Lagrangian on a saddle advice?

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To derive a Lagrangian for a particle on a rotating saddle surface defined by z = x^2 - y^2, one should start with the kinetic term in three-dimensional space and apply a constraint to ensure the particle remains on the saddle. The rotation of the saddle can be incorporated by transforming the coordinates using a rotation matrix that accounts for the angular frequency, w. Specifically, the transformed coordinates, denoted as tilde x and tilde y, involve cosine and sine functions of the angular frequency multiplied by time. Implementing a Lagrange multiplier for the constraint will help in formulating the complete Lagrangian. This approach provides a structured way to model the dynamics of the particle on the rotating saddle.
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Hi,

I am trying to obtain a Lagrangian for a particle moving on the surface of a saddle
z = x^2 - y^2

I have an added complication that the saddle is rotating with some angular frequency, w, and not sure how to incorporate this rotation into my kinetic and potential terms.

This is the kind of thing I am trying to model:
http://www.fas.harvard.edu/~scidemos/OscillationsWaves/SaddleShape/SaddleShape.html
But thought best to assume a particle for now, so don't have to worry about moment of inertia.

Does anyone have any advice on where to begin?

Any help will be much appreciated.

Thanks
 
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The most straightforward way I can think of for such a system is to write down the ordinary kinetic term in R^3, with zero potential term, and then implementing "the particle stays attached to the saddle" as a constraint (i.e., with a Lagrange multiplier). The constraint will look something like

\lambda(t) (z - \tilde x^2 + \tilde y^2)

where

\begin{align*} \tilde x &= \cos (\omega t) \; x - \sin (\omega t) \; y \\ \tilde y &= -\sin (\omega t) \; x + \cos (\omega t) \; y \end{align*}
 
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