Ordinary Differential Equations

Total Page:16

File Type:pdf, Size:1020Kb

Ordinary Differential Equations Ordinary Differential Equations William G. Faris August 16, 1992 Contents 1 Growth and Decay 3 1.1 Linear constant coefficient equations . 3 1.2 Autonomous equations . 4 2 Oscillations 5 2.1 Linear constant coefficient equations . 5 2.1.1 Growth and Decay . 6 2.1.2 Oscillation . 6 2.1.3 Shearing . 7 2.1.4 Inhomogeneous equations . 7 2.2 Autonomous Systems . 9 2.3 Limit cycles . 11 3 Conserved Quantities 13 3.1 Vector fields . 13 3.2 Hamiltonian systems . 14 3.3 Exact equations . 16 3.4 Integrating factors . 17 3.5 Homogeneous equations . 19 4 Forcing 21 4.1 ISETL . 21 4.1.1 Expressions . 21 4.1.2 Statements . 22 4.2 Solving equations . 22 4.3 Linear equations . 24 4.4 Non-linear equations . 25 1 2 CONTENTS 5 Numerics 27 5.1 Existence . 27 5.2 Uniqueness . 28 5.3 Numerics . 28 6 Resonance 31 6.1 Forced linear systems . 31 6.2 Forced constant coefficient linear systems . 32 6.3 Resonance . 33 6.4 General forcing terms . 33 7 Music of the Spheres 35 7.1 The circle . 35 7.2 The plane . 35 7.3 The sphere . 37 Chapter 1 Growth and Decay 1.1 Linear constant coefficient equations The simplest differential equation is the equation of uniform motion: dy = b; (1.1) dt where b is constant. Its solution is y = y0 + bt: (1.2) The next simplest is the equation of growth or decay: dy = ay; (1.3) dt where a is constant. This is the homogeneous linear constant coefficient equation. Its solution is at y = y0e : (1.4) These may be combined in the general linear constant coefficient equa- tion: dy = ay + b; (1.5) dt where a and b are constants. The general solution for a 6= 0 is b y = Ceat − : (1.6) a The solution with y = y0 at t = 0 is b y = y eat + (eat − 1): (1.7) 0 a 3 4 CHAPTER 1. GROWTH AND DECAY 1.2 Autonomous equations The general autonomous equation is dy = f(y): (1.8) dt An equilibrium point is a solution of f(r) = 0. For each equilibrium point we have a solution y = r. Near an equilibrium point f(y) ≈ f 0(r)(y − r). An equilibrium point r is attractive if f 0(r) < 0 and repulsive if f 0(r) > 0. One can attempt to find the general solution of the equation by inte- grating Z 1 Z dy = dt: (1.9) f(y) Problems 1. If a population grows by dp=dt = :05p, how long does it take to double in size? 2. The velocity of a falling body (in the downward direction) is given by dv=dt = g − kv, where g = 32 and k = 1=4. If v = 0 when t = 0, what is the limiting velocity as t ! 1? 3. Consider dy=dt = ay + b where y = y0 when t = 0. Fix t and find the limit of the solution y as a ! 0. 4. A population grows by dp=dt = ap − bp2. Here a > 0, b > 0, and 0 < p < a=b. Find the solution with p = p0 at t = 0. Do this by letting u = 1=p and solving the resulting differential equation for u. 5. Do the same problem by integrating 1=(ap−bp2) dp = dt. Use partial fractions. 6. In the same problem, find the limiting population as t ! 1. 7. Use Phaser to explore the solutions of dx=dt = x − x3. Try many different initial conditions. What pattern emerges? Discuss the limit of x as t ! 1 as a function of the initial condition x0. Chapter 2 Oscillations 2.1 Linear constant coefficient equations The homogeneous linear constant coefficient system is of the form dx = ax + by (2.1) dt dy = cx + dy: (2.2) dt Try a solution of the form x = veλt (2.3) y = weλt: (2.4) We obtain the eigenvalue equation av + bw = λv (2.5) cv + dw = λw: (2.6) This has a non-zero solution only when λ satisfies λ2 −(a+d)λ+ad−bc = 0. We can express the same ideas in matrix notation. The equation is dx = Ax: (2.7) dt The trial solution is x = veλt: (2.8) The eigenvalue equation is Av = λv: (2.9) This has a non-zero solution only when det(λI − A) = 0. 5 6 CHAPTER 2. OSCILLATIONS 2.1.1 Growth and Decay The first case is real and unequal eigenvalues λ1 6= λ2. This takes place when (a − d)2 + 4bc > 0. There are two solutions corresponding to two independent eigenvectors. The general solution is a linear combination of these two. In matrix notation this is λ1t λ2t x = c1v1e + c2v2e : (2.10) When the two eigenvalues are both positive or both negative, the equilib- rium is called a node. When one eigenvalue is positive and one is negative, it is called a saddle. An attractive node corresponds to an overdamped oscillator. 