Hyperbolic Geometry, Surfaces, and 3-Manifolds Bruno Martelli
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Geometric Manifolds
Wintersemester 2015/2016 University of Heidelberg Geometric Structures on Manifolds Geometric Manifolds by Stephan Schmitt Contents Introduction, first Definitions and Results 1 Manifolds - The Group way .................................... 1 Geometric Structures ........................................ 2 The Developing Map and Completeness 4 An introductory discussion of the torus ............................. 4 Definition of the Developing map ................................. 6 Developing map and Manifolds, Completeness 10 Developing Manifolds ....................................... 10 some completeness results ..................................... 10 Some selected results 11 Discrete Groups .......................................... 11 Stephan Schmitt INTRODUCTION, FIRST DEFINITIONS AND RESULTS Introduction, first Definitions and Results Manifolds - The Group way The keystone of working mathematically in Differential Geometry, is the basic notion of a Manifold, when we usually talk about Manifolds we mean a Topological Space that, at least locally, looks just like Euclidean Space. The usual formalization of that Concept is well known, we take charts to ’map out’ the Manifold, in this paper, for sake of Convenience we will take a slightly different approach to formalize the Concept of ’locally euclidean’, to formulate it, we need some tools, let us introduce them now: Definition 1.1. Pseudogroups A pseudogroup on a topological space X is a set G of homeomorphisms between open sets of X satisfying the following conditions: • The Domains of the elements g 2 G cover X • The restriction of an element g 2 G to any open set contained in its Domain is also in G. • The Composition g1 ◦ g2 of two elements of G, when defined, is in G • The inverse of an Element of G is in G. • The property of being in G is local, that is, if g : U ! V is a homeomorphism between open sets of X and U is covered by open sets Uα such that each restriction gjUα is in G, then g 2 G Definition 1.2. -
Black Hole Physics in Globally Hyperbolic Space-Times
Pram[n,a, Vol. 18, No. $, May 1982, pp. 385-396. O Printed in India. Black hole physics in globally hyperbolic space-times P S JOSHI and J V NARLIKAR Tata Institute of Fundamental Research, Bombay 400 005, India MS received 13 July 1981; revised 16 February 1982 Abstract. The usual definition of a black hole is modified to make it applicable in a globallyhyperbolic space-time. It is shown that in a closed globallyhyperbolic universe the surface area of a black hole must eventuallydecrease. The implications of this breakdown of the black hole area theorem are discussed in the context of thermodynamics and cosmology. A modifieddefinition of surface gravity is also given for non-stationaryuniverses. The limitations of these concepts are illustrated by the explicit example of the Kerr-Vaidya metric. Keywocds. Black holes; general relativity; cosmology, 1. Introduction The basic laws of black hole physics are formulated in asymptotically flat space- times. The cosmological considerations on the other hand lead one to believe that the universe may not be asymptotically fiat. A realistic discussion of black hole physics must not therefore depend critically on the assumption of an asymptotically flat space-time. Rather it should take account of the global properties found in most of the widely discussed cosmological models like the Friedmann models or the more general Robertson-Walker space times. Global hyperbolicity is one such important property shared by the above cosmo- logical models. This property is essentially a precise formulation of classical deter- minism in a space-time and it removes several physically unreasonable pathological space-times from a discussion of what the large scale structure of the universe should be like (Penrose 1972). -
Models of 2-Dimensional Hyperbolic Space and Relations Among Them; Hyperbolic Length, Lines, and Distances
Models of 2-dimensional hyperbolic space and relations among them; Hyperbolic length, lines, and distances Cheng Ka Long, Hui Kam Tong 1155109623, 1155109049 Course Teacher: Prof. Yi-Jen LEE Department of Mathematics, The Chinese University of Hong Kong MATH4900E Presentation 2, 5th October 2020 Outline Upper half-plane Model (Cheng) A Model for the Hyperbolic Plane The Riemann Sphere C Poincar´eDisc Model D (Hui) Basic properties of Poincar´eDisc Model Relation between D and other models Length and distance in the upper half-plane model (Cheng) Path integrals Distance in hyperbolic geometry Measurements in the Poincar´eDisc Model (Hui) M¨obiustransformations of D Hyperbolic length and distance in D Conclusion Boundary, Length, Orientation-preserving isometries, Geodesics and Angles Reference Upper half-plane model H Introduction to Upper half-plane model - continued Hyperbolic geometry Five Postulates of Hyperbolic geometry: 1. A straight line segment can be drawn joining any two points. 