Landau Quantization: Classical Particle Motion in a Uniform Magnetic Field

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Homework Help Overview

The problem involves a classical particle with charge q and mass m moving in a uniform magnetic field in two dimensions. The discussion focuses on understanding the trajectory of the particle, evaluating the classical action along that trajectory, and determining the magnetic flux as a function of energy.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Problem interpretation, Assumption checking

Approaches and Questions Raised

  • Participants discuss the Lorentz force law and its implications for the particle's trajectory, questioning how energy affects the trajectory. There are attempts to derive the equations of motion using Hamiltonian dynamics and to express the Lagrangian for the system. Some participants express confusion regarding the vector potential and its relation to the magnetic field.

Discussion Status

The discussion is ongoing, with participants exploring different interpretations of the vector potential and its implications for the magnetic field. Some guidance has been provided regarding the use of the Landau gauge and the formulation of the Lagrangian, but there is no explicit consensus on the trajectory or the evaluation of the classical action.

Contextual Notes

Participants are grappling with the implications of energy on the trajectory and the correct formulation of the vector potential. There are references to class notes and textbooks, indicating reliance on external sources for clarification. The discussion also highlights the concept of gauge invariance in the context of vector potentials.

  • #31
I just integrated v_{x} from 0 to t to get (v_{0})(cos(t\omega) - cos(0)) + x_{0} \longrightarrow (v_{0})cos(t\omega) -v_{0} + x_{0}

although the (-v_{0}) term seems strange to me
 
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  • #32
But, x is not a constant:

<br /> x(t) = x_{0} + \int_{t_{0}}^{t}{v_{x}(t&#039;) \, dt&#039;}<br />
 
  • #33
Right. Integrating v_{x} = v_{0}cos(t\omega) over [t_{0}, t] gives

v_{0}[\omega(sin(t_{0} \omega) - sin(t \omega))] where (sin(t_{0} \omega) is some constant, unless I'm being an idiot.

Oh jeez, I just saw that I did the wrong integral in my last post. Now I think your comment makes sense.
 
  • #34
No!

<br /> \int{\cos{(a t)} \, dt} = \frac{1}{a} \, \sin{(a \, t)}<br />
 
  • #35
Jesus. Embarrassing. Long day.

But we are doing a definite integral, so it should still end up as v_{0}[\frac{1}{\omega}(sin(t_{0} \omega) - sin(t \omega))] shouldn't it? If we set t_{0}=0, then the first sin term vanishes, and we end up with v_{0}[\frac{1}{\omega}(-sin(t \omega))] ?
 
  • #36
Yes, this would be x(t) that you need to substitute in the above expression and integrate again.
 
  • #37
Integrating my LagrangianL = (m/2)[(v_{0})^2 +1] - (q/c)B[(x_{0} - \frac{v_{0}}{\omega} sin(t\omega)][-(v_{0})sin(t\omega)]

Gives

S(t) = [(m(v_{0})^2)/2]\Delta t - <br /> <br /> (q/c)B[\frac{(v_{0})x_{0}}{\omega}](cos(\omega t_{1}) - cos(\omega t_{0})) - <br /> <br /> (q/c)B[\frac{(v_{0})^2}{\omega}]((t_{1})/2 - \frac{sin(2\omega t_{1})}{4\omega} - (t_{0})/2) + \frac{sin(2\omega t_{0})}{4\omega}

This looks more complicated than it should be..
 
  • #38
Ok, do this first:

Take the lagrangian:

<br /> L = \frac{m v^{2}_{0}}{2} \, \left(v^{2}_{x} + v^{2}_{y} \right) - \frac{q B}{c} \, x \, v_{y}<br />

substitute:

<br /> \begin{array}{rcl}<br /> v_{x} &amp; = &amp; v_{0} \, \cos{(\omega \, t)} \\<br /> <br /> v_{y} &amp; = &amp; -v_{0} \, \sin{(\omega \, t)} \\<br /> <br /> x &amp; = &amp; \frac{v_{0}}{\omega} \, \sin{(\omega t)}<br />

and perform integration from 0 to t, by keeping in mind that:

<br /> \omega = \frac{q \, B}{m \, c}<br />

What is the lagrangian as a function of t?

