Differentiable Manifolds
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Differential Geometry: Curvature and Holonomy Austin Christian
University of Texas at Tyler Scholar Works at UT Tyler Math Theses Math Spring 5-5-2015 Differential Geometry: Curvature and Holonomy Austin Christian Follow this and additional works at: https://scholarworks.uttyler.edu/math_grad Part of the Mathematics Commons Recommended Citation Christian, Austin, "Differential Geometry: Curvature and Holonomy" (2015). Math Theses. Paper 5. http://hdl.handle.net/10950/266 This Thesis is brought to you for free and open access by the Math at Scholar Works at UT Tyler. It has been accepted for inclusion in Math Theses by an authorized administrator of Scholar Works at UT Tyler. For more information, please contact [email protected]. DIFFERENTIAL GEOMETRY: CURVATURE AND HOLONOMY by AUSTIN CHRISTIAN A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science Department of Mathematics David Milan, Ph.D., Committee Chair College of Arts and Sciences The University of Texas at Tyler May 2015 c Copyright by Austin Christian 2015 All rights reserved Acknowledgments There are a number of people that have contributed to this project, whether or not they were aware of their contribution. For taking me on as a student and learning differential geometry with me, I am deeply indebted to my advisor, David Milan. Without himself being a geometer, he has helped me to develop an invaluable intuition for the field, and the freedom he has afforded me to study things that I find interesting has given me ample room to grow. For introducing me to differential geometry in the first place, I owe a great deal of thanks to my undergraduate advisor, Robert Huff; our many fruitful conversations, mathematical and otherwise, con- tinue to affect my approach to mathematics. -
Tensor Calculus and Differential Geometry
Course Notes Tensor Calculus and Differential Geometry 2WAH0 Luc Florack March 10, 2021 Cover illustration: papyrus fragment from Euclid’s Elements of Geometry, Book II [8]. Contents Preface iii Notation 1 1 Prerequisites from Linear Algebra 3 2 Tensor Calculus 7 2.1 Vector Spaces and Bases . .7 2.2 Dual Vector Spaces and Dual Bases . .8 2.3 The Kronecker Tensor . 10 2.4 Inner Products . 11 2.5 Reciprocal Bases . 14 2.6 Bases, Dual Bases, Reciprocal Bases: Mutual Relations . 16 2.7 Examples of Vectors and Covectors . 17 2.8 Tensors . 18 2.8.1 Tensors in all Generality . 18 2.8.2 Tensors Subject to Symmetries . 22 2.8.3 Symmetry and Antisymmetry Preserving Product Operators . 24 2.8.4 Vector Spaces with an Oriented Volume . 31 2.8.5 Tensors on an Inner Product Space . 34 2.8.6 Tensor Transformations . 36 2.8.6.1 “Absolute Tensors” . 37 CONTENTS i 2.8.6.2 “Relative Tensors” . 38 2.8.6.3 “Pseudo Tensors” . 41 2.8.7 Contractions . 43 2.9 The Hodge Star Operator . 43 3 Differential Geometry 47 3.1 Euclidean Space: Cartesian and Curvilinear Coordinates . 47 3.2 Differentiable Manifolds . 48 3.3 Tangent Vectors . 49 3.4 Tangent and Cotangent Bundle . 50 3.5 Exterior Derivative . 51 3.6 Affine Connection . 52 3.7 Lie Derivative . 55 3.8 Torsion . 55 3.9 Levi-Civita Connection . 56 3.10 Geodesics . 57 3.11 Curvature . 58 3.12 Push-Forward and Pull-Back . 59 3.13 Examples . 60 3.13.1 Polar Coordinates in the Euclidean Plane . -
Lecture Note on Elementary Differential Geometry