2.1.2 Oscillation The second case is complex conjugate unequal eigenvalues λ = α + i! and λ¯ = α − i! with α = (a + d)=2 and ! > 0. This takes place when (a−d)2 +4bc < 0. There are two independent complex conjugate solutions. These are expressed in terms of eλt = eαtei!t and eλt¯ = eαte−i!t. Their real and imaginary parts are independent real solutions. These are expressed in terms of eαt cos(!t) and eαt sin(!t). In matrix notation we have complex eigenvectors u±iv and the solutions are αt ±i!t x = (c1 ± ic2)e e (u ± iv): (2.11) Taking the real part gives αt αt x = c1e (cos(!t)u − sin(!t)v) − c2e (sin(!t)u + cos(!t)v): (2.12) ±iθ If we write ci ± ic2 = ce , these take the alternate forms x = ceαte±i(!t+θ)(u ± iv): (2.13) and x = ceαt(cos(!t + θ)u − sin(!t + θ)v): (2.14) From this we see that the solution is characterized by an amplitude c and a phase θ. When the two conjugate eigenvalues are pure imaginary, the equilibrium is called a center. When the two conjugate eigenvalues have a non-zero real part, it is called a spiral (or a focus). An center corresponds to an undamped oscillator. An attractive spiral corresponds to an underdamped oscillator. 2.1. LINEAR CONSTANT COEFFICIENT EQUATIONS 7 2.1.3 Shearing The remaining case is when there is only one eigenvalue λ = (a+d)=2. This takes place when (a − d)2 + 4bc = 0. In this case we neeed to try a solution of the form x = peλt + vteλt (2.15) y = qeλt + wteλt: (2.16) We obtain the same eigenvalue equation together with the equation ap + bq = λp + v (2.17) cp + dq = λq + w: (2.18) In practice we do not need to solve for the eigenvector: we merely take p, q determined by the initial conditions and use the last equation to solve for v, w. Im matrix notation this becomes x = peλt + vteλt (2.19) with Ap = λp + v: (2.20) 2.1.4 Inhomogeneous equations The general linear constant coefficient equation is dx = Ax + r: (2.21) dt When A is non-singular we may rewrite this as dx = A(x − s); (2.22) dt where s = −A−1r is constant. Thus x = s is a particular solution. The gen- eral solution is the sum of this particular solution with the general solution of the homogeneous equation. Problems 1. Find the general solution of the system dx = x + 3y dt dy = 5x + 3y: dt 8 CHAPTER 2. OSCILLATIONS 2. Find the solution of this equation with the initial condition x = 1 and y = 3 when t = 0. 3. Use Phaser to sketch the direction field in the above problem. Sketch the given solution in the x, y phase space. Experiment to find a solution that passes very close to the origin, and sketch it. 4. Write the Taylor series of ez about z = 0. Plug in z = iθ, where i2 = −1. Show that eiθ = cos θ + i sin θ. 5. Find the general solution of the system dx = x + 5y dt dy = −x − 3y: dt 6. Find the solution of this equation with the initial condition x = 5 and y = 4 when t = 0. 7. User Phaser to sketch the direction field in the above problem. Use Phaser to find the given solution in phase space. Also plot x versus t and y versus t. 8. A frictionless spring has mass m > 0 and spring constant k > 0. Its displacement and velocity x and y satisfy dx = y dt dy m = −kx: dt Describe the motion. 9. A spring has mass m > 0 and spring constant k > 0 and friction constant f > 0. Its displacement and velocity x and y satisfy dx = y dt dy m = −kx − fy: dt Describe the motion in the case f 2 − 4k < 0 (underdamped). 10. Take m = 1 and k = 1 and f = 0:1. Use Phaser to sketch the direction field and the solution in the phase plane. Also sketch x as a function of t. 2.2. AUTONOMOUS SYSTEMS 9 11. In the preceding problem, describe the motion in the case f 2 − 4k > 0 (overdamped). Is it possible for the oscillator displacement x to overshoot the origin? If so, how many times? 12. An object has mass m > 0 and its displacement and velocity x and y satisfy dx = y dt dy m = 0: dt Describe the motion. 13. Use Phaser to solve the above equation with many initial condition with x = 0 and with varying value of y.
