Imagine you are standing inside a massive, solid cylindrical wire carrying a steady, uniform current. The physics of electromagnetism dictates that the magnetic field you experience depends entirely on where you are relative to the central axis of this wire. This problem is a beautiful exploration of Ampere's Circuital Law, testing our understanding of how magnetic fields behave both inside and outside a current-carrying conductor.
The Master Key
Ampere's Circuital Law
Ampere's Law is to magnetism what Gauss's Law is to electrostatics. It states that the line integral of the magnetic field around any closed loop is proportional to the total current enclosed by that loop:
For a long, straight wire with a circular cross-section, symmetry tells us that the magnetic field lines form concentric circles around the axis. This symmetry makes evaluating the integral incredibly simple: the left side always becomes B(2πr). The real physics lies in determining Ienc, the enclosed current.
Inside the Wire
The Linear Regime
When we are inside the wire, at a distance r<a, our Amperian loop does not enclose the entire current I. Because the current is uniformly distributed, the current density J (current per unit area) is constant: J=πa2I.
The current enclosed by a loop of radius r is simply the current density multiplied by the area of our loop:
Ienc=J×(πr2)=(πa2I)πr2=Ia2r2
Plugging this into Ampere's Law gives us the magnetic field inside the wire:
Bin(2πr)=μ0(Ia2r2)⟹Bin=2πa2μ0Ir
Notice that inside the wire, the magnetic field increases linearly with distance r. For our specific problem, we need the field at r=3a. Let's substitute this value:
B1=2πa2μ0I(3a)=6πaμ0I
Outside the Wire
The Inverse Regime
Now, let's step outside the wire to a distance r>a. Here, our Amperian loop encloses the entire current I. The internal structure of the wire no longer matters; it behaves exactly like an infinitely thin wire located at the central axis.
Ampere's Law gives us the familiar formula:
Bout(2πr)=μ0I⟹Bout=2πrμ0I
Outside the wire, the magnetic field decreases inversely with distance r. We are asked to find the field at r=2a. Substituting this into our formula yields:
The Final Calculation
We now have the magnetic field at both locations. The final step is to find their ratio, B2B1. This is where the elegance of proportionalities shines, as all the constants will perfectly cancel out.
B2B1=4πaμ0I6πaμ0I
And there we have it! The ratio of the magnetic fields is 32. This problem serves as a fantastic reminder to always trust the fundamental laws of physics. Whether you are deep inside a conductor or far out in space, Ampere's Law will always guide you to the right answer.