Classical Limit and Angular frequency

keniwas
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Homework Statement


Show that in classical mechanics, for circular motion, in an arbitrary central potential
V (r), one has w = dE/dL where E is the energy, L is the angular momentum, and w is the
angular frequency of motion around the orbit.

This is the basis for a problem on understanding the correspondence between classical and quantum mechanis in the limit of large circular orbits (i.e. akin to Bohr's atom).

Homework Equations


Total Energy of the system in Circular Motion
E=\frac{1}{2}m(\dot{r}^2+\frac{L^2}{mr^2})+V(\vec{r})
Where
L=r^2\omega m


The Attempt at a Solution


Once I got the energy in terms of angular momentum, I simply took the derivative with respect to L, however this leaves me with the angular velocity \omega and an additional term from the potential (which I can't find any argument as to why it should be zero in this case...)
dE/dL = 0+\frac{L}{mr^2}+\frac{dV}{dL}=\omega+\frac{dV}{dL}

I am clearly missing somthing important in the problem... is my form for the total energy of the system wrong? or is there somthing special about the central potential I am missing?
Any input is greatly appreciated.
 
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I think, simply, as its a circular motion, the r has to be constant making the potential constant. Which makes the derivative zero.

PS--Be a bit more clear in your problem, as I think the \dot{r}^2 is different from the other "r" in the system (though it wouldn't matter for the problem). are you considering a point mass?
 
It would be a point mass (or as close as you can get to one as an electron). The \dot{r}^2 would be the velocity in the radial direction (i.e. a change in the radius of your circular orbit).

I thought something similar to the logic regarding a fixed circular orbit, however if I change my angular momentum will that not nessecarily correspond to a change in the potential of the system? Since a change in angular momentum would change the effective radius?
 
For a circular orbit, the radius must be constant, so \dot{r}=0.

Your potential is given in the functional form V=V(r) suggesting it depends only only the radius, which is constant for a circular orbit

\frac{\partial V}{\partial L}=\frac{\partial r}{\partial L}\frac{\partial V}{\partial r}=(0)\frac{\partial V}{\partial r}
 
Thank you for the help!
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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