The Magnetic Field in Various Situations

14The Magnetic Field in Various Situations

14–1The vector potential

In this chapter we continue our discussion of magnetic fields associated with steady currents—the subject of magnetostatics. The magnetic field is related to electric currents by our basic equations

\label E q : I I : 14 : 1 \FLPdiv \FLPB = 0, \label E q : I I : 14 : 2 c^{2} \FLPcurl \FLPB = \frac{\FLPj}{\epsO} .

We want now to solve these equations mathematically in a general way, that is, without requiring any special symmetry or intuitive guessing. In electrostatics, we found that there was a straightforward procedure for finding the field when the positions of all electric charges are known: One simply works out the scalar potential $ϕ$ by taking an integral over the charges—as in Eq. (4.25). Then if one wants the electric field, it is obtained from the derivatives of $ϕ$ . We will now show that there is a corresponding procedure for finding the magnetic field $\FLPB$ if we know the current density $\FLPj$ of all moving charges.

In electrostatics we saw that (because the curl of $\FLPE$ was always zero) it was possible to represent $\FLPE$ as the gradient of a scalar field $ϕ$ . Now the curl of $\FLPB$ is not always zero, so it is not possible, in general, to represent it as a gradient. However, the divergence of $\FLPB$ is always zero, and this means that we can always represent $\FLPB$ as the curl of another vector field. For, as we saw in Section 2–7, the divergence of a curl is always zero. Thus we can always relate $\FLPB$ to a field we will call $\FLPA$ by

\label E q : I I : 14 : 3 \FLPB = \FLPcurl \FLPA .

Or, by writing out the components,

B_{x} B_{y} B_{z} = (\FLPcurl \FLPA)_{x} = (\FLPcurl \FLPA)_{y} = (\FLPcurl \FLPA)_{z} = \ddp A_{z} y = \ddp A_{x} z = \ddp A_{y} x - \ddp A_{y} z, - \ddp A_{z} x, - \ddp A_{x} y . \label E q : I I : 14 : 4

Writing $\FLPB = \FLPcurl \FLPA$ guarantees that Eq. (14.1) is satisfied, since, necessarily,

\FLPdiv \FLPB = \FLPdiv (\FLPcurl \FLPA) = 0.

The field $\FLPA$ is called the vector potential.

You will remember that the scalar potential $ϕ$ was not completely specified by its definition. If we have found $ϕ$ for some problem, we can always find another potential $ϕ^{'}$ that is equally good by adding a constant:

ϕ^{'} = ϕ + C .

The new potential $ϕ^{'}$ gives the same electric fields, since the gradient $\FLPgrad C$ is zero; $ϕ^{'}$ and $ϕ$ represent the same physics.

Similarly, we can have different vector potentials $\FLPA$ which give the same magnetic fields. Again, because $\FLPB$ is obtained from $\FLPA$ by differentiation, adding a constant to $\FLPA$ doesn’t change anything physical. But there is even more latitude for $\FLPA$ . We can add to $\FLPA$ any field which is the gradient of some scalar field, without changing the physics. We can show this as follows. Suppose we have an $\FLPA$ that gives correctly the magnetic field $\FLPB$ for some real situation, and ask in what circumstances some other new vector potential $\FLPA^{'}$ will give the same field $\FLPB$ if substituted into (14.3). Then $\FLPA$ and $\FLPA^{'}$ must have the same curl:

\FLPB = \FLPcurl \FLPA^{'} = \FLPcurl \FLPA .

Therefore

\FLPcurl \FLPA^{'} - \FLPcurl \FLPA = \FLPcurl (\FLPA^{'} - \FLPA) = \FLPzero .

But if the curl of a vector is zero it must be the gradient of some scalar field, say $ψ$ , so $\FLPA^{'} - \FLPA = \FLPgrad ψ$ . That means that if $\FLPA$ is a satisfactory vector potential for a problem then, for any $ψ$ , at all,

\label E q : I I : 14 : 5 \FLPA^{'} = \FLPA + \FLPgrad ψ

will be an equally satisfactory vector potential, leading to the same field $\FLPB$ .

