Anallagmatic Curves and Inversion About the Unit Hyperbola
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Old-Fashioned Relativity & Relativistic Space-Time Coordinates
Relativistic Coordinates-Classic Approach 4.A.1 Appendix 4.A Relativistic Space-time Coordinates The nature of space-time coordinate transformation will be described here using a fictional spaceship traveling at half the speed of light past two lighthouses. In Fig. 4.A.1 the ship is just passing the Main Lighthouse as it blinks in response to a signal from the North lighthouse located at one light second (about 186,000 miles or EXACTLY 299,792,458 meters) above Main. (Such exactitude is the result of 1970-80 work by Ken Evenson's lab at NIST (National Institute of Standards and Technology in Boulder) and adopted by International Standards Committee in 1984.) Now the speed of light c is a constant by civil law as well as physical law! This came about because time and frequency measurement became so much more precise than distance measurement that it was decided to define the meter in terms of c. Fig. 4.A.1 Ship passing Main Lighthouse as it blinks at t=0. This arrangement is a simplified model for a 1Hz laser resonator. The two lighthouses use each other to maintain a strict one-second time period between blinks. And, strict it must be to do relativistic timing. (Even stricter than NIST is the universal agency BIGANN or Bureau of Intergalactic Aids to Navigation at Night.) The simulations shown here are done using RelativIt. Relativistic Coordinates-Classic Approach 4.A.2 Fig. 4.A.2 Main and North Lighthouses blink each other at precisely t=1. At p recisel y t=1 sec. -
Catoni F., Et Al. the Mathematics of Minkowski Space-Time.. With
Frontiers in Mathematics Advisory Editorial Board Leonid Bunimovich (Georgia Institute of Technology, Atlanta, USA) Benoît Perthame (Ecole Normale Supérieure, Paris, France) Laurent Saloff-Coste (Cornell University, Rhodes Hall, USA) Igor Shparlinski (Macquarie University, New South Wales, Australia) Wolfgang Sprössig (TU Bergakademie, Freiberg, Germany) Cédric Villani (Ecole Normale Supérieure, Lyon, France) Francesco Catoni Dino Boccaletti Roberto Cannata Vincenzo Catoni Enrico Nichelatti Paolo Zampetti The Mathematics of Minkowski Space-Time With an Introduction to Commutative Hypercomplex Numbers Birkhäuser Verlag Basel . Boston . Berlin $XWKRUV )UDQFHVFR&DWRQL LQFHQ]R&DWRQL LDHJOLD LDHJOLD 5RPD 5RPD Italy Italy HPDLOYMQFHQ]R#\DKRRLW Dino Boccaletti 'LSDUWLPHQWRGL0DWHPDWLFD (QULFR1LFKHODWWL QLYHUVLWjGL5RPD²/D6DSLHQ]D³ (1($&5&DVDFFLD 3LD]]DOH$OGR0RUR LD$QJXLOODUHVH 5RPD 5RPD Italy Italy HPDLOERFFDOHWWL#XQLURPDLW HPDLOQLFKHODWWL#FDVDFFLDHQHDLW 5REHUWR&DQQDWD 3DROR=DPSHWWL (1($&5&DVDFFLD (1($&5&DVDFFLD LD$QJXLOODUHVH LD$QJXLOODUHVH 5RPD 5RPD Italy Italy HPDLOFDQQDWD#FDVDFFLDHQHDLW HPDLO]DPSHWWL#FDVDFFLDHQHDLW 0DWKHPDWLFDO6XEMHFW&ODVVL½FDWLRQ*(*4$$ % /LEUDU\RI&RQJUHVV&RQWURO1XPEHU Bibliographic information published by Die Deutsche Bibliothek 'LH'HXWVFKH%LEOLRWKHNOLVWVWKLVSXEOLFDWLRQLQWKH'HXWVFKH1DWLRQDOELEOLRJUD½H GHWDLOHGELEOLRJUDSKLFGDWDLVDYDLODEOHLQWKH,QWHUQHWDWKWWSGQEGGEGH! ,6%1%LUNKlXVHUHUODJ$*%DVHOÀ%RVWRQÀ% HUOLQ 7KLVZRUNLVVXEMHFWWRFRS\ULJKW$OOULJKWVDUHUHVHUYHGZKHWKHUWKHZKROHRUSDUWRIWKH PDWHULDOLVFRQFHUQHGVSHFL½FDOO\WKHULJKWVRIWUDQVODWLRQUHSULQWLQJUHXVHRILOOXVWUD -
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. -
Unifying the Hyperbolic and Spherical 2-Body Problem with Biquaternions
Unifying the Hyperbolic and Spherical 2-Body Problem with Biquaternions Philip Arathoon December 2020 Abstract The 2-body problem on the sphere and hyperbolic space are both real forms of holo- morphic Hamiltonian systems defined on the complex sphere. This admits a natural description in terms of biquaternions and allows us to address questions concerning the hyperbolic system by complexifying it and treating it as the complexification of a spherical system. In this way, results for the 2-body problem on the sphere are readily translated to the hyperbolic case. For instance, we implement this idea to completely classify the relative equilibria for the 2-body problem on hyperbolic 3-space for a strictly attractive potential. Background and outline The case of the 2-body problem on the 3-sphere has recently been considered by the author in [1]. This treatment takes advantage of the fact that S3 is a group and that the action of SO(4) on S3 is generated by the left and right multiplication of S3 on itself. This allows for a reduction in stages, first reducing by the left multiplication, and then reducing an intermediate space by the residual right-action. An advantage of this reduction-by-stages is that it allows for a fairly straightforward derivation of the relative equilibria solutions: the relative equilibria may first be classified in the intermediate reduced space and then reconstructed on the original phase space. For the 2-body problem on hyperbolic space the same idea does not apply. Hyperbolic 3-space H3 cannot be endowed with an isometric group structure and the symmetry group SO(1; 3) does not arise as a direct product of two groups. -