Lecture Note on Elementary Differential Geometry Ling-Wei Luo* Institute of Physics, Academia Sinica July 20, 2019 Abstract This is a note based on a course of elementary differential geometry as I gave the lectures in the NCTU-Yau Journal Club: Interplay of Physics and Geometry at Department of Electrophysics in National Chiao Tung University (NCTU) in Spring semester 2017. The contents of remarks, supplements and examples are highlighted in the red, green and blue frame boxes respectively. The supplements can be omitted at first reading. The basic knowledge of the differential forms can be found in the lecture notes given by Dr. Sheng-Hong Lai (NCTU) and Prof. Jen-Chi Lee (NCTU) on the website. The website address of Interplay of Physics and Geometry is http: //web.it.nctu.edu.tw/~string/journalclub.htm or http://web.it.nctu. edu.tw/~string/ipg/. Contents 1 Curve on E2 ......................................... 1 2 Curve in E3 .......................................... 6 3 Surface theory in E3 ..................................... 9 4 Cartan’s moving frame and exterior differentiation methods .............. 31 1 Curve on E2 We define n-dimensional Euclidean space En as a n-dimensional real space Rn equipped a dot product defined n-dimensional vector space. Tangent vector In 2-dimensional Euclidean space, an( E2 plane,) we parametrize a curve p(t) = x(t); y(t) by one parameter t with re- spect to a reference point o with a fixed Cartesian coordinate frame. The( velocity) vector at point p is given by p_ (t) = x_(t); y_(t) with the norm Figure 1: A curve. p p jp_ (t)j = p_ · p_ = x_ 2 +y _2 ; (1) *Electronic address: [email protected] 1 where x_ := dx/dt. -
DISCRETE DIFFERENTIAL GEOMETRY: an APPLIED INTRODUCTION Keenan Crane • CMU 15-458/858 LECTURE 10: INTRODUCTION to CURVES
DISCRETE DIFFERENTIAL GEOMETRY: AN APPLIED INTRODUCTION Keenan Crane • CMU 15-458/858 LECTURE 10: INTRODUCTION TO CURVES DISCRETE DIFFERENTIAL GEOMETRY: AN APPLIED INTRODUCTION Keenan Crane • CMU 15-458/858 Curves & Surfaces •Much of the geometry we encounter in life well-described by curves and surfaces* (Curves) *Or solids… but the boundary of a solid is a surface! (Surfaces) Much Ado About Manifolds • In general, differential geometry studies n-dimensional manifolds; we’ll focus on low dimensions: curves (n=1), surfaces (n=2), and volumes (n=3) • Why? Geometry we encounter in everyday life/applications • Low-dimensional manifolds are not “baby stuff!” • n=1: unknot recognition (open as of 2021) • n=2: Willmore conjecture (2012 for genus 1) • n=3: Geometrization conjecture (2003, $1 million) • Serious intuition gained by studying low-dimensional manifolds • Conversely, problems involving very high-dimensional manifolds (e.g., data analysis/machine learning) involve less “deep” geometry than you might imagine! • fiber bundles, Lie groups, curvature flows, spinors, symplectic structure, ... • Moreover, curves and surfaces are beautiful! (And in some cases, high- dimensional manifolds have less interesting structure…) Smooth Descriptions of Curves & Surfaces •Many ways to express the geometry of a curve or surface: •height function over tangent plane •local parameterization •Christoffel symbols — coordinates/indices •differential forms — “coordinate free” •moving frames — change in adapted frame •Riemann surfaces (local); Quaternionic functions -
The Ricci Curvature of Rotationally Symmetric Metrics
The Ricci curvature of rotationally symmetric metrics Anna Kervison Supervisor: Dr Artem Pulemotov The University of Queensland 1 1 Introduction Riemannian geometry is a branch of differential non-Euclidean geometry developed by Bernhard Riemann, used to describe curved space. In Riemannian geometry, a manifold is a topological space that locally resembles Euclidean space. This means that at any point on the manifold, there exists a neighbourhood around that point that appears ‘flat’and could be mapped into the Euclidean plane. For example, circles are one-dimensional manifolds but a figure eight is not as it cannot be pro- jected into the Euclidean plane at the intersection. Surfaces such as the sphere and the torus are examples of two-dimensional manifolds. The shape of a manifold is defined by the Riemannian metric, which is a measure of the length of tangent vectors and curves in the manifold. It can be thought of as locally a matrix valued function. The Ricci curvature is one of the most sig- nificant geometric characteristics of a Riemannian metric. It provides a measure of the curvature of the manifold in much the same way the second derivative of a single valued function provides a measure of the curvature of a graph. Determining the Ricci curvature of a metric is difficult, as it is computed from a lengthy ex- pression involving the derivatives of components of the metric up to order two. In fact, without additional simplifications, the formula for the Ricci curvature given by this definition is essentially unmanageable. Rn is one of the simplest examples of a manifold. -
