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Variation of parameters

In mathematics, variation of parameters, also known as variation of constants, is a general method to solve inhomogeneous linear ordinary differential equations.

For first-order inhomogeneous linear differential equations it is usually possible to find solutions via integrating factors or undetermined coefficients with considerably less effort, although those methods leverage heuristics that involve guessing and do not work for all inhomogeneous linear differential equations.

Variation of parameters extends to linear partial differential equations as well, specifically to inhomogeneous problems for linear evolution equations like the heat equation, wave equation, and vibrating plate equation. In this setting, the method is more often known as Duhamel's principle, named after Jean-Marie Duhamel (1797–1872) who first applied the method to solve the inhomogeneous heat equation. Sometimes variation of parameters itself is called Duhamel's principle and vice versa.

History edit

The method of variation of parameters was first sketched by the Swiss mathematician Leonhard Euler (1707–1783), and later completed by the Italian-French mathematician Joseph-Louis Lagrange (1736–1813).[1]

A forerunner of the method of variation of a celestial body's orbital elements appeared in Euler's work in 1748, while he was studying the mutual perturbations of Jupiter and Saturn.[2] In his 1749 study of the motions of the earth, Euler obtained differential equations for the orbital elements.[3] In 1753, he applied the method to his study of the motions of the moon.[4]

Lagrange first used the method in 1766.[5] Between 1778 and 1783, he further developed the method in two series of memoirs: one on variations in the motions of the planets[6] and another on determining the orbit of a comet from three observations.[7] During 1808–1810, Lagrange gave the method of variation of parameters its final form in a third series of papers.[8]

Description of method edit

Given an ordinary non-homogeneous linear differential equation of order n

 

(i)

Let   be a basis of the vector space of solutions of the corresponding homogeneous equation

 

(ii)

Then a particular solution to the non-homogeneous equation is given by

 

(iii)

where the   are differentiable functions which are assumed to satisfy the conditions

 

(iv)

Starting with (iii), repeated differentiation combined with repeated use of (iv) gives

 

(v)

One last differentiation gives

 

(vi)

By substituting (iii) into (i) and applying (v) and (vi) it follows that

 

(vii)

The linear system (iv and vii) of n equations can then be solved using Cramer's rule yielding

 

where   is the Wronskian determinant of the basis   and   is the Wronskian determinant of the basis with the i-th column replaced by  

The particular solution to the non-homogeneous equation can then be written as

 

Intuitive explanation edit

Consider the equation of the forced dispersionless spring, in suitable units:

 

Here x is the displacement of the spring from the equilibrium x = 0, and F(t) is an external applied force that depends on time. When the external force is zero, this is the homogeneous equation (whose solutions are linear combinations of sines and cosines, corresponding to the spring oscillating with constant total energy).

We can construct the solution physically, as follows. Between times   and  , the momentum corresponding to the solution has a net change   (see: Impulse (physics)). A solution to the inhomogeneous equation, at the present time t > 0, is obtained by linearly superposing the solutions obtained in this manner, for s going between 0 and t.

The homogeneous initial-value problem, representing a small impulse   being added to the solution at time  , is

 

The unique solution to this problem is easily seen to be  . The linear superposition of all of these solutions is given by the integral:

 

To verify that this satisfies the required equation:

 
 

as required (see: Leibniz integral rule).

The general method of variation of parameters allows for solving an inhomogeneous linear equation

 

by means of considering the second-order linear differential operator L to be the net force, thus the total impulse imparted to a solution between time s and s+ds is F(s)ds. Denote by   the solution of the homogeneous initial value problem

 

Then a particular solution of the inhomogeneous equation is

 

the result of linearly superposing the infinitesimal homogeneous solutions. There are generalizations to higher order linear differential operators.

In practice, variation of parameters usually involves the fundamental solution of the homogeneous problem, the infinitesimal solutions   then being given in terms of explicit linear combinations of linearly independent fundamental solutions. In the case of the forced dispersionless spring, the kernel   is the associated decomposition into fundamental solutions.