It is usually convenient to take some of the “latitude” out of $\FLPA$ by arbitrarily placing some other condition on it (in much the same way that we found it convenient—often—to choose to make the potential $ϕ$ zero at large distances). We can, for instance, restrict $\FLPA$ by choosing arbitrarily what the divergence of $\FLPA$ must be. We can always do that without affecting $\FLPB$ . This is because although $\FLPA^{'}$ and $\FLPA$ have the same curl, and give the same $\FLPB$ , they do not need to have the same divergence. In fact, $\FLPdiv \FLPA^{'} = \FLPdiv \FLPA + \nabla^{2} ψ$ , and by a suitable choice of $ψ$ we can make $\FLPdiv \FLPA^{'}$ anything we wish.

What should we choose for $\FLPdiv \FLPA$ ? The choice should be made to get the greatest mathematical convenience and will depend on the problem we are doing. For magnetostatics, we will make the simple choice

\label E q : I I : 14 : 6 \FLPdiv \FLPA = 0.

(Later, when we take up electrodynamics, we will change our choice.) Our complete definition¹ of $\FLPA$ is then, for the moment, $\FLPcurl \FLPA = \FLPB$ and $\FLPdiv \FLPA = 0$ .

To get some experience with the vector potential, let’s look first at what it is for a uniform magnetic field $\FLPB_{0}$ . Taking our $z$ -axis in the direction of $\FLPB_{0}$ , we must have

B_{x} B_{y} B_{z} = \ddp A_{z} y = \ddp A_{x} z = \ddp A_{y} x - \ddp A_{y} z - \ddp A_{z} x - \ddp A_{x} y = 0, = 0, = B_{0} . \label E q : I I : 14 : 7

By inspection, we see that one possible solution of these equations is

A_{y} = x B_{0}, A_{x} = 0, A_{z} = 0.

Or we could equally well take

A_{x} = - y B_{0}, A_{y} = 0, A_{z} = 0.

Still another solution is a linear combination of the two:

\label E q : I I : 14 : 8 A_{x} = - \frac{1}{2} y B_{0}, A_{y} = \frac{1}{2} x B_{0}, A_{z} = 0.

It is clear that for any particular field $\FLPB$ , the vector potential $\FLPA$ is not unique; there are many possibilities.

The third solution, Eq. (14.8), has some interesting properties. Since the $x$ -component is proportional to $- y$ and the $y$ -component is proportional to $+ x$ , $\FLPA$ must be at right angles to the vector from the $z$ -axis, which we will call $\FLPr^{'}$ (the “prime” is to remind us that it is not the vector displacement from the origin). Also, the magnitude of $\FLPA$ is proportional to $x^{2} + y^{2}$ and, hence, to $r^{'}$ . So $\FLPA$ can be simply written (for our uniform field) as

\label E q : I I : 14 : 9 \FLPA = \frac{1}{2} \FLPB_{0} \times \FLPr^{'} .

The vector potential $\FLPA$ has the magnitude $B_{0} r^{'} /2$ and rotates about the $z$ -axis as shown in Fig. 14–1. If, for example, the $\FLPB$ field is the axial field inside a solenoid, then the vector potential circulates in the same sense as do the currents of the solenoid.

Fig. 14–1.A uniform magnetic field $\FigB$ in the $z$ -direction corresponds to a vector potential $\FigA$ that rotates about the $z$ -axis, with the magnitude $A = B r^{'} /2$ ( $r^{'}$ is the displacement from the $z$ -axis).

The vector potential for a uniform field can be obtained in another way. The circulation of $\FLPA$ on any closed loop $Γ$ can be related to the surface integral of $\FLPcurl \FLPA$ by Stokes’ theorem, Eq. (3.38):

\label E q : I I : 14 : 10 \oint_{Γ} \FLPA \cdot d \FLPs = inside Γ \int (\FLPcurl \FLPA) \cdot \FLPn d a .

