Lagrangian

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Building on d'Alembert's principle, Newton's second law can be recast in terms of generalized coordinates q_i\, in the form of the Euler-Lagrange equations

\frac{d}{dt} \left( \frac{\partial L}{\partial \dot{q}_i} \right) - \frac{\partial L}{\partial q_i} = Q_i^{(nc)}\,,

where L(q_1, ..., q_n, \dot{q}_1, ..., \dot{q}_n, t)\, is the Lagrangian, which is sometimes called Lagrange's function, and is given by the difference in the kinetic and potential energies:

L(q_i, \dot{q}_i, t) = T(q_i, \dot{q}_i, t) - V(q_i,\dot{q}_i, t)\,,

and where Q_i^{(nc)}\, represent the non-conservative forces, or forces that have otherwise not been included in constructing the potential V\,. In terms of conventional coordinates, T\, is given by

T = \sum_i \frac{1}{2}m_i v_i^2\,,

while, for a conservative system, the potential function V\, is defined through

\mathbf{F}_i = - \boldsymbol{\nabla}_i V\,.
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