2. Any straight line segment can be extended indefinitely in a straight line. 3. A circle may be described with any given point as its center and any distance as its radius. 4. All right angles are congruent. 5. For any given line R and point P not on R, in the plane containing both line R and point P there are at least two distinct lines through P that do not intersect R. Some interesting facts about hyperbolic geometry 1. Rectangles don't exist in hyperbolic geometry. 2. In hyperbolic geometry, all triangles have angle sum < π 3. In hyperbolic geometry if two triangles are similar, they are congruent. -
Arxiv:2008.00328V3 [Math.DS] 28 Apr 2021 Uniformly Hyperbolic and Topologically Mixing
ERGODICITY AND EQUIDISTRIBUTION IN STRICTLY CONVEX HILBERT GEOMETRY FENG ZHU Abstract. We show that dynamical and counting results characteristic of negatively-curved Riemannian geometry, or more generally CAT(-1) or rank- one CAT(0) spaces, also hold for geometrically-finite strictly convex projective structures equipped with their Hilbert metric. More specifically, such structures admit a finite Sullivan measure; with respect to this measure, the Hilbert geodesic flow is strongly mixing, and orbits and primitive closed geodesics equidistribute, allowing us to asymptotically enumerate these objects. In [Mar69], Margulis established counting results for uniform lattices in constant negative curvature, or equivalently for closed hyperbolic manifolds, by means of ergodicity and equidistribution results for the geodesic flows on these manifolds with respect to suitable measures. Thomas Roblin, in [Rob03], obtained analogous ergodicity and equidistribution results in the more general setting of CAT(−1) spaces. These results include ergodicity of the horospherical foliations, mixing of the geodesic flow, orbital equidistribution of the group, equidistribution of primitive closed geodesics, and, in the geometrically finite case, asymptotic counting estimates. Gabriele Link later adapted similar techniques to prove similar results in the even more general setting of rank-one isometry groups of Hadamard spaces in [Lin20]. These results do not directly apply to manifolds endowed with strictly convex projective structures, considered with their Hilbert metrics and associated Bowen- Margulis measures, since strictly convex Hilbert geometries are in general not CAT(−1) or even CAT(0) (see e.g. [Egl97, App. B].) Nevertheless, these Hilbert geometries exhibit substantial similarities to Riemannian geometries of pinched negative curvature. In particular, there is a good theory of Busemann functions and of Patterson-Sullivan measures on these geometries. -
Volume Estimates for Equiangular Hyperbolic Coxeter Polyhedra
Algebraic & Geometric Topology 9 (2009) 1225–1254 1225 Volume estimates for equiangular hyperbolic Coxeter polyhedra CHRISTOPHER KATKINSON An equiangular hyperbolic Coxeter polyhedron is a hyperbolic polyhedron where all dihedral angles are equal to =n for some fixed n Z, n 2. It is a consequence of 2 Andreev’s theorem that either n 3 and the polyhedron has all ideal vertices or that D n 2. Volume estimates are given for all equiangular hyperbolic Coxeter polyhedra. D 57M50; 30F40 1 Introduction An orientable 3–orbifold, Q, is determined by an underlying 3–manifold, XQ and a trivalent graph, †Q , labeled by integers. If Q carries a hyperbolic structure then it is unique by Mostow rigidity, so the hyperbolic volume of Q is an invariant of Q. Therefore, for hyperbolic orbifolds with a fixed underlying manifold, the volume is a function of the labeled graph †. In this paper, methods for estimating the volume of orbifolds of a restricted type in terms of this labeled graph will be described. The orbifolds studied in this paper are quotients of H3 by reflection groups generated by reflections in hyperbolic Coxeter polyhedra. A Coxeter polyhedron is one where each dihedral angle is of the form =n for some n Z, n 2. Given a hyperbolic 2 Coxeter polyhedron P , consider the group generated by reflections through the geodesic planes determined by its faces, .P/. Then .P/ is a Kleinian group which acts on H3 with fundamental domain P . The quotient, O H3= .P/, is a nonorientable D orbifold with singular locus P.2/ , the 2–skeleton of P . -
[Math.GT] 9 Oct 2020 Symmetries of Hyperbolic 4-Manifolds
