Matching Nature with 'Complex Geometry' – an Architectural History
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Quadratic Approximation at a Stationary Point Let F(X, Y) Be a Given
Multivariable Calculus Grinshpan Quadratic approximation at a stationary point Let f(x; y) be a given function and let (x0; y0) be a point in its domain. Under proper differentiability conditions one has f(x; y) = f(x0; y0) + fx(x0; y0)(x − x0) + fy(x0; y0)(y − y0) 1 2 1 2 + 2 fxx(x0; y0)(x − x0) + fxy(x0; y0)(x − x0)(y − y0) + 2 fyy(x0; y0)(y − y0) + higher−order terms: Let (x0; y0) be a stationary (critical) point of f: fx(x0; y0) = fy(x0; y0) = 0. Then 2 2 f(x; y) = f(x0; y0) + A(x − x0) + 2B(x − x0)(y − y0) + C(y − y0) + higher−order terms, 1 1 1 1 where A = 2 fxx(x0; y0);B = 2 fxy(x0; y0) = 2 fyx(x0; y0), and C = 2 fyy(x0; y0). Assume for simplicity that (x0; y0) = (0; 0) and f(0; 0) = 0. [ This can always be achieved by translation: f~(x; y) = f(x0 + x; y0 + y) − f(x0; y0). ] Then f(x; y) = Ax2 + 2Bxy + Cy2 + higher−order terms. Thus, provided A, B, C are not all zero, the graph of f near (0; 0) resembles the quadric surface z = Ax2 + 2Bxy + Cy2: Generically, this quadric surface is either an elliptic or a hyperbolic paraboloid. We distinguish three scenarios: * Elliptic paraboloid opening up, (0; 0) is a point of local minimum. * Elliptic paraboloid opening down, (0; 0) is a point of local maximum. * Hyperbolic paraboloid, (0; 0) is a saddle point. It should certainly be possible to tell which case we are dealing with by looking at the coefficients A, B, and C, and this is the idea behind the Second Partials Test. -
Chapter 11. Three Dimensional Analytic Geometry and Vectors
Chapter 11. Three dimensional analytic geometry and vectors. Section 11.5 Quadric surfaces. Curves in R2 : x2 y2 ellipse + =1 a2 b2 x2 y2 hyperbola − =1 a2 b2 parabola y = ax2 or x = by2 A quadric surface is the graph of a second degree equation in three variables. The most general such equation is Ax2 + By2 + Cz2 + Dxy + Exz + F yz + Gx + Hy + Iz + J =0, where A, B, C, ..., J are constants. By translation and rotation the equation can be brought into one of two standard forms Ax2 + By2 + Cz2 + J =0 or Ax2 + By2 + Iz =0 In order to sketch the graph of a quadric surface, it is useful to determine the curves of intersection of the surface with planes parallel to the coordinate planes. These curves are called traces of the surface. Ellipsoids The quadric surface with equation x2 y2 z2 + + =1 a2 b2 c2 is called an ellipsoid because all of its traces are ellipses. 2 1 x y 3 2 1 z ±1 ±2 ±3 ±1 ±2 The six intercepts of the ellipsoid are (±a, 0, 0), (0, ±b, 0), and (0, 0, ±c) and the ellipsoid lies in the box |x| ≤ a, |y| ≤ b, |z| ≤ c Since the ellipsoid involves only even powers of x, y, and z, the ellipsoid is symmetric with respect to each coordinate plane. Example 1. Find the traces of the surface 4x2 +9y2 + 36z2 = 36 1 in the planes x = k, y = k, and z = k. Identify the surface and sketch it. Hyperboloids Hyperboloid of one sheet. The quadric surface with equations x2 y2 z2 1. -
Calculus & Analytic Geometry
TQS 126 Spring 2008 Quinn Calculus & Analytic Geometry III Quadratic Equations in 3-D Match each function to its graph 1. 9x2 + 36y2 +4z2 = 36 2. 4x2 +9y2 4z2 =0 − 3. 36x2 +9y2 4z2 = 36 − 4. 4x2 9y2 4z2 = 36 − − 5. 9x2 +4y2 6z =0 − 6. 9x2 4y2 6z =0 − − 7. 4x2 + y2 +4z2 4y 4z +36=0 − − 8. 