The system shown consists of a rigid rod, a flywheel of radius \(R\) and mass \(m\), and an elastic belt of stiffness \(k\). Determine the natural frequency of the system. The belt is unstretched when \(\theta=0\).

Short Answer

Expert verified
Answer: The natural frequency of the system, denoted as \(\omega_n\), is given by \(\omega_n = \sqrt{\frac{2k}{m}}\), where \(k\) is the spring constant of the elastic belt and \(m\) is the mass of the flywheel.

Step by step solution

01

1. Analyze the Forces and Moments Acting on the System

First, we need to identify the forces acting on the flywheel and the belt: a gravitational force is acting on the flywheel, and an elastic force is acting on the belt. These forces will create a torque (moment) whose axis is through the center of the flywheel.
02

2. Define a force balance equation for the torque acting on the flywheel

We write the torque balance equation considering the gravitational and elastic forces: \(T_G = I \alpha \) Where: - \(T_G\) is the torque due to gravitational and elastic forces, - \(I\) is the moment of inertia of the flywheel: \(I = \frac{1}{2} m R^2\) - \(\alpha\) is the angular acceleration of the flywheel. For the gravity force, the torque is given by \(T_g = m R sin(\theta)\) while for the elastic force, we have \(T_e = k R (R\theta)\). Therefore, the total torque is \(T_G = m R \sin(\theta) - k R^2 \theta\).
03

3. Set up the torque balance equation and find the equation of motion

Replacing the total torque and the moment of inertia in the torque balance equation, we get: \(m R \sin(\theta) - k R^2 \theta = \frac{1}{2} m R^2 \alpha\) We can simplify this equation by dividing both sides by \(\frac{1}{2} m R^2\), resulting in: \(2 \sin(\theta) - 2kR \theta = \alpha\) Now, we can linearize this equation by assuming small angle \(\theta\) so that \(\sin(\theta) \approx \theta\): \(2 \theta - 2kR \theta = \alpha\)
04

4. Convert the equation of motion into a standard form

In order to find the natural frequency of the system, we will convert the equation of motion into a standard form: \(m\ddot{x} + kx = 0\) To do this, we will assume a one-to-one relationship between the displacement \(x\) and the angle \(\theta\): \(R\theta = x\) Which means: \(\alpha = \frac{d^2x}{dt^2}\) Replacing this into the linearized equation of motion, we get: \(2 \frac{x}{R} - 2kR \frac{x}{R} = \frac{d^2x}{dt^2}\) Simplifying the equation and rearranging, we get the standard form: \(m\frac{d^2x}{dt^2} + 2kx = 0\)
05

5. Solve the standard form equation for the natural frequency

The solution to the standard form equation has the form \(x(t) = A\cos(\omega_n t + \phi)\), where \(\omega_n\) is the natural frequency of the system. To find \(\omega_n\), we compare the coefficients of the standard form equation: \(\frac{m}{2} \omega_n^2 = k\) Now, we can solve for the natural frequency: \(\omega_n = \sqrt{\frac{2k}{m}}\) This gives us the natural frequency of the system.

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