Curves with Rational Chord-Length Parametrization
Curves with rational chord-length parametrization J. Sanchez-Reyes , L. Fernandez-Jambrina Instituto de Matemdtica Aplicada a la Ciencia e Ingenieria, ETS Ingenieros Industrials, Universidad de Castilla-La Mancha, Campus Universitario, 13071-Ciudad Real, Spain ETSI Navales, Universidad Politecnica de Madrid, Arco de la Victoria s/n, 28040-Madrid, Spain Abstract It has been recently proved that rational quadratic circles in standard Bezier form are parameterized by chord-length. If we consider that standard circles coincide with the isoparametric curves in a system of bipolar coordinates, this property comes as a straightforward consequence. General curves with chord-length parametrization are simply the analogue in bipolar coordinates of nonparametric curves. This interpretation furnishes a compact explicit expression for all planar curves with rational chord-length parametrization. In addition to straight lines and circles in standard form, they include remarkable curves, such as the equilateral hyperbola, Lemniscate of Bernoulli and Limacon of Pascal. The extension to 3D rational curves is also tackled. Keywords: Bezier circle; Bipolar coordinates; Chord-length parametrization; Equilateral hyperbola; Lemniscate of Bernoulli 1. Chord-length parametrization Given a parametric curve p(t) over a certain domain t e[a,b], its chord-length at a given point p(7) is defined as (Farm, 2001, 2006): IF|p(0 — A| chord(0 := y A = p(fl), B = p(Z?) (1) |p(0-A| + |p(0-B| where bars denote the modulus of a vector. The curve is said to be chord-length parameterized if chord(f) = t. Chord- length parametrization is clearly invariant with respect to linear transformations of the domain. -
Generating Negative Pedal Curve Through Inverse Function – an Overview *Ramesha
© 2017 JETIR March 2017, Volume 4, Issue 3 www.jetir.org (ISSN-2349-5162) Generating Negative pedal curve through Inverse function – An Overview *Ramesha. H.G. Asst Professor of Mathematics. Govt First Grade College, Tiptur. Abstract This paper attempts to study the negative pedal of a curve with fixed point O is therefore the envelope of the lines perpendicular at the point M to the lines. In inversive geometry, an inverse curve of a given curve C is the result of applying an inverse operation to C. Specifically, with respect to a fixed circle with center O and radius k the inverse of a point Q is the point P for which P lies on the ray OQ and OP·OQ = k2. The inverse of the curve C is then the locus of P as Q runs over C. The point O in this construction is called the center of inversion, the circle the circle of inversion, and k the radius of inversion. An inversion applied twice is the identity transformation, so the inverse of an inverse curve with respect to the same circle is the original curve. Points on the circle of inversion are fixed by the inversion, so its inverse is itself. is a function that "reverses" another function: if the function f applied to an input x gives a result of y, then applying its inverse function g to y gives the result x, and vice versa, i.e., f(x) = y if and only if g(y) = x. The inverse function of f is also denoted. -
An Analysis of Spacetime Numbers
Rowan University Rowan Digital Works Theses and Dissertations 4-30-1999 An analysis of spacetime numbers Nicolae Andrew Borota Rowan University Follow this and additional works at: https://rdw.rowan.edu/etd Recommended Citation Borota, Nicolae Andrew, "An analysis of spacetime numbers" (1999). Theses and Dissertations. 1771. https://rdw.rowan.edu/etd/1771 This Thesis is brought to you for free and open access by Rowan Digital Works. