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Ordinary Differential Equations
Ordinary Differential Equations for Engineers and Scientists Gregg Waterman Oregon Institute of Technology c 2017 Gregg Waterman This work is licensed under the Creative Commons Attribution 4.0 International license. The essence of the license is that You are free to: Share copy and redistribute the material in any medium or format • Adapt remix, transform, and build upon the material for any purpose, even commercially. • The licensor cannot revoke these freedoms as long as you follow the license terms. Under the following terms: Attribution You must give appropriate credit, provide a link to the license, and indicate if changes • were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use. No additional restrictions You may not apply legal terms or technological measures that legally restrict others from doing anything the license permits. Notices: You do not have to comply with the license for elements of the material in the public domain or where your use is permitted by an applicable exception or limitation. No warranties are given. The license may not give you all of the permissions necessary for your intended use. For example, other rights such as publicity, privacy, or moral rights may limit how you use the material. For any reuse or distribution, you must make clear to others the license terms of this work. The best way to do this is with a link to the web page below. To view a full copy of this license, visit https://creativecommons.org/licenses/by/4.0/legalcode. -
New Dirac Delta Function Based Methods with Applications To
New Dirac Delta function based methods with applications to perturbative expansions in quantum field theory Achim Kempf1, David M. Jackson2, Alejandro H. Morales3 1Departments of Applied Mathematics and Physics 2Department of Combinatorics and Optimization University of Waterloo, Ontario N2L 3G1, Canada, 3Laboratoire de Combinatoire et d’Informatique Math´ematique (LaCIM) Universit´edu Qu´ebec `aMontr´eal, Canada Abstract. We derive new all-purpose methods that involve the Dirac Delta distribution. Some of the new methods use derivatives in the argument of the Dirac Delta. We highlight potential avenues for applications to quantum field theory and we also exhibit a connection to the problem of blurring/deblurring in signal processing. We find that blurring, which can be thought of as a result of multi-path evolution, is, in Euclidean quantum field theory without spontaneous symmetry breaking, the strong coupling dual of the usual small coupling expansion in terms of the sum over Feynman graphs. arXiv:1404.0747v3 [math-ph] 23 Sep 2014 2 1. A method for generating new representations of the Dirac Delta The Dirac Delta distribution, see e.g., [1, 2, 3], serves as a useful tool from physics to engineering. Our aim here is to develop new all-purpose methods involving the Dirac Delta distribution and to show possible avenues for applications, in particular, to quantum field theory. We begin by fixing the conventions for the Fourier transform: 1 1 g(y) := g(x) eixy dx, g(x)= g(y) e−ixy dy (1) √2π √2π Z Z To simplify the notation we denote integration over the real line by the absence of e e integration delimiters. -
Modifications of the Method of Variation of Parameters
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector International Joumal Available online at www.sciencedirect.com computers & oc,-.c~ ~°..-cT- mathematics with applications Computers and Mathematics with Applications 51 (2006) 451-466 www.elsevier.com/locate/camwa Modifications of the Method of Variation of Parameters ROBERTO BARRIO* GME, Depto. Matem~tica Aplicada Facultad de Ciencias Universidad de Zaragoza E-50009 Zaragoza, Spain rbarrio@unizar, es SERGIO SERRANO GME, Depto. MatemAtica Aplicada Centro Politdcnico Superior Universidad de Zaragoza Maria de Luna 3, E-50015 Zaragoza, Spain sserrano©unizar, es (Received February PO05; revised and accepted October 2005) Abstract--ln spite of being a classical method for solving differential equations, the method of variation of parameters continues having a great interest in theoretical and practical applications, as in astrodynamics. In this paper we analyse this method providing some modifications and generalised theoretical results. Finally, we present an application to the determination of the ephemeris of an artificial satellite, showing the benefits of the method of variation of parameters for this kind of problems. ~) 2006 Elsevier Ltd. All rights reserved. Keywords--Variation of parameters, Lagrange equations, Gauss equations, Satellite orbits, Dif- ferential equations. 1. INTRODUCTION The method of variation of parameters was developed by Leonhard Euler in the middle of XVIII century to describe the mutual perturbations of Jupiter and Saturn. However, his results were not absolutely correct because he did not consider the orbital elements varying simultaneously. In 1766, Lagrange improved the method developed by Euler, although he kept considering some of the orbital elements as constants, which caused some of his equations to be incorrect. -