Symmetries of hyperbolic 4-manifolds Alexander Kolpakov & Leone Slavich R´esum´e Pour chaque groupe G fini, nous construisons des premiers exemples explicites de 4- vari´et´es non-compactes compl`etes arithm´etiques hyperboliques M, `avolume fini, telles M G + M G que Isom ∼= , ou Isom ∼= . Pour y parvenir, nous utilisons essentiellement la g´eom´etrie de poly`edres de Coxeter dans l’espace hyperbolique en dimension quatre, et aussi la combinatoire de complexes simpliciaux. C¸a nous permet d’obtenir une borne sup´erieure universelle pour le volume minimal d’une 4-vari´et´ehyperbolique ayant le groupe G comme son groupe d’isom´etries, par rap- port de l’ordre du groupe. Nous obtenons aussi des bornes asymptotiques pour le taux de croissance, par rapport du volume, du nombre de 4-vari´et´es hyperboliques ayant G comme le groupe d’isom´etries. Abstract In this paper, for each finite group G, we construct the first explicit examples of non- M M compact complete finite-volume arithmetic hyperbolic 4-manifolds such that Isom ∼= G + M G , or Isom ∼= . In order to do so, we use essentially the geometry of Coxeter polytopes in the hyperbolic 4-space, on one hand, and the combinatorics of simplicial complexes, on the other. This allows us to obtain a universal upper bound on the minimal volume of a hyperbolic 4-manifold realising a given finite group G as its isometry group in terms of the order of the group. We also obtain asymptotic bounds for the growth rate, with respect to volume, of the number of hyperbolic 4-manifolds having a finite group G as their isometry group. -
Hyperbolic Geometry, Fuchsian Groups, and Tiling Spaces
HYPERBOLIC GEOMETRY, FUCHSIAN GROUPS, AND TILING SPACES C. OLIVARES Abstract. Expository paper on hyperbolic geometry and Fuchsian groups. Exposition is based on utilizing the group action of hyperbolic isometries to discover facts about the space across models. Fuchsian groups are character- ized, and applied to construct tilings of hyperbolic space. Contents 1. Introduction1 2. The Origin of Hyperbolic Geometry2 3. The Poincar´eDisk Model of 2D Hyperbolic Space3 3.1. Length in the Poincar´eDisk4 3.2. Groups of Isometries in Hyperbolic Space5 3.3. Hyperbolic Geodesics6 4. The Half-Plane Model of Hyperbolic Space 10 5. The Classification of Hyperbolic Isometries 14 5.1. The Three Classes of Isometries 15 5.2. Hyperbolic Elements 17 5.3. Parabolic Elements 18 5.4. Elliptic Elements 18 6. Fuchsian Groups 19 6.1. Defining Fuchsian Groups 20 6.2. Fuchsian Group Action 20 Acknowledgements 26 References 26 1. Introduction One of the goals of geometry is to characterize what a space \looks like." This task is difficult because a space is just a non-empty set endowed with an axiomatic structure|a list of rules for its points to follow. But, a priori, there is nothing that a list of axioms tells us about the curvature of a space, or what a circle, triangle, or other classical shapes would look like in a space. Moreover, the ways geometry manifests itself vary wildly according to changes in the axioms. As an example, consider the following: There are two spaces, with two different rules. In one space, planets are round, and in the other, planets are flat. -
Apollonian Circle Packings: Dynamics and Number Theory
APOLLONIAN CIRCLE PACKINGS: DYNAMICS AND NUMBER THEORY HEE OH Abstract. We give an overview of various counting problems for Apol- lonian circle packings, which turn out to be related to problems in dy- namics and number theory for thin groups. This survey article is an expanded version of my lecture notes prepared for the 13th Takagi lec- tures given at RIMS, Kyoto in the fall of 2013. Contents 1. Counting problems for Apollonian circle packings 1 2. Hidden symmetries and Orbital counting problem 7 3. Counting, Mixing, and the Bowen-Margulis-Sullivan measure 9 4. Integral Apollonian circle packings 15 5. Expanders and Sieve 19 References 25 1. Counting problems for Apollonian circle packings An Apollonian circle packing is one of the most of beautiful circle packings whose construction can be described in a very simple manner based on an old theorem of Apollonius of Perga: Theorem 1.1 (Apollonius of Perga, 262-190 BC). Given 3 mutually tangent circles in the plane, there exist exactly two circles tangent to all three. Figure 1. Pictorial proof of the Apollonius theorem 1 2 HEE OH Figure 2. Possible configurations of four mutually tangent circles Proof. We give a modern proof, using the linear fractional transformations ^ of PSL2(C) on the extended complex plane C = C [ f1g, known as M¨obius transformations: a b az + b (z) = ; c d cz + d where a; b; c; d 2 C with ad − bc = 1 and z 2 C [ f1g. As is well known, a M¨obiustransformation maps circles in C^ to circles in C^, preserving angles between them. -
On Eigenvalues of Geometrically Finite Hyperbolic Manifolds With