But the integral on the right is equal to the flux of $\FLPB$ through the loop, so

\label E q : I I : 14 : 11 \oint_{Γ} \FLPA \cdot d \FLPs = inside Γ \int \FLPB \cdot \FLPn d a .

So the circulation of $\FLPA$ around any loop is equal to the flux of $\FLPB$ through the loop. If we take a circular loop, of radius $r^{'}$ in a plane perpendicular to a uniform field $\FLPB$ , the flux is just

π r^{'2} B .

If we choose our origin on an axis of symmetry, so that we can take $\FLPA$ as circumferential and a function only of $r^{'}$ , the circulation will be

\oint \FLPA \cdot d \FLPs = 2 π r^{'} A = π r^{'2} B .

We get, as before,

A = \frac{B r ^{'}}{2} .

In the example we have just given, we have calculated the vector potential from the magnetic field, which is opposite to what one normally does. In complicated problems it is usually easier to solve for the vector potential, and then determine the magnetic field from it. We will now show how this can be done.

14–2The vector potential of known currents

Since $\FLPB$ is determined by currents, so also is $\FLPA$ . We want now to find $\FLPA$ in terms of the currents. We start with our basic equation (14.2):

c^{2} \FLPcurl \FLPB = \frac{\FLPj}{\epsO},

which means, of course, that

\label E q : I I : 14 : 12 c^{2} \FLPcurl (\FLPcurl \FLPA) = \frac{\FLPj}{\epsO} .

This equation is for magnetostatics what the equation

\label E q : I I : 14 : 13 \FLPdiv \FLPgrad ϕ = - \frac{ρ}{\epsO}

was for electrostatics.

Our equation (14.12) for the vector potential looks even more like that for $ϕ$ if we rewrite $\FLPcurl (\FLPcurl \FLPA)$ using the vector identity Eq. (2.58):

\label E q : I I : 14 : 14 \FLPcurl (\FLPcurl \FLPA) = \FLPgrad (\FLPdiv \FLPA) - \nabla^{2} \FLPA .

Since we have chosen to make $\FLPdiv \FLPA = 0$ (and now you see why), Eq. (14.12) becomes

\label E q : I I : 14 : 15 \nabla^{2} \FLPA = - \frac{\FLPj}{\epsO c ^{2}} .

This vector equation means, of course, three equations:

\nabla^{2} A_{x} \nabla^{2} A_{y} \nabla^{2} A_{z} = - \frac{j _{x}}{\epsO c ^{2}}, = - \frac{j _{y}}{\epsO c ^{2}}, = - \frac{j _{z}}{\epsO c ^{2}} . \label E q : I I : 14 : 16

And each of these equations is mathematically identical to

\label E q : I I : 14 : 17 \nabla^{2} ϕ = - \frac{ρ}{\epsO} .

All we have learned about solving for potentials when $ρ$ is known can be used for solving for each component of $\FLPA$ when $\FLPj$ is known!

We have seen in Chapter 4 that a general solution for the electrostatic equation (14.17) is

ϕ (1) = \frac{1}{4 π \epsO} \int \frac{ρ ( 2 ) d V _{2}}{r _{12}} .

So we know immediately that a general solution for $A_{x}$ is

\label E q : I I : 14 : 18 A_{x} (1) = \frac{1}{4 π \epsO c ^{2}} \int \frac{j _{x} ( 2 ) d V _{2}}{r _{12}},

and similarly for $A_{y}$ and $A_{z}$ . (Figure 14–2 will remind you of our conventions for $r_{12}$ and $d V_{2}$ .) We can combine the three solutions in the vector form

\label E q : I I : 14 : 19 \FLPA (1) = \frac{1}{4 π \epsO c ^{2}} \int \frac{\FLPj ( 2 ) d V _{2}}{r _{12}},

(You can verify if you wish, by direct differentiation of components, that this integral for $\FLPA$ satisfies $\FLPdiv \FLPA = 0$ so long as $\FLPdiv \FLPj = 0$ , which, as we saw, must happen for steady currents.)