Phase Plane Methods
Chapter 10 Phase Plane Methods Contents 10.1 Planar Autonomous Systems . 680 10.2 Planar Constant Linear Systems . 694 10.3 Planar Almost Linear Systems . 705 10.4 Biological Models . 715 10.5 Mechanical Models . 730 Studied here are planar autonomous systems of differential equations. The topics: Planar Autonomous Systems: Phase Portraits, Stability. Planar Constant Linear Systems: Classification of isolated equilib- ria, Phase portraits. Planar Almost Linear Systems: Phase portraits, Nonlinear classi- fications of equilibria. Biological Models: Predator-prey models, Competition models, Survival of one species, Co-existence, Alligators, doomsday and extinction. Mechanical Models: Nonlinear spring-mass system, Soft and hard springs, Energy conservation, Phase plane and scenes. 680 Phase Plane Methods 10.1 Planar Autonomous Systems A set of two scalar differential equations of the form x0(t) = f(x(t); y(t)); (1) y0(t) = g(x(t); y(t)): is called a planar autonomous system. The term autonomous means self-governing, justified by the absence of the time variable t in the functions f(x; y), g(x; y). ! ! x(t) f(x; y) To obtain the vector form, let ~u(t) = , F~ (x; y) = y(t) g(x; y) and write (1) as the first order vector-matrix system d (2) ~u(t) = F~ (~u(t)): dt It is assumed that f, g are continuously differentiable in some region D in the xy-plane. This assumption makes F~ continuously differentiable in D and guarantees that Picard's existence-uniqueness theorem for initial d ~ value problems applies to the initial value problem dt ~u(t) = F (~u(t)), ~u(0) = ~u0. -
The Following Integration Formulas Will Be Provided on the Exam and You
The following integration formulas will be provided on the exam and you may apply any of these results directly without showing work/proof: Z 1 (ax + b)n+1 (ax + b)n dx = · + C a n + 1 Z 1 eax+b dx = · eax+b + C a Z 1 uax+b dx = · uax+b + C for u > 0; u 6= 1 a ln u Z 1 1 dx = · ln jax + bj + C ax + b a Z 1 sin(ax + b) dx = − · cos(ax + b) + C a Z 1 cos(ax + b) dx = · sin(ax + b) + C a Z 1 sec2(ax + b) dx = · tan(ax + b) + C a Z 1 csc2(ax + b) dx = · cot(ax + b) + C a Z 1 p dx = sin−1(x) + C 1 − x2 Z 1 dx = tan−1(x) + C 1 + x2 Z 1 p dx = sinh−1(x) + C 1 + x2 1 The following formulas for Laplace transform will also be provided f(t) = L−1fF (s)g F (s) = Lff(t)g f(t) = L−1fF (s)g F (s) = Lff(t)g 1 1 1 ; s > 0 eat ; s > a s s − a tf(t) −F 0(s) eatf(t) F (s − a) n! n! tn ; s > 0 tneat ; s > a sn+1 (s − a)n+1 w w sin(wt) ; s > 0 eat sin(wt) ; s > a s2 + w2 (s − a)2 + w2 s s − a cos(wt) ; s > 0 eat cos(wt) ; s > a s2 + w2 (s − a)2 + w2 e−as u(t − a); a ≥ 0 ; s > 0 δ(t − a); a ≥ 0 e−as; s > 0 s u(t − a)f(t) e−asLff(t + a)g δ(t − a)f(t) f(a)e−as Here, u(t) is the unit step (Heaviside) function and δ(t) is the Dirac Delta function Laplace transform of derivatives: Lff 0(t)g = sLff(t)g − f(0) Lff 00(t)g = s2Lff(t)g − sf(0) − f 0(0) Lff (n)(t)g = snLff(t)g − sn−1f(0) − sn−2f 0(0) − · · · − sf (n−2)(0) − f (n−1)(0) Convolution: Lf(f ∗ g)(t)g = Lff(t)gLfg(t)g = Lf(g ∗ f)(t)g 2 1 First Order Linear Differential Equation Differential equations of the form dy + p(t) y = g(t) (1) dt where t is the independent variable and y(t) is the unknown function. -
Second Order Linear Differential Equations Y
Second Order Linear Differential Equations Second order linear equations with constant coefficients; Fundamental solutions; Wronskian; Existence and Uniqueness of solutions; the characteristic equation; solutions of homogeneous linear equations; reduction of order; Euler equations In this chapter we will study ordinary differential equations of the standard form below, known as the second order linear equations : y″ + p(t) y′ + q(t) y = g(t). Homogeneous Equations : If g(t) = 0, then the equation above becomes y″ + p(t) y′ + q(t) y = 0. It is called a homogeneous equation. Otherwise, the equation is nonhomogeneous (or inhomogeneous ). Trivial Solution : For the homogeneous equation above, note that the function y(t) = 0 always satisfies the given equation, regardless what p(t) and q(t) are. This constant zero solution is called the trivial solution of such an equation. © 2008, 2016 Zachary S Tseng B-1 - 1 Second Order Linear Homogeneous Differential Equations with Constant Coefficients For the most part, we will only learn how to solve second order linear equation with constant coefficients (that is, when p(t) and q(t) are constants). Since a homogeneous equation is easier to solve compares to its nonhomogeneous counterpart, we start with second order linear homogeneous equations that contain constant coefficients only: a y″ + b y′ + c y = 0. Where a, b, and c are constants, a ≠ 0. A very simple instance of such type of equations is y″ − y = 0 . The equation’s solution is any function satisfying the equality t y″ = y. Obviously y1 = e is a solution, and so is any constant multiple t −t of it, C1 e . -
5 Mar 2009 a Survey on the Inverse Integrating Factor
