A Review on Metric Symmetries Used in Geometry and Physics K
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Chapter 13 Curvature in Riemannian Manifolds
Chapter 13 Curvature in Riemannian Manifolds 13.1 The Curvature Tensor If (M, , )isaRiemannianmanifoldand is a connection on M (that is, a connection on TM−), we− saw in Section 11.2 (Proposition 11.8)∇ that the curvature induced by is given by ∇ R(X, Y )= , ∇X ◦∇Y −∇Y ◦∇X −∇[X,Y ] for all X, Y X(M), with R(X, Y ) Γ( om(TM,TM)) = Hom (Γ(TM), Γ(TM)). ∈ ∈ H ∼ C∞(M) Since sections of the tangent bundle are vector fields (Γ(TM)=X(M)), R defines a map R: X(M) X(M) X(M) X(M), × × −→ and, as we observed just after stating Proposition 11.8, R(X, Y )Z is C∞(M)-linear in X, Y, Z and skew-symmetric in X and Y .ItfollowsthatR defines a (1, 3)-tensor, also denoted R, with R : T M T M T M T M. p p × p × p −→ p Experience shows that it is useful to consider the (0, 4)-tensor, also denoted R,givenby R (x, y, z, w)= R (x, y)z,w p p p as well as the expression R(x, y, y, x), which, for an orthonormal pair, of vectors (x, y), is known as the sectional curvature, K(x, y). This last expression brings up a dilemma regarding the choice for the sign of R. With our present choice, the sectional curvature, K(x, y), is given by K(x, y)=R(x, y, y, x)but many authors define K as K(x, y)=R(x, y, x, y). Since R(x, y)isskew-symmetricinx, y, the latter choice corresponds to using R(x, y)insteadofR(x, y), that is, to define R(X, Y ) by − R(X, Y )= + . -
3. Sectional Curvature of Lorentzian Manifolds. 1
3. SECTIONAL CURVATURE OF LORENTZIAN MANIFOLDS. 1. Sectional curvature, the Jacobi equation and \tidal stresses". The (3,1) Riemann curvature tensor has the same definition in the rie- mannian and Lorentzian cases: R(X; Y )Z = rX rY Z − rY rX Z − r[X;Y ]Z: If f(t; s) is a parametrized 2-surface in M (immersion) and W (t; s) is a vector field on M along f, we have the Ricci formula: D DW D DW − = R(@ f; @ f)W: @t @s @s @t t s For a variation f(t; s) = γs(t) of a geodesic γ(t) (with variational vector field J(t) = @sfjs=0 along γ(t)) this leads to the Jacobi equation for J: D2J + R(J; γ_ )_γ = 0: dt2 ? The Jacobi operator is the self-adjoint operator on (γ _ ) : Rp[v] = Rp(v; γ_ )_γ. When γ is a timelike geodesic (the worldline of a free-falling massive particle) the physical interpretation of J is the relative displacement (space- like) vector of a neighboring free-falling particle, while the second covariant 00 derivative J represents its relative acceleration. The Jacobi operator Rp gives the \tidal stresses" in terms of the position vector J. In the Lorentzian case, the sectional curvature is defined only for non- degenerate two-planes Π ⊂ TpM. Definition. Let Π = spanfX; Y g be a non-degenerate two-dimensional subspace of TpM. The sectional curvature σXY = σΠ is the real number σ defined by: hR(X; Y )Y; Xi = σhX ^ Y; X ^ Y i: Remark: by a result of J. -
Hyperbolic Geometry
Flavors of Geometry MSRI Publications Volume 31,1997 Hyperbolic Geometry JAMES W. CANNON, WILLIAM J. FLOYD, RICHARD KENYON, AND WALTER R. PARRY Contents 1. Introduction 59 2. The Origins of Hyperbolic Geometry 60 3. Why Call it Hyperbolic Geometry? 63 4. Understanding the One-Dimensional Case 65 5. Generalizing to Higher Dimensions 67 6. Rudiments of Riemannian Geometry 68 7. Five Models of Hyperbolic Space 69 8. Stereographic Projection 72 9. Geodesics 77 10. Isometries and Distances in the Hyperboloid Model 80 11. The Space at Infinity 84 12. The Geometric Classification of Isometries 84 13. Curious Facts about Hyperbolic Space 86 14. The Sixth Model 95 15. Why Study Hyperbolic Geometry? 98 16. When Does a Manifold Have a Hyperbolic Structure? 103 17. How to Get Analytic Coordinates at Infinity? 106 References 108 Index 110 1. Introduction Hyperbolic geometry was created in the first half of the nineteenth century in the midst of attempts to understand Euclid’s axiomatic basis for geometry. It is one type of non-Euclidean geometry, that is, a geometry that discards one of Euclid’s axioms. Einstein and Minkowski found in non-Euclidean geometry a This work was supported in part by The Geometry Center, University of Minnesota, an STC funded by NSF, DOE, and Minnesota Technology, Inc., by the Mathematical Sciences Research Institute, and by NSF research grants. 59 60 J. W. CANNON, W. J. FLOYD, R. KENYON, AND W. R. PARRY geometric basis for the understanding of physical time and space. In the early part of the twentieth century every serious student of mathematics and physics studied non-Euclidean geometry. -
