Some notes. I've been playing around a bit with "Classical Mechanics Lite" to get a better understanding of exactly what's happening in terms of conservation laws, symmetries, and the seemingly derivative-like relationship between linear momentum $\mathbf p = m \mathbf v$ and kinetic energy $T = \frac{1}{2} m \dot{\mathbf x} \cdot \dot{\mathbf x}$. The reason I'm calling this "Classical Mechanics Lite" is because I'm working under the following assumptions:
- The coordinates $x_i$ are Cartesian coordinates (not generalized coordinates).
- Since there's no coordinate curviture, I'm not worrying about distinguishing covariant and contravariant indices, as one would do in usual Classical Mechanics.
- Kinetic energy $T$ is strictly a function of the velocity variables $\dot x_i$ (again, because there is no curvature in the coordinates).
- Potential energy $U$ is strictly a function of the position variables $x_i$ (I'm not worrying about complicated potentials like the one for the Lorentz force).
Here's what I've found so far.
- The $i$th component of net force $m\ddot x_i$ can be written in terms of kinetic energy $T= \frac{1}{2} m \dot{\mathbf x} \cdot \dot{\mathbf x}$ in two ways. My sense is that each of these representations yields a conservation law under the proper conditions. $$\displaystyle m\ddot x_i = \frac{d}{dt} \left( \frac{\partial T}{\partial \dot x_i} \right) \label{1}\tag{1}$$ $$\displaystyle m\ddot x_i = \frac{\partial}{\partial \dot x_i} \left( \frac{dT}{dt} \right) \label{2}\tag{2}$$
- Assuming we're only worried about conservative forces, then by definition of potential energy $U$, we have $m \ddot{\mathbf x} = - \mathbf \nabla U$, so $$ m\ddot x_i = -\frac{\partial U}{\partial x_i} \label{3}\tag{3}.$$
- Combining equations $\ref 1$ and $\ref 3$ gives conservation of momentum $p_i = \partial T / \partial \dot x_i$ when $-\partial U / \partial x_i = 0$, as expected. This explains the derivative relationship between momentum and kinetic energy. $$0 = - \frac{\partial U}{\partial x_i} = \frac{d}{dt} \left( \frac{\partial T}{\partial \dot x_i} \right) \Rightarrow \boxed{p_i = \frac{\partial T}{\partial \dot x_i} \text{ is conserved}}$$
- Combining equations $\ref 2$ and $\ref 3$ almost give conservation of energy in general. $$-\frac{\partial U}{\partial x_i} = \frac{\partial}{\partial \dot x_i} \left( \frac{dT}{dt} \right)$$ $$0 = \frac{\partial}{\partial \dot x_i} \left( \frac{dT}{dt} \right) + \frac{\partial U}{\partial x_i}$$ $$0 = \frac{\partial}{\partial \dot x_i} \left( \frac{dT}{dt} \right) + \frac{\partial}{\partial \dot x_i} \left( \frac{\partial U}{\partial x_k} \dot x_k \right)$$ $$0 = \frac{\partial}{\partial \dot x_i} \left( \frac{dT}{dt} \right) + \frac{\partial}{\partial \dot x_i} \left( \frac{dU}{dt} \right)$$ $$0 = \frac{\partial}{\partial \dot x_i} \left[ \frac{d}{dt} (T+U) \right] \label{4}\tag{4}$$ $$\text{(this is where I get stuck)}$$
My question. Beyond equation $\ref 4$, I'm expecting to find $\frac{d}{dt} (T+U) = 0$, which would imply that $T+U$ is conserved. However, this cannot be directly deduced, even if taken to be true for all $i$s, since it could be possible to find a function $f$ such that $$\frac{d}{dt}(T+U) = f(x,\ddot x,\dddot x, \ldots),$$ where $x$ represnts all of the $x_i$s, $\ddot x$ represents all of the $\ddot x_i$s, etc, and still have the relationship in equation $\ref 4$ satisfied. What additional assumption (ideally rooted in some sort of physical principle or intuition) would need to be taken in order to deduce conservation of energy $T+U$? I feel like just plainly assuming that $f = 0$ is too big of a jump, and isn't based in any sort of physical principle or intuition.