Imagine you are shrinking down to the atomic scale, staring at a hydrogen atom. You see an electron zipping around the nucleus in a perfect circular orbit. But this isn't just a moving particle; it's a tiny, continuous loop of electric current! And wherever there is a current loop, there is a magnetic field. The atom itself is a miniature magnet.
The Setup
An Atom as a Magnet
To understand this atomic magnet, we first need to figure out how much 'current' this single electron is generating. Current is simply the rate of flow of charge. So, if we take the charge of the electron (e) and divide it by the time it takes to complete one full orbit (the time period T), we get our equivalent current:
i=Te
But how long does one orbit take? The time period is the distance traveled divided by the speed: T=v2πR.
To find the velocity v, we turn to Niels Bohr. Bohr's first postulate tells us that the angular momentum of an electron in the ground state (n=1) is quantized:
mvR=2πh
From this, we can isolate the velocity:
v=2πmRh
The Master Equation
Magnetic Moment
Now, let's plug this velocity back into our time period equation:
T=2πmRh2πR=h4π2mR2
With the time period in hand, our equivalent current becomes:
i=h4π2mR2e=4π2mR2eh
The strength of our atomic magnet is measured by its magnetic moment (M), which is the current multiplied by the area of the loop (A=πR2):
M=iA=(4π2mR2eh)(πR2)
Notice how beautifully the R2 and π terms cancel out! We are left with a pristine, fundamental constant:
M=4πmeh
The Elegant Shortcut
Gyromagnetic Ratio
I know that derivation took a few steps, but let's take a breath... there is a much faster, more elegant way to see this.
For any revolving charge, the ratio of its magnetic moment to its angular momentum is a universal constant known as the gyromagnetic ratio. It is simply the charge divided by twice the mass:
LM=2me
Since we already know from Bohr that the angular momentum L=2πh, we can instantly find the magnetic moment:
M=(2me)(2πh)=4πmeh
Physics is incredibly consistent. Two different paths, one identical, beautiful result.
The Twist
Torque in a Magnetic Field
Now for the grand finale. We place our tiny atomic magnet into an external magnetic field B. The problem states that the normal to the orbit makes a 30∘ angle with the magnetic field.
Because the electron is negatively charged, its conventional current flows opposite to its motion. This means its magnetic moment vector M points exactly opposite to the geometric normal of the orbit.
When a magnetic dipole is placed in a magnetic field, it experiences a twisting force—a torque (τ)—that tries to align it with the field. The formula for this torque is the cross product:
τ=M×B
The magnitude of this torque is:
∣τ∣=MBsinθ
Whether you consider the angle to be 30∘ (with the normal) or 150∘ (with the magnetic moment), the sine value is exactly the same: sin(30∘)=21.
Substituting our magnetic moment and the sine value, we get our final answer:
τ=(4πmeh)B(21)=8πmehB
By the right-hand rule, this torque acts perpendicular to both the magnetic moment and the magnetic field. You've just calculated the fundamental twisting force that governs phenomena like Larmor precession in quantum mechanics. Incredible work!