A Crash Course on Connections

Total Page:16

File Type:pdf, Size:1020Kb

A Crash Course on Connections A CRASH COURSE ON CONNECTIONS DOMINGO TOLEDO 1. INTRODUCTION These notes are meant to give a quick view of the theory of connections and curvature for vector bundles. Basically we follow the outline of x2 of [1], see also Appendix C of [3]. The main goal is to explain that the characteristic classes of a Riemannian manifold have local expressions in terms of the metric. These notes are very preliminary. Watch for updates by looking at the date. Comments, corrections, requests for explanations, are all welcome. 2. DEFINITION OF CONNECTIONS AND CURVATURE Everything will be C1. Let E ! M be a smooth bundle over a smooth manifold. We write A0(E) for the space of smooth sections of E and Ak(E) for the space of smooth sections of the vector bundle Λk(T ∗M) ⊗ E. In other words, Ak(E) Is the space of smooth k-forms with coefficients in E. Alterna- k k 0 tively, A (E) = A (M) ⊗A0(M) A (E). 0 1 Definition 1. A connection on E is an R-linear map r : A (E) ! A (E) with the property that (1) r(fs) = df ⊗ s + frs 0 0 holds for all f 2 A (M) and for all s 2 A (E). If p 2 M and X 2 TpM, and ∗ iX : Tp M ! R denotes evaluation at X, then we write (2) rX s = (iX ⊗ id)rs; called the covariant derivative of s at p in the direction of X. The defining equation (1) becomes (3) r(fs) = (Xf)s + frX s In other words, rs puts together the covariant derivatives rX s in the direction ∗ of tangent vectors X 2 TpM into a single element of T M ⊗ E. This element is evaluated on each X 2 TpM by means of (2). The equation (1) means, in particular, that r is a first-order differential operator A0(E) ! A1(E). In other words, (rs)(p) = 0 whenever s is a section that vanishes to second order at p 2 M. A section vanishes to second order at p if and P only if it can be written as s = fisi where fi(p) = 0 and si(p) = 0. This is a Date: March 20, 2016. 1 2 DOMINGO TOLEDO coordinate-free way of saying that in any local coordinate system, s and all its first order partial derivatives vanish at p. Then using (1) we see that X (rs)(p) = (dfi(p) ⊗ si(p) + fi(p)rs(p)) = 0: In particular, this implies that (rs)(p) depends just on the value of s on a neigh- borhood of p, in other words, it is a local operator. But it says much more: Define 0 an equivalence relation on A (E) by saying s1 ∼ s2 if s1 − s2 vanishes to second order at p. Then (rs1)(p) = (rs2)(p). 2.1. Digression into jets. It can be checked that the collection of these equiva- lence classes, as we vary p, forms a vector bundle over M, called the bundle of one-jets of sections of E, denoted J 1(E). There is a well defined evaluation map 1 0 evp : J (E) ! E induced by evp : A (E) ! Ep. The latter has kernel the space of sections that vanish at p, thus the former has kernel the space of one-jets of sec- ∗ tions that vanish at p. This last space is isomorphic to Tp M ⊗ Ep. Thus the bundle J 1(E) fits into an exact sequence ev (4) T ∗M ⊗ E ! J 1(E) −! E 1 0 1 Let jp : A (E) ! J E denote the map that sends s to its equivalence class. A first order differential operator D : A0(E) ! A0(F ) (E and F vector bundles over M) is equivalent to a bundle map or zeroth-order differential operator D~ : J 1E ! F by the rule Ds = Dj~ 1s. Under this equivalence a connection is a bundle map 1 ∗ (5) r~ : J (E) ! T M ⊗ E such that rj~ T ∗M⊗E = id; in other words, a splitting of (4). 