Theorem. In terms of the coordinate frame, the Levi-Civita connection is given by:
|
|
- Kelley Lloyd
- 5 years ago
- Views:
Transcription
1 THE LEVI-CIVITA CONNECTION FOR THE POINCARÉ METRIC We denote complex numbers z = x + yi C where x, y R. Let H 2 denote the upper half-plane with the Poincaré metric: {x + iy x, y R, y > 0} g = dz 2 y 2 We compute the Levi-Civita connection with respect to several different frames. 1. The usual coordinate system on H 2 Let x, y be the coordinate vector fields, so that: 1) 2) g x, x ) = g y, y ) = y 1 g x, y ) = g y, x ) = 0. The vector fields define an orthonormal frame field. ξ := y 1 x η := y 1 y Theorem. In terms of the coordinate frame, the Levi-Civita connection is given by: 3) 4) 5) 6) x x = y 1 y x y = y 1 x y x = y 1 x y y = y 1 y Date: wmg, July 17,
2 2 LEVI-CIVITA CONNECTION In terms of the orthonormal frame, the Levi-Civita connection is given by: ξ ξ = η ξ η = ξ η ξ = 0 η η = 0 Proof. Orthonormality implies gy x, y x ) = 1 is constant, whence and 0 = y gy x, y x ) = 2g y y x ), y x ) = 2yg y y x ), x ) = 2yg x, x ) + yg y x, x )) = 2yy 1 + yg y x ), x ) 7) g y x, x ) = y 3. Differentiating the constant gy y, y ) with respect to x: 8) 0 = 2 x g x y, x ) whence 9) g y x, x ) = 0. Since is symmetric, 10) x y = y x. Combining 9) with 10): g x y, y ) = y 3 and combining with 8), yields 4). Applying 10) again yields 5). Differentiating gy x, y x ) = 1 with respect to x yields: 11) g x x, x ) = 0 Similarly, differentiating with respect to y ; 12) g x x, x ) = y 3 which implies 3). Differentiating gy x, y y ) = 0 with respect to y yields: 13) g y y, x ) = 0 Similarly, 0 = y g y, y ) implies; 14) g y y, y ) = y 3
3 LEVI-CIVITA CONNECTION 3 which implies 6). The routine calculations for the orthonormal frame are omitted. 2. Connection 1-form for orthonormal frame Denote the coframe field dual to the orthonormal frame by: ξ := ydx η := ydy. The covariant differentials of the orthonormal frame are: so the connection form is: [ ] 0 ξ ξ 0 ξ = η ξ η = ξ ξ = y 1 dx [ ] Geodesic curvature of a hypercycle We use these to calculate the geodesic curvature of a hypercycle. The positive imaginary axis ir + is a geodesic with endpoints 0,. The Euclidean rays from 0 subtending an angle θ with ir + are hypercycles re iθ = r cosθ) + i sinθ) ) = r tanhρ) + i sechρ) ) at distance ρ from ir +. The point x 0 + i has coordinates The curve x 0 = tanhρ) sechρ) = sinhρ). γt) := e t x 0 + i) has velocity vector and speed, respectively: 15) γ t) := e t x 0 x + y ) = x 0 ξ + η γ t) = 1 + x 2 0 We compute the accelaration of γt): D dt γt) = x 0 ξ+ηx 0 ξ + η) = x 2 0η x 0 ξ
4 4 LEVI-CIVITA CONNECTION Now reparametrize γt) by unit speed: γt) := x0 e t x 0 + i) and the geodesic curve is the tangential component of the acceleration: D dt γt) = x 0 x 2 0 η x 0 ξ ) which, since γt) has constant speed, equals: D dt γt) = x x 2 0 = sinθ) = tanhρ) Similarly the geodesic curvature of a metric circle of radius ρ equals cothρ). To see this, use the Poincare unit disc model: for z < 1, the metric tensor is: g := 4 dz 2 1 z 2 ) 2 and writing hyperbolic polar coordinates) z = e iθ tanhρ/2) the metric tensor is g = dρ 2 + sinh 2 ρ)dθ 2, with area form da = sinh 2 ρ)dρ dθ. Consider a disc D ρ with hyperbolic) radius ρ. Then its circumference equals 2π sinhρ) and its area 2πcoshρ) 1. Let k g be the geodesic curvature of the metric circle D ρ. Applying the Gauss-Bonnet theorem 2πχΣ) = KdA + k g ds to σ = D ρ obtaining: Σ Σ 2π = 2π coshρ) 1) + k g 2π sinhρ) ), that is, k g = cothρ) as desired.
