\(\)
When discussing dielectrics we learned
Electric fields can induce electric dipoles in materials. When the molecules or atoms themselves are permanent electric dipoles, an external electric field will try to align them. The degree of success depends entirely on how strong the external electric field is, and on the temperature. If the temperature is low, there is very little thermal agitation, making it easier to align those dipoles.
We have a similar situation with magnetic fields. An external magnetic field can induce magnetic dipoles in materials. It induces magnetic dipoles at the atomic scale. When the atoms/molecules themselves have a permanent magnetic dipole moment, the external field will try to align these dipoles. Again, the degree of success depends on the strength of the external field, and again on the temperature. The lower the temperature, the easier it is to align them.
So the material modifies the external field. We often call this external field, the vacuum field. When you bring material into a vacuum field, the field changes. The field inside is different from the external field.
Magnetic dipole moment
If we have a current in a loop, and the current is running clockwise as seen from below, and the area is \(A\), then the magnetic dipole moment \(\vec\mu\) $$ \vec \mu = I\,\vec A \tag{dipole moment} \label{eq:dipolemoment} $$
We define \(\vec A\) according to the righthand corkscrew rule. If we come from below clockwise, then the \(\vec A\) is perpendicular to the surface. So the magnetic dipole moment \(\vec\mu\), is also pointing upwards.
If we have \(N\) of these loops, then the magnetic dipole moment will be \(N\) times larger.
Diamagnetism
When you expose any material to a permanent external magnetic field, it will to some degree, oppose that external field. On an atomic scale, the material will generate an EMF that opposes the external field. This has nothing to do with Lenz law. It has nothing to do with the free electrons in conductors which produce an eddy current in a changing magnetic field.
In other words: when we apply a permanent magnetic field, to any material, a magnetic dipole moment is induced to oppose that field. This can only be understood with quantum mechanics. Here, we’ll make no attempt to explain it, but we will accept it.
The magnetic field inside the material, is always a little bit smaller than then external field, because the dipoles oppose the external field.
Paramagnetism
There are many substances where the atoms/molecules themselves have magnetic dipole moments. You can think of them as being little magnets. If you have no external field, then these dipoles are completely chaotically oriented. So the net magnetic field is zero. They are not permanent magnets.
If you bring a paramagnetic material in a magnetic field, its atomic magnetic dipoles will move their north poles a little bit in the direction of the external magnetic field. They align a little with the external field. The degree of success depends on the strength of that field and the temperature. The lower the temperature, the easier it is. If you remove the external field, immediately there is complete, total chaos. There is no permanent magnetism left.
In nonuniform field
If you bring a paramagnetic material in a nonuniform magnetic field, it will be pulled towards the strong side of that field. Suppose we have a magnet, and we bring paramagnetic material in its field. Let’s consider just one atom of the material.
The atoms magnetic dipole moment would like to align in the direction to support the field. So if we look from above, the current in this atom/molecule runs clockwise direction. That would be the ideal alignment. This current loop will be attracted to the magnet. Let’s look at a point on the left. At that point, the current goes into the screen, and the magnetic field goes diagonal.
The Lorenz force will be in the direction \(\vec I\times\vec B\), and put it up towards the left. At a point on the right, the force will be to the right. So everywhere around this loop, there is a force that is pointing diagonally outwards up. Clearly, there is a net force up. The matter wants to go towards the magnet.
Essential is that the external magnetic field is nonuniform. (In diamagnetic material, the current would be running in the opposite direction, because it opposes the external field.)
The exception
Diamagnetic materials are always pushed towards the weak part of the field. Paramagnetic and ferromagnetic materials that experience a force towards the strong part of the field, if the field itself is nonuniform.
There is one interesting exception. Oxygen at one atmosphere and 300 °K, has a \(\chi_m\) of \(2\times10^{6}\). But liquid oxygen at 90 °K, the \(\chi_m\) is 1,800 times larger. Why?
Liquid, in general, is about thousand times denser than gas at one atmosphere. So you have a thousand times more dipoles per cubic meter that, in principle, can align. So you expect a 1:1 correspondence between the density, and the value of \(\chi_m\). Indeed, you see that this value is substantially larger. It is more than a factor 1000 larger is that the temperature is also lower. That gives us another factor of two.