Sufficient Conditions for Periodicity of a Killing Vector Field Walter C
PROCEEDINGS OF THE AMERICAN MATHEMATICAL SOCIETY Volume 38, Number 3, May 1973 SUFFICIENT CONDITIONS FOR PERIODICITY OF A KILLING VECTOR FIELD WALTER C. LYNGE Abstract. Let X be a complete Killing vector field on an n- dimensional connected Riemannian manifold. Our main purpose is to show that if X has as few as n closed orbits which are located properly with respect to each other, then X must have periodic flow. Together with a known result, this implies that periodicity of the flow characterizes those complete vector fields having all orbits closed which can be Killing with respect to some Riemannian metric on a connected manifold M. We give a generalization of this characterization which applies to arbitrary complete vector fields on M. Theorem. Let X be a complete Killing vector field on a connected, n- dimensional Riemannian manifold M. Assume there are n distinct points p, Pit' " >Pn-i m M such that the respective orbits y, ylt • • • , yn_x of X through them are closed and y is nontrivial. Suppose further that each pt is joined to p by a unique minimizing geodesic and d(p,p¡) = r¡i<.D¡2, where d denotes distance on M and D is the diameter of y as a subset of M. Let_wx, • ■ ■ , wn_j be the unit vectors in TVM such that exp r¡iwi=pi, i=l, • ■ • , n— 1. Assume that the vectors Xv, wx, ■• • , wn_x span T^M. Then the flow cptof X is periodic. Proof. Fix /' in {1, 2, •••,«— 1}. We first show that the orbit yt does not lie entirely in the sphere Sj,(r¡¿) of radius r¡i about p. -
Global Properties of Asymptotically De Sitter and Anti De Sitter Spacetimes
Global properties of asymptotically de Sitter and Anti de Sitter spacetimes Didier A. Solis May, 17, 2006 arXiv:1803.01171v1 [gr-qc] 3 Mar 2018 Ad Majorem Dei Gloriam. To all those who seek to fulfill God's will in their lives. iii ACKNOWLEDGEMENTS I would like to express my deepest gratitude to: • My advisor Dr. Gregory Galloway, for his constant support and help. This dissertation would not had seen the light of day without his continued encour- agement and guidance. • Dr. N. Saveliev, Dr. M. Cai and Dr. O. Alvarez for their valuable comments and thorough revision of this work. • The Faculty and staff at the Math Department for all the knowledge and affec- tion they shared with me. • CONACYT (Consejo Nacional de Ciencia y Tecnolog´ıa)for the financial support granted to the author. • My family: Douglas, Rosalinda, Douglas Jr, Rosil´uand Josu´efor all their prayers and unconditional love. They are indeed the greatest blessing in my life. • All my friends, especially Guille, for always being there for me to share the struggles and joys of life. • To the CSA gang, for being a living example of faith lived in love and hope. • Last but by no means least, to God, without whom there is no math, laughter or music. iv Contents 1 Introduction 1 1.1 Lorentz vector spaces . 1 1.2 Spacetimes . 6 1.2.1 The Levi-Civita connection . 7 1.2.2 Covariant derivative . 11 1.2.3 Geodesics . 12 1.3 Causal theory . 15 1.3.1 Definitions . 15 1.3.2 Global causality conditions . -
Constructing $ P, N $-Forms from $ P $-Forms Via the Hodge Star Operator and the Exterior Derivative
Constructing p, n-forms from p-forms via the Hodge star operator and the exterior derivative Jun-Jin Peng1,2∗ 1School of Physics and Electronic Science, Guizhou Normal University, Guiyang, Guizhou 550001, People’s Republic of China; 2Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University, Guiyang, Guizhou 550001, People’s Republic of China Abstract In this paper, we aim to explore the properties and applications on the operators consisting of the Hodge star operator together with the exterior derivative, whose action on an arbi- trary p-form field in n-dimensional spacetimes makes its form degree remain invariant. Such operations are able to generate a variety of p-forms with the even-order derivatives of the p- form. To do this, we first investigate the properties of the