5 LEVI-CIVITA CONNECTION 5 4. Fermi coordinates around a geodesic Another convenient coordinate system begins with a geodesic and considers the family of geodesics orthogonal to this one. Let u denote the parameter along the geodesic, and v the parameter along the perpendiculars: x = e u tanhv) y = e u sechv). Then sinhv) = x/y and z = x 2 + y 2 = e u and u = 1 2 logx2 + y 2 ). Writing with metric tensor The coordinate 1-forms are: and dual coodinate vector fields: z = e u tanhv) + i sechv)) dz = zdu + i sechv)dv) dz 2 = z 2 du 2 + sech 2 v)dv 2) g = dz 2 y 2 = cosh 2 v)du 2 + dv 2. du = x 2 + y 2 ) 1 x dx + y dy) dv = x 2 + y 2 ) 1/2 y dx x/y dy) u = x x + y y v = yx 2 + y 2 ) 1/2 y x x y ). 5. The Levi-Civita connection in Fermi coordinates Using the coordinates u, v) R 2 with metric tensor g = cosh 2 v)du 2 + dv 2 as above, we compute the Christoffel symbols of the Levi-Civita connection. Since u, v are coordinates, the corresponding vector fields u, v commute: [ u, v ] = 0 and since has zero torsion, u v = v u. Since all the inner products of this basis are constant except for g u, u ), 0 = u g u, v) = v g u, v) = u g v, v) = v g v, v) and g is parallel with respect to, implies v v = 0
6 6 LEVI-CIVITA CONNECTION and differentiating g u, u ) = cosh 2 v) yields u v = v u = tanhv) u u u = sinhv) coshv) v One can modify this coordinate basis to an orhonormal basis by replacing u by U := sechv) u, in which the covariant derivatives are: U U) = tanhv) v, v U) = 0, U v ) = tanhv)u, v v ) = Geodesic curvature in Fermi coordinates Let γt) = ut), vt) ) be a curve. Its velocity is: γ t) = u t) u + v t) v and the square of its speed is: ) 2 ds = u t) cosh 2 vt) ) + v t) 2 dt Its acceleration is: D dt γ t) = u t) + tanh ) vt))u t)v t) u + v t) + tanh vt))u t)v t) u t) 2 cosh vt) ) sinh vt) )) u
7 The cigar soliton, the Rosenau solution, and moving frame calculations
7 The cigar soliton, the Rosenau solution, and moving frame calculations When making local calculations of the connection and curvature, one has the choice of either using local coordinates or moving frames.
More informationUNIVERSITY OF DUBLIN
UNIVERSITY OF DUBLIN TRINITY COLLEGE JS & SS Mathematics SS Theoretical Physics SS TSM Mathematics Faculty of Engineering, Mathematics and Science school of mathematics Trinity Term 2015 Module MA3429
More informationPractice Final Solutions
Practice Final Solutions Math 1, Fall 17 Problem 1. Find a parameterization for the given curve, including bounds on the parameter t. Part a) The ellipse in R whose major axis has endpoints, ) and 6, )
More information1. Geometry of the unit tangent bundle
1 1. Geometry of the unit tangent bundle The main reference for this section is [8]. In the following, we consider (M, g) an n-dimensional smooth manifold endowed with a Riemannian metric g. 1.1. Notations
More informationPart IB GEOMETRY (Lent 2016): Example Sheet 1
Part IB GEOMETRY (Lent 2016): Example Sheet 1 (a.g.kovalev@dpmms.cam.ac.uk) 1. Suppose that H is a hyperplane in Euclidean n-space R n defined by u x = c for some unit vector u and constant c. The reflection
More informationDifferential Geometry Exercises
Differential Geometry Exercises Isaac Chavel Spring 2006 Jordan curve theorem We think of a regular C 2 simply closed path in the plane as a C 2 imbedding of the circle ω : S 1 R 2. Theorem. Given the
More informationPart IB. Geometry. Year
Part IB Year 2017 2016 2015 2014 2013 2012 2011 2010 2009 2008 2007 2006 2005 2004 2003 2002 2001 2017 17 Paper 1, Section I 3G Give the definition for the area of a hyperbolic triangle with interior angles
More informationIntrinsic Geometry. Andrejs Treibergs. Friday, March 7, 2008
Early Research Directions: Geometric Analysis II Intrinsic Geometry Andrejs Treibergs University of Utah Friday, March 7, 2008 2. References Part of a series of thee lectures on geometric analysis. 1 Curvature
More informationExercise 1 (Formula for connection 1-forms) Using the first structure equation, show that
1 Stokes s Theorem Let D R 2 be a connected compact smooth domain, so that D is a smooth embedded circle. Given a smooth function f : D R, define fdx dy fdxdy, D where the left-hand side is the integral
More informationMathematical Relativity, Spring 2017/18 Instituto Superior Técnico
Mathematical Relativity, Spring 2017/18 Instituto Superior Técnico 1. Starting from R αβµν Z ν = 2 [α β] Z µ, deduce the components of the Riemann curvature tensor in terms of the Christoffel symbols.