Even though the value of \(\chi_m\) is extraordinarily high for a paramagnetic material, notice that the field inside would only be 0.35% higher than the vacuum field. But that is enough for liquid oxygen to be attracted by a very strong magnet, provided that it has a very nonuniform field outside the magnet. So the force with which liquid oxygen is pulled towards a magnet can be made larger than the weight of the liquid oxygen.
Ferromagnetism
Again the atoms have permanent magnetic dipole moments. But this time, for reasons which can only be understood with quantum mechanics, there are domains the size of about \(0.1\) to \(0.3\,\rm{mm}\).
Domains
In the domains, the dipoles are all aligned. The number of atoms involved in such a domain is typically \(10^{17}\ldots10^{21}\) atoms. The domains are uniformly distributed throughout the ferromagnetic material. So there may not be any net magnetic field.
When we apply an external field, these domains will be forced to align themselves with the magnetic field. The domains a a whole can flip. The degree of success depends on the strength of the field and the temperature. The lower the temperature, the better, because there is less thermal agitation with adds a certain randomness to the process. Inside the ferromagnetic material, the magnetic field can thousands of times stronger than the external field..
If we remove the external field, some of those domains may stay aligned in the direction that the external field was forcing them. Undoubtedly some domains will flip back, because of the temperature, but some may remain oriented and therefore the material, once it has been exposed to an external magnetic field, may have become permanently magnetic.
The only way you can remove that permanent magnetism could be to bang on it with a hammer. Then these domains get very nervous and randomize themselves. Or you can heat them up to undo the orientation of the domains. The domains themselves will remain, but then they average out not to produce any permanent magnetic field.
In nonuniform field
For the same reason, that paramagnetism is pulled towards the strong field, ferromagnetism will also be pulled towards the strong field. Except in the case of ferromagnetism the forces with which the material is pulled towards the magnet, is much larger than in with paramagnetic material.
If we take a paperclip, you can hang it on the south pole of your magnet, or the north pole of your magnet. Ferromagnetic material is always pulled towards the strong field. If we hang a few of those paperclips on there, and you carefully and slowly remove them, you may notice that after you move them, that the paperclips themselves have become magnetic. You can not do this paramagnetic material, because the forces involved are only a few percent of the weight of the material itself. So if you try it with aluminum, it will not stick to the magnet.
Paramagnetic material will be pulled, with huge forces, towards a strong magnetic field, provided that the magnetic field is nonuniform. When it as a strong gradient. it is pulled towards the strong side.
Dependencies
Relative permeability
In all cases, whether we have diamagnetic, paramagnetic or ferromagnetic material, the magnetic field inside is different from what the field would be without the material. In many cases, but not all, is the field inside the material proportional to the vacuum field. We call this proportionality constant is called the relative permeability, \(\kappa_m\). $$ \vec B_\text{inside} = \kappa_m \, \vec B_\text{vac} \tag{\(\kappa_m\)} \label{eq:kappam} $$
Now we can look at these values for the relative permeability, and we can understand the difference between diamagnetic material, paramagnetic material and ferromagnetic material.
Magnetic susceptibility
In the case of diamagnetic and paramagnetic material, the \(\vec B\)field inside is only slightly different from the vacuum field. It is common to express \(\kappa_m\) in terms as \(1\) plus something that we call magnetic susceptibility, \(\chi_m\). Because if it is very close to \(1\), it is easier to simply list chi of M. $$ \kappa_m = 1 + \chi_m \nonumber $$
Diamagnetic materials
For diamagnetic materials, the values for \(\chi_m\) are all negative. It is slightly smaller than \(1\), because these induced dipoles oppose the external field.
Material  \(\chi_m\) 

\(\rm{Bi}\)  \(1.7\times10^{4}\) 
\(\rm{Cu}\)  \(10^{5}\) 
\(\rm{H_2O}\)  \(10^{5}\) 
\(\rm{N_2}\,(1\,\rm{atm})\)  \(7\times 10^{9}\) 
Paramagnetic materials
For paramagnetic, the \(\chi_m\) is positive, and again the values are small. Inside the material, the magnetic fields is a little larger than the vacuum field.
