Hamiltonian for mass on a smooth fixed hemisphere

Click For Summary
SUMMARY

The discussion focuses on deriving the Hamiltonian for a mass constrained on a smooth fixed hemisphere, referencing Thornton's example 7.10. The potential energy is expressed as \( mgr \cos \theta \), and the generalized momentum \( p_{\theta} \) is calculated as \( mr^2 \dot{\theta} \). The equation of motion derived is \( \ddot{\theta} = -\frac{g}{r} \sin \theta \), indicating a mathematical pendulum's behavior. The discussion emphasizes the importance of using spherical coordinates for a more general case and suggests seeking guidance in a homework forum for deeper understanding.

PREREQUISITES
  • Understanding of Hamiltonian mechanics
  • Familiarity with Lagrangian dynamics
  • Knowledge of spherical coordinates
  • Basic principles of classical mechanics
NEXT STEPS
  • Study Hamiltonian mechanics in detail, focusing on cyclic coordinates
  • Explore Lagrangian dynamics with examples involving potential energy
  • Learn about spherical pendulum dynamics and their equations of motion
  • Review resources on generalized coordinates and momenta in classical mechanics
USEFUL FOR

Students of physics, particularly those studying classical mechanics, and anyone interested in advanced dynamics involving Hamiltonian and Lagrangian formulations.

Jacob Flowers
Messages
1
Reaction score
0
I am trying to figure out how to get the Hamiltonian for a mass on a fixed smooth hemisphere.

Using Thorton from example 7.10 page 252

My main question is about the Potential energy= mgrcosineθ is the generalized momenta Pdotθ supposed to be equal to zero because θ is cyclic? Or is Pdotθ= -∂H/∂θ= mgr sineθ
http://kylejensenphysicsblog.blogspot.com/2016/03/hamiltons-principle-and-lagrangians.htmlSorry for not being able to upload a pictuure or putting dots over P but I don't know how to do so
 
Physics news on Phys.org
But in the link above you don't have a particle on a sphere but on a circle, and then of course ##\dot{r}=0##. So the correct Lagrangian is
$$L=\frac{m}{2} r^2 \dot{\theta}^2+mgr \cos \theta.$$
I also have more conveniently pointed the ##y## axis in direction of ##\vec{g}## such that the stable stationary state is ##\theta=0=\text{const}##. Then you have
$$p_{\theta}=\frac{\partial L}{\partial \dot{\theta}}=mr^2 \dot{\theta} \; \Rightarrow \; \dot{p}_{\theta}=m r^2 \ddot{\theta}=\frac{\partial L}{\partial \theta}=-mgr \sin \theta,$$
and you get the equation of motion for a mathematical pendulum, as you should:
$$\ddot{\theta}=-\frac{g}{r} \sin \theta.$$

For the more general case you should use spherical coordinates
$$\vec{x}=\begin{pmatrix} r \cos \varphi \sin \vartheta \\ r \sin \varphi \sin \vartheta \\ r \cos \vartheta \end{pmatrix},$$
again with ##r=\text{const}##. Now write down the Hamiltonian, and you'll get the equations of motion for a spherical pendulum, but this problem you should discuss in the homework forum since it's way better to get some guidance to solve the problem yourself than just a solution!
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
Replies
5
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 10 ·
Replies
10
Views
7K
  • · Replies 1 ·
Replies
1
Views
4K
Replies
2
Views
1K
Replies
5
Views
3K
  • · Replies 1 ·
Replies
1
Views
3K