More informationHyperbolic Geometry on Geometric Surfaces
Mathematics Seminar, 15 September 2010 Outline Introduction Hyperbolic geometry Abstract surfaces The hemisphere model as a geometric surface The Poincaré disk model as a geometric surface Conclusion Introduction
More informationEquidistant curve coordinate system. Morio Kikuchi
Equidistant curve coordinate system Morio Kiuchi Abstract: An isometry is realized between Poincaré dis of which radius is not limited to 1 and upper half-plane. Poincaré metrics are the same in both regions
More informationPart IB Geometry. Theorems. Based on lectures by A. G. Kovalev Notes taken by Dexter Chua. Lent 2016
Part IB Geometry Theorems Based on lectures by A. G. Kovalev Notes taken by Dexter Chua Lent 2016 These notes are not endorsed by the lecturers, and I have modified them (often significantly) after lectures.
More informationRule ST1 (Symmetry). α β = β α for 1-forms α and β. Like the exterior product, the symmetric tensor product is also linear in each slot :
2. Metrics as Symmetric Tensors So far we have studied exterior products of 1-forms, which obey the rule called skew symmetry: α β = β α. There is another operation for forming something called the symmetric
More informationworked out from first principles by parameterizing the path, etc. If however C is a A path C is a simple closed path if and only if the starting point
III.c Green s Theorem As mentioned repeatedly, if F is not a gradient field then F dr must be worked out from first principles by parameterizing the path, etc. If however is a simple closed path in the
More informationTutorial Exercises: Geometric Connections
Tutorial Exercises: Geometric Connections 1. Geodesics in the Isotropic Mercator Projection When the surface of the globe is projected onto a flat map some aspects of the map are inevitably distorted.
More informationSELECTED SAMPLE FINAL EXAM SOLUTIONS - MATH 5378, SPRING 2013
SELECTED SAMPLE FINAL EXAM SOLUTIONS - MATH 5378, SPRING 03 Problem (). This problem is perhaps too hard for an actual exam, but very instructional, and simpler problems using these ideas will be on the
More informationWilliam P. Thurston. The Geometry and Topology of Three-Manifolds
William P. Thurston The Geometry and Topology of Three-Manifolds Electronic version 1.1 - March 00 http://www.msri.org/publications/books/gt3m/ This is an electronic edition of the 1980 notes distributed
More informationd F = (df E 3 ) E 3. (4.1)
4. The Second Fundamental Form In the last section we developed the theory of intrinsic geometry of surfaces by considering the covariant differential d F, that is, the tangential component of df for a
More informationProblem 1, Lorentz transformations of electric and magnetic
Problem 1, Lorentz transformations of electric and magnetic fields We have that where, F µν = F µ ν = L µ µ Lν ν F µν, 0 B 3 B 2 ie 1 B 3 0 B 1 ie 2 B 2 B 1 0 ie 3 ie 2 ie 2 ie 3 0. Note that we use the
More informationMath 23b Practice Final Summer 2011
Math 2b Practice Final Summer 211 1. (1 points) Sketch or describe the region of integration for 1 x y and interchange the order to dy dx dz. f(x, y, z) dz dy dx Solution. 1 1 x z z f(x, y, z) dy dx dz
More informationChapter 7 Curved Spacetime and General Covariance
Chapter 7 Curved Spacetime and General Covariance In this chapter we generalize the discussion of preceding chapters to extend covariance to more general curved spacetimes. 145 146 CHAPTER 7. CURVED SPACETIME
More informationHomework for Math , Spring 2012
Homework for Math 6170 1, Spring 2012 Andres Treibergs, Instructor April 24, 2012 Our main text this semester is Isaac Chavel, Riemannian Geometry: A Modern Introduction, 2nd. ed., Cambridge, 2006. Please
More informationGeneral Relativity ASTR 2110 Sarazin. Einstein s Equation
General Relativity ASTR 2110 Sarazin Einstein s Equation Curvature of Spacetime 1. Principle of Equvalence: gravity acceleration locally 2. Acceleration curved path in spacetime In gravitational field,
More informationHadamard s Theorem. Rich Schwartz. September 10, The purpose of these notes is to prove the following theorem.