Examples edit

First-order equation edit

 

The complementary solution to our original (inhomogeneous) equation is the general solution of the corresponding homogeneous equation (written below):

 

This homogeneous differential equation can be solved by different methods, for example separation of variables:

 
 
 
 
 
 

The complementary solution to our original equation is therefore:

 

Now we return to solving the non-homogeneous equation:

 

Using the method variation of parameters, the particular solution is formed by multiplying the complementary solution by an unknown function C(x):

 

By substituting the particular solution into the non-homogeneous equation, we can find C(x):

 
 
 
 

We only need a single particular solution, so we arbitrarily select   for simplicity. Therefore the particular solution is:

 

The final solution of the differential equation is:

 

This recreates the method of integrating factors.

Specific second-order equation edit

Let us solve

 

We want to find the general solution to the differential equation, that is, we want to find solutions to the homogeneous differential equation

 

The characteristic equation is:

 

Since   is a repeated root, we have to introduce a factor of x for one solution to ensure linear independence:   and  . The Wronskian of these two functions is

 

Because the Wronskian is non-zero, the two functions are linearly independent, so this is in fact the general solution for the homogeneous differential equation (and not a mere subset of it).

We seek functions A(x) and B(x) so A(x)u1 + B(x)u2 is a particular solution of the non-homogeneous equation. We need only calculate the integrals

 

Recall that for this example

 

That is,

 
 

where   and   are constants of integration.

General second-order equation edit

We have a differential equation of the form

 

and we define the linear operator

 

where D represents the differential operator. We therefore have to solve the equation   for  , where   and   are known.

We must solve first the corresponding homogeneous equation:

 

by the technique of our choice. Once we've obtained two linearly independent solutions to this homogeneous differential equation (because this ODE is second-order) — call them u1 and u2 — we can proceed with variation of parameters.

Now, we seek the general solution to the differential equation   which we assume to be of the form

 

Here,   and   are unknown and   and   are the solutions to the homogeneous equation. (Observe that if   and   are constants, then  .) Since the above is only one equation and we have two unknown functions, it is reasonable to impose a second condition. We choose the following:

 

Now,

 

Differentiating again (omitting intermediary steps)

 

Now we can write the action of L upon uG as

 

Since u1 and u2 are solutions, then

 

We have the system of equations

 

Expanding,

 

So the above system determines precisely the conditions

 
 

We seek A(x) and B(x) from these conditions, so, given

 

we can solve for (A′(x), B′(x))T, so

 

where W denotes the Wronskian of u1 and u2. (We know that W is nonzero, from the assumption that u1 and u2 are linearly independent.) So,

 

While homogeneous equations are relatively easy to solve, this method allows the calculation of the coefficients of the general solution of the inhomogeneous equation, and thus the complete general solution of the inhomogeneous equation can be determined.

Note that   and   are each determined only up to an arbitrary additive constant (the constant of integration). Adding a constant to   or   does not change the value of   because the extra term is just a linear combination of u1 and u2, which is a solution of   by definition.

