The General Theory of Relativity of Einstein

Derivations, Applications and Considerations – by Albert Prins

Appendix 12 — Derivation of the Euler–Lagrange Equation

Appendix 12.1 — Definition of the Functional

We begin with a function \( f_{1} \) that depends on three variables: \(t\), \(x_{1}(t)\) and \( \dot{x}_{1}(t) = \frac{dx_{1}}{dt} \):

\begin{equation} f_{1} = f\!\left(t,\, x_{1}(t),\, \dot{x}_{1}(t)\right). \end{equation}

Here \(x_{1}(t)\) is a function of \(t\), so \(\dot{x}_{1}(t)\) is not zero. In fact, \(t\) is the only independent variable; \(f_{1}\) is therefore a function of a function.

We now consider the functional:

\begin{equation} I_{1} = \int_{t_{1}}^{t_{2}} f\!\left(t,\, x_{1}(t),\, \dot{x}_{1}(t)\right)\, dt. \end{equation}

We seek the extremal value (minimum, maximum, or saddle point) of \(I_{1}\). For this, it must hold that:

\begin{equation} \delta I_{1} = 0. \end{equation}

Appendix 12.2 — Variation of the Path

To prove that \(I_{1}\) is an extremum, we consider a slightly shifted curve:

\begin{equation} x_{2}(t,\lambda) = x_{1}(t) + \lambda\, \xi(t), \end{equation}

where:

  • \(\lambda\) is a small parameter, independent of \(t\),
  • \(\xi(t)\) is an arbitrary but smooth function.

Because the variation must not change the endpoints, it follows that:

\begin{equation} \xi(t_{1}) = 0, \qquad \xi(t_{2}) = 0. \end{equation}

The function \(x_{2}(t,\lambda)\) therefore differs only between \(t_{1}\) and \(t_{2}\), but coincides with \(x_{1}(t)\) at the endpoints.

Appendix 12.3 — Variation of the Functional

vector_12_1

The integral \(I_{2}\) for the neighboring curve is:

\begin{equation} I_{2} = \int_{t_{1}}^{t_{2}} f_{2}\, dt. \end{equation}

With:

\begin{equation} f_{2} = f\!\left(t,\; x_{2}(t,\lambda),\; \frac{d{x}_{2}(t,\lambda)}{dt}\right). \end{equation}

By substituting (6) into equation (4), we obtain:

\begin{equation} I_2=\int_{t_1}^{t_2} f\!\left(t,\; x_{2}(t,\lambda),\; \frac{d{x}_{2}(t,\lambda)}{dt}\right)dt. \end{equation}
\begin{equation} =\int_{t_1}^{t_2} f\!\left(t,\; x_{1}(t)+\lambda\xi(t)),\; \frac{d\left({x}_{1}(t)+\lambda\xi(t)\right)}{dt}\right)dt. \end{equation}
\begin{equation} I_2=\int_{t_1}^{t_2} f\!\left(t,\; x_{1}(t)+\lambda\xi(t)),\; \frac{d{x}_{1}(t)}{dt}+\frac{d\lambda\xi(t)}{dt}\right)dt \end{equation}

Because \(I_{1}\) is an extremal value, \(I_{2}\) must also be extremal for \(\lambda = 0\):

\begin{equation} \lim_{\lambda \to 0} I_{2} = \text{minimum, maximum or saddle point}. \end{equation}

The extremal value is found by taking the derivative with respect to \(\lambda\) and setting it equal to zero:

\begin{equation} \lim_{\lambda \to 0} \frac{d I_{2}}{d\lambda} = 0. \end{equation}

In combination with equation (6):

\begin{equation} \lim_{\lambda \to 0} \frac{d}{d\lambda} \int_{t_{1}}^{t_{2}} f_{2}\, dt = 0, \end{equation}

or:

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \frac{d f_{2}}{d\lambda}\, dt = 0. \end{equation}