Hadamard s Theorem Rich Schwartz September 10, 013 1 The Result and Proof Outline The purpose of these notes is to prove the following theorem. Theorem 1.1 (Hadamard) Let M 1 and M be simply connected,
More informationHyperbolic Discrete Ricci Curvature Flows
Hyperbolic Discrete Ricci Curvature Flows 1 1 Mathematics Science Center Tsinghua University Tsinghua University 010 Unified Framework of Discrete Curvature Flow Unified framework for both Discrete Ricci
More informationPlane hyperbolic geometry
2 Plane hyperbolic geometry In this chapter we will see that the unit disc D has a natural geometry, known as plane hyperbolic geometry or plane Lobachevski geometry. It is the local model for the hyperbolic
More informationThe Geometry of Relativity
The Geometry of Relativity Tevian Dray Department of Mathematics Oregon State University http://www.math.oregonstate.edu/~tevian OSU 4/27/15 Tevian Dray The Geometry of Relativity 1/27 Books The Geometry
More information8.821 String Theory Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 8.81 String Theory Fall 008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.81 F008 Lecture 11: CFT continued;
More informationMTH4101 CALCULUS II REVISION NOTES. 1. COMPLEX NUMBERS (Thomas Appendix 7 + lecture notes) ax 2 + bx + c = 0. x = b ± b 2 4ac 2a. i = 1.
MTH4101 CALCULUS II REVISION NOTES 1. COMPLEX NUMBERS (Thomas Appendix 7 + lecture notes) 1.1 Introduction Types of numbers (natural, integers, rationals, reals) The need to solve quadratic equations:
More informationChapter 14. Basics of The Differential Geometry of Surfaces. Introduction. Parameterized Surfaces. The First... Home Page. Title Page.
Chapter 14 Basics of The Differential Geometry of Surfaces Page 649 of 681 14.1. Almost all of the material presented in this chapter is based on lectures given by Eugenio Calabi in an upper undergraduate
More informationPractice Problems for Exam 3 (Solutions) 1. Let F(x, y) = xyi+(y 3x)j, and let C be the curve r(t) = ti+(3t t 2 )j for 0 t 2. Compute F dr.
1. Let F(x, y) xyi+(y 3x)j, and let be the curve r(t) ti+(3t t 2 )j for t 2. ompute F dr. Solution. F dr b a 2 2 F(r(t)) r (t) dt t(3t t 2 ), 3t t 2 3t 1, 3 2t dt t 3 dt 1 2 4 t4 4. 2. Evaluate the line
More informationThe Geometry of Relativity
The Geometry of Relativity Tevian Dray Department of Mathematics Oregon State University http://www.math.oregonstate.edu/~tevian PNWMAA 4/11/15 Tevian Dray The Geometry of Relativity 1/25 Books The Geometry
More informationClassical differential geometry of two-dimensional surfaces
Classical differential geometry of two-dimensional surfaces 1 Basic definitions This section gives an overview of the basic notions of differential geometry for twodimensional surfaces. It follows mainly
More informationINTRODUCTION TO GEOMETRY
INTRODUCTION TO GEOMETRY ERIKA DUNN-WEISS Abstract. This paper is an introduction to Riemannian and semi-riemannian manifolds of constant sectional curvature. We will introduce the concepts of moving frames,
More information(b) Find the range of h(x, y) (5) Use the definition of continuity to explain whether or not the function f(x, y) is continuous at (0, 0)
eview Exam Math 43 Name Id ead each question carefully. Avoid simple mistakes. Put a box around the final answer to a question (use the back of the page if necessary). For full credit you must show your
More informationMath 5378, Differential Geometry Solutions to practice questions for Test 2
Math 5378, Differential Geometry Solutions to practice questions for Test 2. Find all possible trajectories of the vector field w(x, y) = ( y, x) on 2. Solution: A trajectory would be a curve (x(t), y(t))
More informationHYPERBOLIC GEOMETRY AND PARALLEL TRANSPORT IN R 2 +
HYPERBOLIC GEOMETRY ND PRLLEL TRNSPORT IN R + VINCENT GLORIOSO, BRITTNY LNDRY, ND PHILLIP WHITE bstract. We will examine the parallel transport of tangent vectors along a hyperbolic triangle containing
More informationDIFFERENTIAL GEOMETRY HW 5
DIFFERENTIAL GEOMETRY HW 5 CLAY SHONKWILER 1 Check the calculations above that the Gaussian curvature of the upper half-plane and Poincaré disk models of the hyperbolic plane is 1. Proof. The calculations
More informationA local characterization for constant curvature metrics in 2-dimensional Lorentz manifolds
A local characterization for constant curvature metrics in -dimensional Lorentz manifolds Ivo Terek Couto Alexandre Lymberopoulos August 9, 8 arxiv:65.7573v [math.dg] 4 May 6 Abstract In this paper we
More informationMAT 211 Final Exam. Spring Jennings. Show your work!
