MA4C0 Differential Geometry Course, Taught by Peter Topping, Typeset by Matthew Egginton
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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. -
Lectures on Differential Geometry Math 240C
Lectures on Differential Geometry Math 240C John Douglas Moore Department of Mathematics University of California Santa Barbara, CA, USA 93106 e-mail: [email protected] June 6, 2011 Preface This is a set of lecture notes for the course Math 240C given during the Spring of 2011. The notes will evolve as the course progresses. The starred sections are less central to the course, and may be omitted by some readers. i Contents 1 Riemannian geometry 1 1.1 Review of tangent and cotangent spaces . 1 1.2 Riemannian metrics . 4 1.3 Geodesics . 8 1.3.1 Smooth paths . 8 1.3.2 Piecewise smooth paths . 12 1.4 Hamilton's principle* . 13 1.5 The Levi-Civita connection . 19 1.6 First variation of J: intrinsic version . 25 1.7 Lorentz manifolds . 28 1.8 The Riemann-Christoffel curvature tensor . 31 1.9 Curvature symmetries; sectional curvature . 39 1.10 Gaussian curvature of surfaces . 42 1.11 Matrix Lie groups . 48 1.12 Lie groups with biinvariant metrics . 52 1.13 Projective spaces; Grassmann manifolds . 57 2 Normal coordinates 64 2.1 Definition of normal coordinates . 64 2.2 The Gauss Lemma . 68 2.3 Curvature in normal coordinates . 70 2.4 Tensor analysis . 75 2.5 Riemannian manifolds as metric spaces . 84 2.6 Completeness . 86 2.7 Smooth closed geodesics . 88 3 Curvature and topology 94 3.1 Overview . 94 3.2 Parallel transport along curves . 96 3.3 Geodesics and curvature . 97 3.4 The Hadamard-Cartan Theorem . 101 3.5 The fundamental group* . -
3. Introducing Riemannian Geometry
3. Introducing Riemannian Geometry We have yet to meet the star of the show. There is one object that we can place on a manifold whose importance dwarfs all others, at least when it comes to understanding gravity. This is the metric. The existence of a metric brings a whole host of new concepts to the table which, collectively, are called Riemannian geometry.Infact,strictlyspeakingwewillneeda slightly di↵erent kind of metric for our study of gravity, one which, like the Minkowski metric, has some strange minus signs. This is referred to as Lorentzian Geometry and a slightly better name for this section would be “Introducing Riemannian and Lorentzian Geometry”. However, for our immediate purposes the di↵erences are minor. The novelties of Lorentzian geometry will become more pronounced later in the course when we explore some of the physical consequences such as horizons. 3.1 The Metric In Section 1, we informally introduced the metric as a way to measure distances between points. It does, indeed, provide this service but it is not its initial purpose. Instead, the metric is an inner product on each vector space Tp(M). Definition:Ametric g is a (0, 2) tensor field that is: Symmetric: g(X, Y )=g(Y,X). • Non-Degenerate: If, for any p M, g(X, Y ) =0forallY T (M)thenX =0. • 2 p 2 p p With a choice of coordinates, we can write the metric as g = g (x) dxµ dx⌫ µ⌫ ⌦ The object g is often written as a line element ds2 and this expression is abbreviated as 2 µ ⌫ ds = gµ⌫(x) dx dx This is the form that we saw previously in (1.4). -
Hamilton's Ricci Flow
The University of Melbourne, Department of Mathematics and Statistics Hamilton's Ricci Flow Nick Sheridan Supervisor: Associate Professor Craig Hodgson Second Reader: Professor Hyam Rubinstein Honours Thesis, November 2006. Abstract The aim of this project is to introduce the basics of Hamilton's Ricci Flow. The Ricci flow is a pde for evolving the metric tensor in a Riemannian manifold to make it \rounder", in the hope that one may draw topological conclusions from the existence of such \round" metrics. Indeed, the Ricci flow has recently been used to prove two very deep theorems in topology, namely the Geometrization and Poincar´eConjectures. We begin with a brief survey of the differential geometry that is needed in the Ricci flow, then proceed to introduce its basic properties and the basic techniques used to understand it, for example, proving existence and uniqueness and bounds on derivatives of curvature under the Ricci flow using the maximum principle. We use these results to prove the \original" Ricci flow theorem { the 1982 theorem of Richard Hamilton that closed 3-manifolds which admit metrics of strictly positive Ricci curvature are diffeomorphic to quotients of the round 3-sphere by finite groups of isometries acting freely. We conclude with a qualitative discussion of the ideas behind the proof of the Geometrization Conjecture using the Ricci flow. Most of the project is based on the book by Chow and Knopf [6], the notes by Peter Topping [28] (which have recently been made into a book, see [29]), the papers of Richard Hamilton (in particular [9]) and the lecture course on Geometric Evolution Equations presented by Ben Andrews at the 2006 ICE-EM Graduate School held at the University of Queensland. -
