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Bound Current Density and the Vector Magnetic Field Created by a Magnetized Object 📂Electrodynamics

Bound Current Density and the Vector Magnetic Field Created by a Magnetized Object

Explanation1

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Suppose there is an object magnetized by an external magnetic field. This object will have a magnetization density M\mathbf{M}, and this magnetization density will generate a new magnetic field. The vector potential created by a magnetic dipole is as follows.

A(r)=μ04πm×2 \mathbf{A} (\mathbf{r}) = \dfrac{\mu_{0}}{4\pi}\dfrac{\mathbf{m} \times \crH }{\cR ^2}

Since magnetization density is the dipole moment per unit volume, M=mdτ\mathbf{M}=\dfrac{\mathbf{m}}{d\tau}. By substituting this into the above equation and integrating over the entire volume, the vector potential created by the magnetized object is as follows.

A(r)=μ04πM(r)×2dτ \mathbf{A} (\mathbf{r}) = \dfrac{\mu_{0}}{4\pi} \int\dfrac{ \mathbf{M}(\mathbf{r}^{\prime}) \times \crH }{\cR ^2} d \tau^{\prime}

Given that the gradient of the separation vector is 1=2\nabla^{\prime} \dfrac{1}{\cR} = \dfrac{\crH}{\cR^2},

A(r)=μ04πM(r)×1dτ \mathbf{A} (\mathbf{r}) = \dfrac{\mu_{0}}{4\pi} \int \mathbf{M}(\mathbf{r}^{\prime}) \times \nabla^{\prime}\dfrac{1}{\cR} d \tau^{\prime}

The product rule involving the del operator

×(fA)=(f)×A+f(×A)    A×(f)=f(×A)×(fA) \nabla \times (f \mathbf{A})=(\nabla f)\times \mathbf{A} + f(\nabla \times A) \implies \mathbf{A} \times (\nabla f) = f(\nabla \times \mathbf{A}) -\nabla \times ( f\mathbf{A})

Applying the product rule to the cross product within the integral gives the following.

A(r)=μ04π[1[×M(r)]dτ×M(r)dτ] \mathbf{A} (\mathbf{r}) = \dfrac{\mu_{0}}{4\pi} \left[ \int \frac{1}{\cR}\left[\nabla^{\prime} \times \mathbf{M} (\mathbf{r}^{\prime}) \right] d \tau^{\prime} - \int \nabla^{\prime} \times \dfrac{\mathbf{M}(\mathbf{r^{\prime}})}{\cR}d \tau^{\prime}\right]

Here, Gauss’s theorem is used to swap the second term.

Gauss’s theorem (Divergence theorem)

VFdV=SFdS \int_\mathcal{V} \nabla \cdot \mathbf{ F} dV = \oint _\mathcal{S} \mathbf{F} \cdot d \mathbf{S}

Then the equation becomes as below.

A(r)=μ04π[1[×M(r)]dτ+M(r)×da] \mathbf{A} (\mathbf{r}) = \dfrac{\mu_{0}}{4\pi} \left[ \int \frac{1}{\cR} \left[\nabla^{\prime} \times \mathbf{M} (\mathbf{r}^{\prime}) \right] d \tau^{\prime} + \oint \dfrac{\mathbf{M}(\mathbf{r^{\prime}})}{\cR} \times d \mathbf{a}^{\prime}\right]

Here, the first term can be considered as the potential created by volume current density Jb\mathbf{J}_{b}. The subscript bb stands for bound.

Jb=×M \mathbf{J}_{b}=\nabla \times \mathbf{M}

The second term can be seen as the potential created by surface current density Kb\mathbf{K}_{b}.

Kb=M×n^ \mathbf{K}_{b}=\mathbf{M} \times \hat{\mathbf{n}}

Here, n^\hat{\mathbf{n}} is the unit normal vector perpendicular to each surface. Now, representing the vector potential in terms of bound current density, we get the following.

A(r)=μ04πVJb(r)dτ+μ04πSKb(r)da \mathbf{A} (\mathbf{r})=\dfrac{\mu_{0}}{4\pi} \int_\mathcal{V} \dfrac{\mathbf{J}_{b}(\mathbf{r}^{\prime})}{\cR}d\tau^{\prime}+\dfrac{\mu_{0}}{4\pi}\oint_\mathcal{S}\dfrac{\mathbf{K}_{b} (\mathbf{r}^{\prime})}{\cR}da^{\prime}

Therefore, the vector potential created by the magnetized object is the same as the potential created by the object’s internal volume current density Jb=×M\mathbf{J}_{b}=\nabla \times \mathbf{M} and the surface current density Kb=M×n^\mathbf{K}_{b}=\mathbf{M} \times \hat{\mathbf{n}} on its surface. This is analogous to defining the bound charges ρb\rho_{b} and σb\sigma_{b} and the potential created by a polarized object.


  1. David J. Griffiths, 기초전자기학(Introduction to Electrodynamics, 김진승 역) (4th Edition1 2014), p293-294 ↩︎