2 a Patch of an Open Friedmann-Robertson-Walker Universe
Total Mass of a Patch of a Matter-Dominated Friedmann-Robertson-Walker Universe by Sarah Geller B.S., Massachusetts Institute of Technology (2013) Submitted to the Department of Physics in partial fulfillment of the requirements for the degree of Masters of Science in Physics at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 2017 Massachusetts Institute of Technology 2017. All rights reserved. j A I A A Signature redacted Author ... Department of Physics May 31, 2017 Signature redacted C ertified by ....... ...................... Alan H. Guth V F Weisskopf Professor of Physics and MacVicar Faculty Fellow Thesis Supervisor Accepted by ..... Signature redacted Nergis Mavalvala MASSACHUETT INSTITUTE Associate Department Head of Physics OF TECHNOLOGY (0W JUN 2 7 2017 r LIBRARIES 2 Total Mass of a Patch of a Matter-Dominated Friedmann-Robertson-Walker Universe by Sarah Geller Submitted to the Department of Physics on May 31, 2017, in partial fulfillment of the requirements for the degree of Masters of Science in Physics Abstract In this thesis, I have addressed the question of how to calculate the total relativistic mass for a patch of a spherically-symmetric matter-dominated spacetime of nega- tive curvature. This calculation provides the open-universe analogue to a similar calculation first proposed by Zel'dovich in 1962. I consider a finite, spherically- symmetric (SO(3)) spatial region of a Friedmann-Robertson-Walker (FRW) universe surrounded with a vacuum described by the Schwarzschild metric. Provided that the patch of FRW spacetime is glued along its boundary to a Schwarzschild spacetime in a sufficiently smooth manner, the result is a spatial region of FRW which transitions smoothly to an asymptotically flat exterior region such that spherical symmetry is preserved throughout. -
INTRODUCTION to MANIFOLDS Contents 1. Differentiable Curves 1
INTRODUCTION TO MANIFOLDS TSOGTGEREL GANTUMUR Abstract. We discuss manifolds embedded in Rn and the implicit function theorem. Contents 1. Differentiable curves 1 2. Manifolds 3 3. The implicit function theorem 6 4. The preimage theorem 10 5. Tangent spaces 12 1. Differentiable curves Intuitively, a differentiable curves is a curve with the property that the tangent line at each of its points can be defined. To motivate our definition, let us look at some examples. Example 1.1. (a) Consider the function γ : (0; π) ! R2 defined by ( ) cos t γ(t) = : (1) sin t As t varies in the interval (0; π), the point γ(t) traces out the curve C = [γ] ≡ fγ(t): t 2 (0; π)g ⊂ R2; (2) which is a semicircle (without its endpoints). We call γ a parameterization of C. If γ(t) represents the coordinates of a particle in the plane at time t, then the \instantaneous velocity vector" of the particle at the time moment t is given by ( ) 0 − sin t γ (t) = : (3) cos t Obviously, γ0(t) =6 0 for all t 2 (0; π), and γ is smooth (i.e., infinitely often differentiable). The direction of the velocity vector γ0(t) defines the direction of the line tangent to C at the point p = γ(t). (b) Under the substitution t = s2, we obtain a different parameterization of C, given by ( ) cos s2 η(s) ≡ γ(s2) = : (4) sin s2 p Note that the parameter s must take values in (0; π). (c) Now consider the function ξ : [0; π] ! R2 defined by ( ) cos t ξ(t) = : (5) sin t Date: 2016/11/12 10:49 (EDT). -
Symbols 1-Form, 10 4-Acceleration, 184 4-Force, 115 4-Momentum, 116
