Models of 2-Dimensional Hyperbolic Space and Relations Among Them; Hyperbolic Length, Lines, and Distances
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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). -
More on Parallel and Perpendicular Lines
More on Parallel and Perpendicular Lines By Ma. Louise De Las Peñas et’s look at more problems on parallel and perpendicular lines. The following results, presented Lin the article, “About Slope” will be used to solve the problems. Theorem 1. Let L1 and L2 be two distinct nonvertical lines with slopes m1 and m2, respectively. Then L1 is parallel to L2 if and only if m1 = m2. Theorem 2. Let L1 and L2 be two distinct nonvertical lines with slopes m1 and m2, respectively. Then L1 is perpendicular to L2 if and only if m1m2 = -1. Example 1. The perpendicular bisector of a segment is the line which is perpendicular to the segment at its midpoint. Find equations of the three perpendicular bisectors of the sides of a triangle with vertices at A(-4,1), B(4,5) and C(4,-3). Solution: Consider the triangle with vertices A(-4,1), B(4,5) and C(4,-3), and the midpoints E, F, G of sides AB, BC, and AC, respectively. TATSULOK FirstSecond Year Year Vol. Vol. 12 No.12 No. 1a 2a e-Pages 1 In this problem, our aim is to fi nd the equations of the lines which pass through the midpoints of the sides of the triangle and at the same time are perpendicular to the sides of the triangle. Figure 1 The fi rst step is to fi nd the midpoint of every side. The next step is to fi nd the slope of the lines containing every side. The last step is to obtain the equations of the perpendicular bisectors. -
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. -
A Survey on the Square Peg Problem
A survey on the Square Peg Problem Benjamin Matschke∗ March 14, 2014 Abstract This is a short survey article on the 102 years old Square Peg Problem of Toeplitz, which is also called the Inscribed Square Problem. It asks whether every continuous simple closed curve in the plane contains the four vertices of a square. This article first appeared in a more compact form in Notices Amer. Math. Soc. 61(4), 2014. 1 Introduction In 1911 Otto Toeplitz [66] furmulated the following conjecture. Conjecture 1 (Square Peg Problem, Toeplitz 1911). Every continuous simple closed curve in the plane γ : S1 ! R2 contains four points that are the vertices of a square. Figure 1: Example for Conjecture1. A continuous simple closed curve in the plane is also called a Jordan curve, and it is the same as an injective map from the unit circle into the plane, or equivalently, a topological embedding S1 ,! R2. Figure 2: We do not require the square to lie fully inside γ, otherwise there are counter- examples. ∗Supported by Deutsche Telekom Stiftung, NSF Grant DMS-0635607, an EPDI-fellowship, and MPIM Bonn. This article is licensed under a Creative Commons BY-NC-SA 3.0 License. 1 In its full generality Toeplitz' problem is still open. So far it has been solved affirmatively for curves that are \smooth enough", by various authors for varying smoothness conditions, see the next section. All of these proofs are based on the fact that smooth curves inscribe generically an odd number of squares, which can be measured in several topological ways. -
A Historical Introduction to Elementary Geometry