operators, such as the Laplace-de Rham operator, the codifferential and their combinations, as well as the applications of the arXiv:1909.09921v2 [gr-qc] 23 Mar 2020 operators in the construction of conserved currents. On basis of two general p-forms, then we construct a general n-form with higher-order derivatives. Finally, we propose that such an n-form could be applied to define a generalized Lagrangian with respect to a p-form field according to the fact that it incudes the ordinary Lagrangians for the p-form and scalar fields as special cases. Keywords: p-form; Hodge star; Laplace-de Rham operator; Lagrangian for p-form. ∗ [email protected] 1 1 Introduction Differential forms are a powerful tool developed to deal with the calculus in differential geom- etry and tensor analysis. -
Lecture 8: the Sectional and Ricci Curvatures
LECTURE 8: THE SECTIONAL AND RICCI CURVATURES 1. The Sectional Curvature We start with some simple linear algebra. As usual we denote by ⊗2(^2V ∗) the set of 4-tensors that is anti-symmetric with respect to the first two entries and with respect to the last two entries. Lemma 1.1. Suppose T 2 ⊗2(^2V ∗), X; Y 2 V . Let X0 = aX +bY; Y 0 = cX +dY , then T (X0;Y 0;X0;Y 0) = (ad − bc)2T (X; Y; X; Y ): Proof. This follows from a very simple computation: T (X0;Y 0;X0;Y 0) = T (aX + bY; cX + dY; aX + bY; cX + dY ) = (ad − bc)T (X; Y; aX + bY; cX + dY ) = (ad − bc)2T (X; Y; X; Y ): 1 Now suppose (M; g) is a Riemannian manifold. Recall that 2 g ^ g is a curvature- like tensor, such that 1 g ^ g(X ;Y ;X ;Y ) = hX ;X ihY ;Y i − hX ;Y i2: 2 p p p p p p p p p p 1 Applying the previous lemma to Rm and 2 g ^ g, we immediately get Proposition 1.2. The quantity Rm(Xp;Yp;Xp;Yp) K(Xp;Yp) := 2 hXp;XpihYp;Ypi − hXp;Ypi depends only on the two dimensional plane Πp = span(Xp;Yp) ⊂ TpM, i.e. it is independent of the choices of basis fXp;Ypg of Πp. Definition 1.3. We will call K(Πp) = K(Xp;Yp) the sectional curvature of (M; g) at p with respect to the plane Πp. Remark. The sectional curvature K is NOT a function on M (for dim M > 2), but a function on the Grassmann bundle Gm;2(M) of M. -
Curves of Constant Curvature and Torsion in the the 3-Sphere
CURVES OF CONSTANT CURVATURE AND TORSION IN THE 3-SPHERE DEBRAJ CHAKRABARTI, RAHUL SAHAY, AND JARED WILLIAMS Abstract. We describe the curves of constant (geodesic) curvature and torsion in the three-dimensional round sphere. These curves are the trajectory of a point whose motion is the superposition of two circular motions in orthogonal planes. The global behavior may be periodic or the curve may be dense in a Clifford torus embedded in the three- sphere. This behavior is very different from that of helices in three-dimensional Euclidean space, which also have constant curvature and torsion. 1. Introduction Let pM; x; yq be a three dimensional Riemannian manifold, let I Ď R be an open interval, and let γ : I Ñ M be a smooth curve in M, which we assume to be parametrized by the arc length t. It is well-known that the local geometry of γ is characterized by the curvature κ and the torsion τ. These are functions defined along γ and are the coefficients of the well-known Frenet-Serret formulas [2, Vol. IV, pp. 21-23]: D Tptq “ κptqNptq dt D Nptq “ ´κptqTptq `τptqBptq (1.1) dt D Bptq “ ´ τptqNptq; dt where the orthogonal unit vector fields T; N; B, with T “ γ1, along the unit-speed curve D γ, constitute its Frenet frame and dt denotes covariant differentiation along γ with respect to the arc length t. We will assume that each of the functions κ and τ is either nowhere zero or vanishes identically. Additionally, if κ is identically zero, then τ is also taken to be identically zero. -
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. -
Lecture A2 Conformal Field Theory Killing Vector Fields the Sphere Sn
