TOPOLOGY of FIBER BUNDLES by HAINAN ZHANG B.S

TOPOLOGY of FIBER BUNDLES by HAINAN ZHANG B.S

TOPOLOGY OF FIBER BUNDLES by HAINAN ZHANG B.S., Kansas State University, 2012 A THESIS submitted in partial fulfillment of the requirements for the degree MASTER OF SCIENCE Department of Mathematics College of Arts and Sciences KANSAS STATE UNIVERSITY Manhattan, Kansas 2014 Approved by: Major Professor David Auckly Copyright Hainan Zhang 2014 Abstract This report introduces the fiber bundles. It includes the definitions of fiber bundles such as vector bundles and principal bundles, with some interesting examples. Reduction of the structure groups, and covering homotopy theorem and some specific computation using obstruction classes, Cech cohomology, Stiefel-Whitney classes, and first Chern classes are included. Table of Contents Table of Contents iv List of Figuresv 1 Introduction to Fiber Bundles1 1.1 Trivial Bundles . .4 1.2 Vector Bundles . .4 1.3 Principal Bundles . .4 2 2 Example: The Bundle of Frames (π; SO3; S ; SO2) 6 3 Trivialization and Section 14 4 Reduction of the structure group 17 5 Covering Homotopy Theorem 21 5.1 Hopf-fibration: (S1 ! S3 ! S2)......................... 24 6 Obstruction Theory 25 6.1 Stiefel-Whitney Classes . 32 6.2 Chern Class . 33 7 Cechˇ Cohomology 35 Bibliography 40 iv List of Figures 6.1 Cell decomposition . 27 6.2 Graph one of 1st Stiefel Class under section sigma . 28 6.3 Graph two of 1st Stiefel Class under section sigma . 29 6.4 Graph of 1st Chern class . 31 v Chapter 1 Introduction to Fiber Bundles A fiber bundle is a space that is locally a product space, but globally may have a different topological structure. We can describe it as a continuous surjective map π : E ! B that in small neighborhood U behaves like the projection of U × F to U. Usually, we call the map π the projection of the bundle. The space E, B, F are known as total space, base space, and fiber space respectively. In general, there are two kinds of fiber bundles. The trivial bundle is B × F , the map π is the canonical projection from the product space to the first factor. In the non-trivial case, bundles will have totally different topological structures globally, such as the M¨obius strip and the Klein bottle, as well as non-trivial covering spaces. Definition 1. A fiber bundle is a structure (π; E; B; F ), where E, B, and F are topological spaces and π : E ! B is a continuous surjection satisfying a local triviality condition, which is called the bundle projection. The space E is the total space, B is called the base space of the bundle, and F is the fiber space. The locally triviality condition is that for any point x 2 B, there exists an open neighborhood 1 −1 Ux ⊂ B such that π (Ux) is homeomorphic to the product space Ux × F such that the following diagram commutes: −1 φ π (Ux) / Ux × F π proj Ux (1.1) where proj : Ux × F ! Ux is the natural projection. The set of all f(Uj; φj)g is called a local trivialization of the bundle. Thus for any p in B, the preimage π−1(p) is homeomorphic to F and is called the fiber over p. Every fiber bundle π : E ! B is an open map since the projection of products are open maps. Therefore B carries the quotient topology determined by the map π. Transition Functions If let U = fUαgα2I be a open cover of the base space, then one can construct many different local homeomorphisms by taking different open sets. Then, the nonempty interscetion of two local homeomorphisms will give two different systems for the same point in the over- lap. Transition functions give a invertible transformation of the fiber over the point in two different systems. Given a vector bundle E ! B, and a pair of neighborhood Uα and Uβ over which the bundle trivializes via two homeomorphisms, 2 −1 hα : Uα × F ! π (Uα) (1.2) −1 hβ : Uβ × F ! π (Uβ) (1.3) the composite function αβ is defined to be −1 hα ◦ hβ : Uαβ × F ! Uαβ × F (1.4) where Uαβ is Uα \ Uβ, which is well defined on the overlap by −1 hα ◦ hβ(x; v) := αβ(x; v) = (x; αβ(x)(v)) (1.5) where the map αβ : Uαβ ! Homeo(F) (1.6) sends x to (x) such that αβ(x): F ! F (1.7) is the automorphism of the fiber F with f ! αβ(x)(f) for all f 2 F . Lemma 1. αβ ◦ βγ = αγ. −1 