On Eigenvalues of Geometrically Finite Hyperbolic Manifolds with Infinite Volume Xiaolong Hans Han April 6, 2020 Abstract Let M be an oriented geometrically finite hyperbolic manifold of dimension n ≥ 3 with infinite volume. Then for all k ≥ 0, we provide a lower bound on the k-th eigenvalue of the Laplacian operator acting on functions on M by a constant and the k-th eigenvalue of some neighborhood Mf of the thick part of the convex core. 1. Introduction As analytic data of a manifold, the spectrum of the Laplacian operator acting on func- tions contains rich information about the geometry and topology of a manifold. For example, by results of Cheeger and Buser, with a lower bound on Ricci curvature, the first eigenvalue is equivalent to the Cheeger constant of a manifold, which depends on the geometry of the manifold. The rigidity and richness of hyperbolic geometry make the connection even more intriguing: by Canary [4], for infinite volume, topologically tame hyperbolic 3-manifolds, the 2 bottom of the L -spectrum of −∆, denoted by λ0, is zero if and only if the manifold is not geometrically finite. If λ0 of a geometrically finite, infinite volume hyperbolic manifold is 1, by Canary and Burger [2], the manifold is either the topological interior of a handlebody or an R-bundle over a closed surface, which is a very strong topological restriction. Conversely, if we have data about the geometry of a manifold, we can convert it into data about its spectrum, like lower bounds on eigenvalues, dimensions of eigenspaces, existence of embedded eigenvalues, etc. -
Geodesic Planes in Hyperbolic 3-Manifolds
Geodesic planes in hyperbolic 3-manifolds Curtis T. McMullen, Amir Mohammadi and Hee Oh 28 April 2015 Abstract This paper initiates the study of rigidity for immersed, totally geodesic planes in hyperbolic 3-manifolds M of infinite volume. In the case of an acylindrical 3-manifold whose convex core has totally geodesic boundary, we show that the closure of any geodesic plane is a properly immersed submanifold of M. On the other hand, we show that rigidity fails for quasifuchsian manifolds. Contents 1 Introduction . 1 2 Background . 8 3 Fuchsian groups . 10 4 Zariski dense Kleinian groups . 12 5 Influence of a Fuchsian subgroup . 16 6 Convex cocompact Kleinian groups . 17 7 Acylindrical manifolds . 19 8 Unipotent blowup . 21 9 No exotic circles . 25 10 Thin Cantor sets . 31 11 Isolation and finiteness . 31 A Appendix: Quasifuchsian groups . 34 B Appendix: Bounded geodesic planes . 36 Research supported in part by the Alfred P. Sloan Foundation (A.M.) and the NSF. Typeset 2020-09-23 11:37. 1 Introduction 3 Let M = ΓnH be an oriented complete hyperbolic 3-manifold, presented as the quotient of hyperbolic space by the action of a Kleinian group ∼ + 3 Γ ⊂ G = PGL2(C) = Isom (H ): Let 2 f : H ! M be a geodesic plane, i.e. a totally geodesic immersion of a hyperbolic plane into M. 2 We often identify a geodesic plane with its image, P = f(H ). One can regard P as a 2{dimensional version of a Riemannian geodesic. It is natural to ask what the possibilities are for its closure, V = f(H2) ⊂ M: When M has finite volume, Shah and Ratner showed that strong rigidity properties hold: either V = M or V is a properly immersed surface of finite area [Sh], [Rn2]. -
ISOMETRY TRANSFORMATIONS of HYPERBOLIC 3-MANIFOLDS Sadayoshi KOJIMA 0. Introduction by a Hyperbolic Manifold, We Mean a Riemanni
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Topology and its Applications 29 (1988) 297-307 297 North-Holland ISOMETRY TRANSFORMATIONS OF HYPERBOLIC 3-MANIFOLDS Sadayoshi KOJIMA Department of Information Science, Tokyo Institute of Technology, Ohokayama, Meguro, Tokyo, Japan Received 1 December 1986 Revised 10 June 1987 The isometry group of a compact hyperbolic manifold is known to be finite. We show that every finite group is realized as the full isometry group of some compact hyperbolic 3-manifold. AMS (MOS) Subj. Class.: 57S17, 53C25, 57M99 3-manifold hyperbolic manifold isometry 0. Introduction By a hyperbolic manifold, we mean a Riemannian manifold with constant sectional curvature -1. It is known by several ways that the isometry group of a hyperbolic manifold of finite volume is finite. On the other hand, Greenberg has shown in [3] that every finite group is realized as the full conformal automorphism group of some Riemann surface of hyperbolic type. Since such a Riemann surface, which is a 2-manifold with a conformal structure, inherits a unique conformally equivalent hyperbolic structure through the uniformization theorem, there are no limitations on the group structure of the full isometry group of a hyperbolic manifold in dimension 2. In this paper, we first give a quick proof of the theorem of Greenberg quoted above, and then along the same line we show, raising the dimension by one. Theorem. Every jinite group is realized as the full isometry group of some closed hyperbolic 3 -manifold. An immediate corollary to this is the following. -
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.