4x2 + y2 +4z2 4y 4z 36=0 − − − cone • ellipsoid • elliptic paraboloid • hyperbolic paraboloid • hyperboloid of one sheet • hyperboloid of two sheets 24 TQS 126 Spring 2008 Quinn Calculus & Analytic Geometry III Parametric Equations (§10.1) and Vector Functions (§13.1) Definition. If x and y are given as continuous function x = f(t) y = g(t) over an interval of t-values, then the set of points (x, y)=(f(t),g(t)) defined by these equation is a parametric curve (sometimes called aplane curve). The equations are parametric equations for the curve. Often we think of parametric curves as describing the movement of a particle in a plane over time. Examples. x = 2cos t x = et 0 t π 1 t e y = 3sin t ≤ ≤ y = ln t ≤ ≤ Can we find parameterizations of known curves? the line segment circle x2 + y2 =1 from (1, 3) to (5, 1) Why restrict ourselves to only moving through planes? Why not space? And why not use our nifty vector notation? 25 Definition. If x, y, and z are given as continuous functions x = f(t) y = g(t) z = h(t) over an interval of t-values, then the set of points (x,y,z)= (f(t),g(t), h(t)) defined by these equation is a parametric curve (sometimes called a space curve). -
Structural Forms 1
Key principles The hyperboloid of revolution is a Surface and may be generated by revolving a Hyperbola about its conjugate axis. The outline of the elevation will be a Hyperbola. When the conjugate axis is vertical all horizontal sections are circles. The horizontal section at the mid point of the conjugate axis is known as the Throat. The diagram shows the incomplete construction for drawing a hyperbola in a rectangle. (a) Draw the outline of the both branches of the double hyperbola in the rectangle. The diagram shows the incomplete Elevation of a hyperboloid of revolution. (a) Determine the position of the throat circle in elevation. (b) Draw the outline of the both branches of the double hyperbola in elevation. DESIGN & COMMUNICATION GRAPHICS Structural forms 1 NAME: ______________________________ DATE: _____________ The diagram shows the plan and incomplete elevation of an object based on the hyperboloid of revolution. The focal points and transverse axis of the hyperbola are also shown. (a) Using the given information draw the outline of the elevation.. F The diagram shows the axis, focal points and transverse axis of a double hyperbola. (a) Draw the outline of both branches of the double hyperbola. (b) The difference between the focal distances for any point on a double hyperbola is constant and equal to the length of the transverse axis. (c) Indicate this principle on the drawing below. DESIGN & COMMUNICATION GRAPHICS Structural forms 2 NAME: ______________________________ DATE: _____________ Key principles The diagram shows the plan and incomplete elevation of a hyperboloid of revolution. The hyperboloid of revolution may also be generated by revolving one skew line about another. -
Stereographic Projection Patch Kessler, December 12, 2018
Stereographic Projection Patch Kessler, December 12, 2018 Stereographic projection is a way to flatten out the surface of a ball, such as the celestial sphere, which surrounds the earth and contains all the stars in the sky. The celestial sphere gives order out of chaos. It gives a way to predict star locations at different times, as well as the time of night from the stars. Here is a physical model of the celestial sphere from around 1480. 1480-1481, http://www.artfund.org/artwork/3600/spherical-astrolabe 1 According to legend, Ptolemy (AD 90 - AD 168) thought of stereographic projection after a donkey stepped on his model of the celestial sphere, making it flat. Applying stereographic projection to the celestial sphere results in a planar device called an astrolabe. 16th century islamic astrolabe The tips on the perforated upper plate correspond to stars, while points on the lower plate correspond to viewing directions. For instance, the point on the lower plate that the circles are shrinking towards corresponds to the viewing direction directly overhead (i.e., looking straight up). The stereographic projection of a point X on a sphere S is obtained by drawing a line from the north pole of the sphere through X, and continuing on to the plane G that the sphere is resting on. The projection of X is the point f(X) where this line hits the plane. E X S G f(X) 2 One of the most surprising things about stereographic projection is that circles get mapped to circles. P circle on the sphere E S circle in the plane G Circles that pass through the north pole get mapped to lines, however if you think of a line as an infinite radius circle, then you can say that circles get mapped to circles in all cases. -
