Sorcerer
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What I mean is, if you start with, say, a coordinate of some moving object, (cdt, dx), ignoring the y and z directions, of course, and then divide by proper time, written as ## \frac{dt}{\gamma\ }## , you get (##\gamma \textbf{c}##, ##\gamma\ u_x##), so that second coordinate, the speed times gamma, is what I mean by ##\gamma \textbf{u}## .PeterDonis said:What do you mean by ##\gamma \textbf{u}##?
So, if you multiply by invariant mass it becomes γmu, then if you take the time derivative, and then integrate over distance (after doing some manipulations with the differentials and integrating from 0 to u), you end up with a result that is identical to the relativistic kinetic energy equation.
So that's what I meant by all that. I don't know if it's mere coincidence or not, but it seems interesting to me.