i MATH 119 – Fall 2012: A HISTORICAL INTRODUCTION TO ELEMENTARY GEOMETRY Geometry is an word derived from ancient Greek meaning “earth measure” ( ge = earth or land ) + ( metria = measure ) . Euclid wrote the Elements of geometry between 330 and 320 B.C. It was a compilation of the major theorems on plane and solid geometry presented in an axiomatic style. Near the beginning of the first of the thirteen books of the Elements, Euclid enumerated five fundamental assumptions called postulates or axioms which he used to prove many related propositions or theorems on the geometry of two and three dimensions. POSTULATE 1. Any two points can be joined by a straight line. POSTULATE 2. Any straight line segment can be extended indefinitely in a straight line. POSTULATE 3. Given any straight line segment, a circle can be drawn having the segment as radius and one endpoint as center. POSTULATE 4. All right angles are congruent. POSTULATE 5. (Parallel postulate) If two lines intersect a third in such a way that the sum of the inner angles on one side is less than two right angles, then the two lines inevitably must intersect each other on that side if extended far enough. The circle described in postulate 3 is tacitly unique. Postulates 3 and 5 hold only for plane geometry; in three dimensions, postulate 3 defines a sphere. Postulate 5 leads to the same geometry as the following statement, known as Playfair's axiom, which also holds only in the plane: Through a point not on a given straight line, one and only one line can be drawn that never meets the given line. -
Geometry Course Outline
GEOMETRY COURSE OUTLINE Content Area Formative Assessment # of Lessons Days G0 INTRO AND CONSTRUCTION 12 G-CO Congruence 12, 13 G1 BASIC DEFINITIONS AND RIGID MOTION Representing and 20 G-CO Congruence 1, 2, 3, 4, 5, 6, 7, 8 Combining Transformations Analyzing Congruency Proofs G2 GEOMETRIC RELATIONSHIPS AND PROPERTIES Evaluating Statements 15 G-CO Congruence 9, 10, 11 About Length and Area G-C Circles 3 Inscribing and Circumscribing Right Triangles G3 SIMILARITY Geometry Problems: 20 G-SRT Similarity, Right Triangles, and Trigonometry 1, 2, 3, Circles and Triangles 4, 5 Proofs of the Pythagorean Theorem M1 GEOMETRIC MODELING 1 Solving Geometry 7 G-MG Modeling with Geometry 1, 2, 3 Problems: Floodlights G4 COORDINATE GEOMETRY Finding Equations of 15 G-GPE Expressing Geometric Properties with Equations 4, 5, Parallel and 6, 7 Perpendicular Lines G5 CIRCLES AND CONICS Equations of Circles 1 15 G-C Circles 1, 2, 5 Equations of Circles 2 G-GPE Expressing Geometric Properties with Equations 1, 2 Sectors of Circles G6 GEOMETRIC MEASUREMENTS AND DIMENSIONS Evaluating Statements 15 G-GMD 1, 3, 4 About Enlargements (2D & 3D) 2D Representations of 3D Objects G7 TRIONOMETRIC RATIOS Calculating Volumes of 15 G-SRT Similarity, Right Triangles, and Trigonometry 6, 7, 8 Compound Objects M2 GEOMETRIC MODELING 2 Modeling: Rolling Cups 10 G-MG Modeling with Geometry 1, 2, 3 TOTAL: 144 HIGH SCHOOL OVERVIEW Algebra 1 Geometry Algebra 2 A0 Introduction G0 Introduction and A0 Introduction Construction A1 Modeling With Functions G1 Basic Definitions and Rigid -
1 Euclidean Geometry
Dr. Anna Felikson, Durham University Geometry, 26.02.2015 Outline 1 Euclidean geometry 1.1 Isometry group of Euclidean plane, Isom(E2). A distance on a space X is a function d : X × X ! R,(A; B) 7! d(A; B) for A; B 2 X satisfying 1. d(A; B) ≥ 0 (d(A; B) = 0 , A = B); 2. d(A; B) = d(B; A); 3. d(A; C) ≤ d(A; B) + d(B; C) (triangle inequality). We will use two models of Euclidean plane: p 2 2 a Cartesian plane: f(x; y) j x; y 2 Rg with the distance d(A1;A2) = (x1 − x2) + (y1 − y2) ; a Gaussian plane: fz j z 2 Cg, with the distance d(u; v) = ju − vj. Definition 1.1. A Euclidean isometry is a distance-preserving transformation of E2, i.e. a map f : E2 ! E2 satisfying d(f(A); f(B)) = d(A; B). Corollary 1.2. (a) Every isometry of E2 is a one-to-one map. (b) The composition of any two isometries is an isometry. (c) Isometries of E2 form a group (denoted Isom(E2)). Example 1.3: Translation, rotation, reflection in a line are isometries. Theorem 1.4. Let ABC and A0B0C0 be two congruent triangles. Then there exists a unique isometry sending A to A0, B to B0 and C to C0. Corollary 1.5. Every isometry of E2 is a composition of at most 3 reflections. (In particular, the group Isom(E2) is generated by reflections). Remark: the way to write an isometry as a composition of reflection is not unique. -