Proof. Note αβ is defined to be hα ◦ hβ : Uαβ × F ! Uαβ × F , therefore, αβ ◦ βγ = −1 −1 −1 hα ◦ hβ ◦ hβ ◦ hγ = hα ◦ hγ = αγ. Thus, by this fact, for all x 2 Uα \ Uβ \ Uγ and f 2 F we have αβ ◦ βγ(x; f) = αγ(x; f) ) αβ(x; βγ(x)(f)) = (x; αγ(x)(f)) ) (x; αβ(x)( βγ(x)(f))) = (x; αγ(x)(f)) ) (x; αβ ◦ βγ(x)(f)) = (x; αγ(x)(f)) ) αβ ◦ βγ = αγ 3 1.1 Trivial Bundles Let E = B × F and let π : E ! B be the projection onto the first factor. Then E is a fiber bundle over B. The bundle E is not just a locally product but globally one. Thus, a trivial bundle is homeomorphic to the Cartesian product. Lemma 2. Any fiber bundle over a contractible CW-complex is trivial. Proof. Let B be a contractible CW-complex. Since B is contractible, there is a point x 2 B and a homotopy between idB and the constant map f : B ! fxg. Then, we can define ∗ ∗ ∗ ∗ the pullback with idB(E) w f (E). Therefore, E = IdB and f = B × Ex imply that 1 E w B × Ex, which is a trivial bundle. 1.2 Vector Bundles Definition 2. A vector bundle is a fiber bundle in which every fiber is a vector space. For every point in the base space B, there is an open neighborhood U and a homeomorphism h : U × Rk ! π−1(U) such that for all x 2 U, 1. (π ◦ φ)(x; v) = x for all vectors v in Rk 2. v ! φ(x; v) is an isomorphism between the vector space Rk and π−1(x), and the vector bundle over the fields are defined similarly. 1.3 Principal Bundles A principal bundle P is a mathematical object which formalizes some essential features of the Cartesian product X ×G of a topological space with a structure group G equipped with: 1. An action of G on P , analogous to (x; g)h = (x; gh) for a product space 4 2. A natural projection onto X, this is just the projection onto the first factor, (x; g) ! x Definition 3. A principle G-bundle P , where G denotes any topological group, is a fiber bundle π : P ! X together with a continuous right action P ×G ! P such that G preserves the fibers of P and acts freely and transitively on them i.e. let Px be a fiber over any point x, then 8 x0 and x1 2 Px, 9 some g 2 G such that x0g = x1 The definition implies that each fiber of the bundle is homeomorphic to the group G itself. Unlike the product space, principal bundles P lack a preferred choice of identity section. Likewise, there is no general projection onto G generalizing the projection onto the second factor, X × G ! G which exists for the Cartesian product. 5 Chapter 2 Example: The Bundle of Frames 2 (π; SO3; S ; SO2) Every rotation maps an orthonormal basis of R3 to another orthonormal basis. Like any lin- ear transformation of a finite-dimensional vector space, a rotation can always be represented by a matrix. The orthonormality condition can be expressed as RT R = I, where R is any ro- tation matrix in R3 and I is the 3×3 identity matrix. Matrices for which this property holds are called orthogonal matrices. The group of the orthogonal matrices is called orthogonal T group, and SO3 := fA 2 Mat3×3jA A = I; det(A) = 1g is the subgroup of the orthogo- nal group with determinant +1. It is called the special orthogonal group, and the det(A) = 1 2 Similiarly, SO2 is the orientation preserving orthogonal group in R . In order to carry out a rotation using the point (x, y) to be rotated is written as a vector, then multiplied by a matrix from the rotating angle θ: 2 3 2 3 2 3 x0 cos θ − sin θ x 6 7 6 7 6 7 4 5 = 4 5 4 5 (2.1) y0 sin θ cos θ y 6 where (x0, y0) are the coordinates of the point after rotation, and the formulae for x0 and y0 can be seen to be x0 = x cos θ − y sin θ y0 = x sin θ + y cos θ: Note that unlike higher dimension, the group of vector rotations in R2 is commutative. 2 Before showing the bundle structure of (π; SO3; S ; SO2), let us consider the map πe : 2 T SO3=SO2 ! S defined by πe([A]) = A · e3 where A 2 SO3 and e3 = [0; 0; 1] . Here, the equivalence class of [A] is defined via the equivalence 2 3 B 0 6 7 A ∼ A · 4 5 0 1 where B 2 SO2. We are trying to show that this map is a bijective continuous closed map, therefore, a homeomorphism. 2 3 B 0 6 7 Proof. We first show that this map is well-defined. Let [A1] = [A2], so A1 = A2 · 4 5.

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