We start with a following 'force' equation that we saw earlier.
$\mathbf{p}''=\alpha p_0 \mathbf{k}\times\widehat{\mathbf{p}}'$
Taking a dot product on both sides with $\mathbf{p}'$, we have
$\mathbf{p}'\cdot\mathbf{p}''=\alpha p_0 \mathbf{p}'\cdot(\mathbf{k}\times\widehat{\mathbf{p}}')$
Permuting the RHS and integrating the above, we see that
$\displaystyle \frac{1}{2}\left\vert{\mathbf{p}'}\right\vert^2+\alpha p_0 \int\mathbf{k}\cdot(\mathbf{p}'\times\widehat{\mathbf{p}}')\,dt=\text{const.}$
For any vector $\mathbf{q}$, with straightforward differentiation, we can show that
$\displaystyle \mathbf{q}'\times\widehat{\mathbf{q}}'=\frac{\mathbf{q}\cdot\mathbf{q}'}{\left\vert\mathbf{q}\right\vert^3}(\mathbf{q}\times\mathbf{q}')$
Using this result, the constant vector $\mathbf{m}$ from our earlier post and the fact that $\mathbf{p}\cdot\mathbf{k}=\sqrt{\delta/\alpha}$, we see that
$\displaystyle \mathbf{k}\cdot(\mathbf{p}'\times\widehat{\mathbf{p}}')=\frac{\mathbf{p}\cdot\mathbf{p}'}{p^3}\left(\mathbf{k}\cdot\mathbf{m}-\frac{\delta p_0}{p}\right)$
where $p=\left\vert\mathbf{p}\right\vert$.
Let $u=1/p$. It is easy to see that $u'=-(\mathbf{p}\cdot\mathbf{p}')/p^3$. This makes it almost trivial to integrate the above expression.
With the above, our 'energy' equation becomes
$\displaystyle E=\frac{1}{2}\left\vert{\mathbf{p}'}\right\vert^2-\alpha (\mathbf{k}\cdot\mathbf{m}) \frac{p_0}{p}+\frac{\delta\alpha}{2}\frac{p_0^2}{p^2}$
Now comes the interesting part. If we interpret the first term of the RHS as a measure of kinetic energy, the remaining terms gives us the 'effective potential' energy of the system. That is,
$\displaystyle V_{\text{eff}}(p)=-\alpha (\mathbf{k}\cdot\mathbf{m}) \frac{p_0}{p}+\frac{\delta\alpha}{2}\frac{p_0^2}{p^2}$
But that is exactly in the same form as that of the effective potential of the radial equation of an inverse square central force (Central forces). Therefore, the problem of a sphere on a freely spinning turntable is a Kepler problem in disguise which helps us in utilizing many known results.
For example, it known that the orbital period of a kepler problem can be written in terms of the 'energy' and the coefficient of the '$1/r$' term in the effective potential. Using the same, we can see that the orbital period $T$ for our problem is given by
$$\displaystyle T=\frac{2\pi\text{ }\alpha\text{ }p_0\text{ }(\mathbf{k}\cdot\mathbf{m})}{\left\vert2E\right\vert^{3/2}}$$
Hope you enjoyed the discussion. See ya later.
Until then
Yours Aye
Me
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