Fig. 14–2.The vector potential $\FigA$ at point $1$ is given by an integral over the current elements $\Figj d V$ at all points $2$ .

We have, then, a general method for finding the magnetic field of steady currents. The principle is: the $x$ -component of vector potential arising from a current density $\FLPj$ is the same as the electric potential $ϕ$ that would be produced by a charge density $ρ$ equal to $j_{x} / c^{2}$ —and similarly for the $y$ - and $z$ -components. (This principle works only with components in fixed directions. The “radial” component of $\FLPA$ does not come in the same way from the “radial” component of $\FLPj$ , for example.) So from the vector current density $\FLPj$ , we can find $\FLPA$ using Eq. (14.19)—that is, we find each component of $\FLPA$ by solving three imaginary electrostatic problems for the charge distributions $ρ_{1} = j_{x} / c^{2}$ , $ρ_{2} = j_{y} / c^{2}$ , and $ρ_{3} = j_{z} / c^{2}$ . Then we get $\FLPB$ by taking various derivatives of $\FLPA$ to obtain $\FLPcurl \FLPA$ . It’s a little more complicated than electrostatics, but the same idea. We will now illustrate the theory by solving for the vector potential in a few special cases.

14–3A straight wire

For our first example, we will again find the field of a straight wire—which we solved in the last chapter by using Eq. (14.2) and some arguments of symmetry. We take a long straight wire of radius $a$ , carrying the steady current $I$ . Unlike the charge on a conductor in the electrostatic case, a steady current in a wire is uniformly distributed throughout the cross section of the wire. If we choose our coordinates as shown in Fig. 14–3, the current density vector $\FLPj$ has only a $z$ -component. Its magnitude is

\label E q : I I : 14 : 20 j_{z} = \frac{I}{π a ^{2}}

inside the wire, and zero outside.

Fig. 14–3.A long cylindrical wire along the $z$ -axis with a uniform current density $\Figj$ .

Since $j_{x}$ and $j_{y}$ are both zero, we have immediately

A_{x} = 0, A_{y} = 0.

To get $A_{z}$ we can use our solution for the electrostatic potential $ϕ$ of a wire with a uniform charge density $ρ = j_{z} / c^{2}$ . For points outside an infinite charged cylinder, the electrostatic potential is

ϕ = - \frac{λ}{2 π \epsO} ln r^{'},

where $r^{'} = x^{2} + y^{2}$ and $λ$ is the charge per unit length, $π a^{2} ρ$ . So $A_{z}$ must be

A_{z} = - \frac{π a ^{2} j _{z}}{2 π \epsO c ^{2}} ln r^{'}

for points outside a long wire carrying a uniform current. Since $π a^{2} j_{z} = I$ , we can also write

\label E q : I I : 14 : 21 A_{z} = - \frac{I}{2 π \epsO c ^{2}} ln r^{'}

Now we can find $\FLPB$ from (14.4). There are only two of the six derivatives that are not zero. We get

\label E q : I I : 14 : 22 \label E q : I I : 14 : 23 B_{x} B_{y} B_{z} = - = = \frac{I}{2 π \epsO c ^{2}} \ddp y \frac{I}{2 π \epsO c ^{2}} \ddp y \ddp x 0 \ddp y . ln r^{'} = - ln r^{'} = \frac{I}{2 π \epsO c ^{2}} \frac{y}{r ^{'2}} \frac{I}{2 π \epsO c ^{2}} \frac{x}{r ^{'2}},,

We get the same result as before: $\FLPB$ circles around the wire, and has the magnitude

\label E q : I I : 14 : 24 B = \frac{1}{4 π \epsO c ^{2}} \frac{2 I}{r ^{'}} .

14–4A long solenoid

Next, we consider again the infinitely long solenoid with a circumferential current on the surface of $n I$ per unit length. (We imagine there are $n$ turns of wire per unit length, carrying the current $I$ , and we neglect the slight pitch of the winding.)