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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 .
    [Show full text]
  • 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 .
    [Show full text]
  • 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
    [Show full text]
  • FIRST-ORDER ORDINARY DIFFERENTIAL EQUATIONS III: Numerical and More Analytic Methods
    FIRST-ORDER ORDINARY DIFFERENTIAL EQUATIONS III: Numerical and More Analytic Methods David Levermore Department of Mathematics University of Maryland 30 September 2012 Because the presentation of this material in lecture will differ from that in the book, I felt that notes that closely follow the lecture presentation might be appreciated. Contents 8. First-Order Equations: Numerical Methods 8.1. Numerical Approximations 2 8.2. Explicit and Implicit Euler Methods 3 8.3. Explicit One-Step Methods Based on Taylor Approximation 4 8.3.1. Explicit Euler Method Revisited 4 8.3.2. Local and Global Errors 4 8.3.3. Higher-Order Taylor-Based Methods (not covered) 5 8.4. Explicit One-Step Methods Based on Quadrature 6 8.4.1. Explicit Euler Method Revisited Again 6 8.4.2. Runge-Trapezoidal Method 7 8.4.3. Runge-Midpoint Method 9 8.4.4. Runge-Kutta Method 10 8.4.5. General Runge-Kutta Methods (not covered) 12 9. Exact Differential Forms and Integrating Factors 9.1. Implicit General Solutions 15 9.2. Exact Differential Forms 16 9.3. Integrating Factors 20 10. Special First-Order Equations and Substitution 10.1. Linear Argument Equations (not covered) 25 10.2. Dilation Invariant Equations (not covered) 26 10.3. Bernoulli Equations (not covered) 27 10.4. Substitution (not covered) 29 1 2 8. First-Order Equations: Numerical Methods 8.1. Numerical Approximations. Analytic methods are either difficult or impossible to apply to many first-order differential equations. In such cases direction fields might be the only graphical method that we have covered that can be applied.
    [Show full text]
  • Phase-Space Matrix Representation of Differential Equations for Obtaining the Energy Spectrum of Model Quantum Systems
    Phase-space matrix representation of differential equations for obtaining the energy spectrum of model quantum systems Juan C. Morales, Carlos A. Arango1, a) Department of Chemical Sciences, Universidad Icesi, Cali, Colombia (Dated: 27 August 2021) Employing the phase-space representation of second order ordinary differential equa- tions we developed a method to find the eigenvalues and eigenfunctions of the 1- dimensional time independent Schr¨odinger equation for quantum model systems. The method presented simplifies some approaches shown in textbooks, based on asymptotic analyses of the time-independent Schr¨odinger equation, and power series methods with recurrence relations. In addition, the method presented here facilitates the understanding of the relationship between the ordinary differential equations of the mathematical physics and the time independent Schr¨odinger equation of physical models as the harmonic oscillator, the rigid rotor, the Hydrogen atom, and the Morse oscillator. Keywords: phase-space, model quantum systems, energy spectrum arXiv:2108.11487v1 [quant-ph] 25 Aug 2021 a)Electronic mail: [email protected] 1 I. INTRODUCTION The 1-dimensional time independent Schr¨odinger equation (TISE) can be solved analyt- ically for few physical models. The harmonic oscillator, the rigid rotor, the Hydrogen atom, and the Morse oscillator are examples of physical models with known analytical solution of the TISE (1). The analytical solution of the TISE for a physical model is usually obtained by using the ansatz of a wavefunction as a product of two functions, one of these functions acts as an integrating factor (2), the other function produces a differential equation solv- able either by Frobenius series method or by directly comparing with a template ordinary differential equation (ODE) with known solution (3).
