{*}) \to (\mathbb{R}, \mathcal{A}_1^{*}) by F(t)=t3F(t) = t^3. Its coordinate representation is id∘F∘h−1(s)=(s1/3)3=s\mathrm{id} \circ F \circ h^{-1}(s) = (s^{1/3})^3 = s, the identity, which is C∞C^\infty; and the coordinate representation of the inverse F−1(s)=s1/3F^{-1}(s) = s^{1/3} is h∘F−1∘id−1(t)=(t1/3)3=th \circ F^{-1} \circ \mathrm{id}^{-1}(t) = (t^{1/3})^3 = t, again C∞C^\infty. In other words, “the differentiable structures differ” and “the manifolds differ” are two distinct assertions.

Whether there exist manifolds that are homeomorphic but not diffeomorphic is a deep question. In 1956 Milnor constructed 77-dimensional manifolds homeomorphic but not diffeomorphic to S7S^7 (exotic spheres). Moreover, for n≠4n \ne 4 the differentiable structure on Rn\mathbb{R}^n is known to be the standard one only (for n≥5n \ge 5 this is a 1962 result of Stallings), whereas results in 44-dimensional topology from the 1980s show that R4\mathbb{R}^4 carries uncountably many non-standard differentiable structures.

Exercise 7.1Easy

Let AA be an uncountable set and give X=⨆α∈ARαX = \bigsqcup_{\alpha \in A} \mathbb{R}_\alpha (where each Rα\mathbb{R}_\alpha is a copy of R\mathbb{R}) the disjoint union topology: a set W⊂XW \subset X is open when W∩RαW \cap \mathbb{R}_\alpha is open in Rα\mathbb{R}_\alpha for every α\alpha. Show that XX is Hausdorff and carries a 11-dimensional C∞C^\infty atlas, but is not second countable.

Solution

The Hausdorff condition. Take two distinct points p,q∈Xp, q \in X. If they lie in the same Rα\mathbb{R}_\alpha, then since R\mathbb{R} is Hausdorff they can be separated by disjoint open sets inside Rα\mathbb{R}_\alpha, and those are open in XX. If they lie in different copies Rα\mathbb{R}_\alpha and Rβ\mathbb{R}_\beta, then Rα\mathbb{R}_\alpha and Rβ\mathbb{R}_\beta themselves are disjoint open sets.

The atlas. Put Uα=RαU_\alpha = \mathbb{R}_\alpha and let φα ⁣:Uα→R\varphi_\alpha \colon U_\alpha \to \mathbb{R} be the natural identification. Each (Uα,φα)(U_\alpha, \varphi_\alpha) is a 11-dimensional chart and ⋃αUα=X\bigcup_\alpha U_\alpha = X. For α≠β\alpha \ne \beta we have Uα∩Uβ=∅U_\alpha \cap U_\beta = \emptyset, so compatibility holds automatically, and for α=β\alpha = \beta the transition map is the identity, which is C∞C^\infty. Hence {(Uα,φα)}\{(U_\alpha, \varphi_\alpha)\} is a 11-dimensional C∞C^\infty atlas.

Failure of second countability. Let U\mathcal{U} be a basis for the topology of XX. For each α∈A\alpha \in A choose a point pα∈Rαp_\alpha \in \mathbb{R}_\alpha. Since Rα\mathbb{R}_\alpha is an open set containing pαp_\alpha, the definition of a basis gives some Bα∈UB_\alpha \in \mathcal{U} with pα∈Bα⊂Rαp_\alpha \in B_\alpha \subset \mathbb{R}_\alpha. For α≠β\alpha \ne \beta the sets Bα⊂RαB_\alpha \subset \mathbb{R}_\alpha and Bβ⊂RβB_\beta \subset \mathbb{R}_\beta are disjoint and both non-empty, so Bα≠BβB_\alpha \ne B_\beta. Hence α↦Bα\alpha \mapsto B_\alpha is injective and the cardinality of U\mathcal{U} is at least that of AA, hence uncountable. Therefore no countable basis exists.

