Moving sphere in magnetic field

In summary, the conversation is about solving a problem involving a conducting sphere moving with constant velocity in a constant magnetic field. The task is to find the induced charge distribution on the sphere to first order in v/c in the laboratory inertial reference frame. The person discussing the problem mentions their attempt at a solution, which involved considering a different inertial reference frame and calculating the induced surface charge density. However, their approach was deemed incorrect by their professors. Another person suggests solving the problem exactly for a constant external field at infinity and a fixed potential on the sphere. After some discussion and clarification, the person attempting the problem comes up with an expression for the potential, but is unsure how to calculate the surface charge density from it
  • #1
fluidistic
Gold Member
3,923
261

Homework Statement


I got no credit in an exam for the following exercise and I've been told what's wrong but even then I am unable to solve it correctly.
A conducting sphere with radius R moves with constant velocity ##\vec v =v \hat x## (v <<c) inside a constant magnetic field ##\vec B =B \hat y##. Find the induced charge distribution on the sphere to 1st order in v/c in the laboratory inertial reference frame.

Homework Equations


Fields transformations: ##\vec E '=\gamma (\vec E +\vec \beta \times \vec B ) - \frac{\gamma^2}{\gamma +1} \vec \beta (\vec \beta \cdot \vec E )##
##\vec B' =\gamma (\vec B -\vec \beta \times \vec E ) - \frac{\gamma ^2}{\gamma +1} \vec \beta (\vec \beta \cdot \vec B )##.
Lorentz boost.
##\rho = \gamma \rho'##. Where rho is the charge distribution in the laboratory K and rho' the charge distribution in another inertial reference frame moving with constant velocity with respect to K.

The Attempt at a Solution


My idea was to consider K', an inertial reference frame that would move alongside the conducting sphere. From there, calculate the E' and B' fields "seen" by the sphere. From there, calculate the induced surface charge density ##\sigma '##. And from there simply convert using the fact that ##\sigma = \gamma \sigma '##.
So here I go:
Using the formulae for fields transformations, ##\vec E'=\frac{\gamma v}{c}\hat z## and ##\vec B'=\gamma B \hat y##. Thus for the reference frame K', there's a static EM field. Now the sphere is a perfect conductor so the E' field inside of it must vanish. So that there's a discontinuity in the E' field that is proportional to the surface charge density sigma'. Mathematically, ##\hat n \cdot (\vec E' - \vec E'_{\text{inside}})=\sigma ' /\varepsilon _0##. Where ##\hat n = \hat r'## and as I said, ##\vec E'_{\text{inside}}=\vec 0##.
Furthermore, ##\hat z' \cdot \hat r' = \cos \theta '##.
Therefore ##\sigma '(\theta ') = \varepsilon_0 \frac{\gamma v}{c}\cos (\theta ')##. Now ##\sigma = \varepsilon_0 \frac{\gamma ^2 v}{c}\cos (\theta ')## but I must transform back ##\theta '## into non primed coordinates. I won't do it though, because this answer is completely wrong according to my professors and I don't deserve any credit.
Instead, according to them, what I should have done is to calculate the electric field generated by the surface charge density. The total electric field seen in K' will be the sum of the field I had calculated plus the field due to this charge density.

That's basically what I have been told. But then what? I wasn't asked to calculate the fields... I was asked the charge density. So if I understand them well, I must calculate this new E' field, and from it recalculate the new charge density? This doesn't make any sense to me, I could do this process forever, i.e. calculate the E field generated by a charge density, then calculate the new charge density, then calculate the new E field, then calculate the new charge density, etc. So why should I stop at step 1 or 2? Is it because they asked "to 1st order in v/c" in the problem statement?
 
Physics news on Phys.org
  • #2
You can solve the problem exactly for a constant external field at infinity and a fixed potential on the sphere. From there you can deduce the charge.

Since you are only looking at leading order terms in v/c, you may ignore any gamma factors. However, note that when you cannot, surface charge densities are not related in the same way as volume charge densities, but also depend on the orientation of the surface.
 
