How to Derive Equations of Motion for Colliding Masses in a Central Field?

PhysStudent81
Messages
8
Reaction score
0

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



U = \frac{k}{r}
r = r_{1}(t) - r_{2}(t)

0.5μ\dot{r}^2 = E_{tot} - \frac{k}{r}

dt = \frac{μ}{2}∫\frac{dr}{\sqrt{E_{tot} - \frac{k}{r}}}

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 \frac{1}{r} = \sin^{2}(\theta)) 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:

\frac{dr^{2}}{dt^{2}} = \frac{k}{r^{2}}

but I can't seem to do this (I fee I'm missing something very simple here). I know that if I let r = At^{\frac{2}{3}} this is a solution but it doesn't have enough constants.

Any pointers?

Thanks,

Rob
 
Physics news on Phys.org
PhysStudent81 said:
I try to integrate the above equation it gives me something very complicated (I end up integrating cosec^3 after making the substitution \frac{1}{r} = \sin^{2}(\theta)) which gives me t = t(r), but I can't invert this to give me r = r(t).

Am I doing something wrong?

I think what you are doing is correct. Did you allow for the fact that both k and Etot are negative numbers? Anyway, as you say, you can get an expression for t(r). I agree that the result looks too complicated to invert for r(t).
 
So strange that for such seemingly simple problem there is no closed form result for r(t). t(r) is actually all I wanted so that's ok!
 
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
The value of H equals ## 10^{3}## in natural units, According to : https://en.wikipedia.org/wiki/Natural_units, ## t \sim 10^{-21} sec = 10^{21} Hz ##, and since ## \text{GeV} \sim 10^{24} \text{Hz } ##, ## GeV \sim 10^{24} \times 10^{-21} = 10^3 ## in natural units. So is this conversion correct? Also in the above formula, can I convert H to that natural units , since it’s a constant, while keeping k in Hz ?
Back
Top