image equation


In solving an initial value problemMathworldPlanetmathPlanetmath leading to an ordinary differential equationMathworldPlanetmath, the Laplace transformMathworldPlanetmath offers often a way to simplify the equation: both sides are Laplace transformed.  The transformed equation, the so-called image equation, is in many cases simplier than the original differential equation, since it does not contain the derivatives of the unknown function y⁢(t).  From the image equation one may solve the Laplace transform Y⁢(s) of y⁢(t) and then inverse transform Y⁢(s) getting y⁢(t).

Let’s consider e.g. the ordinary n’th order linear differential equation

a0⁢dn⁢yd⁢t+a1⁢dn-1⁢yd⁢xn-1+…+an-1⁢d⁢yd⁢t+an⁢y⁢(t)=f⁢(t) (1)

subject to the initial conditions

y⁢(0)=y0,y′⁢(0)=y0′,…,yn-1⁢(0)=y0(n-1). (2)

Due to the linearity of the Laplace transform the image equation of (1) is

a0⁢ℒ⁢{dn⁢yd⁢xn}+a1⁢ℒ⁢{dn-1⁢yd⁢xn-1}+…+an⁢ℒ⁢{y⁢(t)}=ℒ⁢{f⁢(t)}. (3)

Denote  ℒ{y(t)}=:Y(s)  and  ℒ{f(t)}=:F(s).  We put into (3) the expressions of the Laplace transforms of the derivatives on the left hand side (see “Laplace transforms of derivatives (http://planetmath.org/LaplaceTransformsOfDerivatives)”) getting

a0⁢[sn⁢Y⁢(s)-(sn-1⁢y0+sn-2⁢y0′+…+y0(n-1))]
+a1⁢[sn-1⁢Y⁢(s)-(sn-2⁢y0+sn-3⁢y0′+…+y0(n-2))]
+…  …  …  …
+an-1⁢[s⁢Y⁢(s)-(y0)]
= F⁢(s).

This equation is simplified to

(a0⁢sn+a1⁢sn-1+…+an-1⁢s+an)⁢Y⁢(s)=
a0⁢[y0⁢sn-1+y0′⁢sn-2+…+y0(n-1)]+
+a1⁢[y0⁢sn-2+y0′⁢sn-3+…+y0(n-2)]+
+…  …  …  …+
+an-2⁢[y0⁢s+y0′]+an-1⁢[y0]+F⁢(s).

For brevity, denote in the last equation the polynomial multiplier of Y⁢(s) by φ⁢(s) and the sum preceding F⁢(s) by ψ⁢(s).  Then the equation can be written as

φ⁢(s)⁢Y⁢(s)=ψ⁢(s)+F⁢(s),

i.e.

Y⁢(s)=ψ⁢(s)φ⁢(s)+F⁢(s)φ⁢(s). (4)

The function Y⁢(s) defined by (4) is the Laplace transform of the solution y⁢(t) of the differential equation (1) which satisfies the initial conditions (2).  If we now find a function y*⁢(t) the Laplace transform of which is the function Y⁢(s) defined by (4), then y*⁢(t) will do for y⁢(t) due to the uniqueness property of Laplace transform expressed in the entry “Mellin’s inverse formula (http://planetmath.org/MellinsInverseFormula)”.
If we seek the solution of (1) satisfying the zero initial conditions

x0=x0′=x0′′=…=x0(n-1)=0,

then  ψ⁢(s)≡0  and

Y⁢(s)=F⁢(s)φ⁢(s),

i.e.

Y⁢(s)=F⁢(s)a0⁢sn+a1⁢sn-1+…+an.

Example.  The 4’th order differential equation

y′′′′⁢(t)+y⁢(t)= 0 (5)

should be solved with the initial conditions

y⁢(0)=y′′′⁢(0)=1,y′⁢(0)=y′′⁢(0)=0.

The image equation of (5) is

s4⁢Y⁢(s)-s3⁢y⁢(0)-s2⁢y′⁢(0)-s⁢y′′⁢(0)-y′′′⁢(0)+Y⁢(s)= 0,

i.e.

(s4+1)⁢Y⁢(s)=s3+1.

Thus one needs to determine the inverse Laplace transform of

Y⁢(s)=14⋅4⁢s3s4+1+1s4+1. (6)

The zeroes of the numerator s4+1 are the eighth roots of unity ei⁢π4, ei⁢3⁢π4, ei⁢5⁢π4, ei⁢7⁢π4, in other words the complex numbersPlanetmathPlanetmath ±1±i2.  By the special case (3) of the Heaviside formula, the first addend of (6) corresponds the original function

14⁢∑±e±1±i2⁢t=et2+e-t22⋅ei⁢t2+e-i⁢t22=cosh⁡t2⁢cos⁡t2.

Utilizing also the general Heaviside formula (http://planetmath.org/HeavisideFormula) (1), one can get from (6) the result

y⁢(t):=cosh⁡t2⁢cos⁡t2+12⁢(cosh⁡t2⁢sin⁡t2-sinh⁡t2⁢cos⁡t2).

References

  • 1 N. Piskunov: Diferentsiaal- ja integraalarvutus kõrgematele tehnilistele õppeasutustele. Teine köide. Viies trükk.  Kirjastus Valgus, Tallinn (1966).

Title image equation
Canonical name ImageEquation
Date of creation 2014-03-20 20:16:56
Last modified on 2014-03-20 20:16:56
Owner pahio (2872)
Last modified by pahio (2872)
Numerical id 13
Author pahio (2872)
Entry type Topic
Classification msc 34A05
Classification msc 44A10