Oscillations of a disc with a smaller disc removed (Feynman ex. 17.23)

  • Thread starter Thread starter ergospherical
  • Start date Start date
  • Tags Tags
    Disc Oscillations
Click For Summary
SUMMARY

The discussion centers on the oscillations of a disc with a smaller disc removed, specifically analyzing the dynamics of the resulting object. The center of mass is calculated to be at a distance of \(h = \frac{5a}{6}\) from the edge, and the moment of inertia about the center \(C\) is derived as \(I_C = \frac{13\pi a^4 \rho}{32}\). The kinetic energy expression is established as \(T = \pi a^4 \rho \dot{\varphi}^2 \left( \frac{115}{192} - \frac{1}{8} \cos{\varphi} \right)\), while the potential energy is given by \(U = \frac{3\pi a^3 \rho g}{4}\left(1- \frac{1}{6} \cos{\varphi} \right)\). The final motion analysis reveals a non-simple harmonic motion, leading to a derived period \(T = \pi \sqrt{\frac{29a}{g}}\) as per the solution manual.

PREREQUISITES
  • Understanding of rotational dynamics and moment of inertia
  • Familiarity with the concepts of center of mass and kinetic energy
  • Knowledge of potential energy in gravitational fields
  • Application of the parallel axis theorem in physics
NEXT STEPS
  • Study the parallel axis theorem and its applications in rotational dynamics
  • Explore the derivation of kinetic and potential energy in oscillatory systems
  • Investigate the conditions for simple harmonic motion in non-linear systems
  • Learn about the effects of mass distribution on oscillation periods in rigid bodies
USEFUL FOR

Physics students, mechanical engineers, and anyone interested in advanced dynamics and oscillatory motion analysis.

ergospherical
Science Advisor
Homework Helper
Education Advisor
Insights Author
Messages
1,100
Reaction score
1,387
Homework Statement
Determine the period of small oscillations, given that the disc rolls without slipping
Relevant Equations
N/A
A disc of radius ##a## has a smaller disc of radius ##a/2## removed. The resulting object has mass ##m##:

1630700847115.png
The centre of mass ##G## is a distance ##h = \dfrac{\pi a^3 - \dfrac{3\pi a^3}{8} }{\dfrac{3\pi a^2}{4}} = \dfrac{5a}{6}## from the edge. The moment of inertia of the shape about the centre ##C## is\begin{align*}
I_C = \dfrac{1}{2}(\pi a^2 \rho)a^2 - \left(\dfrac{\pi a^2 \rho}{4} \right) \left( \dfrac{1}{2} \left(\dfrac{a}{2} \right)^2 + \left(\dfrac{a}{2} \right)^2 \right) = \dfrac{13\pi a^4 \rho}{32}
\end{align*}therefore the moment of inertia about ##G## is $$I_G = I_C + \dfrac{3\pi a^2 \rho}{4} \left(\dfrac{a}{6} \right)^2 = \dfrac{41 \pi a^4 \rho}{96}$$If the angle through which the disc has rotated is denoted ##\varphi##, then the centre of mass ##G## has velocity\begin{align*}
\mathbf{v}_G &= (a\dot{\varphi})\mathbf{\hat{x}} + \boldsymbol{\omega} \times \overrightarrow{CG} = \left(a\dot{\varphi} - \dfrac{a \dot{\varphi}}{6} \cos{\varphi} \right)\mathbf{\hat{x}} + \left(\dfrac{a\dot{\varphi}}{6} \sin{\varphi} \right)\mathbf{\hat{y}} \\

\implies v_G^2 &= \frac{a^2 \dot{\varphi}^2}{36}\left(37 - 12\cos{\varphi} \right)
\end{align*}Therefore the kinetic energy of the body is\begin{align*}
T = \dfrac{1}{2} m v_G^2 + \dfrac{1}{2}I_G \dot{\varphi}^2 = \pi a^4 \rho \dot{\varphi}^2 \left( \dfrac{1}{96}(37 - 12\cos{\varphi}) + \frac{41}{192} \right) = \pi a^4 \rho \dot{\varphi}^2 \left( \dfrac{115}{192} - \dfrac{1}{8} \cos{\varphi} \right)
\end{align*}Meanwhile, the height of the centre of mass ##G## when the body has rotated by ##\varphi## is\begin{align*}
y_G = a(1-\cos{\varphi}) + \dfrac{5a}{6} \cos{\varphi} = a(1- \dfrac{1}{6} \cos{\varphi})
\end{align*}therefore the potential energy is ##U = \dfrac{3\pi a^3 \rho g}{4}\left(1- \dfrac{1}{6} \cos{\varphi} \right)##. Overall I write the energy ##E## as\begin{align*}
\dfrac{1}{\pi a^3 \rho} E &= a \dot{\varphi}^2 \left( \dfrac{115}{192} - \dfrac{1}{8} \cos{\varphi} \right) + \dfrac{3g}{4}\left(1- \dfrac{1}{6} \cos{\varphi} \right) \\ \\

\implies \dot{E} &= 2a \dot{\varphi} \ddot{\varphi}\left( \dfrac{115}{192} - \dfrac{1}{8} \cos{\varphi} \right) + \dfrac{a\dot{\varphi}^3}{8} \sin{\varphi} + \dfrac{g \dot{\varphi}}{8} \sin{\varphi} \overset{!}{=} 0
\end{align*}The motion does not look simple harmonic, at least for finite ##\varphi##. To investigate we can put ##\cos{\varphi} = 1## and ##\sin{\varphi} = \varphi##, and I assume also ##\dot{\varphi}^2 = 0##, which gives\begin{align*}
\ddot{\varphi} + \dfrac{12g}{91a} \varphi = 0 \implies \Omega &= \sqrt{\dfrac{12 g}{91 a}} \\

T &= \pi \sqrt{\dfrac{91a}{3g}}
\end{align*}However in the solution manual they write ##T = \pi \sqrt{29a/g}##?
 
  • Like
Likes   Reactions: Hamiltonian
Physics news on Phys.org
State the parallel axis theorem. Did you use it correctly?
 
  • Like
Likes   Reactions: ergospherical
haruspex said:
State the parallel axis theorem. Did you use it correctly?
ahhhh, kill me
ought to be ##I_G = I_C - \dfrac{3\pi a^2 \rho}{4} \left(\dfrac{a}{6} \right)^2##, right?

[Edit: Yep, I checked it through with ##I_G = \dfrac{37 \pi a^4 \rho}{96}## and it works. Thanks haru! ☺️]
 
Last edited:
  • Like
Likes   Reactions: haruspex

Similar threads

  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 6 ·
Replies
6
Views
2K
Replies
13
Views
1K
Replies
23
Views
2K
  • · Replies 11 ·
Replies
11
Views
1K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 6 ·
Replies
6
Views
1K
Replies
4
Views
3K
Replies
9
Views
2K