Index Symbols B 1-form, 10 Betti number, 589 4-acceleration, 184 Bianchi type-I models, 448 4-force, 115 Bianchi’s differential identities, 60 4-momentum, 116 complex valued, 532–533 total, 122 consequences of in Newman-Penrose 4-velocity, 114 formalism, 549–551 first contracted, 63 second contracted, 63 A bicharacteristic curves, 620 acceleration big crunch, 441 4-acceleration, 184 big-bang cosmological model, 438, 449 Newtonian, 74 Birkhoff’s theorem, 271 action function or functional bivector space, 486 (see also Lagrangian), 594, 598 black hole, 364–433 ADM action, 606 Bondi-Metzner-Sachs group, 240 affine parameter, 77, 79 boost, 110 alternating operation, antisymmetriza- Born-Infeld (or tachyonic) scalar field, tion, 27 467–471 angle field, 44 Boyer-Lindquist coordinate chart, 334, anisotropic fluid, 218–220, 276 399 collapse, 424–431 Brinkman-Robinson-Trautman met- ric, 514 anti-de Sitter space-time, 195, 644, Buchdahl inequality, 262 663–664 bugle, 69 anti-self-dual, 671 antisymmetric oriented tensor, 49 C antisymmetric tensor, 28 canonical energy-momentum-stress ten- antisymmetrization, 27 sor, 119 arc length parameter, 81 canonical or normal forms, 510 arc separation function, 85 Cartesian chart, 44, 68 arc separation parameter, 77 Casimir effect, 638 Arnowitt-Deser-Misner action integral, Cauchy horizon, 403, 416 606 Cauchy problem, 207 atlas, 3 Cauchy-Kowalewski theorem, 207 complete, 3 causal cone, 108 maximal, 3 causal space-time, 663 698 Index 699 causality violation, 663 contravariant index, 51 characteristic hypersurface, 623 contravariant -
Catalogue of Spacetimes
Catalogue of Spacetimes e2 e1 x2 = 2 x = 2 q ∂x2 1 x2 = 1 ∂x1 x1 = 1 x1 = 0 x2 = 0 M Authors: Thomas Müller Visualisierungsinstitut der Universität Stuttgart (VISUS) Allmandring 19, 70569 Stuttgart, Germany [email protected] Frank Grave formerly, Universität Stuttgart, Institut für Theoretische Physik 1 (ITP1) Pfaffenwaldring 57 //IV, 70550 Stuttgart, Germany [email protected] URL: http://go.visus.uni-stuttgart.de/CoS Date: 21. Mai 2014 Co-authors Andreas Lemmer, formerly, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Alcubierre Warp Sebastian Boblest, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart deSitter, Friedmann-Robertson-Walker Felix Beslmeisl, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Petrov-Type D Heiko Munz, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Bessel and plane wave Andreas Wünsch, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Majumdar-Papapetrou, extreme Reissner-Nordstrøm dihole, energy momentum tensor Many thanks to all that have reported bug fixes or added metric descriptions. Contents 1 Introduction and Notation1 1.1 Notation...............................................1 1.2 General remarks...........................................1 1.3 Basic objects of a metric......................................2 1.4 Natural local tetrad and initial conditions for geodesics....................3 1.4.1 Orthonormality condition.................................3 1.4.2 Tetrad transformations...................................4 -
Cambridge University Press 978-1-108-47122-0 — Mathematics for Physicists Alexander Altland , Jan Von Delft Index More Information
Cambridge University Press 978-1-108-47122-0 — Mathematics for Physicists Alexander Altland , Jan von Delft Index More Information Index δ-function basis Gaussian representation, 273 definition, 30 qualitative discussion, 272 local, 418 ǫ–δ criterion, 208 orientation, 96 ∃, there exists, 7 orthonormal, 43, 50 ∀, for all,7 bilinear form, 156 ´ , symbol, 217 bin, 218 n-tuple, 34 bit, 8 Abel, Nils Henrik, 8 calculus, 205 absolute value, 17 canonical, 32 action principle, 334 Cantor, Georg Ferdinand Ludwig Philipp, 13 affine space Cartesian product, 13 definition, 26 Cauchy theorem, 344 Euclidean, 26 Cauchy, Augustin-Louis, 339 point, 25 Cauchy–Schwarz inequality, 40 chaos algebra definition, 325 definition, 71 fractal dimension, 