Consider a bead (mass $m$) on a frictionless hoop (radius $R$) in the presence of gravity. The hoop is spun around an axis parallel to the gravitational acceleration at constant angular speed ($\omega$). This is the typical set up for this problem.
The total energy for this system (using $\phi$ to denote the angle from the bottom of the hoop) is:
$$ E = \frac{p_{\phi}^2}{2mR^2} \color{red}{+} \frac{1}{2} mR^2 \omega^2 \sin^2 \phi + mgR (1- \cos \phi)\tag{1} $$
where
$$p_{\phi} = mR^2\dot{\phi}\tag{2}.$$
The Hamiltonian is:
$$ H = \frac{p_{\phi}^2}{2mR^2} \color{red}{-} \frac{1}{2} mR^2 \omega^2 \sin^2 \phi + mgR (1- \cos \phi).\tag{3} $$
So the difference between the total mechanical energy and the Hamiltonian is:
$$ E-H = mR^2 \omega^2 \sin^2 \phi\tag{4} $$
which is twice the rotational kinetic energy, I think. I'm just trying to get a handle on what this difference means. I wondering about the interpretation for the energy difference between the Hamiltonian and the total mechanical energy for systems where the Hamiltonian is conserved, but it is not equal to the total mechanical energy.