(This XX fails condition 2 of Definition 4.1, so it is not a manifold.)

Exercise 7.2Standard

Let MM and NN be CkC^k manifolds and give M×NM \times N the CkC^k structure of Proposition 5.1. Show the following.

  1. The projections prM ⁣:M×N→M\mathrm{pr}_M \colon M \times N \to M and prN ⁣:M×N→N\mathrm{pr}_N \colon M \times N \to N are both CkC^k.
  2. Let PP be a CkC^k manifold and H ⁣:P→M×NH \colon P \to M \times N. Then HH is CkC^k if and only if prM∘H\mathrm{pr}_M \circ H and prN∘H\mathrm{pr}_N \circ H are both CkC^k.
Solution

1. Take (p,q)∈M×N(p, q) \in M \times N and charts (U,φ)∈A(U,\varphi) \in \mathcal{A}, (V,ψ)∈B(V,\psi) \in \mathcal{B} with p∈Up \in U and q∈Vq \in V. For the product chart (U×V,φ×ψ)(U \times V, \varphi \times \psi) we have prM(U×V)=U⊂U\mathrm{pr}_M(U \times V) = U \subset U, and the coordinate representation is

φ∘prM∘(φ×ψ)−1(u,v)=φ(φ−1(u))=u,\varphi \circ \mathrm{pr}_M \circ (\varphi \times \psi)^{-1}(u, v) = \varphi(\varphi^{-1}(u)) = u,

that is, the projection Rm+n⊃φ(U)×ψ(V)→Rm\mathbb{R}^{m+n} \supset \varphi(U)\times\psi(V) \to \mathbb{R}^m onto the first factor. Being linear, it is C∞C^\infty and in particular CkC^k. The same applies to prN\mathrm{pr}_N.

2. If HH is CkC^k, then by 1 and part 2 (composition) of Proposition 6.5, the maps prM∘H\mathrm{pr}_M \circ H and prN∘H\mathrm{pr}_N \circ H are CkC^k.

Conversely, assume H1=prM∘HH_1 = \mathrm{pr}_M \circ H and H2=prN∘HH_2 = \mathrm{pr}_N \circ H are both CkC^k. Take r∈Pr \in P and charts (U,φ)(U,\varphi), (V,ψ)(V,\psi) with H1(r)∈UH_1(r) \in U and H2(r)∈VH_2(r) \in V. By Proposition 6.4 the maps H1H_1, H2H_2 are continuous, so H1−1(U)∩H2−1(V)H_1^{-1}(U) \cap H_2^{-1}(V) is an open set containing rr. Let (W,χ)(W, \chi) be a chart of PP containing rr, restricted to this open set (by Remark 3.6 this is again a chart). Then H1(W)⊂UH_1(W) \subset U and H2(W)⊂VH_2(W) \subset V, that is, H(W)⊂U×VH(W) \subset U \times V. The coordinate representation is

(φ×ψ)∘H∘χ−1(w)=(φ∘H1∘χ−1(w), ψ∘H2∘χ−1(w)),(\varphi \times \psi) \circ H \circ \chi^{-1}(w) = \big( \varphi \circ H_1 \circ \chi^{-1}(w),\ \psi \circ H_2 \circ \chi^{-1}(w) \big),

and by part 1 of Proposition 6.5 each component is CkC^k on χ(W)\chi(W). A vector-valued map is CkC^k exactly when each of its components is, so the whole map is CkC^k. As rr was arbitrary, HH is CkC^k.

Exercise 7.3Standard

Show that RP1\mathbb{RP}^1 and S1S^1 are diffeomorphic. Hint: identify R2\mathbb{R}^2 with C\mathbb{C} and consider F([z])=z2/∣z∣2F([z]) = z^2/|z|^2.

Solution

Identify R2∋(x0,x1)↔z=x0+ix1∈C\mathbb{R}^2 \ni (x^0, x^1) \leftrightarrow z = x^0 + i x^1 \in \mathbb{C} and define F ⁣:RP1→S1F \colon \mathbb{RP}^1 \to S^1 by F([z])=z2/∣z∣2F([z]) = z^2/|z|^2.