A survey on the inverse integrating factor.∗ Isaac A. Garc´ıa (1) & Maite Grau (1) Abstract The relation between limit cycles of planar differential systems and the inverse integrating factor was first shown in an article of Giacomini, Llibre and Viano appeared in 1996. From that moment on, many research articles are devoted to the study of the properties of the inverse integrating factor and its relation with limit cycles and their bifurcations. This paper is a summary of all the results about this topic. We include a list of references together with the corresponding related results aiming at being as much exhaustive as possible. The paper is, nonetheless, self-contained in such a way that all the main results on the inverse integrating factor are stated and a complete overview of the subject is given. Each section contains a different issue to which the inverse integrating factor plays a role: the integrability problem, relation with Lie symmetries, the center problem, vanishing set of an inverse integrating factor, bifurcation of limit cycles from either a period annulus or from a monodromic ω-limit set and some generalizations. 2000 AMS Subject Classification: 34C07, 37G15, 34-02. Key words and phrases: inverse integrating factor, bifurcation, Poincar´emap, limit cycle, Lie symmetry, integrability, monodromic graphic. arXiv:0903.0941v1 [math.DS] 5 Mar 2009 1 The Euler integrating factor The method of integrating factors is, in principle, a means for solving ordinary differential equations of first order and it is theoretically important. The use of integrating factors goes back to Leonhard Euler. Let us consider a first order differential equation and write the equation in the Pfaffian form ω = P (x, y) dy Q(x, y) dx =0 . -
PHYS2100: Hamiltonian Dynamics and Chaos
PHYS2100: Hamiltonian dynamics and chaos M. J. Davis September 2006 Chapter 1 Introduction Lecturer: Dr Matthew Davis. Room: 6-403 (Physics Annexe, ARC Centre of Excellence for Quantum-Atom Optics) Phone: (334) 69824 email: [email protected] Office hours: Friday 8-10am, or by appointment. Useful texts Rasband: Chaotic dynamics of nonlinear systems. Q172.5.C45 R37 1990. • Percival and Richards: Introduction to dynamics. QA614.8 P47 1982. • Baker and Gollub: Chaotic dynamics: an introduction. QA862 .P4 B35 1996. • Gleick: Chaos: making a new science. Q172.5.C45 G54 1998. • Abramowitz and Stegun, editors: Handbook of mathematical functions: with formulas, graphs, and• mathematical tables. QA47.L8 1975 The lecture notes will be complete: However you can only improve your understanding by reading more. We will begin this section of the course with a brief reminder of a few essential conncepts from the first part of the course taught by Dr Karen Dancer. 1.1 Basics A mechanical system is known as conservative if F dr = 0. (1.1) I · Frictional or dissipative systems do not satisfy Eq. (1.1). Using vector analysis it can be shown that Eq. (1.1) implies that there exists a potential function 1 such that F = V (r). (1.2) −∇ for some V (r). We will assume that conservative systems have time-independent potentials. A holonomic constraint is a constraint written in terms of an equality e.g. r = a, a> 0. (1.3) | | A non-holonomic constraint is written as an inequality e.g. r a. | | ≥ 1.2 Lagrangian mechanics For a mechanical system of N particles with k holonomic constraints, there are a total of 3N k degrees of freedom. -
MTHE / MATH 237 Differential Equations for Engineering Science
i Queen’s University Mathematics and Engineering and Mathematics and Statistics MTHE / MATH 237 Differential Equations for Engineering Science Supplemental Course Notes Serdar Y¨uksel November 26, 2015 ii This document is a collection of supplemental lecture notes used for MTHE / MATH 237: Differential Equations for Engineering Science. Serdar Y¨uksel Contents 1 Introduction to Differential Equations ................................................... .......... 1 1.1 Introduction.................................... ............................................ 1 1.2 Classification of DifferentialEquations ............ ............................................. 1 1.2.1 OrdinaryDifferentialEquations ................. ........................................ 2 1.2.2 PartialDifferentialEquations .................. ......................................... 2 1.2.3 HomogeneousDifferentialEquations .............. ...................................... 2 1.2.4 N-thorderDifferentialEquations................ ........................................ 2 1.2.5 LinearDifferentialEquations ................... ........................................ 2 1.3 SolutionsofDifferentialequations ................ ............................................. 3 1.4 DirectionFields................................. ............................................ 3 1.5 Fundamental Questions on First-Order Differential Equations ...................................... 4 2 First-Order Ordinary Differential Equations .................................................. -
Handbook of Mathematics, Physics and Astronomy Data