Just as we have defined a “surface charge density” $σ$ , we define here a “surface current density” $\FLPJ$ equal to the current per unit length on the surface of the solenoid (which is, of course, just the average $\FLPj$ times the thickness of the thin winding). The magnitude of $\FLPJ$ is, here, $n I$ . This surface current (see Fig. 14–4) has the components:

J_{x} = - J sin ϕ, J_{y} = J cos ϕ, J_{z} = 0.

Now we must find $\FLPA$ for such a current distribution.

Fig. 14–4.A long solenoid with a surface current density $\FigJ$ .

First, we wish to find $A_{x}$ for points outside the solenoid. The result is the same as the electrostatic potential outside a cylinder with a surface charge density

σ = σ_{0} sin ϕ,

with $σ_{0} = - J / c^{2}$ . We have not solved such a charge distribution, but we have done something similar. This charge distribution is equivalent to two solid cylinders of charge, one positive and one negative, with a slight relative displacement of their axes in the $y$ -direction. The potential of such a pair of cylinders is proportional to the derivative with respect to $y$ of the potential of a single uniformly charged cylinder. We could work out the constant of proportionality, but let’s not worry about it for the moment.

The potential of a cylinder of charge is proportional to $ln r^{'}$ ; the potential of the pair is then

ϕ \propto \ddp ln r^{'} y = \frac{y}{r ^{'2}} .

So we know that

\label E q : I I : 14 : 25 A_{x} = - K \frac{y}{r ^{'2}},

where $K$ is some constant. Following the same argument, we would find

\label E q : I I : 14 : 26 A_{y} = K \frac{x}{r ^{'2}} .

Although we said before that there was no magnetic field outside a solenoid, we find now that there is an $\FLPA$ -field which circulates around the $z$ -axis, as in Fig. 14–4. The question is: Is its curl zero?

Clearly, $B_{x}$ and $B_{y}$ are zero, and

B_{z} = \ddp x (K \frac{x}{r ^{'2}}) - \ddp y (- K \frac{y}{r ^{'2}}) = K (\frac{1}{r ^{'2}} - \frac{2 x ^{2}}{r ^{'4}} + \frac{1}{r ^{'2}} - \frac{2 y ^{2}}{r ^{'4}}) = 0.

So the magnetic field outside a very long solenoid is indeed zero, even though the vector potential is not.

We can check our result against something else we know: The circulation of the vector potential around the solenoid should be equal to the flux of $\FLPB$ inside the coil (Eq. 14.11). The circulation is $A \cdot 2 π r^{'}$ or, since $A = K / r^{'}$ , the circulation is $2 π K$ . Notice that it is independent of $r^{'}$ . That is just as it should be if there is no $\FLPB$ outside, because the flux is just the magnitude of $\FLPB$ inside the solenoid times $π a^{2}$ . It is the same for all circles of radius $r^{'} > a$ . We have found in the last chapter that the field inside is $n I / \epsO c^{2}$ , so we can determine the constant $K$ :

2 π K = π a^{2} \frac{n I}{\epsO c ^{2}},

K = \frac{n I a ^{2}}{2 \epsO c ^{2}} .

So the vector potential outside has the magnitude

\label E q : I I : 14 : 27 A = \frac{n I a ^{2}}{2 \epsO c ^{2}} \frac{1}{r ^{'}},

and is always perpendicular to the vector $\FLPr^{'}$ .

We have been thinking of a solenoidal coil of wire, but we would produce the same fields if we rotated a long cylinder with an electrostatic charge on the surface. If we have a thin cylindrical shell of radius $a$ with a surface charge $σ$ , rotating the cylinder makes a surface current $J = σ v$ , where $v = aω$ is the velocity of the surface charge. There will then be a magnetic field $B = σ aω / \epsO c^{2}$ inside the cylinder.

Fig. 14–5.A rotating charged cylinder produces a magnetic field inside. A short radial wire rotating with the cylinder has charges induced on its ends.