2.2. Space of connections. The point of connections is that in a general vector bundle E ! M there is no canonical way to differentiate sections. A connec- tion gives a way to differentiate sections in all directions. First we should prove existence: n (1) In the trivial bundle M × R , or better, in the trivialized bundle, since we are choosing a particular trivialization, A0(E) is the same as (A0(M))n, n vector functions M ! R , and we can define rs = ds, component- wise exterior derivative. More precisely, a section s = (f1; : : : ; fn) where fi : M ! R and we define rs by (6) rs = ds = (df1; : : : dfn) ∗ (2) The difference of two connections is a section of T M ⊗ End(E): If r1 and r2 are connections, then (r1 − r2)(fs) = f(r1 − r2)(s), thus 0 r1 − r2 is linear over A (M), in other words, is a bundle map E ! T ∗M ⊗E, in other words, a section of T ∗M ⊗End(E) = T ∗M ⊗E ⊗E∗, where E∗ is the dual bundle of E. The same computation shows that if r is a connection and A 2 A1(End(E)), then r + A is a connection. So, if a connection exists, the space of connections is an affine space for the infinite-dimensional vector space A1(M; End(E)). A CRASH COURSE ON CONNECTIONS 3 (3) Given E ! M and an open cover fUαg of M with trivializations(bundle n 0 isomorphisms) φα : EjUα ! Uα × R , define a connection rα on EjUα by 0 −1 (7) rαs = (id ⊗ φα )d(φαs) where d(φαs) is as in (6). (4) Let fλαg be a partition of unity subordinate to fUαg. Then define rs = P 0 α rαλαs In summary, connections exist, they form an affine space for the vector space A1(End(E)). 2.3. Connection one-forms. Let E ! M be a vector bundle and choose an open n cover fUαg with local trivializations φα : EjUα ! Uα × R as above. Let feig n denote the standard basis for R and let ei also denote the constant section ei of n −1 Uα × R . Let si = φα (ei). Then fs1; : : : ; sng is a collection of sections of EjUα that forms a basis of Ep for each p 2 Uα. This collection is called a frame of EjUα , or, more briefly, a local frame for E. 0 Recall the connection rα defined in (7) which corresponds to d under φα. In 0 0 terms of the frame fsig, rα is characterized by rαsi = 0 for i = 1; : : : ; n. Definition 2. Let r be a connection on E, and let rα denote its restriction to 0 0 Uα (more precisely, its restriction to A (Uα;EjUα )). Then rα = rα + θα for a 1 unique θα 2 A (Uα; End(E)), called the connection one-form of r with respect to fsig. Let us drop the subscript α and assume that we are working on EjU for which a frame fsig exists. Then we can write j j 1 (8) θ = fθi g; i; j = 1; : : : ; n; where θi 2 A (U) j 1 In other words, fθi g is a matrix of scalar one-forms representing θ 2 A (End(E)). 0 0 j Since r = r + θ and r si = 0, the θi are characterized by n X j (9) rsi = θi sj for i = 1; : : : ; n j=1 Once we have these forms we can find the covariant derivative of any section on U. Namely, any section s on U can be uniquely written as n X i 0 (10) s = ξ si for some ξi 2 A (U): i=1 Then (1) and (9) give us n n n X i i X i i X j rs = (dξ ⊗ si + ξ rsi) = (dξ ⊗ si + ξ θi sj) i=1 i=1 j=1 4 DOMINGO TOLEDO P i j Relabeling the indices in the second term i;j ξ θi sj we get the final formula n n X i X j i (11) rs = (dξ ⊗ si + ξ θjsi) i=1 j=1 for the covariant derivative of any section over U. We can go one step further in (8) and assume that U ⊂ M is the domain of a m 1 m coordinate chart ~x : U ! R where ~x = (x ; : : : ; x ). Then we can write m j X j µ j 0 (12) θi = Γi,µdx ; where Γi,µ 2 A (U); µ=1 and (11) becomes n n m X i X X i j µ (13) rs = (dξ ⊗ si + Γj,µξ dx si) i=1 j=1 µ=1 j The functions Γi,µ are usually called the Christoffel symbols. 2.4. Connections on induced bundles. Let r be a connection on E ! M, let N be a smooth manifold and let f : N ! M be a smooth map. Then we have the induced bundle (or pull-back) f ∗E ! N defined by the requirement that it be a fiber product: f ∗E −! E ## f N −! M ∗ A section s of s E is a map s : N ! E satisfying s(x) 2 Ef(x) for all x 2 N. If r is a connection on E we want to define an induced connection f ∗r on f ∗E. Since f can be quite arbitrary, it is difficult to give a short definition that works in all generality. It seems best to use local frames. Namely, let fUαg be an open cover α −1 of M so that there is a frame fsi g for each EjUα .