Handbook of Mathematics, Physics and Astronomy Data School of Chemical and Physical Sciences c 2017 Contents 1 Reference Data 1 1.1 PhysicalConstants ............................... .... 2 1.2 AstrophysicalQuantities. ....... 3 1.3 PeriodicTable ................................... 4 1.4 ElectronConfigurationsoftheElements . ......... 5 1.5 GreekAlphabetandSIPrefixes. ..... 6 2 Mathematics 7 2.1 MathematicalConstantsandNotation . ........ 8 2.2 Algebra ......................................... 9 2.3 TrigonometricalIdentities . ........ 10 2.4 HyperbolicFunctions. ..... 12 2.5 Differentiation .................................. 13 2.6 StandardDerivatives. ..... 14 2.7 Integration ..................................... 15 2.8 StandardIndefiniteIntegrals . ....... 16 2.9 DefiniteIntegrals ................................ 18 2.10 CurvilinearCoordinateSystems. ......... 19 2.11 VectorsandVectorAlgebra . ...... 22 2.12ComplexNumbers ................................. 25 2.13Series ......................................... 27 2.14 OrdinaryDifferentialEquations . ......... 30 2.15 PartialDifferentiation . ....... 33 2.16 PartialDifferentialEquations . ......... 35 2.17 DeterminantsandMatrices . ...... 36 2.18VectorCalculus................................. 39 2.19FourierSeries .................................. 42 2.20Statistics ..................................... 45 3 Selected Physics Formulae 47 3.1 EquationsofElectromagnetism . ....... 48 3.2 Equations of Relativistic Kinematics and Mechanics . ............. 49 3.3 Thermodynamics and Statistical Physics -
Phaser: an R Package for Phase Plane Analysis of Autonomous ODE Systems by Michael J
CONTRIBUTED RESEARCH ARTICLES 43 phaseR: An R Package for Phase Plane Analysis of Autonomous ODE Systems by Michael J. Grayling Abstract When modelling physical systems, analysts will frequently be confronted by differential equations which cannot be solved analytically. In this instance, numerical integration will usually be the only way forward. However, for autonomous systems of ordinary differential equations (ODEs) in one or two dimensions, it is possible to employ an instructive qualitative analysis foregoing this requirement, using so-called phase plane methods. Moreover, this qualitative analysis can even prove to be highly useful for systems that can be solved analytically, or will be solved numerically anyway. The package phaseR allows the user to perform such phase plane analyses: determining the stability of any equilibrium points easily, and producing informative plots. Introduction Repeatedly, when a system of differential equations is written down, it cannot be solved analytically. This is particularly true in the non-linear case, which unfortunately habitually arises when modelling physical systems. As such, it is common that numerical integration is the only way for a modeller to analyse the properties of their system. Consequently, many software packages exist today to assist in this step. In R, for example, the package deSolve (Soetaert et al., 2010) deals with many classes of differential equation. It allows users to solve first-order stiff and non-stiff initial value problem ODEs, as well as stiff and non-stiff delay differential equations (DDEs), and differential algebraic equations (DAEs) up to index 3. Moreover, it can tackle partial differential equations (PDEs) with the assistance ReacTran (Soetaert and Meysman, 2012). -
Math 6730 : Asymptotic and Perturbation Methods Hyunjoong
Math 6730 : Asymptotic and Perturbation Methods Hyunjoong Kim and Chee-Han Tan Last modified : January 13, 2018 2 Contents Preface 5 1 Introduction to Asymptotic Approximation7 1.1 Asymptotic Expansion................................8 1.1.1 Order symbols.................................9 1.1.2 Accuracy vs convergence........................... 10 1.1.3 Manipulating asymptotic expansions.................... 10 1.2 Algebraic and Transcendental Equations...................... 11 1.2.1 Singular quadratic equation......................... 11 1.2.2 Exponential equation............................. 14 1.2.3 Trigonometric equation............................ 15 1.3 Differential Equations: Regular Perturbation Theory............... 16 1.3.1 Projectile motion............................... 16 1.3.2 Nonlinear potential problem......................... 17 1.3.3 Fredholm alternative............................. 19 1.4 Problems........................................ 20 2 Matched Asymptotic Expansions 31 2.1 Introductory example................................. 31 2.1.1 Outer solution by regular perturbation................... 31 2.1.2 Boundary layer................................ 32 2.1.3 Matching................................... 33 2.1.4 Composite expression............................. 33 2.2 Extensions: multiple boundary layers, etc...................... 34 2.2.1 Multiple boundary layers........................... 34 2.2.2 Interior layers................................. 35 2.3 Partial differential equations............................. 36 2.4 Strongly