  • Like
Likes fluidistic
  • #3
Orodruin said:
You can solve the problem exactly for a constant external field at infinity and a fixed potential on the sphere. From there you can deduce the charge.

Since you are only looking at leading order terms in v/c, you may ignore any gamma factors. However, note that when you cannot, surface charge densities are not related in the same way as volume charge densities, but also depend on the orientation of the surface.
Thank you very much for the explanation/clarification. I'll keep using gamma up until the very end then.
So I solved for the potential outiside of the sphere, considering azimuthal symmetry (so ##\Phi = \Phi (r, \theta)## and doesn't depend on phi, the azimuthal angle). I solved Laplace equation ##\nabla ^2 \Phi =0## in spherical coordinates. I applied 2 boundary conditions, namely that ##\Phi (r=R, \theta ) =V_0## and ##\Phi (r \to \infty , \theta )=-r \gamma \frac{v}{c} \cos \theta##.
So that the general form for the potential ##\Phi (r, \theta )=\sum _{l=1}^\infty (A_l r^l +B_l r^{-l-1})P_l (\cos \theta)## becomes ##\Phi (r,\theta)=\underbrace{-\frac{\gamma v}{c}r \cos \theta }_{A_1rP_1}+\underbrace{\frac{RV_0}{r}}_{B_0P_0/r} + \underbrace{\frac{\gamma vR^3}{cr^2}}_{B_1P_1/r^2}##.
Now I don't really know how to get the surface charge density from it. Some books give the formula ##-\sigma /\varepsilon_0 =\frac{\partial \Phi}{\partial r} \big | _{r=R}##. If so, then I'd get ##\sigma(\theta )=\frac{3\gamma v}{c} \varepsilon _0 \cos \theta + \frac{V_0 \varepsilon _0}{R}## However I don't trust that formula, because I don't see what's wrong with the following:
Matching condition ##\hat n \cdot \vec E=4\pi \sigma(=\sigma /\varepsilon _0)=E## where ##\vec E = - \nabla \Phi##. But if I take the gradient in spherical coordinates, I get a much more complicated relationship between sigma and Phi than the one given in Griffiths for example (the one I posted above).
Therefore I'm not sure which way is correct from there.
 
  • #4
fluidistic said:
I applied 2 boundary conditions, namely that ##\Phi (r=R, \theta ) =V_0## and ##\Phi (r \to \infty , \theta )=-r \gamma \frac{v}{c} \cos \theta##.
So that the general form for the potential ##\Phi (r, \theta )=\sum _{l=1}^\infty (A_l r^l +B_l r^{-l-1})P_l (\cos \theta)## becomes ##\Phi (r,\theta)=\underbrace{-\frac{\gamma v}{c}r \cos \theta }_{A_1rP_1}+\underbrace{\frac{RV_0}{r}}_{B_0P_0/r} + \underbrace{\frac{\gamma vR^3}{cr^2}}_{B_1P_1/r^2}##.
Shouldn't the magnetic field B be a part of your expressions for ##\Phi##?
The last term of your equation for ##\Phi (r,\theta)## is missing the appropriate Legendre polynomial factor.

Now I don't really know how to get the surface charge density from it. Some books give the formula ##-\sigma /\varepsilon_0 =\frac{\partial \Phi}{\partial r} \big | _{r=R}##. If so, then I'd get ##\sigma(\theta )=\frac{3\gamma v}{c} \varepsilon _0 \cos \theta + \frac{V_0 \varepsilon _0}{R}##
OK. You should be able to determine the value of ##V_0## by thinking about what the total induced charge must be.

However I don't trust that formula, because I don't see what's wrong with the following:
Matching condition ##\hat n \cdot \vec E=4\pi \sigma(=\sigma /\varepsilon _0)=E## where ##\vec E = - \nabla \Phi##. But if I take the gradient in spherical coordinates, I get a much more complicated relationship between sigma and Phi than the one given in Griffiths for example (the one I posted above).
Therefore I'm not sure which way is correct from there.

