- #141
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##B=H## holds in vacuo, where ##M=0## (in Gaussian or Heaviside-Lorentz units). What else should be ##M## without matter present?
The magnetic-pole model works, because it's equivalent to assuming the current density to be ##\propto \vec{\nabla} \times \vec{M}##, including possible surface-current densities like in my example of the homogeneously magnetized sphere, which is the most simple example due to symmetry.
In SI units the constitutive equation is ##\vec{B}=\mu_0 (\vec{H}+\vec{M})##. I also mess up where the ##\epsilon_0## and ##\mu_0## should go. The mnemonics is that the material sources like magnetization belong to ##\vec{H}## and then you need ##\mu_0## to get ##\vec{B}## dimensionally correct ;-). By definition of the SI units the macroscopic Maxwell equations read
$$\vec{\nabla} \cdot \vec{B}=0, \quad \vec{\nabla} \times \vec{E}+\partial_t \vec{B}=0$$
and
$$\vec{\nabla} \times \vec{H} -\partial_t \vec{D}=\vec{j}, \quad \vec{\nabla} \cdot \vec{D}=\rho,$$
with ##\rho## and ##\vec{j}## the "free charges and currents", including polarization charge densities ##\rho_{\text{pol}}=\vec{\nabla} \cdot \vec{P}## and magnetization currents ##\vec{j}_{\text{mag}}=\vec{\nabla} \times \vec{M}## with possible surface-charge densities and surface-current densities at boundaries between different media (or a medium and vacuum).
The magnetic-pole model works, because it's equivalent to assuming the current density to be ##\propto \vec{\nabla} \times \vec{M}##, including possible surface-current densities like in my example of the homogeneously magnetized sphere, which is the most simple example due to symmetry.
In SI units the constitutive equation is ##\vec{B}=\mu_0 (\vec{H}+\vec{M})##. I also mess up where the ##\epsilon_0## and ##\mu_0## should go. The mnemonics is that the material sources like magnetization belong to ##\vec{H}## and then you need ##\mu_0## to get ##\vec{B}## dimensionally correct ;-). By definition of the SI units the macroscopic Maxwell equations read
$$\vec{\nabla} \cdot \vec{B}=0, \quad \vec{\nabla} \times \vec{E}+\partial_t \vec{B}=0$$
and
$$\vec{\nabla} \times \vec{H} -\partial_t \vec{D}=\vec{j}, \quad \vec{\nabla} \cdot \vec{D}=\rho,$$
with ##\rho## and ##\vec{j}## the "free charges and currents", including polarization charge densities ##\rho_{\text{pol}}=\vec{\nabla} \cdot \vec{P}## and magnetization currents ##\vec{j}_{\text{mag}}=\vec{\nabla} \times \vec{M}## with possible surface-charge densities and surface-current densities at boundaries between different media (or a medium and vacuum).
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