Velocity Dependent Potential

Glad to hear you got them! For future reference, here are some tips for finding conserved quantities:1) Look for symmetries in the problem. For example, if the problem has cylindrical or spherical symmetry, then the corresponding angular momentum ( L_z or L^2 ) will be conserved.2) Use Noether's theorem. This states that for every continuous symmetry in a system, there exists a corresponding conserved quantity. For example, invariance under time translation leads to conservation of energy, invariance under space translation leads to conservation of linear momentum, etc.3) Use the cyclic coordinate theorem. If a coordinate does not appear explicitly in the Lagrangian, then the corresponding momentum will be cons
  • #1
CNX
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0

Homework Statement



Consider a particle of mass m and charge q that moves in an E-field [itex]\vec{E}=\frac{E_0}{r}\hat{r}[/itex] and a uniform magnetic field [itex]\vec{B}=B_0\hat{k}[/itex]. Find the scalar potential and show the vector potential is given by [itex]\vec{A}=\frac{1}{2}B_0 r \hat{\theta}[/itex]. Then obtain the Lagrange equations of motion and identify the conserved quantities

Homework Equations



Lagrange equations

The Attempt at a Solution



Using cylindrical coords,

[tex]L=T-V=\frac{1}{2}m \left ( \dot{r}^2+\dot{\theta}^2+\dot{z}^2 \right) - e\phi + e\vec{v} \cdot \vec{A}[/tex]

[tex]L = \frac{1}{2}m \left ( \dot{r}^2+\dot{\theta}^2+\dot{z}^2 \right) - eE_0\ln(r) + \frac{1}{2}e\dot{\theta}B_0r[/tex]

Using the Lagrange equation,

[tex]0 = m\ddot{r} + eE_0\frac{1}{r} - \frac{1}{2}e\dot{\theta}B_0[/tex]

[tex]0=m\ddot{\theta}[/tex]

[tex]0=m\ddot{z}[/itex]

Correct?
 
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  • #2
CNX said:

Homework Statement



Consider a particle of mass m and charge q that moves in an E-field [itex]\vec{E}=\frac{E_0}{r}\hat{r}[/itex] and a uniform magnetic field [itex]\vec{B}=B_0\hat{k}[/itex]. Find the scalar potential and show the vector potential is given by [itex]\vec{A}=\frac{1}{2}B_0 r \hat{\theta}[/itex]. Then obtain the Lagrange equations of motion and identify the conserved quantities

It took me a minute to realize that you are using [itex](r,\theta,z)[/itex] as your cylindrical coordinates...ewww :yuck:... that makes things confusing since one usually uses [itex]\vec{r}[/itex] to represent the position of the particle, and hence it is more natural for [itex]r[/itex] to be used as the spherical polar coordinate corresponding to the distance from the origin so that [itex]\vec{r}=r\hat{r}[/itex]. In this case however, [itex]\vec{r}=r\hat{r}+z\hat{z}[/itex] which is not very aesthetic...but, I digress...

The Attempt at a Solution



Using cylindrical coords,

[tex]L=T-V=\frac{1}{2}m \left ( \dot{r}^2+\dot{\theta}^2+\dot{z}^2 \right) - e\phi + e\vec{v} \cdot \vec{A}[/tex]

It is always a good idea to check your units...does the angular term in [itex]\vec{v}=\dot{r}\hat{r}+\dot{\theta}\hat{\theta}+\dot{z}\hat{z}[/itex] have the correct units?

[tex]L = \ldots - eE_0\ln(r) + \ldots[/tex]

Looks like you have a sign error here...remember, [itex]\vec{E}=-\vec{\nabla}}\phi[/itex]

Using the Lagrange equation,

[tex]0=m\ddot{\theta}[/tex]

Correct?