You should get the same result this way. Remember that you are evaluating the gradient at the surface of the sphere where ##r=R##.
 
  • Like
Likes fluidistic
  • #5
TSny said:
Shouldn't the magnetic field B be a part of your expressions for ##\Phi##?
Hmm I don't think so. Do you mean that the B field has an effect on the charge distribution?
The last term of your equation for ##\Phi (r,\theta)## is missing the appropriate Legendre polynomial factor.
Indeed, I made a typo there; on my draft I have the cos theta term.
OK. You should be able to determine the value of ##V_0## by thinking about what the total induced charge must be.
You should get the same result this way. Remember that you are evaluating the gradient at the surface of the sphere where ##r=R##.
The total induced charge must be 0 right? So that the integral of the surface charge density over all theta should be 0. Correct?
And ok, thank you very much for the comment about the gradient and that both formula should yield the same result.
 
  • #6
fluidistic said:
Hmm I don't think so. Do you mean that the B field has an effect on the charge distribution?
In the frame of reference of the sphere, there is an electric field E' which is proportional to B. So, the induced charge should depend on the magnitude of B. Note that your expressions for ##\Phi## do not have the correct dimensions for electric potential.

The total induced charge must be 0 right? So that the integral of the surface charge density over all theta should be 0. Correct?
Yes
 
  • Like
Likes fluidistic
  • #7
TSny said:
In the frame of reference of the sphere, there is an electric field E' which is proportional to B. So, the induced charge should depend on the magnitude of B. Note that your expressions for ##\Phi## do not have the correct dimensions for electric potential.Yes
Oops right, I made a mistake there...
I get [tex]\Phi (r, \theta) =-\frac{\gamma vB}{c}r\cos \theta + \frac{RV_0}{r} +\frac{\gamma v B R^3}{cr^2}\cos \theta[/tex]
If I use a unit system such that ##4\pi \sigma (\theta ) = - \frac{\partial \Phi}{\partial r} \big | _{r=R}##, then I get that ##\sigma (\theta )= \frac{3\gamma vB \cos \theta}{4\pi c}+\frac{V_0}{4\pi R}##.
I am unsure about how to integrate sigma over all angles. Is it just ##\int_0^\pi \sigma (\theta ) d\theta =0##? If so, then I get ##V_0=0##.
But maybe it's ##\int_0^\pi \sigma (\theta ) \sin \theta d\theta =0##? I am really not sure.
 
  • #8
##\sigma## is charge per unit area. So the amount of charge in a patch of area ##dA## of the spherical surface is ##dq = \sigma dA##.
 
  • Like
Likes fluidistic
  • #9
TSny said:
##\sigma## is charge per unit area. So the amount of charge in a patch of area ##dA## of the spherical surface is ##dq = \sigma dA##.
I see. Then I'm probably doing some mistake. If ##dA=R^2 \sin \theta d\theta d\phi##, I get ##V_0=0##.
 
  • #10
fluidistic said:
I see. Then I'm probably doing some mistake. If ##dA=R^2 \sin \theta d\theta d\phi##, I get ##V_0=0##.
Why do you think that answer is wrong?
 
  • #11
I think I see what might be causing confusion. In your summation over ##l## in the expression for ##\Phi(r, \theta)##, the sum should start at ##l = 0##. So, there is an additional ##A_0## term that you left out.

[EDIT: So, you cannot assume that ##B_0 = RV_0##].
 
