Chapter 5 Curvature on Bundles
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Connections on Bundles Md
Dhaka Univ. J. Sci. 60(2): 191-195, 2012 (July) Connections on Bundles Md. Showkat Ali, Md. Mirazul Islam, Farzana Nasrin, Md. Abu Hanif Sarkar and Tanzia Zerin Khan Department of Mathematics, University of Dhaka, Dhaka 1000, Bangladesh, Email: [email protected] Received on 25. 05. 2011.Accepted for Publication on 15. 12. 2011 Abstract This paper is a survey of the basic theory of connection on bundles. A connection on tangent bundle , is called an affine connection on an -dimensional smooth manifold . By the general discussion of affine connection on vector bundles that necessarily exists on which is compatible with tensors. I. Introduction = < , > (2) In order to differentiate sections of a vector bundle [5] or where <, > represents the pairing between and ∗. vector fields on a manifold we need to introduce a Then is a section of , called the absolute differential structure called the connection on a vector bundle. For quotient or the covariant derivative of the section along . example, an affine connection is a structure attached to a differentiable manifold so that we can differentiate its Theorem 1. A connection always exists on a vector bundle. tensor fields. We first introduce the general theorem of Proof. Choose a coordinate covering { }∈ of . Since connections on vector bundles. Then we study the tangent vector bundles are trivial locally, we may assume that there is bundle. is a -dimensional vector bundle determine local frame field for any . By the local structure of intrinsically by the differentiable structure [8] of an - connections, we need only construct a × matrix on dimensional smooth manifold . each such that the matrices satisfy II. -
LECTURE 6: FIBER BUNDLES in This Section We Will Introduce The
LECTURE 6: FIBER BUNDLES In this section we will introduce the interesting class of fibrations given by fiber bundles. Fiber bundles play an important role in many geometric contexts. For example, the Grassmaniann varieties and certain fiber bundles associated to Stiefel varieties are central in the classification of vector bundles over (nice) spaces. The fact that fiber bundles are examples of Serre fibrations follows from Theorem ?? which states that being a Serre fibration is a local property. 1. Fiber bundles and principal bundles Definition 6.1. A fiber bundle with fiber F is a map p: E ! X with the following property: every ∼ −1 point x 2 X has a neighborhood U ⊆ X for which there is a homeomorphism φU : U × F = p (U) such that the following diagram commutes in which π1 : U × F ! U is the projection on the first factor: φ U × F U / p−1(U) ∼= π1 p * U t Remark 6.2. The projection X × F ! X is an example of a fiber bundle: it is called the trivial bundle over X with fiber F . By definition, a fiber bundle is a map which is `locally' homeomorphic to a trivial bundle. The homeomorphism φU in the definition is a local trivialization of the bundle, or a trivialization over U. Let us begin with an interesting subclass. A fiber bundle whose fiber F is a discrete space is (by definition) a covering projection (with fiber F ). For example, the exponential map R ! S1 is a covering projection with fiber Z. Suppose X is a space which is path-connected and locally simply connected (in fact, the weaker condition of being semi-locally simply connected would be enough for the following construction). -
HARMONIC MAPS Contents 1. Introduction 2 1.1. Notational
HARMONIC MAPS ANDREW SANDERS Contents 1. Introduction 2 1.1. Notational conventions 2 2. Calculus on vector bundles 2 3. Basic properties of harmonic maps 7 3.1. First variation formula 7 References 10 1 2 ANDREW SANDERS 1. Introduction 1.1. Notational conventions. By a smooth manifold M we mean a second- countable Hausdorff topological space with a smooth maximal atlas. We denote the tangent bundle of M by TM and the cotangent bundle of M by T ∗M: 2. Calculus on vector bundles Given a pair of manifolds M; N and a smooth map f : M ! N; it is advantageous to consider the differential df : TM ! TN as a section df 2 Ω0(M; T ∗M ⊗ f ∗TN) ' Ω1(M; f ∗TN): There is a general for- malism for studying the calculus of differential forms with values in vector bundles equipped with a connection. This formalism allows a fairly efficient, and more coordinate-free, treatment of many calculations in the theory of harmonic maps. While this approach is somewhat abstract and obfuscates the analytic content of many expressions, it takes full advantage of the algebraic symmetries available and therefore simplifies many expressions. We will develop some of this theory now and use it freely throughout the text. The following exposition will closely fol- low [Xin96]. Let M be a smooth manifold and π : E ! M a real vector bundle on M or rank r: Throughout, we denote the space of smooth sections of E by Ω0(M; E): More generally, the space of differential p-forms with values in E is given by Ωp(M; E) := Ω0(M; ΛpT ∗M ⊗ E): Definition 2.1. -