Now we can raise an interesting question. Suppose we put a short piece of wire $W$ perpendicular to the axis of the cylinder, extending from the axis out to the surface, and fastened to the cylinder so that it rotates with it, as in Fig. 14–5. This wire is moving in a magnetic field, so the $\FLPv \times \FLPB$ forces will cause the ends of the wire to be charged (they will charge up until the $\FLPE$ -field from the charges just balances the $\FLPv \times \FLPB$ force). If the cylinder has a positive charge, the end of the wire at the axis will have a negative charge. By measuring the charge on the end of the wire, we could measure the speed of rotation of the system. We would have an “angular-velocity meter”!

But are you wondering: “What if I put myself in the frame of reference of the rotating cylinder? Then there is just a charged cylinder at rest, and I know that the electrostatic equations say there will be no electric fields inside, so there will be no force pushing charges to the center. So something must be wrong.” But there is nothing wrong. There is no “relativity of rotation.” A rotating system is not an inertial frame, and the laws of physics are different. We must be sure to use equations of electromagnetism only with respect to inertial coordinate systems.

It would be nice if we could measure the absolute rotation of the earth with such a charged cylinder, but unfortunately the effect is much too small to observe even with the most delicate instruments now available.

14–5The field of a small loop; the magnetic dipole

Let’s use the vector-potential method to find the magnetic field of a small loop of current. As usual, by “small” we mean simply that we are interested in the fields only at distances large compared with the size of the loop. It will turn out that any small loop is a “magnetic dipole.” That is, it produces a magnetic field like the electric field from an electric dipole.

Fig. 14–6.A rectangular loop of wire with the current $I$ . What is the magnetic field at $P$ ? ( $R ≫ a$ and $R ≫ b$ .)

We take first a rectangular loop, and choose our coordinates as shown in Fig. 14–6. There are no currents in the $z$ -direction, so $A_{z}$ is zero. There are currents in the $x$ -direction on the two sides of length $a$ . In each leg, the current density (and current) is uniform. So the solution for $A_{x}$ is just like the electrostatic potential from two charged rods (see Fig. 14–7). Since the rods have opposite charges, their electric potential at large distances would be just the dipole potential (Section 6–5). At the point $P$ in Fig. 14–6, the potential would be

\label E q : I I : 14 : 28 ϕ = \frac{1}{4 π \epsO} \frac{\FLPp \cdot \FLPe _{R}}{R ^{2}},

where $\FLPp$ is the dipole moment of the charge distribution. The dipole moment, in this case, is the total charge on one rod times the separation between them:

\label E q : I I : 14 : 29 p = λab .

The dipole moment points in the negative $y$ -direction, so the cosine of the angle between $\FLPR$ and $\FLPp$ is $- y / R$ (where $y$ is the coordinate of $P$ ). So we have

ϕ = - \frac{1}{4 π \epsO} \frac{λab}{R ^{2}} \frac{y}{R} .

Fig. 14–7.The distribution of $j_{x}$ in the current loop of Fig. 14–6.

We get $A_{x}$ simply by replacing $λ$ by $I / c^{2}$ :

\label E q : I I : 14 : 30 A_{x} = - \frac{I ab}{4 π \epsO c ^{2}} \frac{y}{R ^{3}} .

By the same reasoning,

\label E q : I I : 14 : 31 A_{y} = \frac{I ab}{4 π \epsO c ^{2}} \frac{x}{R ^{3}} .

Again, $A_{y}$ is proportional to $x$ and $A_{x}$ is proportional to $- y$ , so the vector potential (at large distances) goes in circles around the $z$ -axis, circulating in the same sense as $I$ in the loop, as shown in Fig. 14–8.

Fig. 14–8.The vector potential of a small current loop at the origin (in the $x y$ -plane); a magnetic dipole field.

The strength of $\FLPA$ is proportional to $I ab$ , which is the current times the area of the loop. This product is called the magnetic dipole moment (or, often, just “magnetic moment”) of the loop. We represent it by $μ$ :

\label E q : I I : 14 : 32 μ = I ab .

The vector potential of a small plane loop of any shape (circle, triangle, etc.) is also given by Eqs. (14.30) and (14.31) provided we replace $I ab$ by

\label E q : I I : 14 : 33 μ = I \cdot (area of the loop) .

