Magnetic Force of Attraction Between Spinning Charged Shells

Click For Summary
SUMMARY

The discussion focuses on calculating the magnetic force of attraction between the northern and southern hemispheres of a spinning charged spherical shell, referencing Griffiths' textbook for guidance. Participants suggest using the uniform B-field inside the sphere and applying the Lorentz force law to find the force on each hemisphere. Key steps include determining the fields, calculating the force on differential area elements, and integrating the vertical components of these forces. The conclusion emphasizes that while the net force on the sphere is zero, the hemispheres exert compressive forces toward each other.

PREREQUISITES
  • Understanding of Griffiths' "Introduction to Electrodynamics" (specifically pages 211-212 and section 2.5.3)
  • Familiarity with the Lorentz force law and magnetic fields
  • Knowledge of surface currents and their effects on magnetic fields
  • Basic integration techniques for calculating forces in physics
NEXT STEPS
  • Review Griffiths' "Introduction to Electrodynamics" for detailed explanations on surface currents and magnetic fields
  • Study the derivation of the B-field for a uniformly charged spinning sphere
  • Learn about the application of boundary conditions in electromagnetism
  • Practice problems involving the integration of forces in electromagnetic contexts
USEFUL FOR

Physics students, educators, and researchers interested in electromagnetism, particularly those tackling advanced problems involving magnetic forces and charged rotating bodies.

ehrenfest
Messages
2,001
Reaction score
1

Homework Statement



Calculate the magnetic force of attraction between the northern and southern hemispheres of a spinning charged spherical shell. (ex. 5.11)

Homework Equations


The Attempt at a Solution



I already looked at this https://www.physicsforums.com/showthread.php?t=42020.

I am stuck figuring out how to proceed. Should I calculate the B-field due to one hemisphere and then integrate over the Lorentz force on the other? Calculating he- B-field due to one hemisphere does not seem fun...
 
Last edited:
Physics news on Phys.org
anyone?
 
Hmm...I'm too lazy to look at Griffiths right now, but here's one approach: consider each hemisphere to be a series of circular current loops. Do you have an expression for the force between two parallel, co-axial current loops? If so, then integrate that over both hemispheres.
 
Actually, that's probably a rather complicated method.

You don't want to look at the B field of each hemisphere separately; you actually want the B field of the entire sphere, because each individual hemisphere exerts a self-force as well.

You should know, from some other formulas in Griffiths, that the B field on the interior of the spinning, charged sphere is uniform, right? It seems to me that you should be able to simply use this uniform field and apply the Lorentz force law.
 
Ben Niehoff said:
You don't want to look at the B field of each hemisphere separately; you actually want the B field of the entire sphere, because each individual hemisphere exerts a self-force as well.

But I thought that is exactly why we should look at each hemisphere individually--we don't want to include the "self-force" in our answer!
 
OK, it was bothering me that I couldn't immediately see how to do this problem, so I dug out Griffiths and looked at it. Here is how to find the solution:

First, read pages 211-212 about surface currents. Note that B is discontinuous at a surface current, and in order to find the force, you must average B_above and B_below. This is what I suspected, but I couldn't figure out why. Luckily, Griffiths points out why: go back and read section 2.5.3 (page 102), and he explains the argument for electric forces on surface charges.

Now, go back to the problem. You have a spinning, charged sphere. Therefore, it experiences both electric and magnetic forces. He asks for the "magnetic force of attraction", so maybe he wants you to ignore the electric force of repulsion; I'm not sure. Anyway, you can use a similar technique to calculate them both:

To find the force on the sphere, you follow these three steps:

1. Find the fields everywhere.
2. Find the force on a differential area element due to the total field.
3. Take only the vertical component of this force, and integrate over each hemisphere separately to get the (opposite and equal) forces on each.

Step 1 is easy: You know that B field is uniform on the interior of the sphere. There is probably a formula somewhere for it; I haven't dug around enough to find it. You don't actually need to calculate the external field, because you can use the boundary conditions for B to find the field immediately outside the sphere, which is all you really need.

For Step 2, apply the boundary conditions to get the field immediately outside the sphere, and average that with the field immediately inside. Now you know that

d{\vec F} = \vec K \times \vec B_{avg} da

For Step 3, simply take the Z component of the above, and integrate over the northern hemisphere. By symmetry, you know the integral over the southern hemisphere is equal and opposite.

Overall, the net force over the entire sphere is zero (after all, how could the sphere push itself in any particular direction?), but the top and bottom of the sphere do compress toward each other, and hopefully you should arrive at the formula given by Griffiths as the answer.
 
Last edited:

Similar threads

  • · Replies 2 ·
Replies
2
Views
4K
Replies
6
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
12
Views
2K
  • · Replies 2 ·
Replies
2
Views
1K
Replies
1
Views
2K
Replies
7
Views
2K
  • · Replies 1 ·
Replies
1
Views
4K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 3 ·
Replies
3
Views
1K