MAT 211 Final Exam. pring 215. Jennings. how your work! Hessian D = f xx f yy (f xy ) 2 (for optimization). Polar coordinates x = r cos(θ), y = r sin(θ), da = r dr dθ. ylindrical coordinates x = r cos(θ),
More informationReview problems for the final exam Calculus III Fall 2003
Review problems for the final exam alculus III Fall 2003 1. Perform the operations indicated with F (t) = 2t ı 5 j + t 2 k, G(t) = (1 t) ı + 1 t k, H(t) = sin(t) ı + e t j a) F (t) G(t) b) F (t) [ H(t)
More informationMath 20C Homework 2 Partial Solutions
Math 2C Homework 2 Partial Solutions Problem 1 (12.4.14). Calculate (j k) (j + k). Solution. The basic properties of the cross product are found in Theorem 2 of Section 12.4. From these properties, we
More informationMetrics and Curvature
Metrics and Curvature How to measure curvature? Metrics Euclidian/Minkowski Curved spaces General 4 dimensional space Cosmological principle Homogeneity and isotropy: evidence Robertson-Walker metrics
More informationPhysics 236a assignment, Week 2:
Physics 236a assignment, Week 2: (October 8, 2015. Due on October 15, 2015) 1. Equation of motion for a spin in a magnetic field. [10 points] We will obtain the relativistic generalization of the nonrelativistic
More informationArc Length and Riemannian Metric Geometry
Arc Length and Riemannian Metric Geometry References: 1 W F Reynolds, Hyperbolic geometry on a hyperboloid, Amer Math Monthly 100 (1993) 442 455 2 Wikipedia page Metric tensor The most pertinent parts
More informationPhysics 325: General Relativity Spring Final Review Problem Set
Physics 325: General Relativity Spring 2012 Final Review Problem Set Date: Friday 4 May 2012 Instructions: This is the third of three review problem sets in Physics 325. It will count for twice as much
More information9 Gauss Differential Geometry and the Pseudo-Sphere
9 Gauss Differential Geometry and the Pseudo-Sphere 9.1 Introduction Through the work of Gauss on differential geometry, it became clear after a painfully slow historic process that there is a model of
More informationTensors - Lecture 4. cos(β) sin(β) sin(β) cos(β) 0
1 Introduction Tensors - Lecture 4 The concept of a tensor is derived from considering the properties of a function under a transformation of the corrdinate system. As previously discussed, such transformations
More informationEQUATIONS OF MOTION: NORMAL AND TANGENTIAL COORDINATES (Section 13.5)
EQUATIONS OF MOTION: NORMAL AND TANGENTIAL COORDINATES (Section 13.5) Today s Objectives: Students will be able to apply the equation of motion using normal and tangential coordinates. APPLICATIONS Race
More informationDifferential Geometry II Lecture 1: Introduction and Motivation
Differential Geometry II Lecture 1: Introduction and Motivation Robert Haslhofer 1 Content of this lecture This course is on Riemannian geometry and the geometry of submanifol. The goal of this first lecture
More informationf dr. (6.1) f(x i, y i, z i ) r i. (6.2) N i=1
hapter 6 Integrals In this chapter we will look at integrals in more detail. We will look at integrals along a curve, and multi-dimensional integrals in 2 or more dimensions. In physics we use these integrals
More information1 + f 2 x + f 2 y dy dx, where f(x, y) = 2 + 3x + 4y, is
1. The value of the double integral (a) 15 26 (b) 15 8 (c) 75 (d) 105 26 5 4 0 1 1 + f 2 x + f 2 y dy dx, where f(x, y) = 2 + 3x + 4y, is 2. What is the value of the double integral interchange the order
More informationDO NOT BEGIN THIS TEST UNTIL INSTRUCTED TO START
Math 265 Student name: KEY Final Exam Fall 23 Instructor & Section: This test is closed book and closed notes. A (graphing) calculator is allowed for this test but cannot also be a communication device
More informationCURVILINEAR MOTION: NORMAL AND TANGENTIAL COMPONENTS
CURVILINEAR MOTION: NORMAL AND TANGENTIAL COMPONENTS Today s Objectives: Students will be able to: 1. Determine the normal and tangential components of velocity and acceleration of a particle traveling
More informationSyllabus. May 3, Special relativity 1. 2 Differential geometry 3
Syllabus May 3, 2017 Contents 1 Special relativity 1 2 Differential geometry 3 3 General Relativity 13 3.1 Physical Principles.......................................... 13 3.2 Einstein s Equation..........................................
