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Hamilton's Equations of Motion

These equations describe the time evolution of a system's phase space coordinates, \dot{q} = \frac{\partial H}{\partial p} and \dot{p} = -\frac{\partial H}{\partial q}, where H is the Hamiltonian.
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The statement of the theorem

Let H(q,p,t):R2NRH(q, p, t): \mathbb{R}^{2N} \to \mathbb{R} be the Hamiltonian function, where q=(q1,,qN)q = (q_1, \dots, q_N) and p=(p1,,pN)p = (p_1, \dots, p_N) are the generalized coordinates and momenta, respectively. The time evolution of the system's phase space coordinates (q,p)(\mathbf{q}, \mathbf{p}) is governed by Hamilton's canonical equations:\n\ndqidt=Hpianddpidt=Hqifor i=1,,N\frac{d q_i}{d t} = \frac{\partial H}{\partial p_i} \quad \text{and} \quad \frac{d p_i}{d t} = -\frac{\partial H}{\partial q_i} \quad \text{for } i = 1, \dots, N
Source: Wikipedia