    [Show full text]
  • Mathematics for Chemistry Prof. Madhav Ranganathan Department of Chemistry Indian Institute of Technology, Kanpur
    Mathematics for Chemistry Prof. Madhav Ranganathan Department of Chemistry Indian Institute of Technology, Kanpur Module - 05 Lecture - 23 Integrating Factors Today I will be talking about the Integrating Factor method, which is a method for solving differential equations; first order differential equations which cannot be expressed as exact differentials. (Refer Slide Time: 00:22) (Refer Slide Time: 00:27) (Refer Slide Time: 02:59) So, just to remind ourselves about exact and in exact differentials. We said that, we can write our first order differential equation as M times dx plus N times dy equal to 0; where M and N are functions of x and y. And what we said is at an exact differential implies. So, exact implies dou N by dou y equal to dou N by dou x. So, then you say it like that. If it is not exact; so if not exact then can we find some function alpha of x y such that alpha times M dx plus alpha times N dy equal to 0 is an exact differential. So, what I mean is that the left hand side is an exact differential. So, what I did is I just took this equation multiplied it by alpha. So, the right hand side will be 0 into alpha which will still be 0. Now, what I have is alpha M and alpha N instead of M and N. Now if this is an exact differential. So, can we find such an alpha? So, this is the main goal of this idea of integrating factor.
    [Show full text]
  • Solving 1St Order Odes
    Solving First Order ODEs Table of contents Solving First Order ODEs ............................................... 1 1. Introduction ..................................... ................. 1 Side: Two ways of writing a semilinear 1st order ODE . .............. 2 2. Integrating factors and separation of variables . ......................... 2 Side: One must be careful when multiplying an ODE by a function .............. 3 Side:Theroadahead .................................. ......... 3 3. Linear1storderequations .......................... ................... 4 Summary: Solving 1st order linear equations . ............... 6 4. Separableequations ............................... .................. 7 Summary: Solvingseparable equations . .............. 9 5. Exactequations ................................... ................ 9 Side:Theoperator“d” ................................ ........... 9 6. Non-exactequations ............................... .................. 12 7. Solvable equations in disguise: Transformation method . ......................... 18 7.1. Homogeneousequation ............................ ............... 18 7.2. dy G a x b y ................................................ 19 dx = ( + ) 7.3. Bernoulliequation .............................. ................ 19 7.4. Equations with linear coefficients (NOT REQUIRED FOR 334 FALL2010) ......... 20 8. Direction field, numerics, and well-posedness theory . ......................... 22 8.1. Directionfield .................................. ............... 22 8.2. Numerics ......................................
    [Show full text]
  • Analytic Solutions for Third Order Ordinary Differential Equations
    2019 HAWAII UNIVERSITY INTERNATIONAL CONFERENCES SCIENCE, TECHNOLOGY & ENGINEERING, ARTS, MATHEMATICS & EDUCATION JUNE 5 - 7, 2019 HAWAII PRINCE HOTEL WAIKIKI, HONOLULU, HAWAII ANALYTIC SOLUTIONS FOR THIRD ORDER ORDINARY DIFFERENTIAL EQUATIONS BECCAR-VARELA, MARIA P. ET AL UNIVERSITY OF TEXAS AT EL PASO EL PASO, TEXAS Dr. Maria P. Beccar-Varela Department of Mathematical Sciences University of Texas at El Paso El Paso, Texas Mr. Md Al Masum Bhuiyan Mr. Osei K. Tweneboah Computational Science Program University of Texas at El Paso El Paso, Texas Dr. Maria C. Mariani Department of Mathematical Sciences and Computational Science Program University of Texas at El Paso El Paso, Texas Analytic Solutions for Third Order Ordinary Differential Equations Synopsis: This work studies an analytic approach for solving higher order ordinary differential equations (ODEs). We develop alternate techniques for solving third order ODEs and discuss possible generalizations to higher order ODEs. The techniques are effective for solving complex ODEs and could be used in other application of sciences such as physics, engineering, and applied sciences. Analytic Solutions for Third Order Ordinary Differential Equations Maria P. Beccar-Varela ∗, Md Al Masum Bhuiyany, Maria C. Marianiz and Osei K. Tweneboahx Abstract This paper focuses on an analytic approach for solving higher order ordinary differential equations (ODEs). We develop a self-adjoint for- mulation and integrating-factor techniques to solve third order ODEs. The necessary conditions for ODEs to be self-adjoint are also pro- vided. Under these conditions, we find the analytic solution of the ODEs. The solutions produced in this work are exact unlike numeri- cal solutions which have approximation errors.