Quadric Surfaces
Quadric Surfaces Six basic types of quadric surfaces: • ellipsoid • cone • elliptic paraboloid • hyperboloid of one sheet • hyperboloid of two sheets • hyperbolic paraboloid (A) (B) (C) (D) (E) (F) 1. For each surface, describe the traces of the surface in x = k, y = k, and z = k. Then pick the term from the list above which seems to most accurately describe the surface (we haven't learned any of these terms yet, but you should be able to make a good educated guess), and pick the correct picture of the surface. x2 y2 (a) − = z. 9 16 1 • Traces in x = k: parabolas • Traces in y = k: parabolas • Traces in z = k: hyperbolas (possibly a pair of lines) y2 k2 Solution. The trace in x = k of the surface is z = − 16 + 9 , which is a downward-opening parabola. x2 k2 The trace in y = k of the surface is z = 9 − 16 , which is an upward-opening parabola. x2 y2 The trace in z = k of the surface is 9 − 16 = k, which is a hyperbola if k 6= 0 and a pair of lines (a degenerate hyperbola) if k = 0. This surface is called a hyperbolic paraboloid , and it looks like picture (E) . It is also sometimes called a saddle. x2 y2 z2 (b) + + = 1. 4 25 9 • Traces in x = k: ellipses (possibly a point) or nothing • Traces in y = k: ellipses (possibly a point) or nothing • Traces in z = k: ellipses (possibly a point) or nothing y2 z2 k2 k2 Solution. The trace in x = k of the surface is 25 + 9 = 1− 4 . -
(Anti-)De Sitter Space-Time
Geometry of (Anti-)De Sitter space-time Author: Ricard Monge Calvo. Facultat de F´ısica, Universitat de Barcelona, Diagonal 645, 08028 Barcelona, Spain. Advisor: Dr. Jaume Garriga Abstract: This work is an introduction to the De Sitter and Anti-de Sitter spacetimes, as the maximally symmetric constant curvature spacetimes with positive and negative Ricci curvature scalar R. We discuss their causal properties and the characterization of their geodesics, and look at p;q the spaces embedded in flat R spacetimes with an additional dimension. We conclude that the geodesics in these spaces can be regarded as intersections with planes going through the origin of the embedding space, and comment on the consequences. I. INTRODUCTION In the case of dS4, introducing the coordinates (T; χ, θ; φ) given by: Einstein's general relativity postulates that spacetime T T is a differential (Lorentzian) manifold of dimension 4, X0 = a sinh X~ = a cosh ~n (4) a a whose Ricci curvature tensor is determined by its mass- energy contents, according to the equations: where X~ = X1;X2;X3;X4 and ~n = ( cos χ, sin χ cos θ, sin χ sin θ cos φ, sin χ sin θ sin φ) with T 2 (−∞; 1), 0 ≤ 1 8πG χ ≤ π, 0 ≤ θ ≤ π and 0 ≤ φ ≤ 2π, then the line element Rµλ − Rgµλ + Λgµλ = 4 Tµλ (1) 2 c is: where Rµλ is the Ricci curvature tensor, R te Ricci scalar T ds2 = −dT 2 + a2 cosh2 [dχ2 + sin2 χ dΩ2] (5) curvature, gµλ the metric tensor, Λ the cosmological con- a 2 stant, G the universal gravitational constant, c the speed of light in vacuum and Tµλ the energy-momentum ten- where the surfaces of constant time dT = 0 have metric 2 2 2 2 sor. -
Geometric Properties of Central Catadioptric Line Images