On a Class of Einstein Space-Time Manifolds
Publ. Math. Debrecen 67/3-4 (2005), 471–480 On a class of Einstein space-time manifolds By ADELA MIHAI (Bucharest) and RADU ROSCA (Paris) Abstract. We deal with a general space-time (M,g) with usual differen- tiability conditions and hyperbolic metric g of index 1, which carries 3 skew- symmetric Killing vector fields X, Y , Z having as generative the unit time-like vector field e of the hyperbolic metric g. It is shown that such a space-time (M,g) is an Einstein manifold of curvature −1, which is foliated by space-like hypersur- faces Ms normal to e and the immersion x : Ms → M is pseudo-umbilical. In addition, it is proved that the vector fields X, Y , Z and e are exterior concur- rent vector fields and X, Y , Z define a commutative Killing triple, M admits a Lorentzian transformation which is in an orthocronous Lorentz group and the distinguished spatial 3-form of M is a relatively integral invariant of the vector fields X, Y and Z. 0. Introduction Let (M,g) be a general space-time with usual differentiability condi- tions and hyperbolic metric g of index 1. We assume in this paper that (M,g) carries 3 skew-symmetric Killing vector fields (abbr. SSK) X, Y , Z having as generative the unit time-like vector field e of the hyperbolic metric g (see[R1],[MRV].Therefore,if∇ is the Levi–Civita connection and ∧ means the wedge product of vector Mathematics Subject Classification: 53C15, 53D15, 53C25. Key words and phrases: space-time, skew-symmetric Killing vector field, exterior con- current vector field, orthocronous Lorentz group. -
GEOMETRIC INTERPRETATIONS of CURVATURE Contents 1. Notation and Summation Conventions 1 2. Affine Connections 1 3. Parallel Tran
GEOMETRIC INTERPRETATIONS OF CURVATURE ZHENGQU WAN Abstract. This is an expository paper on geometric meaning of various kinds of curvature on a Riemann manifold. Contents 1. Notation and Summation Conventions 1 2. Affine Connections 1 3. Parallel Transport 3 4. Geodesics and the Exponential Map 4 5. Riemannian Curvature Tensor 5 6. Taylor Expansion of the Metric in Normal Coordinates and the Geometric Interpretation of Ricci and Scalar Curvature 9 Acknowledgments 13 References 13 1. Notation and Summation Conventions We assume knowledge of the basic theory of smooth manifolds, vector fields and tensors. We will assume all manifolds are smooth, i.e. C1, second countable and Hausdorff. All functions, curves and vector fields will also be smooth unless otherwise stated. Einstein summation convention will be adopted in this paper. In some cases, the index types on either side of an equation will not match and @ so a summation will be needed. The tangent vector field @xi induced by local i coordinates (x ) will be denoted as @i. 2. Affine Connections Riemann curvature is a measure of the noncommutativity of parallel transporta- tion of tangent vectors. To define parallel transport, we need the notion of affine connections. Definition 2.1. Let M be an n-dimensional manifold. An affine connection, or connection, is a map r : X(M) × X(M) ! X(M), where X(M) denotes the space of smooth vector fields, such that for vector fields V1;V2; V; W1;W2 2 X(M) and function f : M! R, (1) r(fV1 + V2;W ) = fr(V1;W ) + r(V2;W ), (2) r(V; aW1 + W2) = ar(V; W1) + r(V; W2), for all a 2 R. -
Differential Geometry Lecture 17: Geodesics and the Exponential
