Lagrangian for a particle in a bowl with parabolic curvature

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Homework Help Overview

The problem involves a particle of mass moving inside a bowl shaped by a paraboloid of revolution. Participants are tasked with writing the Lagrangian and the Euler-Lagrange equations for this system, focusing on the kinetic and potential energy components in cylindrical coordinates.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants discuss the formulation of the Lagrangian, including potential and kinetic energy expressions. There are attempts to derive the Euler-Lagrange equations for both coordinates involved. Some participants express confusion regarding the derivatives and the implications of the particle moving without slipping.

Discussion Status

There is ongoing exploration of the correct expressions for the Lagrangian and its derivatives. Some participants have pointed out potential errors in the calculations, while others are questioning the physical interpretation of the problem, particularly regarding the conditions of motion without slipping or friction. The discussion reflects a mix of clarifications and attempts to resolve misunderstandings.

Contextual Notes

Participants are considering the implications of the particle's motion, including the assumption of constant radius and its effects on angular velocity. There is a suggestion that the problem may have intended to describe motion without friction rather than without slipping, leading to further exploration of the constraints involved.

vbrasic
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Homework Statement


A particle of mass ##m## moves without slipping inside a bowl generated by the paraboloid of revolution ##z=b\rho^2,## where ##b## is a positive constant. Write the Lagrangian and Euler-Lagrange equation for this system.

Homework Equations


$$\frac{\partial\mathcal{L}}{\partial q_i}-\frac{d}{dt}\frac{\partial\mathcal{L}}{\partial \dot{q_i}}$$

The Attempt at a Solution


Potential energy is given by, $$V=mgz=mgb\rho^2.$$ Kinetic energy in cylindrical coordinates is given by, $$T=\dot{\rho}^2+\rho^2\dot{\theta}^2+\dot{z}^2=\dot{\rho}^2+\rho^2\dot{\theta}^2+4b^2\rho^2\dot{\rho}^2.$$ Then the Lagrangian is, $$\mathcal{L}=\dot{\rho}^2+\rho^2\dot{\theta}^2+4b^2\rho^2\dot{\rho}^2-mgb\rho^2.$$ Then, we can write the Euler-Lagrange equations for both ##\theta## and ##\rho##. The ##\theta## equation is very simple. We have, $$\frac{\partial\mathcal{L}}{\partial\theta}=0,$$ and $$\frac{d}{dt}\frac{\partial\mathcal{L}}{\partial\dot{\theta}}=\frac{d}{dt}\bigg(2\rho^2\dot{\theta}\bigg)=4\rho\dot{\rho}\dot{\theta}+2\rho^2\ddot{\theta}.$$ So the Euler-Lagrange equation reads, $$4\rho\dot{\rho}\dot{\theta}+2\rho^2\ddot{\theta}=0.$$ I'm getting messy with my derivatives in the ##\rho## equations. Any help would be appreciated.
 
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vbrasic said:

Homework Statement


A particle of mass ##m## moves without slipping inside a bowl generated by the paraboloid of revolution ##z=b\rho^2,## where ##b## is a positive constant. Write the Lagrangian and Euler-Lagrange equation for this system.

Homework Equations


$$\frac{\partial\mathcal{L}}{\partial q_i}-\frac{d}{dt}\frac{\partial\mathcal{L}}{\partial \dot{q_i}}$$