See also edit

Notes edit

  1. ^ See:
    • Forest Ray Moulton, An Introduction to Celestial Mechanics, 2nd ed. (first published by the Macmillan Company in 1914; reprinted in 1970 by Dover Publications, Inc., Mineola, New York), page 431.
    • Edgar Odell Lovett (1899) "The theory of perturbations and Lie's theory of contact transformations," The Quarterly Journal of Pure and Applied Mathematics, vol. 30, pages 47–149; see especially pages 48–61.
  2. ^ Euler, L. (1748) "Recherches sur la question des inégalités du mouvement de Saturne et de Jupiter, sujet proposé pour le prix de l'année 1748, par l’Académie Royale des Sciences de Paris" [Investigations on the question of the differences in the movement of Saturn and Jupiter; this subject proposed for the prize of 1748 by the Royal Academy of Sciences (Paris)] (Paris, France: G. Martin, J.B. Coignard, & H.L. Guerin, 1749).
  3. ^ Euler, L. (1749) "Recherches sur la précession des équinoxes, et sur la nutation de l’axe de la terre," Histoire [or Mémoires ] de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 289–325 [published in 1751].
  4. ^ Euler, L. (1753) Theoria motus lunae: exhibens omnes ejus inaequalitates ... [The theory of the motion of the moon: demonstrating all of its inequalities ... ] (Saint Petersburg, Russia: Academia Imperialis Scientiarum Petropolitanae [Imperial Academy of Science (St. Petersburg)], 1753).
  5. ^ Lagrange, J.-L. (1766) “Solution de différens problèmes du calcul integral,” Mélanges de philosophie et de mathématique de la Société royale de Turin, vol. 3, pages 179–380.
  6. ^ See:
    • Lagrange, J.-L. (1781) "Théorie des variations séculaires des élémens des Planetes. Premiere partie, ... ," Nouveaux Mémoires de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 199–276.
    • Lagrange, J.-L. (1782) "Théorie des variations séculaires des élémens des Planetes. Seconde partie, ... ," Nouveaux Mémoires de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 169–292.
    • Lagrange, J.-L. (1783) "Théorie des variations périodiques des mouvemens des Planetes. Premiere partie, ... ," Nouveaux Mémoires de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 161–190.
  7. ^ See:
    • Lagrange, J.-L. (1778) "Sur le probleme de la détermination des orbites des cometes d'après trois observations, premier mémoire" (On the problem of determining the orbits of comets from three observations, first memoir), Nouveaux Mémoires de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 111–123 [published in 1780].
    • Lagrange, J.-L. (1778) "Sur le probleme de la détermination des orbites des cometes d'après trois observations, second mémoire", Nouveaux Mémoires de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 124–161 [published in 1780].
    • Lagrange, J.-L. (1783) "Sur le probleme de la détermination des orbites des cometes d'après trois observations. Troisième mémoire, dans lequel on donne une solution directe et générale du problème.", Nouveaux Mémoires de l'Académie Royale des Sciences et Belles-lettres (Berlin), pages 296–332 [published in 1785].
  8. ^ See:
    • Lagrange, J.-L. (1808) “Sur la théorie des variations des éléments des planètes et en particulier des variations des grands axes de leurs orbites,” Mémoires de la première Classe de l’Institut de France. Reprinted in: Joseph-Louis Lagrange with Joseph-Alfred Serret, ed., Oeuvres de Lagrange (Paris, France: Gauthier-Villars, 1873), vol. 6, pages 713–768.
    • Lagrange, J.-L. (1809) “Sur la théorie générale de la variation des constantes arbitraires dans tous les problèmes de la méchanique,” Mémoires de la première Classe de l’Institut de France. Reprinted in: Joseph-Louis Lagrange with Joseph-Alfred Serret, ed., Oeuvres de Lagrange (Paris, France: Gauthier-Villars, 1873), vol. 6, pages 771–805.
    • Lagrange, J.-L. (1810) “Second mémoire sur la théorie générale de la variation des constantes arbitraires dans tous les problèmes de la méchanique, ... ,” Mémoires de la première Classe de l’Institut de France. Reprinted in: Joseph-Louis Lagrange with Joseph-Alfred Serret, ed., Oeuvres de Lagrange (Paris, France: Gauthier-Villars, 1873), vol. 6, pages 809–816.

References edit

  • Coddington, Earl A.; Levinson, Norman (1955). Theory of Ordinary Differential Equations. McGraw-Hill.
  • Boyce, William E.; DiPrima, Richard C. (2005). Elementary Differential Equations and Boundary Value Problems (8th ed.). Wiley. pp. 186–192, 237–241.
  • Teschl, Gerald (2012). Ordinary Differential Equations and Dynamical Systems. American Mathematical Society.

