The Curl of Magnetic Potential

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Homework Help Overview

The discussion revolves around the mathematical operation of taking the curl of a magnetic potential, specifically A(r) = (u/4π)(m × R/r^3), where u is the permeability of free space, m is the magnetic dipole moment, R is the position vector, and r is the distance from the magnetic field. Participants are exploring the derivation of the resulting expression after applying the curl operation.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss different methods for calculating the curl, including using Cartesian components and spherical coordinates. There are questions about the appropriateness of using all three partial derivatives in the del operator and the application of vector identities.

Discussion Status

Some participants have offered guidance on using vector identities and have suggested methods for approaching the problem. There is an acknowledgment of the need to clarify calculations and identities used in the derivation process. Multiple interpretations of the problem-solving approach are being explored.

Contextual Notes

Participants express uncertainty regarding the use of spherical versus Cartesian coordinates and the implications of using different mathematical identities. There is a mention of homework rules that restrict providing direct solutions, emphasizing a collaborative effort to understand the problem better.

quantumfoam
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Hi guys! I recently saw on Wiki that given a magnetic potential A(r)=(u/4π)(mXR/r^3) ,( where u is the permeability of free space, m is the magnetic dipole moment of a magnetic field, R is the position vector, and r is the distance from the magnetic field ) upon taking the curl of the magnetic potential A(r), one obtains (u/4π)([3(m•r)R/r^5]-[m/r^3]). Can someone show me how they ended up with this result? I would like a step by step process please.(: the wiki article is called Magnetic Moment under the section called Effects of an External Magnetic Field on a Magnetic Moment.
 
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quantumfoam said:
Hi guys! I recently saw on Wiki that given a magnetic potential A(r)=(u/4π)(mXR/r^3) ,( where u is the permeability of free space, m is the magnetic dipole moment of a magnetic field, R is the position vector, and r is the distance from the magnetic field ) upon taking the curl of the magnetic potential A(r), one obtains (u/4π)([3(m•r)R/r^5]-[m/r^3]). Can someone show me how they ended up with this result?

I would like a step by step process please.(: the wiki article is called Magnetic Moment under the section called Effects of an External Magnetic Field on a Magnetic Moment.
That's not how we do things in the Homework section of PF. We're not even allowed to give such help. But we can try to help you work your way through such a problem.

One way to get the result, is to write A(r) in terms of it's Cartesian components, then take the curl. I suppose you could also take the curl directly in spherical coordinates.
 
I'm sorry! Well I thought about doing it in spherical coordinates but I was not sure if I should use the whole three partials in the del operator.
 
quantumfoam said:
I'm sorry! Well I thought about doing it in spherical coordinates but I was not sure if I should use the whole three partials in the del operator.
Yes, use all three partials.
 
quantumfoam said:
I'm sorry! Well I thought about doing it in spherical coordinates but I was not sure if I should use the whole three partials in the del operator.

I don't think there is any advantage is using spherical coordinates. Try using the identity:

\nabla \times (a \times b)=(b \cdot \nabla) a-b(\nabla \cdot a)<br /> -(a \cdot \nabla) b+a(\nabla \cdot b)<br />

If you set a to be m and b to be ##\frac{\vec r}{r^3}##, the first two terms vanish because m is a constant. The last one vanishes because ##\frac{\vec r}{r^3}## is divergence free. So you only have to puzzle out what the third term means.
 
Thank you very much! (:
 
Is there any other identity I could use for (a(div))b? I did the calculation but I think I did it wrong. I'm missing the second term in the curl of the magnetic potential. The (m/r^3) term
 
quantumfoam said:
Is there any other identity I could use for (a(div))b? I did the calculation but I think I did it wrong. I'm missing the second term in the curl of the magnetic potential. The (m/r^3) term

Show what you did. You'll need to use the quotient rule on the dervivatives ##\frac{\vec r}{r^3}##.
 
Well, at first I used the identity (a(div))b= (div(a))b-b(div(a)). Was that a correct move?
 
  • #10
Oh! I get it! Nevermind! I didn't think to carry out the quotient rule. That makes a lot more sense! Thank you!
 
  • #11
So I should calculate using the radial term of the spherical version of the del operator?
 
  • #12
That's the only way I see to take the derivative of R/r^3.
 
  • #13
quantumfoam said:
That's the only way I see to take the derivative of R/r^3.

R/r^3 is just (x,y,z)/(x^2+y^2+z^2)^(3/2). It worked out pretty ok for me in cartesian coordinates.
 
  • #14
Would it be a little easier with spherical coordinates?
 
  • #15
quantumfoam said:
Would it be a little easier with spherical coordinates?

Maybe. I didn't try it that way. I just know it's not hard in cartesian.
 
  • #16
I will try it! Thank you!
 

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