The Language of Differential Forms
Appendix A The Language of Differential Forms This appendix—with the only exception of Sect.A.4.2—does not contain any new physical notions with respect to the previous chapters, but has the purpose of deriving and rewriting some of the previous results using a different language: the language of the so-called differential (or exterior) forms. Thanks to this language we can rewrite all equations in a more compact form, where all tensor indices referred to the diffeomorphisms of the curved space–time are “hidden” inside the variables, with great formal simplifications and benefits (especially in the context of the variational computations). The matter of this appendix is not intended to provide a complete nor a rigorous introduction to this formalism: it should be regarded only as a first, intuitive and oper- ational approach to the calculus of differential forms (also called exterior calculus, or “Cartan calculus”). The main purpose is to quickly put the reader in the position of understanding, and also independently performing, various computations typical of a geometric model of gravity. The readers interested in a more rigorous discussion of differential forms are referred, for instance, to the book [22] of the bibliography. Let us finally notice that in this appendix we will follow the conventions introduced in Chap. 12, Sect. 12.1: latin letters a, b, c,...will denote Lorentz indices in the flat tangent space, Greek letters μ, ν, α,... tensor indices in the curved manifold. For the matter fields we will always use natural units = c = 1. Also, unless otherwise stated, in the first three Sects. -
Math 704: Part 1: Principal Bundles and Connections
MATH 704: PART 1: PRINCIPAL BUNDLES AND CONNECTIONS WEIMIN CHEN Contents 1. Lie Groups 1 2. Principal Bundles 3 3. Connections and curvature 6 4. Covariant derivatives 12 References 13 1. Lie Groups A Lie group G is a smooth manifold such that the multiplication map G × G ! G, (g; h) 7! gh, and the inverse map G ! G, g 7! g−1, are smooth maps. A Lie subgroup H of G is a subgroup of G which is at the same time an embedded submanifold. A Lie group homomorphism is a group homomorphism which is a smooth map between the Lie groups. The Lie algebra, denoted by Lie(G), of a Lie group G consists of the set of left-invariant vector fields on G, i.e., Lie(G) = fX 2 X (G)j(Lg)∗X = Xg, where Lg : G ! G is the left translation Lg(h) = gh. As a vector space, Lie(G) is naturally identified with the tangent space TeG via X 7! X(e). A Lie group homomorphism naturally induces a Lie algebra homomorphism between the associated Lie algebras. Finally, the universal cover of a connected Lie group is naturally a Lie group, which is in one to one correspondence with the corresponding Lie algebras. Example 1.1. Here are some important Lie groups in geometry and topology. • GL(n; R), GL(n; C), where GL(n; C) can be naturally identified as a Lie sub- group of GL(2n; R). • SL(n; R), O(n), SO(n) = O(n) \ SL(n; R), Lie subgroups of GL(n; R). -
Minimal and Totally Geodesic Unit Sections of the Unit Sphere Bundles
Вiсник Харкiвського нацiонального унiверситету iменi В.Н. Каразiна Серiя "Математика, прикладна математика i механiка" УДК 514 № 1030, 2012, с.54–70 Minimal and totally geodesic unit sections of the unit sphere bundles. A. Yampolsky Харкiвський нацiональный унiверситет механiко-математичний факультет, кафедра геометрiї, майдан Свободи, 4, 61022, Харкiв, Україна [email protected] We consider a real vector bundle E of rank p and a unit sphere bundle E1 ⊂ E n over the Riemannian M with the Sasaki-type metric. A unit section of E1 gives rise to a submanifold in E1. We give some examples of local minimal unit sections and present a complete description of local totally geodesic unit sections of E1 in the simplest non-trivial case p = 2 and n = 2. Keywords: Sasaki metric, unit sphere bundle, totally geodesic unit section. Ямпольський О. Л., Мiнiмальнi i цiлком геодезичнi одиничнi перерiзи сферичних розшарувань. Ми розглядаємо векторне розшарування E рангу p та одиничне розшарування E1 ⊂ E над рiмановим многовидом M n з метрикою Сасакi. Ми наводимо приклади мiнiмальних перерiзiв i надаємо повне вирiшення задачi про цiлком геодезичнi перерiзи E1 у найпростiшому нетривiальному випадку, коли p = 2 i n = 2. Ключовi слова: метрика Сасакi, одиничне розшарування, цiлком геодезичний одиничний перерiз. Ямпольский А. Л., Минимальные и вполне геодезические сечения единичных сферических расслоений. Мы рассматриваем вещественное векторное расслоение E ранга p и единичное расслоение n E1 над римановым многообразием M с метрикой Сасаки. Мы приводим примеры локальных минимальных единичных сечений и даем полное решение задачи существования локальных вполне геодезических сечений E1 в простейшем нетривиальном случае, когда p = 2 и n = 2. Ключевые слова: метрика Сасаки, сферическое расслоение, вполне геодезическое единичное сечение. -