External links edit

  • Online Notes / Proof by Paul Dawkins, Lamar University.
  • PlanetMath page.
  • A NOTE ON LAGRANGE’S METHOD OF VARIATION OF PARAMETERS

variation, parameters, mathematics, variation, parameters, also, known, variation, constants, general, method, solve, inhomogeneous, linear, ordinary, differential, equations, first, order, inhomogeneous, linear, differential, equations, usually, possible, fin. In mathematics variation of parameters also known as variation of constants is a general method to solve inhomogeneous linear ordinary differential equations For first order inhomogeneous linear differential equations it is usually possible to find solutions via integrating factors or undetermined coefficients with considerably less effort although those methods leverage heuristics that involve guessing and do not work for all inhomogeneous linear differential equations Variation of parameters extends to linear partial differential equations as well specifically to inhomogeneous problems for linear evolution equations like the heat equation wave equation and vibrating plate equation In this setting the method is more often known as Duhamel s principle named after Jean Marie Duhamel 1797 1872 who first applied the method to solve the inhomogeneous heat equation Sometimes variation of parameters itself is called Duhamel s principle and vice versa Contents 1 History 2 Description of method 3 Intuitive explanation 4 Examples 4 1 First order equation 4 2 Specific second order equation 4 3 General second order equation 5 See also 6 Notes 7 References 8 External linksHistory editThe method of variation of parameters was first sketched by the Swiss mathematician Leonhard Euler 1707 1783 and later completed by the Italian French mathematician Joseph Louis Lagrange 1736 1813 1 A forerunner of the method of variation of a celestial body s orbital elements appeared in Euler s work in 1748 while he was studying the mutual perturbations of Jupiter and Saturn 2 In his 1749 study of the motions of the earth Euler obtained differential equations for the orbital elements 3 In 1753 he applied the method to his study of the motions of the moon 4 Lagrange first used the method in 1766 5 Between 1778 and 1783 he further developed the method in two series of memoirs one on variations in the motions of the planets 6 and another on determining the orbit of a comet from three observations 7 During 1808 1810 Lagrange gave the method of variation of parameters its final form in a third series of papers 8 Description of method editGiven an ordinary non homogeneous linear differential equation of order n y n x i 0 n 1 a i x y i x b x displaystyle y n x sum i 0 n 1 a i x y i x b x nbsp i Let y 1 x y n x displaystyle y 1 x ldots y n x nbsp be a basis of the vector space of solutions of the corresponding homogeneous equation y n x i 0 n 1 a i x y i x 0 displaystyle y n x sum i 0 n 1 a i x y i x 0 nbsp ii Then a particular solution to the non homogeneous equation is given by y p x i 1 n c i x y i x displaystyle y p x sum i 1 n c i x y i x nbsp iii where the c i x displaystyle c i x nbsp are differentiable functions which are assumed to satisfy the conditions i 1 n c i x y i j x 0 j 0 n 2 displaystyle sum i 1 n c i x y i j x 0 quad j 0 ldots n 2 nbsp iv Starting with iii repeated differentiation combined with repeated use of iv gives y p j x i 1 n c i x y i j x j 0 n 1 displaystyle y p j x sum i 1 n c i x y i j x quad j 0 ldots n 1 nbsp v One last differentiation gives y p n x i 1 n c i x y i n 1 x i 1 n c i x y i n x displaystyle y p n x sum i 1 n c i x y i n 1 x sum i 1 n c i x y i n x nbsp vi By substituting iii into i and applying v and vi it follows that i 1 n c i x y i n 1 x b x displaystyle sum i 1 n c i x y i n 1 x b x nbsp vii The linear system iv and vii of n equations can then be solved using Cramer s rule yielding c i x W i x W x i 1 n displaystyle c i x frac W i x W x quad i 1 ldots n nbsp where W x displaystyle W x nbsp is the Wronskian determinant of the basis