More informationIntroduction to Differential Geometry
More about Introduction to Differential Geometry Lecture 7 of 10: Dominic Joyce, Oxford University October 2018 EPSRC CDT in Partial Differential Equations foundation module. These slides available at
More informationMLC Practice Final Exam
Name: Section: Recitation/Instructor: INSTRUCTIONS Fill in your name, etc. on this first page. Without fully opening the exam, check that you have pages 1 through 13. Show all your work on the standard
More informationChristoffel Symbols. 1 In General Topologies. Joshua Albert. September 28, W. First we say W : λ n = x µ (λ) so that the world
Christoffel Symbols Joshua Albert September 28, 22 In General Topoloies We have a metric tensor nm defined by, Note by some handy theorem that for almost any continuous function F (L), equation 2 still
More informationENGI 4430 Parametric Vector Functions Page dt dt dt
ENGI 4430 Parametric Vector Functions Page 2-01 2. Parametric Vector Functions (continued) Any non-zero vector r can be decomposed into its magnitude r and its direction: r rrˆ, where r r 0 Tangent Vector:
More informationDerivatives in General Relativity
Derivatives in General Relativity One of the problems with curved space is in dealing with vectors how do you add a vector at one point in the surface of a sphere to a vector at a different point, and
More informationj=1 ωj k E j. (3.1) j=1 θj E j, (3.2)
3. Cartan s Structural Equations and the Curvature Form Let E,..., E n be a moving (orthonormal) frame in R n and let ωj k its associated connection forms so that: de k = n ωj k E j. (3.) Recall that ωj
More information8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS
8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS Lecturer: McGreevy Scribe: Francesco D Eramo October 16, 2008 Today: 1. the boundary of AdS 2. Poincaré patch 3. motivate boundary
More informationEuler Characteristic of Two-Dimensional Manifolds
Euler Characteristic of Two-Dimensional Manifolds M. Hafiz Khusyairi August 2008 In this work we will discuss an important notion from topology, namely Euler Characteristic and we will discuss several
More informationGeometric Modelling Summer 2016
Geometric Modelling Summer 2016 Exercises Benjamin Karer M.Sc. http://gfx.uni-kl.de/~gm Benjamin Karer M.Sc. Geometric Modelling Summer 2016 1 Dierential Geometry Benjamin Karer M.Sc. Geometric Modelling
More informationSpacetime and 4 vectors
Spacetime and 4 vectors 1 Minkowski space = 4 dimensional spacetime Euclidean 4 space Each point in Minkowski space is an event. In SR, Minkowski space is an absolute structure (like space in Newtonian
More informationMATHS 267 Answers to Stokes Practice Dr. Jones
MATH 267 Answers to tokes Practice Dr. Jones 1. Calculate the flux F d where is the hemisphere x2 + y 2 + z 2 1, z > and F (xz + e y2, yz, z 2 + 1). Note: the surface is open (doesn t include any of the
More informationInstructions: No books. No notes. Non-graphing calculators only. You are encouraged, although not required, to show your work.
Exam 3 Math 850-007 Fall 04 Odenthal Name: Instructions: No books. No notes. Non-graphing calculators only. You are encouraged, although not required, to show your work.. Evaluate the iterated integral
More informationHyperbolic Analytic Geometry
Chapter 6 Hyperbolic Analytic Geometry 6.1 Saccheri Quadrilaterals Recall the results on Saccheri quadrilaterals from Chapter 4. Let S be a convex quadrilateral in which two adjacent angles are right angles.
