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# Euler–Lagrange equation-(only for study)

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In calculus of variations, the Euler–Lagrange equationEuler's equation, or Lagrange's equation, is a differential equation whose solutions are the functions for which a given functional is stationary. It was developed by Swiss mathematician Leonhard Euler and Italian mathematician Joseph Louis Lagrange in the 1750s.

Because a differentiable functional is stationary at its local maxima and minima, the Euler–Lagrange equation is useful for solving optimization problems in which, given some functional, one seeks the function minimizing (or maximizing) it. This is analogous to Fermat's theorem in calculus, stating that where a differentiable function attains its local extrema, itsderivative is zero.

In Lagrangian mechanics, because of Hamilton's principle of stationary action, the evolution of a physical system is described by the solutions to the Euler–Lagrange equation for theaction of the system. In classical mechanics, it is equivalent to Newton's laws of motion, but it has the advantage that it takes the same form in any system of generalized coordinates, and it is better suited to generalizations.

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## History

The Euler–Lagrange equation was developed in the 1750s by Euler and Lagrange in connection with their studies of the tautochrone problem. This is the problem of determining a curve on which a weighted particle will fall to a fixed point in a fixed amount of time, independent of the starting point.

Lagrange solved this problem in 1755 and sent the solution to Euler. Both further developed Lagrange's method and applied it to mechanics, which led to the formulation of Lagrangian mechanics. Their correspondence ultimately led to the calculus of variations, a term coined by Euler himself in 1766.

## Statement

The Euler–Lagrange equation is an equation satisfied by a function, q, of a real argument, t, which is a stationary point of the functional $displaystyle S(q) = int_a^b L(t,q(t),q'(t)), mathrm{d}t$

where:

• q is the function to be found: begin{align} q colon [a, b] subset mathbb{R} & to X t & mapsto x = q(t) end{align}
such that q is differentiable, q(a) = xa, and q(b) = xb;
• q′ is the derivative of q: begin{align} q' colon [a, b] & to T_{q(t)}X t & mapsto v = q'(t) end{align}
TX being the tangent bundle of X (the space of possible values of derivatives of functions with values in X);
• L is a real-valued function with continuous first partial derivatives: begin{align} L colon [a, b] times X times TX & to mathbb{R} (t, x, v) & mapsto L(t, x, v). end{align}

The Euler–Lagrange equation, then, is given by $L_x(t,q(t),q'(t))-frac{mathrm{d}}{mathrm{d}t}L_v(t,q(t),q'(t)) = 0.$

where Lx and Lv denote the partial derivatives of L with respect to the second and third arguments, respectively.

If the dimension of the space X is greater than 1, this is a system of differential equations, one for each component: $frac{partial L(t,q(t),q'(t))}{partial x_i}-frac{mathrm{d}}{mathrm{d}t}frac{partial L(t,q(t),q'(t))}{partial v_i} = 0 quad text{for } i = 1, dots, n.$

## Examples

A standard example is finding the real-valued function on the interval [ab], such that f(a) = c and f(b) = d, the length of whose graph is as short as possible. The length of the graph of f is: $ell (f) = int_{a}^{b} sqrt{1+(f'(x))^2},mathrm{d}x,$

the integrand function being L(xyy′) = 1 + y′ ² evaluated at (xyy′) = (xf(x), f′(x)).

The partial derivatives of L are: $frac{partial L(x, y, y')}{partial y'} = frac{y'}{sqrt{1 + y'^2}} quad text{and} quad frac{partial L(x, y, y')}{partial y} = 0.$

By substituting these into the Euler–Lagrange equation, we obtain begin{align} frac{mathrm{d}}{mathrm{d}x} frac{f'(x)}{sqrt{1 + (f'(x))^2}} &= 0 frac{f'(x)}{sqrt{1 + (f'(x))^2}} &= C = text{constant} Rightarrow f'(x)&= frac{C}{sqrt{1-C^2}} := A Rightarrow f(x) &= Ax + B end{align}

that is, the function must have constant first derivative, and thus its graph is a straight line.