Material  \(\chi_m\)  Temperature 

\(\rm{Al}\)  \(+2\times10^{5}\)  \(\approx 300\,^oK\) 
\(\rm{O_2\,(1\,\rm{atm})}\)  \(+2\times10^{6}\)  \(\approx 300\,^oK\) 
\(\rm{O_2\,(\rm{liquid})}\)  \(+3.5\times10^{3}\)  \(90\,^oK\) 
Ferromagnetic materials
For ferromagnetic materials, it would be absurd to list \(\chi_m\) because it is so large that you can forget about the \(1\). So \(\chi_m\) is about the same as \(\kappa_m\) $$ \chi_m \approx \kappa_m \approx 10^2 \ldots 10^5 \nonumber $$ If \(\kappa_m\) is ten thousand, you would have a field inside the ferromagnetic material that is \(10,000\times\) larger than the vacuum field. There is a limit, that we discuss next time.
The three most common ferromagnetic materials are cobalt, nickel and iron. Gadolinium is ferromagnetic in the winter, when the temperature is below 16 °C, but is paramagnetic in the summer.
Curie point
So paramagnetic and ferromagnetic properties depend on the temperature. (Diamagnetic properties do not depend on the temperature.)
At very low temperatures, there is very little thermal agitation. So we can then easier align those dipoles. So the values for \(\kappa_m\) will be different. If you cool ferromagnetic material, you expect the \(\kappa_m\) to go up. You get a stronger field inside.
If you make the material very hot, then it can lose its ferromagnetic properties completely. At a very precise temperature the domains fall apart. The domains themselves no longer exist. That is also something that you need quantum mechanics for to understand. We call this the Curie temperature. For iron this is 1043 °K, or 770 °C, where all of a sudden all the domains disappear and the material becomes paramagnetic.
In other words, if ferromagnetic material would be hanging on a magnet and you heat it up above the Curie point, it will fall off.
Maximum dipole moment
As we have seen: in paramagnetic and ferromagnetic, the \(\kappa_m\) is the result of the intrinsic dipoles of atoms/molecules are aligning with the external field.
The question is: how large can the magnetic dipole moment of a single atom be? How strong can we have a field inside ferromagnetic material? In other words, if we were able to align all the dipole moments of all the atoms, what is the maximum that we can achieve.
Bohr magnetron
To calculate the magnetic dipole moment of an atom, you have to do some quantum mechanics, and that is beyond our scope. We will derive it in a classical way.
Assuming a hydrogen atom, with a proton in the center, and an electron with orbit radius \(R\). The electron \(e^\) moves with velocity \(v\), so the current goes in the opposite direction.
The mass, charge and Bohr radius of an electron $$ \begin{align*} m_e &= 9.1\times10^{31}\,\rm{kg} \\ e &= 1.6\times 10^{10}\,\rm{C} \\ R &= 6\times 10^{11}\,\rm{m} \end{align*} $$
The current running around the proton, creates a magnetic field, so the dipole moment \(\vec u\) is upwards
Recall the magnetic dipole moment from equation \(\eqref{eq:dipolemoment}\)
$$ \vec\mu = I \vec A \nonumber $$
The area \(A\) is simply $$ A = \pi R^2 \approx 8\times10^{21}\,\rm{m} \nonumber $$
For the current we have to combine knowledge Newtonian mechanics and electro magnetics. The electron goes around, because the proton and electron attract each other. So there is a Coulomb force \(\vec F\).