FROM DIFFERENTIATION in AFFINE SPACES to CONNECTIONS Jovana -Duretic 1. Introduction Definition 1. We Say That a Real Valued
THE TEACHING OF MATHEMATICS 2015, Vol. XVIII, 2, pp. 61–80 FROM DIFFERENTIATION IN AFFINE SPACES TO CONNECTIONS Jovana Dureti´c- Abstract. Connections and covariant derivatives are usually taught as a basic concept of differential geometry, or more precisely, of differential calculus on smooth manifolds. In this article we show that the need for covariant derivatives may arise, or at lest be motivated, even in a linear situation. We show how a generalization of the notion of a derivative of a function to a derivative of a map between affine spaces naturally leads to the notion of a connection. Covariant derivative is defined in the framework of vector bundles and connections in a way which preserves standard properties of derivatives. A special attention is paid on the role played by zero–sets of a first derivative in several contexts. MathEduc Subject Classification: I 95, G 95 MSC Subject Classification: 97 I 99, 97 G 99, 53–01 Key words and phrases: Affine space; second derivative; connection; vector bun- dle. 1. Introduction Definition 1. We say that a real valued function f :(a; b) ! R is differen- tiable at a point x0 2 (a; b) ½ R if a limit f(x) ¡ f(x ) lim 0 x!x0 x ¡ x0 0 exists. We denote this limit by f (x0) and call it a derivative of a function f at a point x0. We can write this limit in a different form, as 0 f(x0 + h) ¡ f(x0) (1) f (x0) = lim : h!0 h This expression makes sense if the codomain of a function is Rn, or more general, if the codomain is a normed vector space. -
Math 396. Covariant Derivative, Parallel Transport, and General Relativity
Math 396. Covariant derivative, parallel transport, and General Relativity 1. Motivation Let M be a smooth manifold with corners, and let (E, ∇) be a C∞ vector bundle with connection over M. Let γ : I → M be a smooth map from a nontrivial interval to M (a “path” in M); keep in mind that γ may not be injective and that its velocity may be zero at a rather arbitrary closed subset of I (so we cannot necessarily extend the standard coordinate on I near each t0 ∈ I to part of a local coordinate system on M near γ(t0)). In pseudo-Riemannian geometry E = TM and ∇ is a specific connection arising from the metric tensor (the Levi-Civita connection; see §4). A very fundamental concept is that of a (smooth) section along γ for a vector bundle on M. Before we give the official definition, we consider an example. Example 1.1. To each t0 ∈ I there is associated a velocity vector 0 ∗ γ (t0) = dγ(t0)(∂t|t0 ) ∈ Tγ(t0)(M) = (γ (TM))(t0). Hence, we get a set-theoretic section of the pullback bundle γ∗(TM) → I by assigning to each time 0 t0 the velocity vector γ (t0) at that time. This is not just a set-theoretic section, but a smooth section. Indeed, this problem is local, so pick t0 ∈ I and an open U ⊆ M containing γ(J) for an open ∞ neighborhood J ⊆ I around t0, with J and U so small that U admits a C coordinate system {x1, . , xn}. Let γi = xi ◦ γ|J ; these are smooth functions on J since γ is a smooth map from I into M. -
WHAT IS a CONNECTION, and WHAT IS IT GOOD FOR? Contents 1. Introduction 2 2. the Search for a Good Directional Derivative 3 3. F
WHAT IS A CONNECTION, AND WHAT IS IT GOOD FOR? TIMOTHY E. GOLDBERG Abstract. In the study of differentiable manifolds, there are several different objects that go by the name of \connection". I will describe some of these objects, and show how they are related to each other. The motivation for many notions of a connection is the search for a sufficiently nice directional derivative, and this will be my starting point as well. The story will by necessity include many supporting characters from differential geometry, all of whom will receive a brief but hopefully sufficient introduction. I apologize for my ungrammatical title. Contents 1. Introduction 2 2. The search for a good directional derivative 3 3. Fiber bundles and Ehresmann connections 7 4. A quick word about curvature 10 5. Principal bundles and principal bundle connections 11 6. Associated bundles 14 7. Vector bundles and Koszul connections 15 8. The tangent bundle 18 References 19 Date: 26 March 2008. 1 1. Introduction In the study of differentiable manifolds, there are several different objects that go by the name of \connection", and this has been confusing me for some time now. One solution to this dilemma was to promise myself that I would some day present a talk about connections in the Olivetti Club at Cornell University. That day has come, and this document contains my notes for this talk. In the interests of brevity, I do not include too many technical details, and instead refer the reader to some lovely references. My main references were [2], [4], and [5]. -