y 1 x y n x displaystyle y 1 x ldots y n x nbsp and W i x displaystyle W i x nbsp is the Wronskian determinant of the basis with the i th column replaced by 0 0 b x displaystyle 0 0 ldots b x nbsp The particular solution to the non homogeneous equation can then be written as i 1 n y i x W i x W x d x displaystyle sum i 1 n y i x int frac W i x W x mathrm d x nbsp Intuitive explanation editConsider the equation of the forced dispersionless spring in suitable units x t x t F t displaystyle x t x t F t nbsp Here x is the displacement of the spring from the equilibrium x 0 and F t is an external applied force that depends on time When the external force is zero this is the homogeneous equation whose solutions are linear combinations of sines and cosines corresponding to the spring oscillating with constant total energy We can construct the solution physically as follows Between times t s displaystyle t s nbsp and t s d s displaystyle t s ds nbsp the momentum corresponding to the solution has a net change F s d s displaystyle F s ds nbsp see Impulse physics A solution to the inhomogeneous equation at the present time t gt 0 is obtained by linearly superposing the solutions obtained in this manner for s going between 0 and t The homogeneous initial value problem representing a small impulse F s d s displaystyle F s ds nbsp being added to the solution at time t s displaystyle t s nbsp is x t x t 0 x s 0 x s F s d s displaystyle x t x t 0 quad x s 0 x s F s ds nbsp The unique solution to this problem is easily seen to be x t F s sin t s d s displaystyle x t F s sin t s ds nbsp The linear superposition of all of these solutions is given by the integral x t 0 t F s sin t s d s displaystyle x t int 0 t F s sin t s ds nbsp To verify that this satisfies the required equation x t 0 t F s cos t s d s displaystyle x t int 0 t F s cos t s ds nbsp x t F t 0 t F s sin t s d s F t x t displaystyle x t F t int 0 t F s sin t s ds F t x t nbsp as required see Leibniz integral rule The general method of variation of parameters allows for solving an inhomogeneous linear equation L x t F t displaystyle Lx t F t nbsp by means of considering the second order linear differential operator L to be the net force thus the total impulse imparted to a solution between time s and s ds is F s ds Denote by x s displaystyle x s nbsp the solution of the homogeneous initial value problem L x t 0 x s 0 x s F s d s displaystyle Lx t 0 quad x s 0 x s F s ds nbsp Then a particular solution of the inhomogeneous equation is x t 0 t x s t d s displaystyle x t int 0 t x s t ds nbsp the result of linearly superposing the infinitesimal homogeneous solutions There are generalizations to higher order linear differential operators In practice variation of parameters usually involves the fundamental solution of the homogeneous problem the infinitesimal solutions x s displaystyle x s nbsp then being given in terms of explicit linear combinations of linearly independent fundamental solutions In the case of the forced dispersionless spring the kernel sin t s sin t cos s sin s cos t displaystyle sin t s sin t cos s sin s cos t nbsp is the associated decomposition into fundamental solutions Examples editFirst order equation edit y p x y q x displaystyle y p x y q x nbsp The complementary solution to our original inhomogeneous equation is the general solution of the corresponding homogeneous equation written below y p x y 0 displaystyle y p x y 0 nbsp This homogeneous differential equation can be solved by different methods for example separation of variables d d x y p x y 0 displaystyle frac d dx y p x y 0 nbsp d y d x p x y displaystyle frac dy dx p x y nbsp d y y p x d x displaystyle dy over y p x dx nbsp 1 y d y p x d x displaystyle int frac 1 y dy int p x dx nbsp ln y p x d x C displaystyle ln y int p x dx C nbsp y e p x d x C C 0 e p x d x displaystyle y pm e int p x dx C C 0 e int p x dx nbsp The complementary solution to our original equation is therefore y c C 0 e p x d x displaystyle y c C 0 e int p x dx nbsp