We leave the proof of this to you.

We can put our equation in vector form if we define the direction of the vector $\FLPmu$ to be the normal to the plane of the loop, with a positive sense given by the right-hand rule (Fig. 14–8). Then we can write

\label E q : I I : 14 : 34 \FLPA = \frac{1}{4 π \epsO c ^{2}} \frac{\FLPmu \times \FLPR}{R ^{3}} = \frac{1}{4 π \epsO c ^{2}} \frac{\FLPmu \times \FLPe _{R}}{R ^{2}} .

We have still to find $\FLPB$ . Using (14.33) and (14.34), together with (14.4), we get

\label E q : I I : 14 : 35 B_{x} = - \ddp z \frac{μ}{4 π \epsO c ^{2}} \frac{x}{R ^{3}} = \dots \frac{3 x z}{R ^{5}}

(where by $\dots$ we mean $μ /4 π \epsO c^{2}$ ),

B_{y} B_{z} = \ddp z (- \dots \frac{y}{R ^{3}}) = \dots \frac{3 y z}{R ^{5}}, = \ddp x (\dots \frac{x}{R ^{3}}) - \ddp y (- \dots \frac{y}{R ^{3}}) = - \dots (\frac{1}{R ^{3}} - \frac{3 z ^{2}}{R ^{5}}) . \label E q : I I : 14 : 36

The components of the $\FLPB$ -field behave exactly like those of the $\FLPE$ -field for a dipole oriented along the $z$ -axis. (See Eqs. (6.14) and (6.15); also Fig. 6–4.) That’s why we call the loop a magnetic dipole. The word “dipole” is slightly misleading when applied to a magnetic field because there are no magnetic “poles” that correspond to electric charges. The magnetic “dipole field” is not produced by two “charges,” but by an elementary current loop.

It is curious, though, that starting with completely different laws, $\FLPdiv \FLPE = ρ / \epsO$ and $\FLPcurl \FLPB = \FLPj / \epsO c^{2}$ , we can end up with the same kind of a field. Why should that be? It is because the dipole fields appear only when we are far away from all charges or currents. So through most of the relevant space the equations for $\FLPE$ and $\FLPB$ are identical: both have zero divergence and zero curl. So they give the same solutions. However, the sources whose configuration we summarize by the dipole moments are physically quite different—in one case, it’s a circulating current; in the other, a pair of charges, one above and one below the plane of the loop for the corresponding field.

14–6The vector potential of a circuit

Fig. 14–9.For a fine wire $\Figj d V$ is the same as $I d \Figs$ .

We are often interested in the magnetic fields produced by circuits of wire in which the diameter of the wire is very small compared with the dimensions of the whole system. In such cases, we can simplify the equations for the magnetic field. For a thin wire we can write our volume element as

d V = S d s

where $S$ is the cross-sectional area of the wire and $d s$ is the element of distance along the wire. In fact, since the vector $d \FLPs$ is in the same direction as $\FLPj$ , as shown in Fig. 14–9 (and we can assume that $\FLPj$ is constant across any given cross section), we can write a vector equation:

\label E q : I I : 14 : 37 \FLPj d V = j S d \FLPs .

But $j S$ is just what we call the current $I$ in a wire, so our integral for the vector potential (14.19) becomes

\label E q : I I : 14 : 38 \FLPA (1) = \frac{1}{4 π \epsO c ^{2}} \int \frac{I d \FLPs _{2}}{r _{12}}

(see Fig. 14–10). (We assume that $I$ is the same throughout the circuit. If there are several branches with different currents, we should, of course, use the appropriate $I$ for each branch.)

Fig. 14–10.The magnetic field of a wire can be obtained from an integral around the circuit.

Again, we can find the fields from (14.38) either by integrating directly or by solving the corresponding electrostatic problems.

14–7The law of Biot and Savart

In studying electrostatics we found that the electric field of a known charge distribution could be obtained directly with an integral, Eq. (4.16):

\FLPE (1) = \frac{1}{4 π \epsO} \int \frac{ρ ( 2 ) \FLPe _{12} d V _{2}}{r _{12}^{2}} .

