Ok, let's do the calculation for an idealized model: A bead is gliding along a rigid rod, which is rotating at constant angular speed. Let ##(r,\varphi)## be the usual polar coordinates. Then the position vector of the bead is
$$\vec{r}=\begin{pmatrix} r \cos(\omega t) \\ r \sin(\omega t) \end{pmatrix}.$$
The velocity is
$$\dot{\vec{r}} = \dot{r} \begin{pmatrix} \cos(\omega t) \\ \sin(\omega t) \end{pmatrix} + \omega r \begin{pmatrix} -\sin(\omega t) \\ \cos(\omega t) \end{pmatrix}.$$
Lagrangian is
$$L=T=\frac{m}{2} \dot{\vec{r}}^2 = \frac{m}{2} (\dot{r}^2 + \omega^2 r^2).$$
The equation of motion is given by the Euler-Lagrange equation,
$$\frac{\mathrm{d}}{\mathrm{d} t} \frac{\partial L}{\partial \dot{r}}=\frac{\partial L}{\partial r},$$
i.e.,
$$m \ddot{r} = m \omega^2 r \; \Rightarrow \; r(t)=A \cosh(\omega t) + B \sinh(\omega t),$$
i.e., the bead is flying radially out.
Of course, the equation of motion, here derived entirely in the inertial frame, can be reinterpreted as the equation of motion from the point of view of the non-inertial frame, co-rotating with the rod, leading to the centri-fugal force on the right-hand side.