Lecture A2 conformal field theory Killing vector fields The sphere Sn is invariant under the group SO(n + 1). The Minkowski space is invariant under the Poincar´egroup, which includes translations, rotations, and Lorentz boosts. For µ a general Riemannian manifold M, take a tangent vector field ξ = ξ ∂µ and consider the infinitesimal coordinate transformation, xµ xµ + ǫξµ, ( ǫ 1). → | |≪ Question 1: Show that the metric components gµν transforms as ρ 2 2 gµν gµν + ǫ (∂µξν + ∂νξµ + ξ ∂ρ) + 0(ǫ )= gµν + ǫ ( µξν + νξµ) + 0(ǫ ). → ∇ ∇ The metric is invariant under the infinitesimal transformation by ξ iff µξν + νξµ = 0. A ∇ ∇ tangent vector field satisfying this equation is called a Killing vector field. µ Question 2: Suppose we have two tangent vector fields, ξa = ξa ∂µ (a = 1, 2). Show that their commutator ν µ ν µ [ξ ,ξ ] = (ξ ∂νξ ξ ∂ν ξ )∂µ 1 2 1 2 − 2 1 ν µ is also a tangent vector field. Explain why ξ1 ∂νξ2 is not a tangent vector field in general. Question 3: Suppose there are two Killing vector fields, ξa (a = 1, 2). One can consider an infinitesimal transformation, ga, corresponding to each of them. Namely, µ µ µ ga : x x + ǫξ , (a = 1, 2). → a −1 −1 Show that g1g2g1 g2 is generated by the commutator, [ξ1,ξ2]. If the metric is invariant under infinitesimal transformations generated by ξ1,ξ2, it should also be invariant under their commutator, [ξ1,ξ2]. Thus, the space of Killing vector fields is closed under the commutator – it makes a Lie algebra. -
Chapter 5 Differential Geometry
Chapter 5 Differential Geometry III 5.1 The Lie derivative 5.1.1 The Pull-Back Following (2.28), we considered one-parameter groups of diffeomor- phisms γt : R × M → M (5.1) such that points p ∈ M can be considered as being transported along curves γ : R → M (5.2) with γ(0) = p. Similarly, the diffeomorphism γt can be taken at fixed t ∈ R, defining a diffeomorphism γt : M → M (5.3) which maps the manifold onto itself and satisfies γt ◦ γs = γs+t. We have seen the relationship between vector fields and one-parameter groups of diffeomorphisms before. Let now v be a vector field on M and γ from (5.2) be chosen such that the tangent vectorγ ˙(t) defined by d (˙γ(t))( f ) = ( f ◦ γ)(t) (5.4) dt is identical with v,˙γ = v. Then γ is called an integral curve of v. If this is true for all curves γ obtained from γt by specifying initial points γ(0), the result is called the flow of v. The domain of definition D of γt can be a subset of R× M.IfD = R× M, the vector field is said to be complete and γt is called the global flow of v. If D is restricted to open intervals I ⊂ R and open neighbourhoods U ⊂ M, thus D = I × U ⊂ R × M, the flow is called local. 63 64 5 Differential Geometry III Pull-back Let now M and N be two manifolds and φ : M → N a map from M onto N. -
Conformal Killing Forms on Riemannian Manifolds
Conformal Killing forms on Riemannian manifolds Uwe Semmelmann October 22, 2018 Abstract Conformal Killing forms are a natural generalization of conformal vector fields on Riemannian manifolds. They are defined as sections in the kernel of a conformally invariant first order differential operator. We show the existence of conformal Killing forms on nearly K¨ahler and weak G2-manifolds. Moreover, we give a complete de- scription of special conformal Killing forms. A further result is a sharp upper bound on the dimension of the space of conformal Killing forms. 1 Introduction A classical object of differential geometry are Killing vector fields. These are by definition infinitesimal isometries, i.e. the flow of such a vector field preserves a given metric. The space of all Killing vector fields forms the Lie algebra of the isometry group of a Riemannian manifold and the number of linearly independent Killing vector fields measures the degree of symmetry of the manifold. It is known that this number is bounded from above by the dimension of the isometry group of the standard sphere and, on compact manifolds, equality is attained if and only if the manifold is isometric to the standard sphere or the real projective space. Slightly more generally one can consider conformal vector fields, i.e. vector fields with a flow preserving a given conformal class of metrics. There are several geometric conditions which force a conformal vector field to be Killing. Much less is known about a rather natural generalization of conformal vector fields, the so-called conformal Killing forms. These are p-forms ψ satisfying for any vector field X the differential equation 1 y 1 ∗ ∗ ∇X ψ − p+1 X dψ + n−p+1 X ∧ d ψ = 0 , (1.1) arXiv:math/0206117v1 [math.DG] 11 Jun 2002 where n is the dimension of the manifold, ∇ denotes the covariant derivative of the Levi- Civita connection, X∗ is 1-form dual to X and y is the operation dual to the wedge product.