Recommended publications
  • When Is a Connection a Metric Connection?
    NEW ZEALAND JOURNAL OF MATHEMATICS Volume 38 (2008), 225–238 WHEN IS A CONNECTION A METRIC CONNECTION? Richard Atkins (Received April 2008) Abstract. There are two sides to this investigation: first, the determination of the integrability conditions that ensure the existence of a local parallel metric in the neighbourhood of a given point and second, the characterization of the topological obstruction to a globally defined parallel metric. The local problem has been previously solved by means of constructing a derived flag. Herein we continue the inquiry to the global aspect, which is formulated in terms of the cohomology of the constant sheaf of sections in the general linear group. 1. Introduction A connection on a manifold is a type of differentiation that acts on vector fields, differential forms and tensor products of these objects. Its importance lies in the fact that given a piecewise continuous curve connecting two points on the manifold, the connection defines a linear isomorphism between the respective tangent spaces at these points. Another fundamental concept in the study of differential geometry is that of a metric, which provides a measure of distance on the manifold. It is well known that a metric uniquely determines a Levi-Civita connection: a symmetric connection for which the metric is parallel. Not all connections are derived from a metric and so it is natural to ask, for a symmetric connection, if there exists a parallel metric, that is, whether the connection is a Levi-Civita connection. More generally, a connection on a manifold M, symmetric or not, is said to be metric if there exists a parallel metric defined on M.
    [Show full text]
  • A Mathematical Derivation of the General Relativistic Schwarzschild
    A Mathematical Derivation of the General Relativistic Schwarzschild Metric An Honors thesis presented to the faculty of the Departments of Physics and Mathematics East Tennessee State University In partial fulfillment of the requirements for the Honors Scholar and Honors-in-Discipline Programs for a Bachelor of Science in Physics and Mathematics by David Simpson April 2007 Robert Gardner, Ph.D. Mark Giroux, Ph.D. Keywords: differential geometry, general relativity, Schwarzschild metric, black holes ABSTRACT The Mathematical Derivation of the General Relativistic Schwarzschild Metric by David Simpson We briefly discuss some underlying principles of special and general relativity with the focus on a more geometric interpretation. We outline Einstein’s Equations which describes the geometry of spacetime due to the influence of mass, and from there derive the Schwarzschild metric. The metric relies on the curvature of spacetime to provide a means of measuring invariant spacetime intervals around an isolated, static, and spherically symmetric mass M, which could represent a star or a black hole. In the derivation, we suggest a concise mathematical line of reasoning to evaluate the large number of cumbersome equations involved which was not found elsewhere in our survey of the literature. 2 CONTENTS ABSTRACT ................................. 2 1 Introduction to Relativity ...................... 4 1.1 Minkowski Space ....................... 6 1.2 What is a black hole? ..................... 11 1.3 Geodesics and Christoffel Symbols ............. 14 2 Einstein’s Field Equations and Requirements for a Solution .17 2.1 Einstein’s Field Equations .................. 20 3 Derivation of the Schwarzschild Metric .............. 21 3.1 Evaluation of the Christoffel Symbols .......... 25 3.2 Ricci Tensor Components .................
