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PhysStudent81
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Homework Statement
I have two masses of finite width, m_1 and m_2. The force is Newton's gravity, so U = k/r. I want to work out their relevant equations of motions r_1(t) and r_2(t) as they start off from rest and collide. I don't want to consider any rotational motion.
Homework Equations
[itex]U = \frac{k}{r}[/itex]
[itex]r = r_{1}(t) - r_{2}(t)[/itex]
0.5μ[itex]\dot{r}^2 = E_{tot} - \frac{k}{r}[/itex]
dt = [itex]\frac{μ}{2}[/itex]∫[itex]\frac{dr}{\sqrt{E_{tot} - \frac{k}{r}}}[/itex]
The Attempt at a Solution
I try to integrate the above equation it gives me something very complicated (I end up integrating cosec^3 after making the substitution [itex] \frac{1}{r} = \sin^{2}(\theta) [/itex]) which gives me t = t(r), but I can't invert this to give me r = r(t).
Am I doing something wrong? Is there another way of doing it that doesn't involve lagrangian or hamiltonian dynamics (which I haven't studied).
Another way would be to solve the the 2nd order differential equation directly:
[itex]\frac{dr^{2}}{dt^{2}} = \frac{k}{r^{2}}[/itex]
but I can't seem to do this (I fee I'm missing something very simple here). I know that if I let [itex] r = At^{\frac{2}{3}}[/itex] this is a solution but it doesn't have enough constants.
Any pointers?
Thanks,
Rob