    [Show full text]
  • Solving Linear First-Order Differential Equations Leonard Euler's Integrating Factor Method
    Ursinus College Digital Commons @ Ursinus College Transforming Instruction in Undergraduate Differential Equations Mathematics via Primary Historical Sources (TRIUMPHS) Summer 2020 Solving Linear First-Order Differential Equations Leonard Euler's Integrating Factor Method Adam E. Parker Wittenberg University Follow this and additional works at: https://digitalcommons.ursinus.edu/triumphs_differ Part of the Curriculum and Instruction Commons, Educational Methods Commons, Higher Education Commons, and the Science and Mathematics Education Commons Click here to let us know how access to this document benefits ou.y Recommended Citation Parker, Adam E., "Solving Linear First-Order Differential Equations Leonard Euler's Integrating Factor Method" (2020). Differential Equations. 4. https://digitalcommons.ursinus.edu/triumphs_differ/4 This Course Materials is brought to you for free and open access by the Transforming Instruction in Undergraduate Mathematics via Primary Historical Sources (TRIUMPHS) at Digital Commons @ Ursinus College. It has been accepted for inclusion in Differential Equations by an authorized administrator of Digital Commons @ Ursinus College. For more information, please contact [email protected]. Solving Linear First-Order Differential Equations Leonard Euler’s Integrating Factor Method Adam E. Parker∗ May 26, 2021 1 Introduction In 1926, British mathematician E. L. Ince (1891–1941) described the typical evolution of solution techniques from calculus (and differential equations and science in general).1 1111111111111111111111111111111111111111 The early history of the infinitesimal calculus abounds in instances of problems solved through the agency of what were virtually differential equations; it is even true to say that the problem of integration, which may be regarded as the solution of the simplest of all types of differential equations, was a practical problem even in the middle of the sixteenth century.
    [Show full text]
  • Ordinary Differential Equations Math 22B-002, Spring 2017 Final Exam: Solutions 1. [15 Pts.] Solve the Initial Value Problem
    Ordinary Differential Equations Math 22B-002, Spring 2017 Final Exam: Solutions 1. [15 pts.] Solve the initial value problem 6y00 − y0 − y = 0; y(0) = 10; y0(0) = 0: Solution. • The characteristic equation is 6r2 −r −1 = 0 with roots r = 1=2; −1=3, so the general solution is x=2 −x=3 y(x) = c1e + c2e : • The initial conditions are satisfied if 1 1 c + c = 10; c − c = 0 1 2 2 1 3 2 whose solution is c1 = 4, c2 = 6, so y(x) = 4ex=2 + 6e−x=3: 1 2. [20 pts.] (a) Let y0 is an arbitrary constant. Find the solution y(x) of the initial-value problem 0 y − 2xy = x; y(0) = y0: (b) For what initial value y0 does the solution remain bounded as x ! +1? What is the solution in that case? Solution. • The ODE is first-order, linear, and nohomogeneous, so we use the in- tegrating factor method. • The integrating factor with coefficient p(x) = −2x is given by Z µ(x) = exp − 2x dx = e−x2 : • Multiplying the ODE by the integrating factor and writing the left- hand side as an exact derivative, we get that 2 0 2 e−x y = xe−x ; so 2 Z 2 1 2 e−x y(x) = xe−x dx + c = − ex + c; 2 and the general solution is 1 2 y(x) = − + cex : 2 • The initial condition gives y0 = −1=2 + c, so c = y0 + 1=2 and 1 1 2 y(x) = − + y + ex : 2 0 2 • (b) The solution remains bounded as x ! 1 if c = 0 and y0 = −1=2.
    [Show full text]