The Coulomb force is $$ \begin{align*} F &= \frac{q_1\,q_2\,K}{4\pi\varepsilon_0\,r^2} \\ &= \frac{e^2}{4\pi\varepsilon_0\,r^2} \end{align*} $$
From Newtonian mechanics we know that, the centripetal force (the force that holds it in orbit)
$$ F = m\,v^2 \nonumber $$
Combining these, allows us to calculate the velocity of the electron $$ \begin{align*} \frac{e^2}{4\pi\varepsilon_0\,R^{\cancel{2}}} &= \frac{m\,v^2}{\cancel{R}} \\ \implies v &= \sqrt{\frac{e^2}{m\,4\pi\,\varepsilon_0\,R}} \\ &\approx 2.3 \times 10^{6}\,\rm{m/s} \end{align*} \nonumber $$
To find the current, we first find the time \(T\) that it takes the electron to go around $$ \begin{align*} T &= \frac{2\pi\,R}{v} \\ &\approx 1.4\times10^{16}\,\rm{sec} \end{align*} $$
At every one point on the radius, every \(1.4\times10^{16}\) seconds, the electron goes by. The definition of current is: charge per unit time $$ \begin{align*} I &= \frac{e}{T} \\ &= 1.1\times 10^{3}\,\rm{A} \end{align*} $$
This is a lot. One electron going around a proton represents a current of a milliampere! Now we have the magnetic moment \(\mu\) $$ \begin{align*} \mu &= I\,A \\ &\approx (1.1\times 10^{3})(8\times10^{21}) \end{align*} $$
This \(\mu_b\) is called the Bohr magneton $$ \shaded{ \mu_b\approx 9.3\times 10^{24}\,\rm{Am^2} } \tag{Bohr magnetron} $$
What we can’t understand with our current knowledge, but will with quantum mechanics, is that the magnetic moment of all electrons in orbit can only be a multiple of this number, nothing in between. It is quantization. It includes even zero, which is even harder to understand.
Spin
In addition to a dipole moment due to the electron going around the proton, the electron itself is a charge which spins around its own axis. That means that a charge is going around on the spinning scale of the electron. That magnetic dipole moment is always the value \(\mu\).
So the net magnetic dipole moment of an atom or molecule is now the vectorial sum of all these dipole moments, of all these electrons going around, the orbital dipole moments, and now you have to add these spin dipoles.
Some of these cancel each other out. The net result is that most atoms/molecules have dipole moments which are either one Bohr magneton or two Bohr magnetons. That is what we will use discussing how strong a field we can create if we align all those magnetic dipoles.
The magnetic field that is produced inside a material when we expose it to an external field, that magnetic field \(\vec B\) is the vacuum field that we can create with a solenoid, plus what we will call \(\vec B^\prime\) $$ \vec B = \vec B_{vac} + \vec B^\prime \tag{net field} \label{eq:netfield} $$
Here \(\vec B^\prime\) is the result of aligning these dipoles. The degree of success depends on the strength of the external field and of course the temperature.
A big if
If, a big if, they \(\vec B^\prime\) is linearly proportional to \(\vec B_{vac}\), then we can write what we saw earlier $$ \begin{align*} B^\prime &= \chi_m\,\vec B_{vac}, & (\vec B = \vec B_{vac} + \vec B^\prime) \\ \implies \vec B &= (1 + \chi_m) \vec B_{vac} \\ &= \kappa_m\,\vec B_{vac} \end{align*} $$
This is only a meaningful equation if the sum of the alignment of all these dipoles can be written as linearly proportional with the external field. Let’s explore that in more detail.
Saturation
With paramagnetic material, the linearity always holds up, but with ferromagnetic material that is not the case. With ferromagnetic material is relative easy to align those dipoles, because they already group in domains and the domains flip in unison.
As we will see, with ferromagnetic material we can go into what we call saturation, where all the dipoles are aligned in the same direction. That leaves the question: how strong would that field be?
We will make a rough calculation that gives a pretty good feeling for the numbers. We choose a material whereby the magnetic dipole moment is two Bohr magnetrons $$ \mu = 2\,\mu_b \nonumber $$
We take the situation where they’re all aligned. The illustration shows the electron path around the nuclei in a solid material, so the atoms are nicely packed
All the dipole moments are nicely aligned, so all the magnetic fields support each other. We want to find the magnetic field in one atom. Note that this looks like a solenoid, where you have windings and currents going around.
Remember for a solenoid
$$ B = \mu_0\,I\,\underline{\frac{N}{l}} \nonumber $$
We need to figure out what would be the factor \(\frac{N}{l}\). Let’s take a material where the atom density \(\mathcal N\) is $$ \mathcal N = 10^{29}\,\rm{atoms/m^3} \nonumber $$
Now we have to introduce the magnetic moment, the two Bohr magnetons.