    [Show full text]
  • Lecture 24/25: Riemannian Metrics
    Lecture 24/25: Riemannian metrics An inner product on Rn allows us to do the following: Given two curves intersecting at a point x Rn,onecandeterminetheanglebetweentheir tangents: ∈ cos θ = u, v / u v . | || | On a general manifold, we would again like to have an inner product on each TpM.Theniftwocurvesintersectatapointp,onecanmeasuretheangle between them. Of course, there are other geometric invariants that arise out of this structure. 1. Riemannian and Hermitian metrics Definition 24.2. A Riemannian metric on a vector bundle E is a section g Γ(Hom(E E,R)) ∈ ⊗ such that g is symmetric and positive definite. A Riemannian manifold is a manifold together with a choice of Riemannian metric on its tangent bundle. Chit-chat 24.3. A section of Hom(E E,R)isasmoothchoiceofalinear map ⊗ gp : Ep Ep R ⊗ → at every point p.Thatg is symmetric means that for every u, v E ,wehave ∈ p gp(u, v)=gp(v, u). That g is positive definite means that g (v, v) 0 p ≥ for all v E ,andequalityholdsifandonlyifv =0 E . ∈ p ∈ p Chit-chat 24.4. As usual, one can try to understand g in local coordinates. If one chooses a trivializing set of linearly independent sections si ,oneob- tains a matrix of functions { } gij = gp((si)p, (sj)p). By symmetry of g,thisisasymmetricmatrix. 85 n Example 24.5. T R is trivial. Let gij = δij be the constant matrix of functions, so that gij(p)=I is the identity matrix for every point. Then on n n every fiber, g defines the usual inner product on TpR ∼= R .
    [Show full text]
  • Laplacians in Geometric Analysis
    LAPLACIANS IN GEOMETRIC ANALYSIS Syafiq Johar syafi[email protected] Contents 1 Trace Laplacian 1 1.1 Connections on Vector Bundles . .1 1.2 Local and Explicit Expressions . .2 1.3 Second Covariant Derivative . .3 1.4 Curvatures on Vector Bundles . .4 1.5 Trace Laplacian . .5 2 Harmonic Functions 6 2.1 Gradient and Divergence Operators . .7 2.2 Laplace-Beltrami Operator . .7 2.3 Harmonic Functions . .8 2.4 Harmonic Maps . .8 3 Hodge Laplacian 9 3.1 Exterior Derivatives . .9 3.2 Hodge Duals . 10 3.3 Hodge Laplacian . 12 4 Hodge Decomposition 13 4.1 De Rham Cohomology . 13 4.2 Hodge Decomposition Theorem . 14 5 Weitzenb¨ock and B¨ochner Formulas 15 5.1 Weitzenb¨ock Formula . 15 5.1.1 0-forms . 15 5.1.2 k-forms . 15 5.2 B¨ochner Formula . 17 1 Trace Laplacian In this section, we are going to present a notion of Laplacian that is regularly used in differential geometry, namely the trace Laplacian (also called the rough Laplacian or connection Laplacian). We recall the definition of connection on vector bundles which allows us to take the directional derivative of vector bundles. 1.1 Connections on Vector Bundles Definition 1.1 (Connection). Let M be a differentiable manifold and E a vector bundle over M. A connection or covariant derivative at a point p 2 M is a map D : Γ(E) ! Γ(T ∗M ⊗ E) 1 with the properties for any V; W 2 TpM; σ; τ 2 Γ(E) and f 2 C (M), we have that DV σ 2 Ep with the following properties: 1.
    [Show full text]
  • 2. Chern Connections and Chern Curvatures1
    1 2. Chern connections and Chern curvatures1 Let V be a complex vector space with dimC V = n. A hermitian metric h on V is h : V £ V ¡¡! C such that h(av; bu) = abh(v; u) h(a1v1 + a2v2; u) = a1h(v1; u) + a2h(v2; u) h(v; u) = h(u; v) h(u; u) > 0; u 6= 0 where v; v1; v2; u 2 V and a; b; a1; a2 2 C. If we ¯x a basis feig of V , and set hij = h(ei; ej) then ¤ ¤ ¤ ¤ h = hijei ­ ej 2 V ­ V ¤ ¤ ¤ ¤ where ei 2 V is the dual of ei and ei 2 V is the conjugate dual of ei, i.e. X ¤ ei ( ajej) = ai It is obvious that (hij) is a hermitian positive matrix. De¯nition 0.1. A complex vector bundle E is said to be hermitian if there is a positive de¯nite hermitian tensor h on E. r Let ' : EjU ¡¡! U £ C be a trivilization and e = (e1; ¢ ¢ ¢ ; er) be the corresponding frame. The r hermitian metric h is represented by a positive hermitian matrix (hij) 2 ¡(­; EndC ) such that hei(x); ej(x)i = hij(x); x 2 U Then hermitian metric on the chart (U; ') could be written as X ¤ ¤ h = hijei ­ ej For example, there are two charts (U; ') and (V; Ã). We set g = à ± '¡1 :(U \ V ) £ Cr ¡¡! (U \ V ) £ Cr and g is represented by matrix (gij). On U \ V , we have X X X ¡1 ¡1 ¡1 ¡1 ¡1 ei(x) = ' (x; "i) = à ± à ± ' (x; "i) = à (x; gij"j) = gijà (x; "j) = gije~j(x) j j For the metric X ~ hij = hei(x); ej(x)i = hgike~k(x); gjle~l(x)i = gikhklgjl k;l that is h = g ¢ h~ ¢ g¤ 12008.04.30 If there are some errors, please contact to: [email protected] 2 Example 0.2 (Fubini-Study metric on holomorphic tangent bundle T 1;0Pn).