Now we return to solving the non homogeneous equation y p x y q x displaystyle y p x y q x nbsp Using the method variation of parameters the particular solution is formed by multiplying the complementary solution by an unknown function C x y p C x e p x d x displaystyle y p C x e int p x dx nbsp By substituting the particular solution into the non homogeneous equation we can find C x C x e p x d x C x p x e p x d x p x C x e p x d x q x displaystyle C x e int p x dx C x p x e int p x dx p x C x e int p x dx q x nbsp C x e p x d x q x displaystyle C x e int p x dx q x nbsp C x q x e p x d x displaystyle C x q x e int p x dx nbsp C x q x e p x d x d x C 1 displaystyle C x int q x e int p x dx dx C 1 nbsp We only need a single particular solution so we arbitrarily select C 1 0 displaystyle C 1 0 nbsp for simplicity Therefore the particular solution is y p e p x d x q x e p x d x d x displaystyle y p e int p x dx int q x e int p x dx dx nbsp The final solution of the differential equation is y y c y p C 0 e p x d x e p x d x q x e p x d x d x displaystyle begin aligned y amp y c y p amp C 0 e int p x dx e int p x dx int q x e int p x dx dx end aligned nbsp This recreates the method of integrating factors Specific second order equation edit Let us solve y 4 y 4 y cosh x displaystyle y 4y 4y cosh x nbsp We want to find the general solution to the differential equation that is we want to find solutions to the homogeneous differential equation y 4 y 4 y 0 displaystyle y 4y 4y 0 nbsp The characteristic equation is l 2 4 l 4 l 2 2 0 displaystyle lambda 2 4 lambda 4 lambda 2 2 0 nbsp Since l 2 displaystyle lambda 2 nbsp is a repeated root we have to introduce a factor of x for one solution to ensure linear independence u 1 e 2 x displaystyle u 1 e 2x nbsp and u 2 x e 2 x displaystyle u 2 xe 2x nbsp The Wronskian of these two functions is W e 2 x x e 2 x 2 e 2 x e 2 x 2 x 1 e 2 x e 2 x 2 x 1 2 x e 2 x e 2 x e 4 x displaystyle W begin vmatrix e 2x amp xe 2x 2e 2x amp e 2x 2x 1 end vmatrix e 2x e 2x 2x 1 2xe 2x e 2x e 4x nbsp Because the Wronskian is non zero the two functions are linearly independent so this is in fact the general solution for the homogeneous differential equation and not a mere subset of it We seek functions A x and B x so A x u1 B x u2 is a particular solution of the non homogeneous equation We need only calculate the integrals A x 1 W u 2 x b x d x B x 1 W u 1 x b x d x displaystyle A x int 1 over W u 2 x b x mathrm d x B x int 1 over W u 1 x b x mathrm d x nbsp Recall that for this example b x cosh x displaystyle b x cosh x nbsp That is A x 1 e 4 x x e 2 x cosh x d x x e 2 x cosh x d x 1 18 e x 9 x 1 e 2 x 3 x 1 C 1 displaystyle A x int 1 over e 4x xe 2x cosh x mathrm d x int xe 2x cosh x mathrm d x 1 over 18 e x left 9 x 1 e 2x 3x 1 right C 1 nbsp B x 1 e 4 x e 2 x cosh x d x e 2 x cosh x d x 1 6 e x 3 e 2 x C 2 displaystyle B x int 1 over e 4x e 2x cosh x mathrm d x int e 2x cosh x mathrm d x 1 over 6 e x left 3 e 2x right C 2 nbsp where C 1 displaystyle C 1 nbsp and C 2 displaystyle C 2 nbsp are constants of integration General second order equation edit We have a differential equation of the form u p x u q x u f x displaystyle u p x u q x u f x nbsp and we define the linear operator L D 2 p x D q x displaystyle L D 2 p x D q x nbsp where D represents the differential operator We therefore have to solve the equation L u x f x displaystyle Lu x f x nbsp for u x displaystyle u x nbsp where L displaystyle L nbsp and f x displaystyle f x nbsp are known We must solve first the corresponding homogeneous equation u p x u q x u 0 displaystyle u p x u q x u 0 nbsp by the technique of our choice Once we ve obtained two linearly independent solutions to this homogeneous differential equation because this ODE is second order call them u1 and u2 we can proceed with variation of parameters Now we seek the general solution to the differential equation u G x displaystyle u G x nbsp which we assume to be of the form u G x A x u 1 x B x u 2 x displaystyle u G x