Weyl's Spin Connection
THE SPIN CONNECTION IN WEYL SPACE c William O. Straub, PhD Pasadena, California “The use of general connections means asking for trouble.” —Abraham Pais In addition to his seminal 1929 exposition on quantum mechanical gauge invariance1, Hermann Weyl demonstrated how the concept of a spinor (essentially a flat-space two-component quantity with non-tensor- like transformation properties) could be carried over to the curved space of general relativity. Prior to Weyl’s paper, spinors were recognized primarily as mathematical objects that transformed in the space of SU (2), but in 1928 Dirac showed that spinors were fundamental to the quantum mechanical description of spin—1/2 particles (electrons). However, the spacetime stage that Dirac’s spinors operated in was still Lorentzian. Because spinors are neither scalars nor vectors, at that time it was unclear how spinors behaved in curved spaces. Weyl’s paper provided a means for this description using tetrads (vierbeins) as the necessary link between Lorentzian space and curved Riemannian space. Weyl’selucidation of spinor behavior in curved space and his development of the so-called spin connection a ab ! band the associated spin vector ! = !ab was noteworthy, but his primary purpose was to demonstrate the profound connection between quantum mechanical gauge invariance and the electromagnetic field. Weyl’s 1929 paper served to complete his earlier (1918) theory2 in which Weyl attempted to derive electrodynamics from the geometrical structure of a generalized Riemannian manifold via a scale-invariant transformation of the metric tensor. This attempt failed, but the manifold he discovered (known as Weyl space), is still a subject of interest in theoretical physics. -
The Riemann Curvature Tensor
The Riemann Curvature Tensor Jennifer Cox May 6, 2019 Project Advisor: Dr. Jonathan Walters Abstract A tensor is a mathematical object that has applications in areas including physics, psychology, and artificial intelligence. The Riemann curvature tensor is a tool used to describe the curvature of n-dimensional spaces such as Riemannian manifolds in the field of differential geometry. The Riemann tensor plays an important role in the theories of general relativity and gravity as well as the curvature of spacetime. This paper will provide an overview of tensors and tensor operations. In particular, properties of the Riemann tensor will be examined. Calculations of the Riemann tensor for several two and three dimensional surfaces such as that of the sphere and torus will be demonstrated. The relationship between the Riemann tensor for the 2-sphere and 3-sphere will be studied, and it will be shown that these tensors satisfy the general equation of the Riemann tensor for an n-dimensional sphere. The connection between the Gaussian curvature and the Riemann curvature tensor will also be shown using Gauss's Theorem Egregium. Keywords: tensor, tensors, Riemann tensor, Riemann curvature tensor, curvature 1 Introduction Coordinate systems are the basis of analytic geometry and are necessary to solve geomet- ric problems using algebraic methods. The introduction of coordinate systems allowed for the blending of algebraic and geometric methods that eventually led to the development of calculus. Reliance on coordinate systems, however, can result in a loss of geometric insight and an unnecessary increase in the complexity of relevant expressions. Tensor calculus is an effective framework that will avoid the cons of relying on coordinate systems. -
Chapter 1 I. Fibre Bundles
Chapter 1 I. Fibre Bundles 1.1 Definitions Definition 1.1.1 Let X be a topological space and let U be an open cover of X.A { j}j∈J partition of unity relative to the cover Uj j∈J consists of a set of functions fj : X [0, 1] such that: { } → 1) f −1 (0, 1] U for all j J; j ⊂ j ∈ 2) f −1 (0, 1] is locally finite; { j }j∈J 3) f (x)=1 for all x X. j∈J j ∈ A Pnumerable cover of a topological space X is one which possesses a partition of unity. Theorem 1.1.2 Let X be Hausdorff. Then X is paracompact iff for every open cover of X there exists a partition of unity relative to . U U See MAT1300 notes for a proof. Definition 1.1.3 Let B be a topological space with chosen basepoint . A(locally trivial) fibre bundle over B consists of a map p : E B such that for all b B∗there exists an open neighbourhood U of b for which there is a homeomorphism→ φ : p−1(U)∈ p−1( ) U satisfying ′′ ′′ → ∗ × π φ = p U , where π denotes projection onto the second factor. If there is a numerable open cover◦ of B|by open sets with homeomorphisms as above then the bundle is said to be numerable. 1 If ξ is the bundle p : E B, then E and B are called respectively the total space, sometimes written E(ξ), and base space→ , sometimes written B(ξ), of ξ and F := p−1( ) is called the fibre of ξ.