generalized coordinate

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Normally the configuration of a system can be described by specifying the positions \mathbf{r}_i\, of all its components on some manifold, which is usually taken to be Cartesian coordinates on the Euclidean space \mathbb{R}^3\,. These coordinates are democratic in that every component is treated on the same footing. On the other hand, the system may have a number of symmetries which may not be evident in the chosen coordinate system, or there may exist a number of constraints which introduce dependence among these coordinates. In such cases, we may parameterize the m\, coordinates \mathbf{r}_i\, in terms of n\, variables q_i\, which are termed generalized coordinates:


\begin{matrix}
\mathbf{r}_1=\mathbf{r}_1(q_1, q_2, ..., q_n, t),\\
\mathbf{r}_2=\mathbf{r}_2(q_1, q_2, ..., q_n, t),\\
\vdots\\
\mathbf{r}_m=\mathbf{r}_m(q_1, q_2, ..., q_n, t),
\end{matrix}\,

where we have allowed the coordinate transformation to be time dependent. If the system has k\, degrees of freedom, there exist 3m - k\, constraint equations of the form f_j(\mathbf{r}_i) = 0\,. The technique is most useful when these k\, degrees of freedom are precisely described by n\, generalized coordinates; that is, when n = k\,. One then says that the constraints f_j(\mathbf{r}_i) = 0\, are implicit in the coordinates q_i\,.

Furthermore, the time derivatives of the generalized coordinates q_i\,,

\dot{q}_i = \frac{dq_i}{dt}\,,

are known as generalized velocities.

back to Lagrangian mechanics
on to d'Alembert's principle
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