Last edited:
  • #12
TSny said:
Why do you think that answer is wrong?
I thought that this would have caused problem if I had assumed that ##V_0=0## when I applied the boundary conditions but that would have been fine I guess, so ok, I accept this as answer.
So overall I get a charge density 3 times greater than what I did in my original attempt. I get that ##\sigma ' (\theta ')=\frac{3\gamma vB \cos \theta}{4\pi c}##. Where the primes mean as seen from the system K'. Now I need to transform this for K. I can write ##z'=r' \cos \theta '##. So that ##\cos \theta '=z'/r' =z/r'=\frac{z}{\sqrt{x'^2+y^2+z^2}} = \frac{z}{\sqrt{\gamma ^2 (x-vt)^2 +y^2 +z^2}}##.
Thus [tex]\sigma (x,y,z)=\frac{3\gamma vBz}{4\pi c \sqrt{\gamma^2 (x-vt)^2 +y^2+z^2}}[/tex]. From here I could approximate gamma by something with v/c (I haven't seen the approximation yet).
Is this correct?
 
  • #13
TSny said:
I think I see what might be causing confusion. In your summation over ##l## in the expression for ##\Phi(r, \theta)##, the sum should start at ##l = 0##. So, there is an additional ##A_0## term that you left out.

[EDIT: So, you cannot assume that ##B_0 = RV_0##].
Hmm but from ##\Phi (r \to \infty, \theta)=-r \cos \theta \frac{\gamma vB}{c}## this seems to imply that ##A_0=0## to me.
 
  • #14
For ##r \gg R##, ##\Phi \rightarrow -E' r \cos \theta +C##
where ##C## is a constant to be determined. For general boundary conditions you cannot assume ##C = 0##.

[EDIT: You should be able to show that ##C=0## only when ##V_0 = \frac{Q}{4 \pi \epsilon_0 R}##, where ##Q## is the net charge of the sphere.]
 
Last edited:
  • Like
Likes fluidistic
  • #15
fluidistic said:
So overall I get a charge density 3 times greater than what I did in my original attempt. I get that ##\sigma ' (\theta ')=\frac{3\gamma vB \cos \theta}{4\pi c}##. Where the primes mean as seen from the system K'. Now I need to transform this for K. I can write ##z'=r' \cos \theta '##. So that ##\cos \theta '=z'/r' =z/r'=\frac{z}{\sqrt{x'^2+y^2+z^2}} = \frac{z}{\sqrt{\gamma ^2 (x-vt)^2 +y^2 +z^2}}##.
Thus [tex]\sigma (x,y,z)=\frac{3\gamma vBz}{4\pi c \sqrt{\gamma^2 (x-vt)^2 +y^2+z^2}}[/tex]. From here I could approximate gamma by something with v/c (I haven't seen the approximation yet).
Is this correct?
I suspect that you are just supposed to describe how the charge is distributed over the sphere in the K frame. I don't think you need to express ##\sigma## as a function of ##x, y, z, t## in the K frame. Just express ##\sigma## as a function of spherical coordinates ##\theta, \phi## on the sphere from the point of view of the K frame.

Since you are only required to express the answer to first order in ##v/c##, you don't need to worry about effects of the Lorentz transformation from the K' frame back to the K frame. In the K' frame, you found that ##\sigma## is already proportional to ##v/c##. Any relativistic effects of transforming back to the K frame from the K' frame would just introduce higher order terms in ##v/c##.

So, unless I'm overlooking something, I think you are done. :smile:

But this exercise is showing how relativity provides a nice way to solve the problem by going to the frame of reference of the moving sphere and using the fact that in this frame there will be a uniform E' field that induces the charge distribution on the sphere. If you stayed in the K frame, you would have to try to find the induced charge distribution by finding a distribution of charge where the magnetic force on the (moving) charge distribution is balanced by the electric force due to the electric field produced by the induced charge. (Yuck!)
 
  • Like
Likes fluidistic
  • #16
Thanks for all the comments.
TSny said:
I suspect that you are just supposed to describe how the charge is distributed over the sphere in the K frame. I don't think you need to express ##\sigma## as a function of ##x, y, z, t## in the K frame. Just express ##\sigma## as a function of spherical coordinates ##\theta, \phi## on the sphere from the point of view of the K frame.
Hmm I really don't see how to do this. I don't see how to avoid the r dependency either.
 
