Euler-Lagrange Differential Equation


The Euler-Lagrange differential equation is the fundamental equation of calculus of variations. It states that if J is defined by an integral of the form

J=intf(t,y,y^.)dt,

(1)

where

y^.=(dy)/(dt),

(2)

then J has a stationary value if the Euler-Lagrange differential equation

(partialf)/(partialy)-d/(dt)((partialf)/(partialy^.))=0

(3)

is satisfied.

If time-derivative notation y^. is replaced instead by space-derivative notation y_x, the equation becomes

(partialf)/(partialy)-d/(dx)(partialf)/(partialy_x)=0.

(4)

The Euler-Lagrange differential equation is implemented as EulerEquations[f, u[x], x] in the Wolfram Language package VariationalMethods` .

In many physical problems, f_x (the partial derivative of f with respect to x) turns out to be 0, in which case a manipulation of the Euler-Lagrange differential equation reduces to the greatly simplified and partially integrated form known as the Beltrami identity,

f-y_x(partialf)/(partialy_x)=C.

(5)

For three independent variables (Arfken 1985, pp. 924-944), the equation generalizes to

(partialf)/(partialu)-partial/(partialx)(partialf)/(partialu_x)-partial/(partialy)(partialf)/(partialu_y)-partial/(partialz)(partialf)/(partialu_z)=0.

(6)

Problems in the calculus of variations often can be solved by solution of the appropriate Euler-Lagrange equation.

To derive the Euler-Lagrange differential equation, examine

since deltaq^.=d(deltaq)/dt. Now, integrate the second term by parts using

so

int(partialL)/(partialq^.)(d(deltaq))/(dt)dt=int(partialL)/(partialq^.)d(deltaq)=[(partialL)/(partialq^.)deltaq]_(t_1)^(t_2)-int_(t_1)^(t_2)(d/(dt)(partialL)/(partialq^.)dt)deltaq.

(13)

Combining (◇) and (◇) then gives

deltaJ=[(partialL)/(partialq^.)deltaq]_(t_1)^(t_2)+int_(t_1)^(t_2)((partialL)/(partialq)-d/(dt)(partialL)/(partialq^.))deltaqdt.

(14)

But we are varying the path only, not the endpoints, so deltaq(t_1)=deltaq(t_2)=0 and (14) becomes

deltaJ=int_(t_1)^(t_2)((partialL)/(partialq)-d/(dt)(partialL)/(partialq^.))deltaqdt.

(15)

We are finding the stationary values such that deltaJ=0. These must vanish for any small change deltaq, which gives from (15),

(partialL)/(partialq)-d/(dt)((partialL)/(partialq^.))=0.

(16)

This is the Euler-Lagrange differential equation.

The variation in J can also be written in terms of the parameter kappa as

where

and the first, second, etc., variations are

The second variation can be re-expressed using

d/(dt)(v^2lambda)=v^2lambda^.+2vv^.lambda,

(25)

so

I_2+[v^2lambda]_2^1=int_1^2[v^2(f_(yy)+lambda^.)+2vv^.(f_(yy^.)+lambda)+v^.^2f_(y^.y^.)]dt.

(26)

But

[v^2lambda]_2^1=0.

(27)

Now choose lambda such that

f_(y^.y^.)(f_(yy)+lambda^.)=(f_(yy^.)+lambda)^2

(28)

and z such that

f_(yy^.)+lambda=-(f_(yy^.))/z(dz)/(dt)

(29)

so that z satisfies

f_(y^.y^.)z^..+f^._(y^.y^.)z^.-(f_(yy)-f^._(yy^.))z=0.

(30)

It then follows that


See also

Beltrami Identity, Brachistochrone Problem, Calculus of Variations, Euler-Lagrange Derivative, Functional Derivative, Variation

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References

Arfken, G. Mathematical Methods for Physicists, 3rd ed. Orlando, FL: Academic Press, 1985.Forsyth, A. R. Calculus of Variations. New York: Dover, pp. 17-20 and 29, 1960.Goldstein, H. Classical Mechanics, 2nd ed. Reading, MA: Addison-Wesley, p. 44, 1980.Lanczos, C. The Variational Principles of Mechanics, 4th ed. New York: Dover, pp. 53 and 61, 1986.Morse, P. M. and Feshbach, H. "The Variational Integral and the Euler Equations." §3.1 in Methods of Theoretical Physics, Part I. New York: McGraw-Hill, pp. 276-280, 1953.

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Euler-Lagrange Differential Equation

Cite this as:

Weisstein, Eric W. "Euler-Lagrange Differential Equation." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/Euler-LagrangeDifferentialEquation.html

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