More informationMATH 4030 Differential Geometry Lecture Notes Part 4 last revised on December 4, Elementary tensor calculus
MATH 4030 Differential Geometry Lecture Notes Part 4 last revised on December 4, 205 Elementary tensor calculus We will study in this section some basic multilinear algebra and operations on tensors. Let
More informationHomework for Math , Spring 2008
Homework for Math 4530 1, Spring 2008 Andrejs Treibergs, Instructor April 18, 2008 Please read the relevant sections in the text Elementary Differential Geometry by Andrew Pressley, Springer, 2001. You
More informationSolutions to old Exam 3 problems
Solutions to old Exam 3 problems Hi students! I am putting this version of my review for the Final exam review here on the web site, place and time to be announced. Enjoy!! Best, Bill Meeks PS. There are
More informationMTH4101 Calculus II. Carl Murray School of Mathematical Sciences Queen Mary University of London Spring Lecture Notes
MTH40 Calculus II Carl Murray School of Mathematical Sciences Queen Mary University of London Spring 20 Lecture Notes Complex Numbers. Introduction We have already met several types of numbers. Natural
More information274 Curves on Surfaces, Lecture 4
274 Curves on Surfaces, Lecture 4 Dylan Thurston Notes by Qiaochu Yuan Fall 2012 4 Hyperbolic geometry Last time there was an exercise asking for braids giving the torsion elements in PSL 2 (Z). A 3-torsion
More informationIs there a magnification paradox in gravitational lensing?
Is there a magnification paradox in gravitational lensing? Olaf Wucknitz wucknitz@astro.uni-bonn.de Astrophysics seminar/colloquium, Potsdam, 26 November 2007 Is there a magnification paradox in gravitational
More informationMAY THE FORCE BE WITH YOU, YOUNG JEDIS!!!
Final Exam Math 222 Spring 2011 May 11, 2011 Name: Recitation Instructor s Initials: You may not use any type of calculator whatsoever. (Cell phones off and away!) You are not allowed to have any other
More informationOn the cosmic no-hair conjecture in the Einstein-Vlasov setting
On the cosmic no-hair conjecture in the Einstein-Vlasov setting KTH, Royal Institute of Technology, Stockholm Recent Advances in Mathematical General Relativity Institut Henri Poincaré, Paris September
More informationReview Sheet for the Final
Review Sheet for the Final Math 6-4 4 These problems are provided to help you study. The presence of a problem on this handout does not imply that there will be a similar problem on the test. And the absence
More informationfor 2 1/3 < t 3 1/3 parametrizes
Solution to Set 4, due Friday April 1) Section 5.1, Problem ) Explain why the path parametrized by ft) = t, t 1 ) is not smooth. Note this is true more specifically if the interval of t contains t = 1
More informationMath 132 Information for Test 2
Math 13 Information for Test Test will cover material from Sections 5.6, 5.7, 5.8, 6.1, 6., 6.3, 7.1, 7., and 7.3. The use of graphing calculators will not be allowed on the test. Some practice questions
More informationSec. 1.1: Basics of Vectors
Sec. 1.1: Basics of Vectors Notation for Euclidean space R n : all points (x 1, x 2,..., x n ) in n-dimensional space. Examples: 1. R 1 : all points on the real number line. 2. R 2 : all points (x 1, x
More informationMath 211, Fall 2014, Carleton College
A. Let v (, 2, ) (1,, ) 1, 2, and w (,, 3) (1,, ) 1,, 3. Then n v w 6, 3, 2 is perpendicular to the plane, with length 7. Thus n/ n 6/7, 3/7, 2/7 is a unit vector perpendicular to the plane. [The negation
More informationx + ye z2 + ze y2, y + xe z2 + ze x2, z and where T is the
1.(8pts) Find F ds where F = x + ye z + ze y, y + xe z + ze x, z and where T is the T surface in the pictures. (The two pictures are two views of the same surface.) The boundary of T is the unit circle
More information7a3 2. (c) πa 3 (d) πa 3 (e) πa3
1.(6pts) Find the integral x, y, z d S where H is the part of the upper hemisphere of H x 2 + y 2 + z 2 = a 2 above the plane z = a and the normal points up. ( 2 π ) Useful Facts: cos = 1 and ds = ±a sin
More information1. (30 points) In the x-y plane, find and classify all local maxima, local minima, and saddle points of the function. f(x, y) = 3y 2 2y 3 3x 2 + 6xy.