325 Grassmann, 161 Lyapunov exponent, 325 alternating form strange attractor, 325 exterior product, 161 characteristic polynomial, 101 maximal degree, 158 closure of degree p, 157 group operation, 7 one-form, 150 interval, 17 pullback, 163 set, 17 top-form, 158 co- and contravariant transformation, 152 volume form, 165 commutator, 183 wedge product, 161 completeness Ampère’s law, 457 relation, 134 analysis, 205 vectors, 30 angle complex conjugate, 15 azimuthal, 423 complex function between vectors, 40 analytic, 338 polar, 423 branch cut, 356 angular momentum, 152 branch point, 356 ansatz, 42 contour integral, 342 anti-derivative, 220 definition, 338 antisymmetric symbol, 12 extended singularity, 346 area element holomorphic, 338 definition, 245 meromorphic, 347 polar coordinates, 246 pole, 347 asymptotic expansion, 267 singularity, -
DIFFERENTIAL GEOMETRY of CURVES and SURFACES 7. Geodesics and the Theorem of Gauss-Bonnet 7.1
DIFFERENTIAL GEOMETRY OF CURVES AND SURFACES 7. Geodesics and the Theorem of Gauss-Bonnet 7.1. Geodesics on a Surface. The goal of this section is to give an answer to the following question. Question. What kind of curves on a given surface should be the analogues of straight lines in the plane? Let’s understand first what means “straight” line in the plane. If you want to go from a point in a plane “straight” to another one, your trajectory will be such a line. In other words, a straight line has the property that if we fix two points P and Q on it, then the piece of between P Land Q is the shortest curve in the plane which joins the two points. Now, if insteadL of a plane (“flat” surface) you need to go from P to Q in a land with hills and valleys (arbitrary surface), which path will you take? This is how the notion of geodesic line arises: “Definition” 7.1.1. Let S be a surface. A curve α : I S parametrized by arc length → is called a geodesic if for any two points P = α(s1), Q = α(s2) on the curve which are sufficiently close to each other, the piece of the trace of α between P and Q is the shortest of all curves in S which join P and Q. There are at least two inconvenients concerning this definition: first, why did we say that P and Q are “sufficiently close to each other”?; second, this definition will certainly not allow us to do any explicit examples (for instance, find the geodesics on a hyperbolic paraboloid). -
Space Curves
AML710 CAD LECTURE 11 SPACE CURVES Space Curves Intrinsic properties Synthetic curves SPACE CURVES A curve which may pass through any region of three- dimensional space, as contrasted to a plane curve which must lie on a single plane. Space curves are very general form of curves ¾ The generation of curves is a problem of curve fitting for given set of points or approximating a curve for these data points ¾ Curve Applications Many real engineering designs need curved mechanical parts, civil engineering designs, architectural designs, aeronautics, ship building ¾ Synthetic Curves The limitations of the analytic curves prompt us to study the synthetic curves 1 SPACE CURVES - Definitions ¾ Curve definition A continuously differentiable curve (function) is called smooth. To define the curvature it is convenient to use the Frenet frame, which is actually a pair of orthogonal coordinates having origin at the point of interest, P. n b P t Frenet Frame ¾ Curvature dt Frenet formulae = k(s).v(s).n(s) ds dn Binormal b=txn = −k(s).v(s).t(s) ds SPACE CURVES An example of a space curve A helix can be generated by the following parametric relations x = r cost y = r sin t z = bt r,b ≠ 0, − ∞ ≤ t ≤ ∞ 50 40 30 20 10 0 5 5 0 0 -5 -5 2 SPACE CURVES Exercise 1 A cubical parabola can be generated by the following parametric relations. Generate the space curve and also its components (x,t), (y,t) and (z,t). x = t y = t 2 z = t 3 0 ≤ t ≤1 SPACE CURVES Another example of a space curve The seam on a tennis ball can be generated by the following parametric relations