A x u 1 x B x u 2 x nbsp Here A x displaystyle A x nbsp and B x displaystyle B x nbsp are unknown and u 1 x displaystyle u 1 x nbsp and u 2 x displaystyle u 2 x nbsp are the solutions to the homogeneous equation Observe that if A x displaystyle A x nbsp and B x displaystyle B x nbsp are constants then L u G x 0 displaystyle Lu G x 0 nbsp Since the above is only one equation and we have two unknown functions it is reasonable to impose a second condition We choose the following A x u 1 x B x u 2 x 0 displaystyle A x u 1 x B x u 2 x 0 nbsp Now u G x A x u 1 x B x u 2 x A x u 1 x B x u 2 x A x u 1 x A x u 1 x B x u 2 x B x u 2 x A x u 1 x B x u 2 x A x u 1 x B x u 2 x A x u 1 x B x u 2 x displaystyle begin aligned u G x amp left A x u 1 x B x u 2 x right amp left A x u 1 x right left B x u 2 x right amp A x u 1 x A x u 1 x B x u 2 x B x u 2 x amp A x u 1 x B x u 2 x A x u 1 x B x u 2 x amp A x u 1 x B x u 2 x end aligned nbsp Differentiating again omitting intermediary steps u G x A x u 1 x B x u 2 x A x u 1 x B x u 2 x displaystyle u G x A x u 1 x B x u 2 x A x u 1 x B x u 2 x nbsp Now we can write the action of L upon uG as L u G A x L u 1 x B x L u 2 x A x u 1 x B x u 2 x displaystyle Lu G A x Lu 1 x B x Lu 2 x A x u 1 x B x u 2 x nbsp Since u1 and u2 are solutions then L u G A x u 1 x B x u 2 x displaystyle Lu G A x u 1 x B x u 2 x nbsp We have the system of equations u 1 x u 2 x u 1 x u 2 x A x B x 0 f displaystyle begin bmatrix u 1 x amp u 2 x u 1 x amp u 2 x end bmatrix begin bmatrix A x B x end bmatrix begin bmatrix 0 f end bmatrix nbsp Expanding A x u 1 x B x u 2 x A x u 1 x B x u 2 x 0 f displaystyle begin bmatrix A x u 1 x B x u 2 x A x u 1 x B x u 2 x end bmatrix begin bmatrix 0 f end bmatrix nbsp So the above system determines precisely the conditions A x u 1 x B x u 2 x 0 displaystyle A x u 1 x B x u 2 x 0 nbsp A x u 1 x B x u 2 x L u G f displaystyle A x u 1 x B x u 2 x Lu G f nbsp We seek A x and B x from these conditions so given u 1 x u 2 x u 1 x u 2 x A x B x 0 f displaystyle begin bmatrix u 1 x amp u 2 x u 1 x amp u 2 x end bmatrix begin bmatrix A x B x end bmatrix begin bmatrix 0 f end bmatrix nbsp we can solve for A x B x T so A x B x u 1 x u 2 x u 1 x u 2 x 1 0 f 1 W u 2 x u 2 x u 1 x u 1 x 0 f displaystyle begin bmatrix A x B x end bmatrix begin bmatrix u 1 x amp u 2 x u 1 x amp u 2 x end bmatrix 1 begin bmatrix 0 f end bmatrix frac 1 W begin bmatrix u 2 x amp u 2 x u 1 x amp u 1 x end bmatrix begin bmatrix 0 f end bmatrix nbsp where W denotes the Wronskian of u1 and u2 We know that W is nonzero from the assumption that u1 and u2 are linearly independent So A x 1 W u 2 x f x B x 1 W u 1 x f x A x 1 W u 2 x f x d x B x 1 W u 1 x f x d x displaystyle begin aligned A x amp 1 over W u 2 x f x amp B x amp 1 over W u 1 x f x A x amp int 1 over W u 2 x f x mathrm d x amp B x amp int 1 over W u 1 x f x mathrm d x end aligned nbsp While homogeneous equations are relatively easy to solve this method allows the calculation of the coefficients of the general solution of the inhomogeneous equation and thus the complete general solution of the inhomogeneous equation can be determined Note that A x displaystyle A x nbsp and B x displaystyle B x nbsp are each determined only up to an arbitrary additive constant the constant of integration Adding a constant to A x displaystyle A x nbsp or B x displaystyle B x nbsp does not change the value of L u G x displaystyle Lu G x nbsp because the extra term is just a linear combination of u1 and u2 which is a solution of L displaystyle L nbsp by definition See also editAlekseev Grobner formula a generalization of the variation of constants formula Reduction of orderNotes edit See Forest Ray Moulton An Introduction to Celestial Mechanics 2nd ed first published by the Macmillan Company in 1914 reprinted in 1970 by Dover Publications Inc Mineola New York page 431 Edgar Odell Lovett 1899 The theory of perturbations and Lie s theory of contact transformations The Quarterly Journal of Pure and Applied Mathematics vol 30 