Appendix 12.4 — Differentiation with respect to the variation parameter

We had:

\begin{equation} \lim_{\lambda \to 0} \frac{d}{d\lambda} \int_{t_{1}}^{t_{2}}\left( f_{2}\, dt\right) = 0. \end{equation}
Since this is a product of two functions, we apply the rule of partial differentiation:

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{d f_{2}}{d\lambda}\, dt + f_{2}\, \frac{d}{d\lambda}(dt) \right) = 0. \end{equation}

Since \(t\) and \(\lambda\) are independent, we have:

\begin{equation} \frac{d t}{d\lambda} = 0, \end{equation}
so the second term vanishes:

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \frac{d f_{2}}{d\lambda}\, dt = 0 \end{equation}

Appendix 12.5 — Expansion of \( \frac{d f_{2}}{d\lambda} \)

As mentioned earlier, \(f_2\) is a function of three variables:

\begin{equation} f_{2} = f\!\left(t,\; x_{2},\; \dot{x}_{2}\right). \end{equation}

We now apply the chain rule:

\begin{equation} \frac{d f_{2}}{d\lambda} = \frac{\partial f_{2}}{\partial t}\frac{dt}{d\lambda} + \frac{\partial f_{2}}{\partial x_{2}}\frac{dx_{2}}{d\lambda} + \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d\dot{x}_{2}}{d\lambda} \end{equation}
thus:

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{\partial f_{2}}{\partial t}\frac{dt}{d\lambda} + \frac{\partial f_{2}}{\partial x_{2}}\frac{dx_{2}}{d\lambda} + \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d\dot{x}_{2}}{d\lambda} \right)\, dt = 0 \end{equation}

Since \(t\) and \(\lambda\) are independent, the first term is zero:

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{\partial f_{2}}{\partial t}\cdot 0 + \frac{\partial f_{2}}{\partial x_{2}}\frac{dx_{2}}{d\lambda} + \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d\dot{x}_{2}}{d\lambda} \right)\, dt = 0 \end{equation}
\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{\partial f_{2}}{\partial x_{2}}\frac{dx_{2}}{d\lambda} + \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d\dot{x}_{2}}{d\lambda} \right)\, dt = 0 \end{equation}

Since:

\begin{equation} \frac{d\dot{x}_{2}}{d\lambda} =\frac{d^2x_2}{dtd\lambda} = \frac{d}{dt}\left(\frac{dx_{2}}{d\lambda}\right) \end{equation}
equation (22), together with (24), leads to:

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{\partial f_{2}}{\partial x_{2}}\frac{dx_{2}}{d\lambda} + \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d}{dt}\left(\frac{dx_{2}}{d\lambda}\right) \right)dt=0 \end{equation}

\begin{equation} \lim_{\lambda \to 0} \left( \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial x_{2}}\frac{dx_{2}}{d\lambda}dt + \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d}{dt}\left(\frac{dx_{2}}{d\lambda}\right)dt \right)=0 \end{equation}

Appendix 12.6 — Integration by Parts

We now integrate the second term by parts:

\begin{equation} \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d}{dt}\left(\frac{dx_{2}}{d\lambda}\right)\, dt = \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial \dot{x}_{2}} d\left(\frac{dx_{2}}{d\lambda}\right) \end{equation}
\begin{equation} = \left[ \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{dx_{2}}{d\lambda} \right]_{t_{1}}^{t_{2}} - \int_{t_{1}}^{t_{2}} \frac{dx_{2}}{d\lambda}\, \frac{d}{dt}\left( \frac{\partial f_{2}}{\partial \dot{x}_{2}} \right) \, dt. \end{equation}

The derivative of \(x_2\) with respect to \(\lambda\) is obtained by differentiating equation (4):

\begin{equation} \frac{dx_2(t,\lambda)}{d\lambda}=\frac{d\left(x_1(t)+\lambda\xi(t)\right)}{d\lambda}=0+\xi(t)=\xi(t) \end{equation}