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of Rowan Digital Works. For more information, please contact [email protected]. AN ANALYSIS OF SPACETIME NUMBERS by Nicolae Andrew Borota A Thesis Submitted in partial fulfillment of the requirements of the Masters of Arts Degree of The Graduate School at Rowan University 04/30/99 Approved by Date Approved A/P/ i- 30 /F?7 ABSTRACT Nicolae Andrew Borota An Analysis of Spacetime Numbers 1999 Thesis Mathematics The familiar complex numbers begin by considering the solution to the equation i = -1, which is not a real number. A two-dimensional number system arises of the form z = x + iy. Spacetime numbers are based upon the simple relation j = 1, with the corresponding two-dimensional number system z = x + jt. It seems odd that anything useful can come from this simple idea, since the solutions of our j equation are the familiar real numbers +1 and -1. However, many interesting applications arise from these new numbers. The most useful aspect of spacetime numbers is in solving problems in the areas of special and general relativity. These areas deal with the notion of space-time, hence the name "spacetime numbers." My goal is to explain in a direct, yet simple manner, the use of these special numbers. -
Strophoids, a Family of Cubic Curves with Remarkable Properties
Strophoids, a family of cubic curves with remarkable properties Hellmuth Stachel [email protected] — http://www.geometrie.tuwien.ac.at/stachel 6th International Conference on Engineering Graphics and Design University Transilvania, June 11–13, Brasov/Romania Table of contents 1. Definition of Strophoids 2. Associated Points 3. Strophoids as a Geometric Locus June 12, 2015: 6th Internat. Conference on Engineering Graphics and Design, Brasov/Romania 1/29 replacements 1. Definition of Strophoids ′ F Definition: An irreducible cubic is called circular if it passes through the absolute circle-points. asymptote A circular cubic is called strophoid ′ if it has a double point (= node) with G orthogonal tangents. F g A strophoid without an axis of y G symmetry is called oblique, other- wise right. S S : (x 2 + y 2)(ax + by) − xy =0 with a, b ∈ R, (a, b) =6 (0, 0). In x N fact, S intersects the line at infinity at (0 : 1 : ±i) and (0 : b : −a). June 12, 2015: 6th Internat. Conference on Engineering Graphics and Design, Brasov/Romania 2/29 1. Definition of Strophoids F ′ The line through N with inclination angle ϕ intersects S in the point asymptote 2 2 ′ sϕ c ϕ s ϕ cϕ G X = , . a cϕ + b sϕ a cϕ + b sϕ F g y G X This yields a parametrization of S. S ϕ = ±45◦ gives the points G, G′. ϕ The tangents at the absolute circle- N x points intersect in the focus F . June 12, 2015: 6th Internat. Conference on Engineering Graphics and Design, Brasov/Romania 3/29 1. -
And Innovative Research of Emerging Technologies
WWW.JETIR.ORG [email protected] An International Open Access Journal UGC and ISSN Approved | ISSN: 2349-5162 INTERNATIONAL JOURNAL OF EMERGING TECHNOLOGIES AND INNOVATIVE RESEARCH JETIR.ORG INTERNATIONAL JOURNAL OF EMERGING TECHNOLOGIES AND INNOVATIVE RESEARCH International Peer Reviewed, Open Access Journal ISSN: 2349-5162 | Impact Factor: 5.87 UGC and ISSN Approved Journals. Website: www. jetir.org Website: www.jetir.org JETIR INTERNATIONAL JOURNAL OF EMERGING TECHNOLOGIES AND INNOVATIVE RESEARCH (ISSN: 2349-5162) International Peer Reviewed, Open Access Journal ISSN: 2349-5162 | Impact Factor: 5.87 | UGC and ISSN Approved ISSN (Online): 2349-5162 This work is subjected to be copyright. All rights are reserved whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, re-use of illusions, recitation, broadcasting, reproduction on microfilms or in any other way, and storage in data banks. Duplication of this publication of parts thereof is permitted only under the provision of the copyright law, in its current version, and permission of use must always be obtained from JETIR www.jetir.org Publishers. International Journal of Emerging Technologies and Innovative Research is published under the name of JETIR publication and URL: www.jetir.org. © JETIR Journal Published in India Typesetting: Camera-ready by author, data conversation by JETIR Publishing Services – JETIR Journal. JETIR Journal, WWW. JETIR.ORG ISSN (Online): 2349-5162 International Journal of Emerging Technologies and Innovative Research (JETIR) is published in online form over Internet. This journal is published at the Website http://www.jetir.org maintained by JETIR Gujarat, India. © 2017 JETIR March 2017, Volume 4, Issue 3 www.jetir.org (ISSN-2349-5162) Generating Negative pedal curve through Inverse function – An Overview *Ramesha. -
On Bivectors and Jay-Vectors - 2 - M