Geometric Properties of Central Catadioptric Line Images Jo˜aoP. Barreto and Helder Araujo Institute of Systems and Robotics Dept. of Electrical and Computer Engineering University of Coimbra Coimbra, Portugal {jpbar, helder}@isr.uc.pt http://www.isr.uc.pt/˜jpbar Abstract. It is highly desirable that an imaging system has a single effective viewpoint. Central catadioptric systems are imaging systems that use mirrors to enhance the field of view while keeping a unique center of projection. A general model for central catadioptric image formation has already been established. The present paper exploits this model to study the catadioptric projection of lines. The equations and geometric properties of general catadioptric line imaging are derived. We show that it is possible to determine the position of both the effec- tive viewpoint and the absolute conic in the catadioptric image plane from the images of three lines. It is also proved that it is possible to identify the type of catadioptric system and the position of the line at infinity without further infor- mation. A methodology for central catadioptric system calibration is proposed. Reconstruction aspects are discussed. Experimental results are presented. All the results presented are original and completely new. 1 Introduction Many applications in computer vision, such as surveillance and model acquisition for virtual reality, require that a large field of view is imaged. Visual control of motion can also benefit from enhanced fields of view [1,2,4]. One effective way to enhance the field of view of a camera is to use mirrors [5,6,7,8,9]. The general approach of combining mirrors with conventional imaging systems is referred to as catadioptric image formation [3]. -
Surfaces in 3-Space
Differential Geometry of Some SURFACES IN 3-SPACE Nicholas Wheeler December 2015 Introduction. Recent correspondence with Ahmed Sebbar concerning the theory of unimodular 3 3 circulant matrices1 × x y z det z x y = x3 + y3 + z3 3xyz = 1 y z x − brought to my attention a surface Σ in R3 which, I was informed, is encountered in work of H. Jonas (1915, 1921) and, because of its form when plotted, is known as “Jonas’ hexenhut” (witch’s hat). I was led by Google from “hexenhut” to a monograph B¨acklund and Darboux Transformations: Geometry and Modern Applications in Soliton Theory, by C. Rogers & W. K. Schief (2002). These are subjects in which I have had longstanding interest, but which I have not thought about for many years. I am inspired by those authors’ splendid book to revisit this subject area. In part one I assemble the tools that play essential roles in the theory of surfaces in R3, and in part two use those tools to develop the properties of some specific surfaces—particularly the pseudosphere, because it was the cradle in which was born the sine-Gordon equation, which a century later became central to the physical theory of solitons.2 part one Concepts & Tools Essential to the Theory of Surfaces in 3-Space Fundamental forms. Relative to a Cartesian frame in R3, surfaces Σ can be described implicitly f(x, y, z) = 0 but for the purposes of differential geometry must be described parametrically x(u, v) r(u, v) = y(u, v) z(u, v) 1 See “Simplest generalization of Pell’s Problem,” (September, 2015). -
Chapter 3 Quadratic Curves, Quadric Surfaces
Chapter 3 Quadratic curves, quadric surfaces In this chapter we begin our study of curved surfaces. We focus on the quadric surfaces. To do this, we also need to look at quadratic curves, such as ellipses. We discuss: Equations and parametric descriptions of the plane quadratic curves: circles, ellipses, ² hyperbolas and parabolas. Equations and parametric descriptions of quadric surfaces, the 2{dimensional ana- ² logues of quadratic curves. We also discuss aspects of matrices, since they are relevant for our discussion. 