Well defined. For λ∈R∖{0}\lambda \in \mathbb{R} \setminus \{0\} we have (λz)2/∣λz∣2=λ2z2/(λ2∣z∣2)=z2/∣z∣2(\lambda z)^2/|\lambda z|^2 = \lambda^2 z^2/(\lambda^2 |z|^2) = z^2/|z|^2, so the value does not depend on the representative. Also ∣z2/∣z∣2∣=1|z^2/|z|^2| = 1, so the value lies in S1S^1.

Bijectivity. We may normalise ∣z∣=1|z| = 1, and then F([z])=z2F([z]) = z^2. For any w∈S1w \in S^1 there are exactly two zz with ∣z∣=1|z|=1 and z2=wz^2 = w, namely zz and −z-z, which form a single equivalence class. Hence FF is a bijection.

Smoothness. Take the chart φ0([1:u])=u\varphi_0([1 : u]) = u of RP1\mathbb{RP}^1, so that z=1+iuz = 1 + iu, and

F(φ0−1(u))=(1+iu)21+u2=1−u21+u2+i 2u1+u2,F(\varphi_0^{-1}(u)) = \frac{(1+iu)^2}{1+u^2} = \frac{1 - u^2}{1+u^2} + i\,\frac{2u}{1+u^2},

that is, the point (a,b)=((1−u2)/(1+u2), 2u/(1+u2))(a, b) = \big((1-u^2)/(1+u^2),\ 2u/(1+u^2)\big) of S1S^1. On the S1S^1 side we use the stereographic projection from the north pole (0,1)(0,1), namely φN(a,b)=a/(1−b)\varphi_N(a,b) = a/(1-b). We have F(φ0−1(u))=(0,1)F(\varphi_0^{-1}(u)) = (0,1) only when 1−u2=01 - u^2 = 0 and 2u=1+u22u = 1 + u^2, that is, only for u=1u = 1, so we restrict the domain to u≠1u \ne 1. There

1−b=1−2u1+u2=(1−u)21+u2,φN∘F∘φ0−1(u)=1−u2(1−u)2=1+u1−u,1 - b = 1 - \frac{2u}{1+u^2} = \frac{(1-u)^2}{1+u^2}, \qquad \varphi_N \circ F \circ \varphi_0^{-1}(u) = \frac{1-u^2}{(1-u)^2} = \frac{1+u}{1-u},

which is C∞C^\infty for u≠1u \ne 1. Near u=1u = 1 we replace the chart on the S1S^1 side by the stereographic projection from the south pole, φS(a,b)=a/(1+b)\varphi_S(a,b) = a/(1+b). Since 1+b=(1+u)2/(1+u2)1 + b = (1+u)^2/(1+u^2), we get φS∘F∘φ0−1(u)=(1−u)/(1+u)\varphi_S \circ F \circ \varphi_0^{-1}(u) = (1-u)/(1+u), which is C∞C^\infty for u≠−1u \ne -1. As u=−1u = -1 is not near u=1u = 1, these two charts cover the domain of φ0\varphi_0. Near the remaining point [0:1][0:1] we use the chart φ1([s:1])=s\varphi_1([s : 1]) = s and carry out the same computation with z=s+iz = s + i; again a rational expression results, so the map is C∞C^\infty. Hence FF is C∞C^\infty.

Smoothness of the inverse. The expression g(u)=(1+u)/(1−u)g(u) = (1+u)/(1-u) obtained above is a bijection from u≠1u \ne 1 onto s≠−1s \ne -1, with inverse g−1(s)=(s−1)/(s+1)g^{-1}(s) = (s-1)/(s+1). This is C∞C^\infty for s≠−1s \ne -1, and it is exactly the coordinate representation φ0∘F−1∘φN−1\varphi_0 \circ F^{-1} \circ \varphi_N^{-1}. The other pairs of charts give rational expressions in the same way, with denominators that do not vanish on the respective domains. Hence F−1F^{-1} is also C∞C^\infty, and FF is a diffeomorphism.