### Classical mechanics

#### Basic method

To find the equations of motions for a given system, one only has to follow these steps:

• From the kinetic energy $T$, and the potential energy $V$, compute the Lagrangian $L = T - V$.
• Compute $frac{partial L}{partial q}$.
• Compute $frac{partial L}{partial dot{q}}$ and from it, $frac{d}{dt}frac{partial L}{partial dot{q}}$. It is important that $dot{q}$ be treated as a complete variable in its own right, and not as a derivative.
• Equate $frac{partial L}{partial q} = frac{d}{dt}frac{partial L}{partial dot{q}}$. This is the Euler–Lagrange equation.
• Solve the differential equation obtained in the preceding step. At this point, $dot{q}$ is treated "normally". Note that the above might be a system of equations and not simply one equation.

#### Particle in a conservative force field

The motion of a single particle in a conservative force field (for example, the gravitational force) can be determined by requiring the action to be stationary, by Hamilton's principle. The action for this system is $S = int_{t_0}^{t_1} L(t, mathbf{x}(t), mathbf{dot{x}}(t)),mathrm{d}t$

where x(t) is the position of the particle at time t. The dot above is Newton's notation for the time derivative: thus (t) is the particle velocity, v(t). In the equation above, L is theLagrangian (the kinetic energy minus the potential energy): $L(t, mathbf{x}, mathbf{v}) = frac{1}{2}m sum_{i=1} ^{3} v_i^2 - U(mathbf{x}),$

where:

• m is the mass of the particle (assumed to be constant in classical physics);
• vi is the i-th component of the vector v in a Cartesian coordinate system (the same notation will be used for other vectors);
• U is the potential of the conservative force.

In this case, the Lagrangian does not vary with its first argument t. (By Noether's theorem, such symmetries of the system correspond to conservation laws. In particular, the invariance of the Lagrangian with respect to time implies the conservation of energy.)

By partial differentiation of the above Lagrangian, we find: $frac{partial L(t,mathbf{x},mathbf{v})}{partial x_i} = -frac{partial U(mathbf{x})}{partial x_i} = F_i (mathbf{x})quad text{and} quad frac{partial L(t,mathbf{x},mathbf{v})}{partial v_i} = m v_i = p_i,$

where the force is F = −U (the negative gradient of the potential, by definition of conservative force), and p is the momentum. By substituting these into the Euler–Lagrange equation, we obtain a system of second-order differential equations for the coordinates on the particle's trajectory, $F_i(mathbf{x}(t)) = frac{mathrm d}{mathrm{d}t} m dot{x}_i(t) = m ddot{x}_i(t),$

which can be solved on the interval [t0t1], given the boundary values xi(t0) and xi(t1). In vector notation, this system reads $mathbf{F}(mathbf{x}(t)) = mmathbf{ddot x}(t)$

or, using the momentum, $mathbf{F} = frac {mathrm{d}mathbf{p}} {mathrm{d}t}$

which is Newton's second law.

## Variations for several functions, several variables, and higher derivatives

### Single function of single variable with higher derivatives

The stationary values of the functional $I[f] = int_{x_0}^{x_1} mathcal{L}(x, f, f', f'', dots, f^{(n)})~mathrm{d}x ~;~~ f' := cfrac{mathrm{d}f}{mathrm{d}x}, ~f'' := cfrac{mathrm{d}^2f}{mathrm{d}x^2}, ~ f^{(n)} := cfrac{mathrm{d}^nf}{mathrm{d}x^n}$

can be obtained from the Euler–Lagrange equation $cfrac{partial mathcal{L}}{partial f} - cfrac{mathrm{d}}{mathrm{d} x}left(cfrac{partial mathcal{L}}{partial f'}right) + cfrac{mathrm{d}^2}{mathrm{d} x^2}left(cfrac{partial mathcal{L}}{partial f''}right) - dots + (-1)^n cfrac{mathrm{d}^n}{mathrm{d} x^n}left(cfrac{partial mathcal{L}}{partial f^{(n)}}right) = 0$

under fixed boundary conditions for the function itself as well as for the first $n-1$ derivatives (i.e. for all $f^{(i)}, i in {0, ..., n-1}$). The endpoint values of the highest derivative $f^{(n)}$ remain flexible.