    [Show full text]
  • Kähler Manifolds, Ricci Curvature, and Hyperkähler Metrics
    K¨ahlermanifolds, Ricci curvature, and hyperk¨ahler metrics Jeff A. Viaclovsky June 25-29, 2018 Contents 1 Lecture 1 3 1.1 The operators @ and @ ..........................4 1.2 Hermitian and K¨ahlermetrics . .5 2 Lecture 2 7 2.1 Complex tensor notation . .7 2.2 The musical isomorphisms . .8 2.3 Trace . 10 2.4 Determinant . 11 3 Lecture 3 11 3.1 Christoffel symbols of a K¨ahler metric . 11 3.2 Curvature of a Riemannian metric . 12 3.3 Curvature of a K¨ahlermetric . 14 3.4 The Ricci form . 15 4 Lecture 4 17 4.1 Line bundles and divisors . 17 4.2 Hermitian metrics on line bundles . 18 5 Lecture 5 21 5.1 Positivity of a line bundle . 21 5.2 The Laplacian on a K¨ahlermanifold . 22 5.3 Vanishing theorems . 25 6 Lecture 6 25 6.1 K¨ahlerclass and @@-Lemma . 25 6.2 Yau's Theorem . 27 6.3 The @ operator on holomorphic vector bundles . 29 1 7 Lecture 7 30 7.1 Holomorphic vector fields . 30 7.2 Serre duality . 32 8 Lecture 8 34 8.1 Kodaira vanishing theorem . 34 8.2 Complex projective space . 36 8.3 Line bundles on complex projective space . 37 8.4 Adjunction formula . 38 8.5 del Pezzo surfaces . 38 9 Lecture 9 40 9.1 Hirzebruch Signature Theorem . 40 9.2 Representations of U(2) . 42 9.3 Examples . 44 2 1 Lecture 1 We will assume a basic familiarity with complex manifolds, and only do a brief review today. Let M be a manifold of real dimension 2n, and an endomorphism J : TM ! TM satisfying J 2 = −Id.