Exercise 7.4Hard

Let A∈GL(n,R)A \in GL(n, \mathbb{R}) and consider the quotient Rn/Λ\mathbb{R}^n/\Lambda by the lattice Λ=AZn={Am:m∈Zn}\Lambda = A\mathbb{Z}^n = \{Am : m \in \mathbb{Z}^n\}. Show that Rn/Λ\mathbb{R}^n/\Lambda is an nn-dimensional C∞C^\infty manifold and that it is diffeomorphic to Tn=Rn/ZnT^n = \mathbb{R}^n/\mathbb{Z}^n.

Solution

It is a manifold. Since AA is a linear homeomorphism, Λ=AZn\Lambda = A\mathbb{Z}^n is a discrete closed subgroup of Rn\mathbb{R}^n. In particular δ=min⁡{∣v∣:v∈Λ, v≠0}\delta = \min\{|v| : v \in \Lambda,\ v \ne 0\} exists and δ>0\delta > 0 (as Λ\Lambda is discrete and closed, only finitely many of its points lie in a bounded closed ball centred at the origin). Let πΛ ⁣:Rn→Rn/Λ\pi_\Lambda \colon \mathbb{R}^n \to \mathbb{R}^n/\Lambda be the quotient map. By the same arguments as in Example 5.4, the map πΛ\pi_\Lambda is open, Rn/Λ\mathbb{R}^n/\Lambda is second countable, and it is Hausdorff because R=d−1(Λ)R = d^{-1}(\Lambda) (with d(x,y)=y−xd(x,y) = y-x) is closed. Taking an open set VV of diameter less than δ\delta, the restriction πΛ∣V\pi_\Lambda|_V is a homeomorphism, so (πΛ(V),(πΛ∣V)−1)(\pi_\Lambda(V), (\pi_\Lambda|_V)^{-1}) is a chart, and the transition maps are translations by elements of Λ\Lambda (locally constant), hence C∞C^\infty. Therefore Rn/Λ\mathbb{R}^n/\Lambda is an nn-dimensional C∞C^\infty manifold.

They are diffeomorphic. Since x−y∈Zn  ⟺  Ax−Ay∈Λx - y \in \mathbb{Z}^n \iff Ax - Ay \in \Lambda, the map Aˉ(π(x))=πΛ(Ax)\bar{A}(\pi(x)) = \pi_\Lambda(Ax) is well defined. As AA is bijective and AZn=ΛA\mathbb{Z}^n = \Lambda, the map Aˉ\bar{A} is bijective, with inverse the map A−1‾\overline{A^{-1}} induced by A−1A^{-1}.

Let us check smoothness. Choose V⊂RnV \subset \mathbb{R}^n small enough to give a chart of TnT^n and such that A(V)A(V) has diameter less than δ\delta (such a VV exists around each point since AA is continuous). Then Aˉ(π(V))=πΛ(A(V))\bar{A}(\pi(V)) = \pi_\Lambda(A(V)), and the coordinate representation is

(πΛ∣A(V))−1∘Aˉ∘π∣V=A∣V.(\pi_\Lambda|_{A(V)})^{-1} \circ \bar{A} \circ \pi|_V = A|_V .

Indeed, for x∈Vx \in V the left-hand side takes πΛ(Ax)\pi_\Lambda(Ax) back to its representative in A(V)A(V), and since Ax∈A(V)Ax \in A(V) that value is AxAx. The linear map AA is C∞C^\infty, so Aˉ\bar{A} is C∞C^\infty. Applying the same argument to A−1A^{-1} shows that A−1‾=Aˉ−1\overline{A^{-1}} = \bar{A}^{-1} is C∞C^\infty. Hence Aˉ\bar{A} is a diffeomorphism.

(On the other hand, if Rn/Λ\mathbb{R}^n/\Lambda is given the metric induced by the standard inner product of Rn\mathbb{R}^n, differences in the shape of the lattice persist as differences of lengths and angles. That two spaces may be diffeomorphic yet metrically different is where Riemannian geometry begins.)