Since the function \(\xi(t)\) is zero at the boundaries of the integral (see equation (5)), the left part of the right-hand term in equation (27) vanishes:

\begin{equation} \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d}{dt}\left(\frac{dx_{2}}{d\lambda}\right)\, dt = \left[ \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{dx_{2}}{d\lambda} \right]_{t_{1}}^{t_{2}} - \int_{t_{1}}^{t_{2}} \frac{dx_{2}}{d\lambda}\, \frac{d}{dt}\left( \frac{\partial f_{2}}{\partial \dot{x}_{2}} \right) \, dt \end{equation}

This therefore gives:

\begin{equation} \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial \dot{x}_{2}} \frac{d}{dt}\left(\frac{dx_{2}}{d\lambda}\right)\, dt = - \int_{t_{1}}^{t_{2}} \frac{dx_{2}}{d\lambda}\, \frac{d}{dt}\left( \frac{\partial f_{2}}{\partial \dot{x}_{2}} \right) \, dt \end{equation}

This result combined with equation (25) leads to:

\begin{equation} \lim_{\lambda \to 0} \left( \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial x_2}\frac{dx_2}{d\lambda}\, dt + \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial \dot x_2}\, \frac{d\left(\frac{dx_2}{d\lambda}\right)}{dt}dt \right) = 0 \end{equation}

\begin{equation} \lim_{\lambda \to 0} \left( \int_{t_{1}}^{t_{2}} \frac{\partial f_{2}}{\partial x_2}\frac{dx_2}{d\lambda}\, dt - \int_{t_{1}}^{t_{2}} \frac{dx_{2}}{d\lambda}\, \frac{d}{dt}\left( \frac{\partial f_{2}}{\partial \dot{x}_{2}}\right)dt \right) = 0 \end{equation}

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{\partial f_{2}}{\partial x_2}\frac{dx_2}{d\lambda} - \frac{dx_{2}}{d\lambda}\, \frac{d}{dt} \left(\frac{\partial f_{2}}{\partial \dot{x}_{2}}\right)\right)dt = 0 \end{equation}

\begin{equation} \lim_{\lambda \to 0} \int_{t_{1}}^{t_{2}} \left( \frac{\partial f_{2}}{\partial x_2} - \, \frac{d}{dt} \left(\frac{\partial f_{2}}{\partial \dot{x}_{2}}\right)\right)\frac{dx_2}{d\lambda}dt = 0 \end{equation}

To make this integral zero, we require that:

\begin{equation} \lim_{\lambda \to 0} \left( \frac{\partial f_{2}}{\partial x_2} - \, \frac{d}{dt} \left(\frac{\partial f_{2}}{\partial \dot{x}_{2}}\right)\right) = 0 \end{equation}

\begin{equation} \frac{\partial f_{2}}{\partial x_2} - \, \frac{d}{dt} \left(\frac{\partial f_{2}}{\partial \dot{x}_{2}}\right) = 0 \end{equation}

Now \(\lambda\) has completely disappeared and we have obtained a general expression for the condition that a function must satisfy in order for the integral \(I\) to have an extremal value.

We started with equation (1) for our derivation, but we could make this starting point even more general by considering a function such as:

\begin{equation} f_1=f\left(t,x_1(t),\frac{dx_1(t)}{dt}, x_2(t), \frac{dx_2(t)}{dt} \text{..............}x_n(t),\frac{dx_n(t)}{dt} \right) \end{equation}

This would have led to a more general form of equation (37):

\begin{equation} \frac{\partial f}{\partial x_n} - \, \frac{d}{dt} \left(\frac{\partial f}{\partial \dot{x_n}}\right) = 0 \end{equation}

Or in another notation:

\begin{equation} \frac{d}{dt} \left(\frac{\partial f}{\partial \dot{x_n}}\right) = \frac{\partial f}{\partial x_n} \end{equation}
Equation (40) is the Euler–Lagrange equation. It gives the condition that a function must satisfy in order for the integral \(I\) to have an extremal value.

This forms the foundation of the calculus of variations, classical mechanics, field theory, and general relativity.