    [Show full text]
  • Riemannian Geometry and Multilinear Tensors with Vector Fields on Manifolds Md
    International Journal of Scientific & Engineering Research, Volume 5, Issue 9, September-2014 157 ISSN 2229-5518 Riemannian Geometry and Multilinear Tensors with Vector Fields on Manifolds Md. Abdul Halim Sajal Saha Md Shafiqul Islam Abstract-In the paper some aspects of Riemannian manifolds, pseudo-Riemannian manifolds, Lorentz manifolds, Riemannian metrics, affine connections, parallel transport, curvature tensors, torsion tensors, killing vector fields, conformal killing vector fields are focused. The purpose of this paper is to develop the theory of manifolds equipped with Riemannian metric. I have developed some theorems on torsion and Riemannian curvature tensors using affine connection. A Theorem 1.20 named “Fundamental Theorem of Pseudo-Riemannian Geometry” has been established on Riemannian geometry using tensors with metric. The main tools used in the theorem of pseudo Riemannian are tensors fields defined on a Riemannian manifold. Keywords: Riemannian manifolds, pseudo-Riemannian manifolds, Lorentz manifolds, Riemannian metrics, affine connections, parallel transport, curvature tensors, torsion tensors, killing vector fields, conformal killing vector fields. —————————— —————————— I. Introduction (c) { } is a family of open sets which covers , that is, 푖 = . Riemannian manifold is a pair ( , g) consisting of smooth 푈 푀 manifold and Riemannian metric g. A manifold may carry a (d) ⋃ is푈 푖푖 a homeomorphism푀 from onto an open subset of 푀 ′ further structure if it is endowed with a metric tensor, which is a 푖 . 푖 푖 휑 푈 푈 natural generation푀 of the inner product between two vectors in 푛 ℝ to an arbitrary manifold. Riemannian metrics, affine (e) Given and such that , the map = connections,푛 parallel transport, curvature tensors, torsion tensors, ( ( ) killingℝ vector fields and conformal killing vector fields play from푖 푗 ) to 푖 푗 is infinitely푖푗 −1 푈 푈 푈 ∩ 푈 ≠ ∅ 휓 important role to develop the theorem of Riemannian manifolds.
    [Show full text]
  • 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.
    [Show full text]
  • General Relativity Fall 2019 Lecture 11: the Riemann Tensor
    General Relativity Fall 2019 Lecture 11: The Riemann tensor Yacine Ali-Ha¨ımoud October 8th 2019 The Riemann tensor quantifies the curvature of spacetime, as we will see in this lecture and the next. RIEMANN TENSOR: BASIC PROPERTIES α γ Definition { Given any vector field V , r[αrβ]V is a tensor field. Let us compute its components in some coordinate system: σ σ λ σ σ λ r[µrν]V = @[µ(rν]V ) − Γ[µν]rλV + Γλ[µrν]V σ σ λ σ λ λ ρ = @[µ(@ν]V + Γν]λV ) + Γλ[µ @ν]V + Γν]ρV 1 = @ Γσ + Γσ Γρ V λ ≡ Rσ V λ; (1) [µ ν]λ ρ[µ ν]λ 2 λµν where all partial derivatives of V µ cancel out after antisymmetrization. σ Since the left-hand side is a tensor field and V is a vector field, we conclude that R λµν is a tensor field as well { this is the tensor division theorem, which I encourage you to think about on your own. You can also check that explicitly from the transformation law of Christoffel symbols. This is the Riemann tensor, which measures the non-commutation of second derivatives of vector fields { remember that second derivatives of scalar fields do commute, by assumption. It is completely determined by the metric, and is linear in its second derivatives. Expression in LICS { In a LICS the Christoffel symbols vanish but not their derivatives. Let us compute the latter: 1 1 @ Γσ = @ gσδ (@ g + @ g − @ g ) = ησδ (@ @ g + @ @ g − @ @ g ) ; (2) µ νλ 2 µ ν λδ λ νδ δ νλ 2 µ ν λδ µ λ νδ µ δ νλ since the first derivatives of the metric components (thus of its inverse as well) vanish in a LICS.
    [Show full text]
  • Solving the Geodesic Equation
    Solving the Geodesic Equation Jeremy Atkins December 12, 2018 Abstract We find the general form of the geodesic equation and discuss the closed form relation to find Christoffel symbols. We then show how to use metric independence to find Killing vector fields, which allow us to solve the geodesic equation when there are helpful symmetries. We also discuss a more general way to find Killing vector fields, and some of their properties as a Lie algebra. 1 The Variational Method We will exploit the following variational principle to characterize motion in general relativity: The world line of a free test particle between two timelike separated points extremizes the proper time between them. where a test particle is one that is not a significant source of spacetime cur- vature, and a free particles is one that is only under the influence of curved spacetime. Similarly to classical Lagrangian mechanics, we can use this to de- duce the equations of motion for a metric. The proper time along a timeline worldline between point A and point B for the metric gµν is given by Z B Z B µ ν 1=2 τAB = dτ = (−gµν (x)dx dx ) (1) A A using the Einstein summation notation, and µ, ν = 0; 1; 2; 3. We can parame- terize the four coordinates with the parameter σ where σ = 0 at A and σ = 1 at B. This gives us the following equation for the proper time: Z 1 dxµ dxν 1=2 τAB = dσ −gµν (x) (2) 0 dσ dσ We can treat the integrand as a Lagrangian, dxµ dxν 1=2 L = −gµν (x) (3) dσ dσ and it's clear that the world lines extremizing proper time are those that satisfy the Euler-Lagrange equation: @L d @L − = 0 (4) @xµ dσ @(dxµ/dσ) 1 These four equations together give the equation for the worldline extremizing the proper time.