  • J. M. Lee, Introduction to Smooth Manifolds, 2nd edition, Springer, 2013 — Chapter 1 “Smooth Manifolds”, Chapter 2 “Smooth Maps”. Charts, atlases and maximal atlases are treated exactly as in this article.
  • Y. Matsushima, Tayōtai Nyūmon (in Japanese), Shōkabō, 1965 — the chapter on the definition of a differentiable manifold and atlases. A standard Japanese introduction.
  • Y. Matsumoto, Tayōtai no Kiso (in Japanese), University of Tokyo Press, 1988 — the chapter on the definition of a manifold and concrete examples, written carefully from the topological preliminaries onwards.
  • B. Riemann, “Über die Hypothesen, welche der Geometrie zu Grunde liegen”, Abhandlungen der Königlichen Gesellschaft der Wissenschaften zu Göttingen 13 (1868) — the 1854 inaugural lecture in which the notion of a manifold was first put forward.
  • L. A. Steen and J. A. Seebach, Jr., Counterexamples in Topology, 2nd edition, Springer, 1978 — counterexamples such as the line with two origins and the long line are collected here.
  • J. Milnor, “On manifolds homeomorphic to the 7-sphere”, Annals of Mathematics 64 (1956), 399–405 — the first construction of exotic spheres.

Appendix: Assembling a manifold from charts

Section titled “Appendix: Assembling a manifold from charts”

Putting the topology in afterwards. In this article we built manifolds by first providing a topological space MM and then placing charts on it. In practice, however, fixing the topology first can be laborious. For RPn\mathbb{RP}^n, for instance, we had to bring in 2×22 \times 2 minors just to verify that the quotient topology is Hausdorff.

In such cases the order can be reversed. Suppose we are given a set MM, a family of subsets {Uα}α∈A\{U_\alpha\}_{\alpha \in A} and injections φα ⁣:Uα→Rn\varphi_\alpha \colon U_\alpha \to \mathbb{R}^n satisfying the following five conditions. (i) Each φα(Uα)\varphi_\alpha(U_\alpha) is open in Rn\mathbb{R}^n. (ii) For all α,β\alpha, \beta, the set φα(Uα∩Uβ)\varphi_\alpha(U_\alpha \cap U_\beta) is open in Rn\mathbb{R}^n. (iii) Whenever Uα∩Uβ≠∅U_\alpha \cap U_\beta \ne \emptyset, the map φβ∘φα−1 ⁣:φα(Uα∩Uβ)→φβ(Uα∩Uβ)\varphi_\beta \circ \varphi_\alpha^{-1} \colon \varphi_\alpha(U_\alpha \cap U_\beta) \to \varphi_\beta(U_\alpha \cap U_\beta) is CkC^k. (iv) Countably many of the UαU_\alpha cover MM. (v) For any two distinct points p,qp, q of MM, either some UαU_\alpha contains both, or there are α,β\alpha, \beta with p∈Uαp \in U_\alpha, q∈Uβq \in U_\beta and Uα∩Uβ=∅U_\alpha \cap U_\beta = \emptyset.

Then there is exactly one topology together with a CkC^k structure on MM making each (Uα,φα)(U_\alpha, \varphi_\alpha) a chart. The topology is defined by taking {φα−1(B):α∈A, B⊂φα(Uα)\{\varphi_\alpha^{-1}(B) : \alpha \in A,\ B \subset \varphi_\alpha(U_\alpha) an open ball}\} as a basis; condition (iv) guarantees second countability and (v) the Hausdorff condition. A proof is in Lee’s textbook (the Smooth Manifold Chart Lemma in Chapter 1).

Why this viewpoint pays. In this form, building a manifold reduces uniformly to “lay out charts and check that the transition maps are CkC^k”. The spaces SnS^n, RPn\mathbb{RP}^n and TnT^n of §5 can all be rebuilt by this procedure. Moreover, for manifolds with boundary as treated in Stokes’ theorem (general form), and for total spaces of fibre bundles and other spaces that are naturally defined by gluing, this construction is in practice the only route available.

not audited

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