Open cmp0xff opened 7 months ago
We have a few options to specify the system:
If we focus on closed systems with exact solutions, I suggest we focus on 2 and 3, making 1 optional.
These are the King in numeric simulations. For exact solutions, however, they are often not the best specifications. For examples, in Kepler problem, we are likely to be forced to convert initial conditions to the energy and angular momentum, before we can proceed.
By definition, all exactly solvable conserved systems have integrals of motion. These quantities have special importance in analytical mechanics.
Typical examples include
Good examples include
Currently we provide users intermediate variables which are used for analytical or numerical purposes. Maybe we should remove them.
In the Lagrangian action of an undamped simple harmonic oscillator (#34), one can easily find the first integral $$\frac{1}{2} m \dot x^2 + \frac{1}{2} m \omega^2 x^2 \equiv E \eqqcolon \frac{1}{2} m \omega^2 x_0^2\,,$$ where $E$ is the integral or motion (constant), having the interpretation of energy, and $x_0$ can be interpreted as the maximal displacement.
Integrating this first-order differential equation directly gives rise to another constant of motion $t_0$, $$t-t_0 = \frac{1}{\omega} \arccos \frac{x}{x_0}\,.$$ In other words, the motion of the system is directly given by the two constant $(x_0, t_0)$, in this framework of Lagrangian mechanics.
I propose we add the initial condition $(x_0, t_0)$, in addition to $(x_0, v_0)$, the latter of which is closer to the second-order differential equation of motion, which is less appealing in analytical mechanics.