    [Show full text]
  • A Geodesic Connection in Fréchet Geometry
    A geodesic connection in Fr´echet Geometry Ali Suri Abstract. In this paper first we propose a formula to lift a connection on M to its higher order tangent bundles T rM, r 2 N. More precisely, for a given connection r on T rM, r 2 N [ f0g, we construct the connection rc on T r+1M. Setting rci = rci−1 c, we show that rc1 = lim rci exists − and it is a connection on the Fr´echet manifold T 1M = lim T iM and the − geodesics with respect to rc1 exist. In the next step, we will consider a Riemannian manifold (M; g) with its Levi-Civita connection r. Under suitable conditions this procedure i gives a sequence of Riemannian manifolds f(T M, gi)gi2N equipped with ci c1 a sequence of Riemannian connections fr gi2N. Then we show that r produces the curves which are the (local) length minimizer of T 1M. M.S.C. 2010: 58A05, 58B20. Key words: Complete lift; spray; geodesic; Fr´echet manifolds; Banach manifold; connection. 1 Introduction In the first section we remind the bijective correspondence between linear connections and homogeneous sprays. Then using the results of [6] for complete lift of sprays, we propose a formula to lift a connection on M to its higher order tangent bundles T rM, r 2 N. More precisely, for a given connection r on T rM, r 2 N [ f0g, we construct its associated spray S and then we lift it to a homogeneous spray Sc on T r+1M [6]. Then, using the bijective correspondence between connections and sprays, we derive the connection rc on T r+1M from Sc.
    [Show full text]
  • Hodge Theory of SKT Manifolds
    Hodge theory and deformations of SKT manifolds Gil R. Cavalcanti∗ Department of Mathematics Utrecht University Abstract We use tools from generalized complex geometry to develop the theory of SKT (a.k.a. pluriclosed Hermitian) manifolds and more generally manifolds with special holonomy with respect to a metric connection with closed skew-symmetric torsion. We develop Hodge theory on such manifolds show- ing how the reduction of the holonomy group causes a decomposition of the twisted cohomology. For SKT manifolds this decomposition is accompanied by an identity between different Laplacian operators and forces the collapse of a spectral sequence at the first page. Further we study the de- formation theory of SKT structures, identifying the space where the obstructions live. We illustrate our theory with examples based on Calabi{Eckmann manifolds, instantons, Hopf surfaces and Lie groups. Contents 1 Linear algebra 3 2 Intrinsic torsion of generalized Hermitian structures8 2.1 The Nijenhuis tensor....................................9 2.2 The intrinsic torsion and the road to integrability.................... 10 2.3 The operators δ± and δ± ................................. 12 3 Parallel Hermitian and bi-Hermitian structures 12 4 SKT structures 14 5 Hodge theory 19 5.1 Differential operators, their adjoints and Laplacians.................. 19 5.2 Signature and Euler characteristic of almost Hermitian manifolds........... 20 5.3 Hodge theory on parallel Hermitian manifolds...................... 22 5.4 Hodge theory on SKT manifolds............................. 23 5.5 Relation to Dolbeault cohomology............................ 23 5.6 Hermitian symplectic structures.............................. 27 6 Hodge theory beyond U(n) 28 6.1 Integrability......................................... 29 Keywords. Strong KT structure, generalized complex geometry, generalized K¨ahlergeometry, Hodge theory, instan- tons, deformations.
    [Show full text]