  • #17
Let the center of the sphere in the K frame be at the origin of coordinates at t = 0. At this instant of time, you can use spherical coordinates to describe the charge distribution. I would think that's all that is asked for. The distribution of charge over the surface of the sphere does not change with time. You could go further and write the distribution as a function of x, y, z, and t for any time t, as you essentially did. But you would need to restrict the values of x, y, and z so that the point (x,y,z) lies on the surface of the sphere at time t. But I don't see the point of doing all that.

Note that to first order in v/c, ##\gamma## can be approximated by 1: ##\frac{1}{\sqrt{1-v^2/c^2}} \approx 1 + \frac{v^2}{2c^2}##.
So you can set all gamma factors to 1 as pointed out by Orodruin in post #2.

I don't know how your professor wanted you to approach the problem.
 
  • Like
Likes fluidistic
  • #18
TSny said:
Let the center of the sphere in the K frame be at the origin of coordinates at t = 0. At this instant of time, you can use spherical coordinates to describe the charge distribution. I would think that's all that is asked for. The distribution of charge over the surface of the sphere does not change with time. You could go further and write the distribution as a function of x, y, z, and t for any time t, as you essentially did. But you would need to restrict the values of x, y, and z so that the point (x,y,z) lies on the surface of the sphere at time t. But I don't see the point of doing all that.

Note that to first order in v/c, ##\gamma## can be approximated by 1: ##\frac{1}{\sqrt{1-v^2/c^2}} \approx 1 + \frac{v^2}{2c^2}##.
So you can set all gamma factors to 1 as pointed out by Orodruin in post #2.

I don't know how your professor wanted you to approach the problem.
Ok thank you very much for everything. So I'd give as answer ##\sigma (\theta) =\frac{3vB \cos \theta}{4\pi c }## neglecting the fact that the sphere doesn't appear spherical. Yeah I don't know either what my professor was expecting from me. Next time I'll ask him if I have doubts on what he's expecting.

Edit: In post #15 you wrote sigma in terms of theta and phi, what did you have in mind about phi?
 
  • #19
fluidistic said:
Edit: In post #15 you wrote sigma in terms of theta and phi, what did you have in mind about phi?
Sorry, I didn't mean to imply that there would be phi dependence. Sigma will just depend on theta, at least to order v/c.
 
  • Like
Likes fluidistic

What is a moving sphere in a magnetic field?

A moving sphere in a magnetic field refers to a situation where a spherical object is placed within a magnetic field and experiences a force due to the interaction between the magnetic field and the object's magnetic properties.

What is the equation for the force exerted on a moving sphere in a magnetic field?

The force exerted on a moving sphere in a magnetic field can be calculated using the equation F = qv x B, where F is the force, q is the charge of the object, v is its velocity, and B is the strength of the magnetic field.

How does the direction of the force on a moving sphere in a magnetic field depend on the direction of motion?

The direction of the force exerted on a moving sphere in a magnetic field is perpendicular to both the direction of the object's motion and the direction of the magnetic field. This is known as the right-hand rule.

What are some real-life applications of a moving sphere in a magnetic field?

A moving sphere in a magnetic field has various applications, including in electric motors, generators, and magnetic levitation systems. It can also be used to study the properties of materials and to measure the strength of magnetic fields.

What factors can affect the force on a moving sphere in a magnetic field?

The force on a moving sphere in a magnetic field can be affected by factors such as the strength of the magnetic field, the velocity and charge of the object, and the angle between the direction of motion and the direction of the magnetic field.

Similar threads

  • Advanced Physics Homework Help
Replies
3
Views
863
  • Advanced Physics Homework Help
Replies
1
Views
423
  • Advanced Physics Homework Help
Replies
5
Views
1K
Replies
1
Views
376
  • Advanced Physics Homework Help
Replies
2
Views
909
  • Advanced Physics Homework Help
Replies
2
Views
1K
  • Advanced Physics Homework Help
Replies
13
Views
2K
Replies
2
Views
717
  • Advanced Physics Homework Help
Replies
1
Views
589
  • Advanced Physics Homework Help
Replies
1
Views
2K
Back
Top