Differential geometry Lecture 17: Geodesics and the exponential map David Lindemann University of Hamburg Department of Mathematics Analysis and Differential Geometry & RTG 1670 3. July 2020 David Lindemann DG lecture 17 3. July 2020 1 / 44 1 Geodesics 2 The exponential map 3 Geodesics as critical points of the energy functional 4 Riemannian normal coordinates 5 Some global Riemannian geometry David Lindemann DG lecture 17 3. July 2020 2 / 44 Recap of lecture 16: constructed covariant derivatives along curves defined parallel transport studied the relation between a given connection in the tangent bundle and its parallel transport maps introduced torsion tensor and metric connections, studied geometric interpretation defined the Levi-Civita connection of a pseudo-Riemannian manifold David Lindemann DG lecture 17 3. July 2020 3 / 44 Geodesics Recall the definition of the acceleration of a smooth curve n 00 n γ : I ! R , that is γ 2 Γγ (T R ). Question: Is there a coordinate-free analogue of this construc- tion involving connections? Answer: Yes, uses covariant derivative along curves. Definition Let M be a smooth manifold, r a connection in TM ! M, 0 and γ : I ! M a smooth curve. Then rγ0 γ 2 Γγ (TM) is called the acceleration of γ (with respect to r). Of particular interest is the case if the acceleration of a curve vanishes, that is if its velocity vector field is parallel: Definition A smooth curve γ : I ! M is called geodesic with respect to a 0 given connection r in TM ! M if rγ0 γ = 0. David Lindemann DG lecture 17 3. -
Differential Geometry Lecture 18: Curvature
Differential geometry Lecture 18: Curvature David Lindemann University of Hamburg Department of Mathematics Analysis and Differential Geometry & RTG 1670 14. July 2020 David Lindemann DG lecture 18 14. July 2020 1 / 31 1 Riemann curvature tensor 2 Sectional curvature 3 Ricci curvature 4 Scalar curvature David Lindemann DG lecture 18 14. July 2020 2 / 31 Recap of lecture 17: defined geodesics in pseudo-Riemannian manifolds as curves with parallel velocity viewed geodesics as projections of integral curves of a vector field G 2 X(TM) with local flow called geodesic flow obtained uniqueness and existence properties of geodesics constructed the exponential map exp : V ! M, V neighbourhood of the zero-section in TM ! M showed that geodesics with compact domain are precisely the critical points of the energy functional used the exponential map to construct Riemannian normal coordinates, studied local forms of the metric and the Christoffel symbols in such coordinates discussed the Hopf-Rinow Theorem erratum: codomain of (x; v) as local integral curve of G is d'(TU), not TM David Lindemann DG lecture 18 14. July 2020 3 / 31 Riemann curvature tensor Intuitively, a meaningful definition of the term \curvature" for 3 a smooth surface in R , written locally as a graph of a smooth 2 function f : U ⊂ R ! R, should involve the second partial derivatives of f at each point. How can we find a coordinate- 3 free definition of curvature not just for surfaces in R , which are automatically Riemannian manifolds by restricting h·; ·i, but for all pseudo-Riemannian manifolds? Definition Let (M; g) be a pseudo-Riemannian manifold with Levi-Civita connection r. -
On Riemannian Manifolds Endowed with a Locally Conformal Cosymplectic Structure
ON RIEMANNIAN MANIFOLDS ENDOWED WITH A LOCALLY CONFORMAL COSYMPLECTIC STRUCTURE ION MIHAI, RADU ROSCA, AND VALENTIN GHIS¸OIU Received 18 September 2004 and in revised form 7 September 2005 We deal with a locally conformal cosymplectic manifold M(φ,Ω,ξ,η,g)admittingacon- formal contact quasi-torse-forming vector field T. The presymplectic 2-form Ω is a lo- cally conformal cosymplectic 2-form. It is shown that T is a 3-exterior concurrent vector field. Infinitesimal transformations of the Lie algebra of ∧M are investigated. The Gauss map of the hypersurface Mξ normal to ξ is conformal and Mξ × Mξ is a Chen submanifold of M × M. 1. Introduction Locally conformal cosymplectic manifolds have been investigated by Olszak and Rosca [7] (see also [6]). In the present paper, we consider a (2m + 1)-dimensional Riemannian manifold M(φ, Ω,ξ,η,g) endowed with a locally conformal cosymplectic structure. We assume that M admits a principal vector field (or a conformal contact quasi-torse-forming), that is, ∇T = sdp + T ∧ ξ = sdp + η ⊗ T − T ⊗ ξ, (1.1) with ds = sη. First, we prove certain geometrical properties of the vector fields T and φT. The exis- tence of T and φT is determined by an exterior differential system in involution (in the sense of Cartan [3]). The principal vector field T is 3-exterior concurrent (see also [8]), it defines a Lie relative contact transformation of the co-Reeb form η, and the Lie differential of T with respect to T is conformal to T.ThevectorfieldφT is an infinitesimal transfor- mation of generators T and ξ.Thevectorfieldsξ, T,andφT commute and the distri- bution DT ={T,φT,ξ} is involutive. -