3.1 Plane quadratic curves 3.1.1 From linear to quadratic equations Lines in the plane R2 are represented by linear equations and linear parametric descriptions. Degree 2 equations also correspond to curves you undoubtedly have come across before: circles, ellipses, hyperbolas and parabolas. This section is devoted to these curves. They will reoccur when we consider quadric surfaces, a class of fascinating shapes, since the intersection of a quadric surface with a plane consists of a quadratic curve. Lines di®er from quadratic curves in various respects, one of which is that all lines look the same (only their position in the plane may di®er), but that quadratic curves may truely di®er in shape. 3.1.2 The general equation of a quadratic curve The general equation of a line in R2 is ax + by = c. When we also allow terms of degree 2 in the variables x and y, i.e., x2, xy and y2, we obtain quadratic equations like x2 + y2 = 1, a circle. ² x2 + 2x + y = 3, a parabola; probably you recognize it as such if it is rewritten in the ² form y = 3 x2 2x or y = (x + 1)2 + 4. -
11.5: Quadric Surfaces
c Dr Oksana Shatalov, Spring 2013 1 11.5: Quadric surfaces REVIEW: Parabola, hyperbola and ellipse. • Parabola: y = ax2 or x = ay2. y y x x 0 0 y x2 y2 • Ellipse: + = 1: x a2 b2 0 Intercepts: (±a; 0)&(0; ±b) x2 y2 x2 y2 • Hyperbola: − = 1 or − + = 1 a2 b2 a2 b2 y y x x 0 0 Intercepts: (±a; 0) Intercepts: (0; ±b) c Dr Oksana Shatalov, Spring 2013 2 The most general second-degree equation in three variables x; y and z: 2 2 2 Ax + By + Cz + axy + bxz + cyz + d1x + d2y + d3z + E = 0; (1) where A; B; C; a; b; c; d1; d2; d3;E are constants. The graph of (1) is a quadric surface. Note if A = B = C = a = b = c = 0 then (1) is a linear equation and its graph is a plane (this is the case of degenerated quadric surface). By translations and rotations (1) can be brought into one of the two standard forms: Ax2 + By2 + Cz2 + J = 0 or Ax2 + By2 + Iz = 0: In order to sketch the graph of a surface determine the curves of intersection of the surface with planes parallel to the coordinate planes. The obtained in this way curves are called traces or cross-sections of the surface. Quadric surfaces can be classified into 5 categories: ellipsoids, hyperboloids, cones, paraboloids, quadric cylinders. (shown in the table, see Appendix.) The elements which characterize each of these categories: 1. Standard equation. 2. Traces (horizontal ( by planes z = k), yz-traces (by x = 0) and xz-traces (by y = 0). -
Lesson 9: Volume and Cavalieri's Principle
NYS COMMON CORE MATHEMATICS CURRICULUM Lesson 9 M3 PRECALCULUS AND ADVANCED TOPICS Lesson 9: Volume and Cavalieri’s Principle Student Outcomes . Students will be able to give an informal argument using Cavalieri’s principle for the formula for the volume of a sphere and other solid figures (G-GMD.A.2). Lesson Notes The opening uses the idea of cross sections to establish a connection between the current lesson and the previous lessons. In particular, ellipses and hyperbolas are seen as cross sections of a cone, and Cavalieri’s volume principle is based on cross-sectional areas. This principle is used to explore the volume of pyramids, cones, and spheres. Classwork Opening (2 minutes) Scaffolding: . A cutout of a cone is available in Geometry, Module 3, Lesson 7 to make picturing this exercise easier. Use the cutout to model determining that a circle is a possible cross section of a cone. “Conic Sections” by Magister Mathematicae is licensed under CC BY-SA 3.0 http://creativecommons.org/licenses/by-sa/3.0/deed.en In the previous lesson, we saw how the ellipse, parabola, and hyperbola can come together in the context of a satellite orbiting a body such as a planet; we learned that the velocity of the satellite determines the shape of its orbit. Another context in which these curves and a circle arise is in slicing a cone. The intersection of a plane with a solid is called a cross section of the solid. Lesson 9: Volume and Cavalieri’s Principle Date: 2/9/15 144 This work is licensed under a © 2015 Common Core, Inc.