Mass rotating on ellipse track

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Homework Statement


A body with mass ##m## can move without any friction on ellipse that ##(x/a)^2+(y/b)^2=1## describe. In ##y## direction homogeneous gravity field ##g## is present. For generalized coordinate we take angle ##\alpha ## defined with ##x=acos\alpha ##, ##y=bsin\alpha ##. Find equilibrium position and frequency of oscillation around that position.

Homework Equations


The Attempt at a Solution



##L=T-V##

##T=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)## and ##V=mgsin\alpha ##.

##L=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)-mgsin\alpha ##

##\frac{\partial L}{\partial \alpha }-\frac{\mathrm{d} }{\mathrm{d} t}\frac{\partial L}{\partial \dot{\alpha }}=0=-mgbcos\alpha -2mr\dot{r}\dot{\alpha }-mr^2\ddot{\alpha }=0##

So finally

##\ddot{\alpha }+\frac{2\dot{r}}{r}\dot{\alpha }+\frac{gb}{r^2}cos\alpha =0##.

For equilibrium position:

##cos\alpha =0## so ##\alpha =-\frac{\pi}{2}##

Now for frequency, I am guessing I can write:

##\ddot{\alpha }+\frac{2\dot{r}}{r}\dot{\alpha }+\frac{gb}{r^2}\alpha =0##

But this will be like horrible to calculate, since ##r=\sqrt{a^2cos^2\alpha +b^2sin^2\alpha }##...

Hmmm, is that ok? :/
 
Last edited:
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Your generalized coordinate is not the polar angle, don't mix them.

At some point you'll have to approximate the kinetic and potential energy for small oscillations, otherwise you won't find a meaningful solution.
 
Note that the parameter t (called the eccentric anomaly in astronomy) is not the angle of (X(t),Y(t)) with the X-axis.

You can use the more general form described above that (and simplify it), but then you need a different variable and you don't use the one the problem statement suggested.
 
hmmm...

##\vec{r}=(acos\alpha ,bsin\alpha )## and ##r^2=a^2cos^2\alpha +b^2sin^2\alpha ##

##\dot{\vec{r}}=\dot{\alpha }(-asin\alpha ,bcos\alpha )## and ##\dot{r}^2=\dot{\alpha }^2(a^2sin^2\alpha +b^2cos^2\alpha )##.

Than ##L=T-V=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)-mgbsin\alpha ##

##L=\frac{1}{2}m(\dot{\alpha }^2(a^2sin^2\alpha +b^2cos^2\alpha )+\dot{\alpha }^2(a^2cos^2\alpha +b^2sin^2\alpha ))-mgbsin\alpha ##

which leaves me with ##L=\frac{1}{2}m\dot{\alpha }^2(a^2+b^2)-mgbsin\alpha ##

Now ##\frac{\mathrm{d} }{\mathrm{d} t}\frac{\partial L}{\partial \dot{\alpha }}-\frac{\partial L}{\partial \alpha }=m\ddot{\alpha }(a^2+b^2)+mgcos\alpha=0##

and finally ##\ddot{\alpha }+\frac{gb}{a^2+b^2}cos\alpha=0##.

Which leaves me with equilibrium position at ##\pi/2## and therefore frequency ## \omega ^2=\frac{gb}{a^2+b^2}##

However, this has to be wrong (don't ask me why), but if ##a=b##, than the track would be a simple circle and I would expect frequency something like ##\omega ^2=\frac{g}{R}##... Hmmm?
 
One more question, I would expect that ##T## is independent of cartesian or polar coordinates, but obviously this is not the case:

##T=\frac{1}{2}m(\dot{x}^2+\dot{y}^2)=\frac{1}{2}m\dot{\alpha }^2(a^2sin^2\alpha + b^2cos^2\alpha )## and

##T=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)=\frac{1}{2}m\dot{\alpha }^2(a^2+b^2)##.How is that so?
 
Your second equation is wrong because, as explained, α is NOT the polar coordinate.
 
Last edited:
Aaaaaaaaaaaaaaaaaaaaaaaaa,

Now I can see what the problem is! Aha! HA! Ok! I can't believe it took me so long.

Well than let's forget about polar coordinates and do everything in cartesian.

This brings me to ##\omega ^2=\frac{gb}{a^2}##
 
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