Particle in an Orbit: Central Force Motion and Radial Equation

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The discussion focuses on the motion of a particle under a central force defined by $$\underline{F(r)} = -mk\left[\frac{3}{r^2} - 2\frac{a}{r^3}\right] \hat{r}$$. The radial equation of motion is derived as $$\ddot{r} - \frac{9}{4} \frac{ka}{r^3} = -\frac{3k}{r^2}$$, which simplifies to a linear form $$u''(\theta) + 9u(\theta) = 12/a$$ by substituting $$u(\theta) = 1/r(t)$$. The solution yields the orbit equation $$r = \frac{3a}{4 - \cos(3 \theta)}$$, indicating a bounded trajectory with specific minima and maxima at defined angles.

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  • #31
Since r is periodic w.r.t. the angle, the orbit has to be closed. But it is not repeated every 120 degrees. It is repeated every 360 degrees.
 
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  • #32
voko said:
Since r is periodic w.r.t. the angle, the orbit has to be closed. But it is not repeated every 120 degrees. It is repeated every 360 degrees.

Maybe I misused the word 'repeated' and I see what you mean. This is the last part of this question:

The angle between successive maxima and minima is called the apsidal angle. Derive an expression for ##dr/d\theta = \dot{r}/\dot{\theta}## by extracting ##\dot{r}## from the expression for the energy and using ##\dot{\theta} = h/r^2##. Use this expression to determine the apsidal angle and compare with your result previously.

The energy is conserved so I was given that ##E = T + U,\,U = mk[\frac{9}{8} a/r^2 - 3/r]##. T = 0 initially (since ##\dot{r} ##= 0) and so E = U = -15mk/8a, with the condition r(0) = a.

My problem is that when I rearrange for ##\dot{r}##, it appears I will have a negative under the square root. I believe what I am rearranging is the following: $$-\frac{15}{8} mk/a = \frac{m}{2}\dot{r}^2 + mk[\frac{9}{8}\frac{a}{r^2} - \frac{3}{r}]$$ Rearranging gives $$\dot{r} = \sqrt{-\frac{15}{8} mk/a - 3mk/r - 9mka/8r^2}$$ which is a negative under the square root.

EDIT: The potential U was given to us in the question as ##mk [\frac{9}{8} a/r^2 - 3/r]##
 
  • #33
Without analyzing it further, there is clearly a sign error in the 1/r term after rearranging.
 
  • #34
voko said:
Without analyzing it further, there is clearly a sign error in the 1/r term after rearranging.

I get the apsidal angle to be ##\theta = \frac{2 \pi}{3}##. This agrees with the difference between the maxima and minima earlier. Just one more question: what exactly does the question mean by the geometrical significance of the max and min r? I would say that the particle can never go below 3a/5 and never beyond a, but this seems to be more of a physical significance rather than the geometry.
 
  • #36
  • #37
The only geometrical statement that I could make would involve the other two trajectories, but I am not sure if this is what is needed (since they don't mention the other two orbits in the question)
 
  • #38
Perhaps you could compare that to an elliptical orbit.
 
  • #39
voko said:
Perhaps you could compare that to an elliptical orbit.

So maybe that the particle on the elliptical orbit has the same r(min) and r(max)
 
  • #40
The apsidal angle is defined as the angle between successive minima and maxima so the answer was pi/3. We just defined the apsidal angle properly today in lectures and the method used to obtain the apsidal angle was an integral. I understand this method. The way I found the angle (which I did before seeing the integral method) was as follows:

Since we have a functional form for r, I just subbed it into the resulting energy equation. I then solved for r'(θ) =0. This gave me the n2π/3. Since we know this corresponds to maxima as shown earlier, and since we know there is a change in concavity between two maxima, then this must correspond to a minima (as my sketch of the orbit showed). Hence to get the apsidal angle I would then divide by 2 to get nπ/3. Want the difference between successive max/min so I take the angle to be π/3.

Is this okay? (Very recently, I have become aware that some of the TAs at my university mark like computers and I think the method they will mark against will be via the integral). So if you think it is okay, I will argue will them. Obviously, I am aware that my method is not the most general, but I did what I did before going over the integral method.

Many thanks.
 
  • #41
There is nothing wrong with your method. You found an explicit expression for minima and maxima, and that is enough to find the apsidal angle. If there was not a specific requirement to use a particular method to solve the problem, you should be fine. After all, this is physics, and there is usually more than one way to solve a problem.
 
  • #42
Thanks voko.
 

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