We take a length of one meter. Each loop has area \(A\), so the volume of this “solenoid” is $$ \rm{vol} = A\,\rm{m^2}\times 1\,\rm{m} = A\,\rm{m^3} \nonumber $$
But the number of atoms per cubic meter is \(mathcal N\), so the number of atoms (windings) in this solenoid per meter is $$ \rm{windings} = A\,\mathcal N \nonumber $$
Now the factor \(A\mathcal N\) is our factor \(\frac{N}{l}\), so for this assumed material we can write $$ \begin{align*} B &= \mu_0 \, \underline{I \, A}\, \mathcal N, & (IA = \mu = 2\mu_b) \\ &= u_0\,2\mu_b\,\mathcal N \\ &\approx (1.25\times10^{6})\,2\,(9.3\times10^{24})(10^{29}) \\ &\approx 2.3\,\rm{T} \end{align*} $$
Let’s use this number and understand what’s going to happen in that ferromagnetic material.
Inside the ferromagnetic material
If we take ferromagnetic material and expose it to an external field, a vacuum field. So we stick it in a solenoid, and we choose the current through the solenoid. The vacuum field is linearly proportional to the current through the solenoid
The strength of the solenoid’s vacuum field is
$$ B = \mu_0\,I\,\underline{\frac{N}{l}} \nonumber $$ Don’t confuse this the atomic scale magnetic field.
When we stick the ferromagnetic material inside the solenoid, the magnetic field there is \(B\)
We can’t plot it on a 1:1scale because \(\kappa_m\) for ferromagnetic material is so large, say \(1000\), because the field inside will be \(1000\times\) higher. If it were to scale then \(\tan\alpha = \kappa_m \approx 10^3\).
At the beginning we get a nice linear curve, but now slowly we’re beginning to reach saturation, where all these dipoles are going to be aligned. What you see then is that this curve bends over and over and will finally reach \(2.3\,\rm{T}\) that we just calculated for our imaginary material plus \(B_{vac}\).
We will now call the \(2.3\,\rm{T}\) field \(B^\prime\). This is the field that is the result of the alignment of all those dipoles. So when I increase the vacuum field, (B^\prime\) goes into saturation and settle for \(2.3\,\rm{T}\) and can no longer increase because all the magnetic dipoles are aligned.
So at point \(A\) the field is no longer \(1000\times\) stronger than the vacuum field. We’re no longer in the linear part. You could also think of it as \(\kappa_m\) being smaller than a thousand. It is no longer proportional to the value of one thousand.
If the temperature of the material is lower, it’s easier to align them, so you will achieve saturation earlier and the cure will go steeper towards saturation.
When it reaches point \(B\), when \(B^\prime\) goes into saturation, we can only increase the \(B\)field in the material, by increasing the vacuum field. Because \(B^\prime\) is not going to go up again. It will go up very slowly, because the huge multiplication factor of \(1000\times\) is gone now. So the growth is very slow.
Hysteresis curve
What happens once we have driven the material into saturation? What happens when we change the current and make the vacuum field zero again? Now you get a very unusual behavior.
Let’s assume that positive current, creates a vacuum field to the right, and a negative (reversed) current creates a vacuum field to the left.
Varying the external field
 O to B – This part of the curve is called “virginal”. Again, we start with zero current and increase it until saturation. At that point \(B\), all the domains have flipped in the direction of the vacuum field. The material itself is now magnetic. We have created permanent magnetism.

B to P – We reduce the current to zero. The vacuum field is still to the left. At point \(P\)
 \(B_{vac}=0\), but
 \(B^\prime\) is still to the right, so
 the net field \(B\) is to the right.

P to Q – We reverse the current, and slowly increase it from zero. So the vacuum field is now to the left. This brings us to location \(Q\), where we have something bizarre: the vacuum field is to the left, but there is no magnetic field inside the material.
 \(B_{vac}\) is to the left, but
 \(B^\prime\) is still to the right (because the domains are still aligned to the right), so
 the net field \(B\) is zero
 Q to R – We increasing the (reverse) current. So the vacuum field remains to the left. At point \(R\), the material goes into saturation again.

R to B – We bring the current back to zero and we arrive at point \(S\). There we have permanent magnetism again because some domains stay aligned towards the left.
 the vacuum field is zero, and
 \(B^\prime\) points to the right.