The Attempt at a Solution


Potential energy is given by, $$V=mgz=mgb\rho^2.$$ Kinetic energy in cylindrical coordinates is given by, $$T=\dot{\rho}^2+\rho^2\dot{\theta}^2+\dot{z}^2=\dot{\rho}^2+\rho^2\dot{\theta}^2+4b^2\rho^2\dot{\rho}^2.$$ Then the Lagrangian is, $$\mathcal{L}=\dot{\rho}^2+\rho^2\dot{\theta}^2+4b^2\rho^2\dot{\rho}^2-mgb\rho^2.$$ Then, we can write the Euler-Lagrange equations for both ##\theta## and ##\rho##. The ##\theta## equation is very simple. We have, $$\frac{\partial\mathcal{L}}{\partial\theta}=0,$$ and $$\frac{d}{dt}\frac{\partial\mathcal{L}}{\partial\dot{\theta}}=\frac{d}{dt}\bigg(2\rho^2\dot{\theta}\bigg)=4\rho\dot{\rho}\dot{\theta}+2\rho^2\ddot{\theta}.$$ So the Euler-Lagrange equation reads, $$4\rho\dot{\rho}\dot{\theta}+2\rho^2\ddot{\theta}=0.$$ I'm getting messy with my derivatives in the ##\rho## equations. Any help would be appreciated.
Your work looks correct so far except for a factor of ##\frac 1 2 m## missing from T and its partials. That doesn't matter in your partials with respect to ##θ## and ##\dot θ##, but it will in the partials with respect to ##ρ## and ##\dot ρ##. If you would post your results so far for partials with respect to ##ρ## and ##\dot ρ##, maybe we could point out where you are going wrong.
 
vbrasic said:
A particle of mass ##m## moves without slipping inside a bowl
How can the particle move without slipping? I can't visualize that.
 
TSny said:
How can the particle move without slipping? I can't visualize that.
I think the idea is that a ball is rolling in a bowl without slipping.
 
If it's a ball, then it will be a really difficult problem. There would be the additional kinetic energy of rotation of the ball. Also, a (non-holonomic) constraint condition would need to be included that corresponds to the rolling without slipping.

Maybe the problem meant to state that the particle moves without friction rather than without slipping.
 
TSny said:
Maybe the problem meant to state that the particle moves without friction rather than without slipping.

Yes, I meant without friction.
 
The Lagrangian (with the m/2 factor added), is, $$\mathcal{L}=\frac{1}{2}m(\dot{\rho}^2+\rho^2\dot{\theta}^2+4b^2\rho^2\dot{\rho}^2)-mgb\rho^2.$$ So, $$\frac{\partial\mathcal{L}}{\partial\rho}=m\rho\dot{\theta}^2+4mb^2\rho\dot{\rho^2}-2mgb\rho,$$ and, $$\frac{\partial\mathcal{L}}{\partial\dot{\rho}}=m\dot{\rho}+4mb\rho^2\dot{\rho}.$$ Taking the time derivative, we have, $$\frac{d}{dt}\frac{\partial\mathcal{L}}{\partial\dot{\rho}}=m\ddot{\rho}+4mb(2\rho\dot{\rho}^2+\rho^2\ddot{\rho}).$$ Do my derivatives look alright?
 
Your ##b## should be ##b^2## in these two equations:
vbrasic said:
$$\frac{\partial\mathcal{L}}{\partial\dot{\rho}}=m\dot{\rho}+4mb\rho^2\dot{\rho}.$$
$$\frac{d}{dt}\frac{\partial\mathcal{L}}{\partial\dot{\rho}}=m\ddot{\rho}+4mb(2\rho\dot{\rho}^2+\rho^2\ddot{\rho}).$$
Otherwise, they look right.
 
  • #10
tnich said:
Your ##b## should be ##b^2## in these two equations:

Otherwise, they look right.
As a final question. Supposing that ##\rho## is constant, we have that ##\dot{\rho}=\ddot{\rho}=0,## so the Euler-Lagrange equation for ##\rho## reads $$0\frac{mp\dot{\theta}^2-2mgb\rho}{(m+4mb^2\rho^2)}\to\dot{\theta}=\sqrt{2gb}.$$ Does it physically make sense that change in angular velocity has no dependence in radius if the path is circular with constant radius?
 
  • #11
vbrasic said:
As a final question. Supposing that ##\rho## is constant, we have that ##\dot{\rho}=\ddot{\rho}=0,## so the Euler-Lagrange equation for ##\rho## reads $$0\frac{mp\dot{\theta}^2-2mgb\rho}{(m+4mb^2\rho^2)}\to\dot{\theta}=\sqrt{2gb}.$$ Does it physically make sense that change in angular velocity has no dependence in radius if the path is circular with constant radius?
I think it does. Assuming that ##\dot ρ = 0##, the components of radial acceleration and gravitational acceleration tangent to the paraboloid surface must sum to zero. Try setting up that equation and you will get the result ##\dot{\theta}=\sqrt{2gb}##.
 

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