Be careful with this equation, remember that it is a full time derivative (not a partial derivative) in the Euler-Lagrange equation:
[tex]\frac{d}{dt}\frac{\partial L}{\partial \dot{\theta}}\neq m\ddot{\theta}[/tex]
 
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  • #3
My attempt at corrections (Note the change in coordinate labels):

Using cylindrical coords [itex](\rho, \theta, z)[/itex],

[tex]L=T-V=\frac{1}{2}m \left ( \dot{\rho}^2+\rho\dot{\theta}^2+\dot{z}^2 \right) - e\phi + e\vec{v} \cdot \vec{A}[/tex]

[tex]L = \frac{1}{2}m \left ( \dot{\rho}^2+\rho\dot{\theta}^2+\dot{z}^2 \right) + eE_0\ln(\rho) + \frac{1}{2}e\dot{\theta}B_0 \rho^2[/tex]

Using the Lagrange equation,

[tex]0 = m\ddot{\rho} - m\rho\ddot{\theta}^2 - eE_0\frac{1}{\rho} - e\dot{\theta}B_0\rho[/tex]

[tex]0=m\rho^2 \ddot{\theta} + 2m\rho\dot{\rho}\dot{\theta} + e B_0\rho\dot{\rho}[/tex]

[tex]0=m\ddot{z}[/itex]
 
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  • #4
CNX said:
My attempt at corrections (Note the change in coordinate labels):

Using cylindrical coords [itex](\rho, \theta, z)[/itex],

[tex]L=T-V=\frac{1}{2}m \left ( \dot{\rho}^2+\rho\dot{\theta}^2+\dot{z}^2 \right) - e\phi + e\vec{v} \cdot \vec{A}[/tex]

[tex]L = \frac{1}{2}m \left ( \dot{\rho}^2+\rho\dot{\theta}^2+\dot{z}^2 \right) + eE_0\ln(\rho) + \frac{1}{2}e\dot{\theta}B_0 \rho^2[/tex]

Surely you meant to put some brackets in there:

[tex]L=T-V=\frac{1}{2}m \left ( \dot{\rho}^2+(\rho\dot{\theta})^2+\dot{z}^2 \right) - e\phi + e\vec{v} \cdot \vec{A}[/tex]

[tex]L = \frac{1}{2}m \left ( \dot{\rho}^2+(\rho\dot{\theta})^2+\dot{z}^2 \right) + eE_0\ln(\rho) + \frac{1}{2}e\dot{\theta}B_0 \rho^2[/tex]

Using the Lagrange equation,

[tex]0 = m\ddot{\rho} - m\rho\ddot{\theta}^2 - eE_0\frac{1}{\rho} - e\dot{\theta}B_0\rho[/tex]

[tex]0=m\rho^2 \ddot{\theta} + 2m\rho\dot{\rho}\dot{\theta} + e B_0\rho\dot{\rho}[/tex]

[tex]0=m\ddot{z}[/itex]

The first one should be:

[tex]0 = m\ddot{\rho} - m\rho\dot{\theta}^2 - eE_0\frac{1}{\rho} - e\dot{\theta}B_0\rho[/tex]

Other than that everything looks good :smile:...You can double check your answers by comparing them to what you get from the Lorentz Force law; you should get the same equations of motion.

How about the conserved quantities...what are you getting for those?
 
  • #5
Thanks. Wouldn't [itex]\dot{z}[/itex] be the conserved quantity?
 
  • #6
Sure, the axial component of the velocity ( [itex]\dot{z}[/itex] ) or the axial momentum ( [itex]p_z=m\dot{z}[/itex] ) is conserved, but is that the only conserved quantity?...How does one typically go about finding the conserved quantities in Lagrangian or Hamiltonian dynamics?
 
  • #7
Thanks I got them
 

1. What is velocity dependent potential?

Velocity dependent potential is a type of potential energy that depends on an object's velocity. It is often used in physics to describe the motion of particles in a system.

2. How is velocity dependent potential different from other types of potential energy?

Unlike other types of potential energy, which only depend on the position of an object, velocity dependent potential also takes into account the object's velocity. This means that the potential energy can change as the object moves, and is not constant at a specific point.

3. What is an example of a velocity dependent potential?

One example of a velocity dependent potential is the Coulomb potential, which describes the potential energy between two charged particles in motion. The potential energy in this case depends on both the distance between the particles and their velocities.

4. How is velocity dependent potential used in scientific research?

Velocity dependent potential is commonly used in fields such as particle physics, astrophysics, and fluid dynamics to study the motion of particles and systems. It allows scientists to better understand how objects move and interact with each other in different environments.

5. How is velocity dependent potential related to kinetic energy?

Velocity dependent potential and kinetic energy are closely related. When an object is moving in a system with velocity dependent potential, some of its kinetic energy is converted into potential energy. This potential energy can then be converted back into kinetic energy as the object continues to move and interact with the potential field.

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