 Again we have permanent magnetism.
 S to P – We reverse the current back to the clockwise direction, and increase the current until the material is back in saturation.
Memory
We call this the hysteresis curve. For a given value of the current / vacuum field, we have two possibilities for the magnetic field \(B\). When I expose this material to an external field, I can’t calculate what the magnetic field inside the material will be. It depends on the history of the material.
\(\kappa_m\)
Looking at point \(Q\) and \(Q\), and you ask for \(\kappa_m\), it is almost a ridiculous question. Because \(\kappa_m\) is defined in equation \(\eqref{eq:kappam}\)
$$ \vec B_\text{inside} = \kappa_m \, \vec B_\text{vac} \nonumber $$
At those points we have a vacuum field, but no net field inside, so \(\kappa_m\) has to be zero. In the second and fourth quadrant it is even more bizarre, because \(\kappa_m\) has to be negative.
Removing the permanent magnetism
To make the material virginal again
 By taking the material out and heating it up above the Curie point, so the domains completely fall apart. Then you cool it again below the Curie point.
 The other way is banging it with a hammer and hope for the best.
 The other way is called demagnetization. That is what happens when you steal a book in the library and the alarm goes off. Someone hasn’t demagnetized the magnetic strip in the book. To demagnetize, one would slowly reduce an AC current through the solenoid.
Effect on external field
If we bring ferromagnetic material in the vicinity of a magnet, we change the magnetic field configuration. Suppose we have a magnet and we bring ferromagnetic material close by
The material will see the vacuum field, so its domains try to align a bit. It will get a south and north pole and create a field in the same direction. It will support the external field. The net result is that the field inside the material becomes very strong.
The external field lines will get sucked into the ferromagnetic material. The external field elsewhere will weaken.
The last Maxwell’s equation
Let’s look at the Maxwell equations as we have them so far.
 Gauss’s law $$ \newcommand{oiint}{\subset\!\!\supset\kern1.65em\iint} \color{blue} \phi = \oiint_S \vec E \cdot d\vec A = \frac{\sum_i Q_i}{\kappa\,\varepsilon_0} \nonumber $$ The electric flux through a closed surface is equal to all the charge inside divided by \(\kappa \varepsilon_0\). With electric fields, the \(\kappa\) always lowers the field inside the material. But nothing going to change here.
 Gauss’s law for magnetism $$ \newcommand{oiint}{\subset\!\!\supset\kern1.65em\iint} \color{brown} \oiint_S \vec B \cdot d\vec A = 0 \nonumber $$ This tells us that magnetic monopoles don’t exist. (Or at least we think they don’t exist.)
 Faraday’s law $$ \color{green} \oint_C \vec E\cdot d\vec l = \frac{d}{dt}\iint_R \vec B \cdot d\vec A \nonumber $$ When you move conducting loops in magnetic fields, you create electricity. This doesn’t require any adjustment in terms of \(\kappa_m\) either.
 Ampère’s law amended by Maxwell $$ \color{purple} \oint \vec B \cdot d\vec l = \mu_0\left(I_\rm{encl} + \varepsilon_0\kappa \frac{d}{dt} \iint_S \vec E\cdot d\vec A \right) \nonumber $$ Tells us the magnetic field for vacuum. Now we know that’s not true anymore.
Ampère’s law with Maxwell’s addition needs to be adjusted by a factor of \(\kappa_m\), the relative permeability. $$ \shaded{ \oint \vec B \cdot d\vec l = \textcolor{purple}{\kappa_m}\, \mu_0\left(I_\rm{encl} + \varepsilon_0\kappa \frac{d}{dt} \iint_S \vec E\cdot d\vec A \right) } \tag{Ampère/Maxwell add} \label{eq:maxwell4} $$
This \(\kappa_m\) is perfectly kosher for paramagnetic and diamagnetic materials. But with ferromagnetic material, you have to be very careful as we have seen with the hysteresis phenomenon. There are even situations where \(\kappa_m\) is negative; where \(\kappa_m\) is zero; and where \(\kappa_m\) can as high as \(10^3\). So we have to be very careful when applying this equation without thinking.
This moment is very special, because we have all four Maxwell’s equations in place. Hope you can appreciate them.