Chapter 7 Geodesics on Riemannian Manifolds
Chapter 7 Geodesics on Riemannian Manifolds 7.1 Geodesics, Local Existence and Uniqueness If (M,g)isaRiemannianmanifold,thentheconceptof length makes sense for any piecewise smooth (in fact, C1) curve on M. Then, it possible to define the structure of a metric space on M,whered(p, q)isthegreatestlowerboundofthe length of all curves joining p and q. Curves on M which locally yield the shortest distance between two points are of great interest. These curves called geodesics play an important role and the goal of this chapter is to study some of their properties. 489 490 CHAPTER 7. GEODESICS ON RIEMANNIAN MANIFOLDS Given any p M,foreveryv TpM,the(Riemannian) norm of v,denoted∈ v ,isdefinedby∈ " " v = g (v,v). " " p ! The Riemannian inner product, gp(u, v), of two tangent vectors, u, v TpM,willalsobedenotedby u, v p,or simply u, v .∈ # $ # $ Definition 7.1.1 Given any Riemannian manifold, M, a smooth parametric curve (for short, curve)onM is amap,γ: I M,whereI is some open interval of R. For a closed→ interval, [a, b] R,amapγ:[a, b] M is a smooth curve from p =⊆γ(a) to q = γ(b) iff→γ can be extended to a smooth curve γ:(a ", b + ") M, for some ">0. Given any two points,− p, q →M,a ∈ continuous map, γ:[a, b] M,isa" piecewise smooth curve from p to q iff → (1) There is a sequence a = t0 <t1 < <tk 1 <t = b of numbers, t R,sothateachmap,··· − k i ∈ γi = γ ! [ti,ti+1], called a curve segment is a smooth curve, for i =0,...,k 1. -
A. Vector and Affine Spaces
A. Vector and affine spaces This appendix reviews basic facts about vector and affine spaces, including the notions of metric and orientation. To a large extent, the treatment follows Malament (2009). A.1. Matrices Definition 34. An m n matrix is a rectangular table of mn real numbers A , where ⇥ ij 1 i m and 1 j n, arrayed as follows: A A A 11 12 ··· 1n 0 A21 A22 A2n 1 ··· (A.1) . .. B . C B C BA A A C B m1 m2 mnC @ ··· A The operation of matrix multiplication is defined as follows. Definition 35. Given an m n matrix A and an n p matrix B, their matrix product AB ⇥ ⇥ is the m p matrix with entries (AB)i , where ⇥ k i i j (AB) k = A jB k (A.2) Note that this uses the Einstein summation convention: repeated indices are summed over. Definition 36. Given an m n matrix Ai , its transpose is an n m matrix denoted by ⇥ j ⇥ A j, and defined by the condition that for all 1 i m and 1 j n, A j = Ai , i i j An element of Rn can be identified with an n 1 matrix; as such, an m n matrix A ⇥ ⇥ encodes a map A : Rm Rn. Such a map is linear, in the sense that for any xi, yi Rm ! 2 97 and any a, b R, 2 i j j i j i j A j(ax + by )=a(A jx )+b(A jy ) (A.3) And, in fact, any linear map from Rm to Rn corresponds to some matrix. -
Exterior Derivative
Exterior derivative On a differentiable manifold, the exterior derivative extends the concept of the differential of a function to differential forms of higher degree. e exterior derivative was first described in its current form by Élie Cartan in 1899; it allows for a natural, metric-independent generalization of Stokes' theorem, Gauss's theorem, and Green's theorem from vector calculus. If a k-form is thought of as measuring the flux through an infinitesimal k-parallelotope, then its exterior derivative can be thought of as measuring the net flux through the boundary of a (k + 1)-parallelotope. Contents Definition In terms of axioms In terms of local coordinates In terms of invariant formula Examples Stokes' theorem on manifolds Further properties Closed and exact forms de Rham cohomology Naturality Exterior derivative in vector calculus Gradient Divergence Curl Invariant formulations of grad, curl, div, and Laplacian See also Notes References Definition e exterior derivative of a differential form of degree k is a differential form of degree k + 1. If f is a smooth function (a 0-form), then the exterior derivative of f is the differential of f . at is, df is the unique 1-form such that for every smooth vector field X, df (X) = dX f , where dX f is the directional derivative of f in the direction of X. ere are a variety of equivalent definitions of the exterior derivative of a general k-form. In terms of axioms e exterior derivative is defined to be the unique ℝ-linear mapping from k-forms to (k + 1)-forms satisfying the following properties: 1.