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]. -
Hyperbolic Geometry on a Hyperboloid, the American Mathematical Monthly, 100:5, 442-455, DOI: 10.1080/00029890.1993.11990430
William F. Reynolds (1993) Hyperbolic Geometry on a Hyperboloid, The American Mathematical Monthly, 100:5, 442-455, DOI: 10.1080/00029890.1993.11990430. (c) 1993 The American Mathematical Monthly 1985 Mathematics Subject Classification 51 M 10 HYPERBOLIC GEOMETRY ON A HYPERBOLOID William F. Reynolds Department of Mathematics, Tufts University, Medford, MA 02155 E-mail: [email protected] 1. Introduction. Hardly anyone would maintain that it is better to begin to learn geography from flat maps than from a globe. But almost all introductions to hyperbolic non-Euclidean geometry, except [6], present plane models, such as the projective and conformal disk models, without even mentioning that there exists a model that has the same relation to plane models that a globe has to flat maps. This model, which is on one sheet of a hyperboloid of two sheets in Minkowski 3-space and which I shall call H2, is over a hundred years old; Killing and Poincar´eboth described it in the 1880's (see Section 14). It is used by differential geometers [29, p. 4] and physicists (see [21, pp. 724-725] and [23, p. 113]). Nevertheless it is not nearly so well known as it should be, probably because, like a globe, it requires three dimensions. The main advantages of this model are its naturalness and its symmetry. Being embeddable (distance function and all) in flat space-time, it is close to our picture of physical reality, and all its points are treated alike in this embedding. Once the strangeness of the Minkowski metric is accepted, it has the familiar geometry of a sphere in Euclidean 3-space E3 as a guide to definitions and arguments. -
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. -
Hyperbolic Geometry, Surfaces, and 3-Manifolds Bruno Martelli
Hyperbolic geometry, surfaces, and 3-manifolds Bruno Martelli Dipartimento di Matematica \Tonelli", Largo Pontecorvo 5, 56127 Pisa, Italy E-mail address: martelli at dm dot unipi dot it version: december 18, 2013 Contents Introduction 1 Copyright notices 1 Chapter 1. Preliminaries 3 1. Differential topology 3 1.1. Differentiable manifolds 3 1.2. Tangent space 4 1.3. Differentiable submanifolds 6 1.4. Fiber bundles 6 1.5. Tangent and normal bundle 6 1.6. Immersion and embedding 7 1.7. Homotopy and isotopy 7 1.8. Tubolar neighborhood 7 1.9. Manifolds with boundary 8 1.10. Cut and paste 8 1.11. Transversality 9 2. Riemannian geometry 9 2.1. Metric tensor 9 2.2. Distance, geodesics, volume. 10 2.3. Exponential map 11 2.4. Injectivity radius 12 2.5. Completeness 13 2.6. Curvature 13 2.7. Isometries 15 2.8. Isometry group 15 2.9. Riemannian manifolds with boundary 16 2.10. Local isometries 16 3. Measure theory 17 3.1. Borel measure 17 3.2. Topology on the measure space 18 3.3. Lie groups 19 3.4. Haar measures 19 4. Algebraic topology 19 4.1. Group actions 19 4.2. Coverings 20 4.3. Discrete groups of isometries 20 v vi CONTENTS 4.4. Cell complexes 21 4.5. Aspherical cell-complexes 22 Chapter 2. Hyperbolic space 25 1. The models of hyperbolic space 25 1.1. Hyperboloid 25 1.2. Isometries of the hyperboloid 26 1.3. Subspaces 27 1.4. The Poincar´edisc 29 1.5. The half-space model 31 1.6.