What is the integral of this from 0 to t?
 
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  • #39
I get that L=(v_{0})^2[\frac{m}{2} + (sin(\omega t)^2)

Have I done anything stupid so far?
 
  • #40
First of all, your equation is dimensionally inconsistent. In the large parentheses, the first term has a dimension of mass, and the second term is dimensionless.
 
  • #41
All I did was cancel the omega in the x term and the omega in the v_{y} term, which I got from plugging in the provided equations.

Sigh. How did I manage to mess THAT up?
 
  • #42
The vector potential term from the Lagrangian has the product:

<br /> x v_{x} = \frac{v_{0}}{\omega} \, \sin{(\omega t)} \, v_{0} \, \cos{(\omega t)} = \frac{v^{2}_{0}}{\omega} \sin{(\omega t)} \, \cos{(\omega t)}<br />

using the double angle formula:

<br /> \sin{(2 \alpha)} = 2 \, \sin{(\alpha)} \, \cos{(\alpha)}<br />

this product can be further simplified as:

<br /> \frac{v^{2}_{0}}{2 \omega} \, \sin{(2 \omega t)}<br />

However, this product is also multiplied by q \, B/c in the Lagrangian. Using the definition of the cyclotron frequency \omega = q \, B/(m \, c), what is:

<br /> \frac{q B}{\omega c} = ?<br />

The kinetic energy term has the sum of squares:

<br /> v^{2}_{x} + v^{2}_{y} = ?<br />

What is this sum equal to? What is it multiplied by in the Lagrangian?
 
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  • #43
<br /> \frac{q B}{\omega c} = ?<br />\frac{qB}{\omega c} = \frac{qBmc}{Bc} = qm[/tex]<br /> <br /> The kinetic energy term has the sum of squares:<br /> <br /> &lt;br /&gt; v^{2}_{x} + v^{2}_{y} = ?&lt;br /&gt;<br /> <br /> What is this sum equal to? What is it multiplied by in the Lagrangian?<br /> <br /> &lt;br /&gt; v^{2}_{x} + v^{2}_{y} = ((v_{0})^2)((cos(\omega t))^2 + (sin(\omega t))^2) = ((v_{0})^2)&lt;br /&gt;<br /> <br /> This is then multiplied by \frac{m}{2}
 
  • #44
Whaddya mean?
 
  • #45
Sonny Liston said:
<br /> \frac{q B}{\omega c} = ?<br />


\frac{qB}{\omega c} = \frac{qBmc}{Bc} = qm[/tex]<br />
<br /> This is incorrect.<br /> <br /> <blockquote data-attributes="" data-quote="Sonny Liston" data-source="post: 2985775" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> Sonny Liston said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> The kinetic energy term has the sum of squares:<br /> <br /> &lt;br /&gt; v^{2}_{x} + v^{2}_{y} = ?&lt;br /&gt;<br /> <br /> What is this sum equal to? What is it multiplied by in the Lagrangian?<br /> <br /> &lt;br /&gt; v^{2}_{x} + v^{2}_{y} = ((v_{0})^2)((cos(\omega t))^2 + (sin(\omega t))^2) = ((v_{0})^2)&lt;br /&gt;<br /> <br /> This is then multiplied by \frac{m}{2} </div> </div> </blockquote>This is correct.
 
  • #46
I didn't see the charge term in the original cyclotron frequency. In that case, we don't get qm, we get m.
 
  • #47
Sonny Liston said:
I didn't see the charge term in the original cyclotron frequency. In that case, we don't get qm, we get m.

Yes. So, what is the final expression for the Lagrangian L?
 