As we have seen, it is usually more work to evaluate this integral—there are really three integrals, one for each component—than to do the integral for the potential and take its gradient.

There is a similar integral which relates the magnetic field to the currents. We already have an integral for $\FLPA$ , Eq. (14.19); we can get an integral for $\FLPB$ by taking the curl of both sides:

\FLPB (1) \label E q : I I : 14 : 39 = \FLPcurl \FLPA (1) = \FLPcurl [\frac{1}{4 π \epsO c ^{2}} \int \frac{\FLPj ( 2 ) d V _{2}}{r _{12}}] .

Now we must be careful: The curl operator means taking the derivatives of $\FLPA (1)$ , that is, it operates only on the coordinates $(x_{1}, y_{1}, z_{1})$ . We can move the $\FLPcurl$ operator inside the integral sign if we remember that it operates only on variables with the subscript $1$ , which of course, appear only in

\label E q : I I : 14 : 40 r_{12} = [(x_{1} - x_{2})^{2} + (y_{1} - y_{2})^{2} + (z_{1} - z_{2})^{2}]^{1/2} .

We have, for the $x$ -component of $\FLPB$ ,

B_{x} \label E q : I I : 14 : 41 = \ddp A_{z} y_{1} - \ddp A_{y} z_{1} = \frac{1}{4 π \epsO c ^{2}} \int [j_{z} \ddp y_{1} (\frac{1}{r _{12}}) - j_{y} \ddp z_{1} (\frac{1}{r _{12}})] d V_{2} = - \frac{1}{4 π \epsO c ^{2}} \int [j_{z} \frac{y _{1} - y _{2}}{r _{12}^{3}} - j_{y} \frac{z _{1} - z _{2}}{r _{12}^{3}}] d V_{2} .

The quantity in brackets is just the negative of the $x$ -component of

\frac{\FLPj \times \FLPr _{12}}{r _{12}^{3}} = \frac{\FLPj \times \FLPe _{12}}{r _{12}^{2}}

Corresponding results will be found for the other components, so we have

\label E q : I I : 14 : 42 \FLPB (1) = \frac{1}{4 π \epsO c ^{2}} \int \frac{\FLPj ( 2 ) \times \FLPe _{12}}{r _{12}^{2}} d V_{2} .

The integral gives $\FLPB$ directly in terms of the known currents. The geometry involved is the same as that shown in Fig. 14–2.

If the currents exist only in circuits of small wires we can, as in the last section, immediately do the integral across the wire, replacing $\FLPj d V$ by $I d \FLPs$ , where $d \FLPs$ is an element of length of the wire. Then, using the symbols in Fig. 14–10,

\label E q : I I : 14 : 43 \FLPB (1) = - \frac{1}{4 π \epsO c ^{2}} \int \frac{I \FLPe _{12} \times d \FLPs _{2}}{r _{12}^{2}} .

(The minus sign appears because we have reversed the order of the cross product.) This equation for $\FLPB$ is called the Biot-Savart law, after its discoverers. It gives a formula for obtaining directly the magnetic field produced by wires carrying currents.

You may wonder: “What is the advantage of the vector potential if we can find $\FLPB$ directly with a vector integral? After all, $\FLPA$ also involves three integrals!” Because of the cross product, the integrals for $\FLPB$ are usually more complicated, as is evident from Eq. (14.41). Also, since the integrals for $\FLPA$ are like those of electrostatics, we may already know them. Finally, we will see that in more advanced theoretical matters (in relativity, in advanced formulations of the laws of mechanics, like the principle of least action to be discussed later, and in quantum mechanics) the vector potential plays an important role.

Our definition still does not uniquely determine $\FLPA$ . For a unique specification we would also have to say something about how the field $\FLPA$ behaves on some boundary, or at large distances. It is sometimes convenient, for example, to choose a field which goes to zero at large distances. ↩

[

Inspection with a Free-Flying Space Manipulator

Explorer