### Several functions of one variable

If the problem involves finding several functions ( $f_1, f_2, dots, f_n$) of a single independent variable ( $x$) that define an extremum of the functional $I[f_1,f_2, dots, f_n] = int_{x_0}^{x_1} mathcal{L}(x, f_1, f_2, dots, f_n, f_1', f_2', dots, f_n')~mathrm{d}x ~;~~ f_i' := cfrac{mathrm{d}f_i}{mathrm{d}x}$

then the corresponding Euler–Lagrange equations are begin{align} cfrac{partial mathcal{L}}{partial f_i} - cfrac{d}{dx}left(cfrac{partial mathcal{L}}{partial f_i'}right) = 0 end{align}

### Single function of several variables

A multi-dimensional generalization comes from considering a function on n variables. If Ω is some surface, then $I[f] = int_{Omega} mathcal{L}(x_1, dots , x_n, f, f_{x_1}, dots , f_{x_n}), mathrm{d}mathbf{x},! ~;~~ f_{x_i} := cfrac{partial f}{partial x_i}$

is extremized only if f satisfies the partial differential equation $frac{partial mathcal{L}}{partial f} - sum_{i=1}^{n} frac{partial}{partial x_i} frac{partial mathcal{L}}{partial f_{x_i}} = 0. ,!$

When n = 2 and $mathcal{L}$ is the energy functional, this leads to the soap-film minimal surface problem.

### Several functions of several variables

If there are several unknown functions to be determined and several variables such that $I[f_1,f_2,dots,f_m] = int_{Omega} mathcal{L}(x_1, dots , x_n, f_1, dots, f_m, f_{1,1}, dots , f_{1,n}, dots, f_{m,1}, dots, f_{m,n}) , mathrm{d}mathbf{x},! ~;~~ f_{j,i} := cfrac{partial f_j}{partial x_i}$

the system of Euler–Lagrange equations is begin{align} frac{partial mathcal{L}}{partial f_1} - sum_{i=1}^{n} frac{partial}{partial x_i} frac{partial mathcal{L}}{partial f_{1,i}} & = 0 frac{partial mathcal{L}}{partial f_2} - sum_{i=1}^{n} frac{partial}{partial x_i} frac{partial mathcal{L}}{partial f_{2,i}} & = 0 dots quad dots qquad dots & frac{partial mathcal{L}}{partial f_m} - sum_{i=1}^{n} frac{partial}{partial x_i} frac{partial mathcal{L}}{partial f_{m,i}} & = 0. end{align}

### Single function of two variables with higher derivatives

If there is a single unknown function f to be determined that is dependent on two variables x1 and x2 and if the functional depends on higher derivatives of f up to n-th order such that begin{align} I[f] & = int_{Omega} mathcal{L}(x_1, x_2, f, f_{,1}, f_{,2}, f_{,11}, f_{,12}, f_{,22}, dots, f_{,22dots 2}), mathrm{d}mathbf{x} & qquad quad f_{,i} := cfrac{partial f}{partial x_i} ; , quad f_{,ij} := cfrac{partial^2 f}{partial x_ipartial x_j} ; , ;; dots end{align}

then the Euler–Lagrange equation is begin{align} frac{partial mathcal{L}}{partial f} & - frac{partial}{partial x_1}left(frac{partial mathcal{L}}{partial f_{,1}}right) - frac{partial}{partial x_2}left(frac{partial mathcal{L}}{partial f_{,2}}right) + frac{partial^2}{partial x_1^2}left(frac{partial mathcal{L}}{partial f_{,11}}right) + frac{partial^2}{partial x_1partial x_2}left(frac{partial mathcal{L}}{partial f_{,12}}right) + frac{partial^2}{partial x_2^2}left(frac{partial mathcal{L}}{partial f_{,22}}right) & - dots + (-1)^n frac{partial^n}{partial x_2^n}left(frac{partial mathcal{L}}{partial f_{,22dots 2}}right) = 0 end{align}

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