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THE GEOMETRY OF CENTRAL FORCES

Section 11.1 Equations of Motion: Harmonic Oscillator

Using conservation of energy, let’s explore the motion of a classical harmonic oscillator.
The statement of energy conservation:
\begin{equation} E = T + U\tag{11.1.1} \end{equation}
becomes
\begin{equation} E = \frac12 m \dot{x}^2 + \frac12 (x-x_0)^2\tag{11.1.2} \end{equation}
(11.1.2) can be solved for \(\dot{x}\) to give:
\begin{equation} \dot{x} = \pm\sqrt{\frac{2}{m}\bigl(E-\frac12 (x-x_0)^2\bigr)}\tag{11.1.3} \end{equation}

Activity 6.

Explore how the kinetic energy \(\frac12 m \dot{x}^2\) of a harmonic oscillator is affected by the shape of the potential (shown in blue) (which depends on the parameters \(k\) and \(x_0\)) and the value of the total energy (shown in green).
Figure 13. The potential for the classical harmonic oscillator is shown in blue. For a given potential, the total energy \(E\text{,}\) shown in green will determine the resulting motion.