Ricerche di Matematica (2019) 68, 859–882. https://doi.org/10.1007/s11587-019-00442-2 On bivectors and jay-vectors M. Hayes School of Mechanical and Materials Engineering, University College, Dublin N. H. Scott∗ School of Mathematics, University of East Anglia, Norwich Research Park, Norwich NR4 7TJ Received: 5 February 2019 Revised: 25 March 2019 Published: 6 April 2019 · · Note from the second author. This is joint work with my erstwhile PhD supervisor at the University of East Anglia, Norwich, Professor Mike Hayes, late of University College Dublin. Since Mike’s unfortunate death I have endeavoured to finish the work in a man- ner he would have approved of. This paper is dedicated to Colette Hayes, Mike’s widow. Abstract A combination a+ib where i2 = 1 and a, b are real vectors is called a bivector. − Gibbs developed a theory of bivectors, in which he associated an ellipse with each bivector. He obtained results relating pairs of conjugate semi-diameters and in particular considered the implications of the scalar product of two bivectors being zero. This paper is an attempt to develop a similar formulation for hyperbolas by the use of jay-vectors — a jay-vector is a linear combination a +jb of real vectors a and b, where j2 = +1 but j is not a real number, so j = 1. The implications 6 ± of the vanishing of the scalar product of two jay-vectors is also considered. We show how to generate a triple of conjugate semi-diameters of an ellipsoid from any arXiv:2004.14154v1 [math.GM] 27 Apr 2020 orthonormal triad. -
Hyperbolic Functions∗
Hyperbolic functions∗ Attila M´at´e Brooklyn College of the City University of New York November 30, 2020 Contents 1 Hyperbolic functions 1 2 Connection with the unit hyperbola 2 2.1 Geometricmeaningoftheparameter . ......... 3 3 Complex exponentiation: connection with trigonometric functions 3 3.1 Trigonometric representation of complex numbers . ............... 4 3.2 Extending the exponential function to complex numbers. ................ 5 1 Hyperbolic functions The hyperbolic functions are defined as follows ex e−x ex + e−x sinh x ex e−x sinh x = − , cosh x = , tanh x = = − 2 2 cosh x ex + e−x 1 2 sech x = = , ... cosh x ex + e−x The following formulas are easy to establish: (1) cosh2 x sinh2 x = 1, sech2 x = 1 tanh2 x, − − sinh(x + y) = sinh x cosh y + cosh x sinh y cosh(x + y) = cosh x cosh y + sinh x sinh y; the analogy with trigonometry is clear. The differentiation formulas also show a lot of similarity: ′ ′ (sinh x) = cosh x, (cosh x) = sinh x, ′ ′ (tanh x) = sech2 x = 1 tanh2 x, (sech x) = tanh x sech x. − − Hyperbolic functions can be used instead of trigonometric substitutions to evaluate integrals with quadratic expressions under the square root. For example, to evaluate the integral √x2 1 − dx Z x2 ∗Written for the course Mathematics 1206 at Brooklyn College of CUNY. 1 for x > 0, we can use the substitution x = cosh t with t 0.1 We have √x2 1 = sinh t and dt = sinh xdx, and so ≥ − √x2 1 sinh t − dx = sinh tdt = tanh2 tdt = (1 sech2 t) dt = t tanh t + C. -
Newton's Parabola Observed from Pappus
Applied Physics Research; Vol. 11, No. 2; 2019 ISSN 1916-9639 E-ISSN 1916-9647 Published by Canadian Center of Science and Education Newton’s Parabola Observed from Pappus’ Directrix, Apollonius’ Pedal Curve (Line), Newton’s Evolute, Leibniz’s Subtangent and Subnormal, Castillon’s Cardioid, and Ptolemy’s Circle (Hodograph) (09.02.2019) Jiří Stávek1 1 Bazovského, Prague, Czech Republic Correspondence: Jiří Stávek, Bazovského 1228, 163 00 Prague, Czech Republic. E-mail: [email protected] Received: February 2, 2019 Accepted: February 20, 2019 Online Published: February 25, 2019 doi:10.5539/apr.v11n2p30 URL: http://dx.doi.org/10.5539/apr.v11n2p30 Abstract Johannes Kepler and Isaac Newton inspired generations of researchers to study properties of elliptic, hyperbolic, and parabolic paths of planets and other astronomical objects orbiting around the Sun. The books of these two Old Masters “Astronomia Nova” and “Principia…” were originally written in the geometrical language. However, the following generations of researchers translated the geometrical language of these Old Masters into the infinitesimal calculus independently discovered by Newton and Leibniz. In our attempt we will try to return back to the original geometrical language and to present several figures with possible hidden properties of parabolic orbits. For the description of events on parabolic orbits we will employ the interplay of the directrix of parabola discovered by Pappus of Alexandria, the pedal curve with the pedal point in the focus discovered by Apollonius of Perga (The Great Geometer), and the focus occupied by our Sun discovered in several stages by Aristarchus, Copernicus, Kepler and Isaac Newton (The Great Mathematician).