  • #48
L = \frac{m(v_{0})^2}{2} - \frac{m(v_{0})^2}{2\omega}sin(2t\omega)
 
  • #49
Sonny Liston said:
L = \frac{m(v_{0})^2}{2} - \frac{m(v_{0})^2}{2\omega}sin(2t\omega)

Where did the extra \omega come from in the second term? C'mon man. Concentrate on your algebra. This is taking too long.
 
  • #50
S(t) = [\frac{m((v_{0})^2)}{2}]t + [\frac{m((v_{0})^2)}{2}]\frac{(cos(2t\omega) + 1}{2\omega}

Extra omega eliminated here. Sorry about that.
 
  • #51
(Again, you kept an extra \omega in the second term.) I see you corrected that.

Also:

<br /> \int_{0}^{t}{\sin{(2 \omega t)} \, dt} = -\left.\frac{1}{2 \omega} \, \cos{(\omega t)}\right|^{t}_{0} = \frac{1}{2\omega} \, \left[1 - \cos{(2 \omega t)}\right]<br />

Finally, what will be the change in S during one period (take t = 2\pi/\omega in the above formula)?
 
  • #52
1 - cos (2 \omega \frac{(2\pi}{\omega}) = 0, so it is appropriately periodic.
 
  • #53
No, the first term is proportional to t and is not periodic.
 
  • #54
Assuming that's satisfactory, may I ask you one last quick question (you are a saint, by the way. I have been unbelievably useless throughout this.) How would I go about evaluating the magnetic flux through the classical trajectory as a function of the energy?

In case you're wondering about my remarkable ignorance, I'm a math student who never took classical mechanics and is in a quantum course, so all the classical mechanics stuff is new to me. Thanks again.
 
  • #55
What does the trajectory look like? What are its dimensions in terms of the quantities we have already defined? What is the magnetic flux from a homogeneous magnetic field perpendicular through a contour?
 
  • #56
In my notes, I have that it is given by \frac{1}{2\pi}\oint A dx, and the baby E&M book I am looking at says that it can be given by the Area of the surface dotted with the B field times cos(theta), for theta the angle between the B field and the surface.

But since the B field is homogeneous in the z-direction, \theta = \frac{\pi}{2} and cos=0, so something must be really flawed in my reasoning.
 
  • #57
Sonny Liston said:
In my notes, I have that it is given by \frac{1}{2\pi}\oint A dx, and the baby E&M book I am looking at says that it can be given by the Area of the surface dotted with the B field times cos(theta), for theta the angle between the B field and the surface.

But since the B field is homogeneous in the z-direction, \theta = \frac{\pi}{2} and cos=0, so something must be really flawed in my reasoning.

Yes, they are both equal due to Stokes' Theorem:

<br /> \phi_{m} = \int_{S}{\left(\mathbf{B} \cdot \hat{\mathbf{n}}\right) \, da} = \oint{\mathbf{A} \cdot d\mathbf{l}}<br />

So, there is no factor of 1/(2\pi) if you use the circulation of the vector potential.
 
  • #58
So there is nothing wrong in my reasoning and the flux actually is zero? It seems odd to ask me to evaluate it "as a function of the energy" then.
 
  • #59
No, it is not zero. I didn't see the part where you say it's zero. Since \mathbf{A} has only a zero component, you need to evaluate:

<br /> \oint{\mathbf{A} \cdot d\mathbf{l}} = \oint{A_{y} \, dy} = B \int_{0}^{T}{x(t) \, v_{y}(t)}<br />

where T = 2\pi/\omega is the period of the trajectory and i used A_{y} = B \, x.
 
  • #60
B\int x(t) v_{y} (t) = B \frac{-(v_{0})^2}{\omega} \int (sin(\omega t)^2)

Using (sin(\omega t)^2) = \frac{1 - cos (2\omega t)}{2} and doing the integral, I get

\Phi = B\pi(- \frac{v_{0}}{\omega})^2
 

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