pages 47 149 see especially pages 48 61 Euler L 1748 Recherches sur la question des inegalites du mouvement de Saturne et de Jupiter sujet propose pour le prix de l annee 1748 par l Academie Royale des Sciences de Paris Investigations on the question of the differences in the movement of Saturn and Jupiter this subject proposed for the prize of 1748 by the Royal Academy of Sciences Paris Paris France G Martin J B Coignard amp H L Guerin 1749 Euler L 1749 Recherches sur la precession des equinoxes et sur la nutation de l axe de la terre Histoire or Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 289 325 published in 1751 Euler L 1753 Theoria motus lunae exhibens omnes ejus inaequalitates The theory of the motion of the moon demonstrating all of its inequalities Saint Petersburg Russia Academia Imperialis Scientiarum Petropolitanae Imperial Academy of Science St Petersburg 1753 Lagrange J L 1766 Solution de differens problemes du calcul integral Melanges de philosophie et de mathematique de la Societe royale de Turin vol 3 pages 179 380 See Lagrange J L 1781 Theorie des variations seculaires des elemens des Planetes Premiere partie Nouveaux Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 199 276 Lagrange J L 1782 Theorie des variations seculaires des elemens des Planetes Seconde partie Nouveaux Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 169 292 Lagrange J L 1783 Theorie des variations periodiques des mouvemens des Planetes Premiere partie Nouveaux Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 161 190 See Lagrange J L 1778 Sur le probleme de la determination des orbites des cometes d apres trois observations premier memoire On the problem of determining the orbits of comets from three observations first memoir Nouveaux Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 111 123 published in 1780 Lagrange J L 1778 Sur le probleme de la determination des orbites des cometes d apres trois observations second memoire Nouveaux Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 124 161 published in 1780 Lagrange J L 1783 Sur le probleme de la determination des orbites des cometes d apres trois observations Troisieme memoire dans lequel on donne une solution directe et generale du probleme Nouveaux Memoires de l Academie Royale des Sciences et Belles lettres Berlin pages 296 332 published in 1785 See Lagrange J L 1808 Sur la theorie des variations des elements des planetes et en particulier des variations des grands axes de leurs orbites Memoires de la premiere Classe de l Institut de France Reprinted in Joseph Louis Lagrange with Joseph Alfred Serret ed Oeuvres de Lagrange Paris France Gauthier Villars 1873 vol 6 pages 713 768 Lagrange J L 1809 Sur la theorie generale de la variation des constantes arbitraires dans tous les problemes de la mechanique Memoires de la premiere Classe de l Institut de France Reprinted in Joseph Louis Lagrange with Joseph Alfred Serret ed Oeuvres de Lagrange Paris France Gauthier Villars 1873 vol 6 pages 771 805 Lagrange J L 1810 Second memoire sur la theorie generale de la variation des constantes arbitraires dans tous les problemes de la mechanique Memoires de la premiere Classe de l Institut de France Reprinted in Joseph Louis Lagrange with Joseph Alfred Serret ed Oeuvres de Lagrange Paris France Gauthier Villars 1873 vol 6 pages 809 816 References editCoddington Earl A Levinson Norman 1955 Theory of Ordinary Differential Equations McGraw Hill Boyce William E DiPrima Richard C 2005 Elementary Differential Equations and Boundary Value Problems 8th ed Wiley pp 186 192 237 241 Teschl Gerald 2012 Ordinary Differential Equations and Dynamical Systems American Mathematical Society External links editOnline Notes Proof by Paul Dawkins Lamar University PlanetMath page A NOTE ON LAGRANGE S METHOD OF VARIATION OF PARAMETERS Retrieved from https en wikipedia org w index php title Variation of parameters amp oldid 1188558059, wikipedia, wiki, book, books, library,

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