APPM 35 FINAL EXAM FALL 13 INSTUTIONS: Electronic devices, books, and crib sheets are not permitted. Write your name and your instructor s name on the front of your bluebook. Work all problems. Show your
More information1. (a) (5 points) Find the unit tangent and unit normal vectors T and N to the curve. r (t) = 3 cos t, 0, 3 sin t, r ( 3π
1. a) 5 points) Find the unit tangent and unit normal vectors T and N to the curve at the point P 3, 3π, r t) 3 cos t, 4t, 3 sin t 3 ). b) 5 points) Find curvature of the curve at the point P. olution:
More information1 First and second variational formulas for area
1 First and second variational formulas for area In this chapter, we will derive the first and second variational formulas for the area of a submanifold. This will be useful in our later discussion on
More information27. Folds (I) I Main Topics A What is a fold? B Curvature of a plane curve C Curvature of a surface 10/10/18 GG303 1
I Main Topics A What is a fold? B Curvature of a plane curve C Curvature of a surface 10/10/18 GG303 1 http://upload.wikimedia.org/wikipedia/commons/a/ae/caledonian_orogeny_fold_in_king_oscar_fjord.jpg
More informationNIL. Let M be R 3 equipped with the metric in which the following vector. fields, U = and. are an orthonormal basis.
NIL KEVIN WHYTE Let M be R 3 equipped with the metric in which the following vector fields: U = x + y z V = y and W = z are an orthonormal basis. 1. Preliminaries Since we re given the metric via an orthonormal
More informationQuantum Black Hole and Information. Lecture (1): Acceleration, Horizon, Black Hole
Quantum Black Hole and Information Soo-Jong Rey @ copyright Lecture (1): Acceleration, Horizon, Black Hole [Convention: c = 1. This can always be reinstated from dimensional analysis.] Today, we shall
More informationWithout fully opening the exam, check that you have pages 1 through 12.
MTH 34 Solutions to Exam April 9th, 8 Name: Section: Recitation Instructor: INSTRUTIONS Fill in your name, etc. on this first page. Without fully opening the exam, check that you have pages through. Show
More informationEinstein Toolkit Workshop. Joshua Faber Apr
Einstein Toolkit Workshop Joshua Faber Apr 05 2012 Outline Space, time, and special relativity The metric tensor and geometry Curvature Geodesics Einstein s equations The Stress-energy tensor 3+1 formalisms
More informationMath 350 Solutions for Final Exam Page 1. Problem 1. (10 points) (a) Compute the line integral. F ds C. z dx + y dy + x dz C
Math 35 Solutions for Final Exam Page Problem. ( points) (a) ompute the line integral F ds for the path c(t) = (t 2, t 3, t) with t and the vector field F (x, y, z) = xi + zj + xk. (b) ompute the line
More informationSpecial Relativity. Chapter The geometry of space-time
Chapter 1 Special Relativity In the far-reaching theory of Special Relativity of Einstein, the homogeneity and isotropy of the 3-dimensional space are generalized to include the time dimension as well.
More informationNEW LIFTS OF SASAKI TYPE OF THE RIEMANNIAN METRICS
NEW LIFTS OF SASAKI TYPE OF THE RIEMANNIAN METRICS Radu Miron Abstract One defines new elliptic and hyperbolic lifts to tangent bundle T M of a Riemann metric g given on the base manifold M. They are homogeneous
More informationProperties of the Pseudosphere
Properties of the Pseudosphere Simon Rubinstein Salzedo May 25, 2004 Euclidean, Hyperbolic, and Elliptic Geometries Euclid began his study of geometry with five axioms. They are. Exactly one line may drawn
More informationMath 234 Exam 3 Review Sheet
Math 234 Exam 3 Review Sheet Jim Brunner LIST OF TOPIS TO KNOW Vector Fields lairaut s Theorem & onservative Vector Fields url Divergence Area & Volume Integrals Using oordinate Transforms hanging the
More informationWithout fully opening the exam, check that you have pages 1 through 10.
MTH 234 Solutions to Exam 2 April 11th 216 Name: Section: Recitation Instructor: INSTRUTIONS Fill in your name, etc. on this first page. Without fully opening the exam, check that you have pages 1 through
More informationTensors, and differential forms - Lecture 2
Tensors, and differential forms - Lecture 2 1 Introduction The concept of a tensor is derived from considering the properties of a function under a transformation of the coordinate system. A description
More informationSolutions to Practice Test 3
Solutions to Practice Test 3. (a) Find the equation for the plane containing the points (,, ), (, 2, ), and (,, 3). (b) Find the area of the triangle with vertices (,, ), (, 2, ), and (,, 3). Answer: (a)
More information