The Setup
Light Meets Metal
Imagine a beam of light, specifically with a wavelength of 6561 A˚, striking a metal surface. This light carries energy in discrete packets called photons. When these photons hit the metal, they can transfer their energy to electrons. If the energy is sufficient, it knocks the electrons right out of the metal! This is the famous photoelectric effect.
But the story doesn't end there. Once these electrons are free, they are immediately subjected to a uniform magnetic field of 3×10−4 T that is perpendicular to their motion. As we know from electromagnetism, a moving charge in a perpendicular magnetic field experiences a force that causes it to move in a circular path.
The Magnetic Dance
The magnetic force acts as the centripetal force keeping the electron in its circular orbit. The radius r of this path is given by the equation:
We are told that the largest circular path has a radius of 10 mm. For the radius to be at its maximum, the velocity of the electron must also be at its maximum, vmax. Rearranging our formula to solve for this maximum velocity, we get:
Calculating the Kinetic Energy
Now that we have an expression for the maximum velocity, we can determine the maximum kinetic energy (Kmax) of these ejected electrons. The standard formula for kinetic energy is:
Substituting our expression for vmax into this equation yields:
Kmax=21m(mBer)2=2mB2e2r2
This gives us the kinetic energy in Joules. However, in atomic physics, it is much more convenient to work in electron-volts (eV). To convert Joules to eV, we simply divide by the elementary charge e:
Kmax(eV)=2m⋅eB2e2r2=2mB2er2
Now, let's plug in the given values: B=3×10−4 T, e=1.6×10−19 C, r=10 mm=10−2 m, and m=9.1×10−31 kg.
Kmax=2×(9.1×10−31)(3×10−4)2×(1.6×10−19)×(10−2)2
Kmax=2×9.19×1.6×10−3110−8×10−19×10−4
Notice how beautifully the powers of ten cancel out! The numerator's powers sum to 10−31, which perfectly cancels the denominator's 10−31. We are left with:
The Photon's Contribution
We know the kinetic energy of the electrons after they leave the metal. But how much energy did the incident light bring in the first place? The energy E of a photon is calculated using Planck's equation:
A very useful shortcut when dealing with wavelengths in Angstroms is to use the approximation hc≈12400 eV⋅A˚. Using our given wavelength of 6561 A˚:
Einstein's Equation to the Rescue
Finally, we bring it all together using Einstein's photoelectric equation. This principle of energy conservation states that the energy of the incoming photon is used to overcome the metal's work function ϕ (the binding energy), with the remainder becoming the kinetic energy of the ejected electron:
We want to find the work function ϕ, so we rearrange the equation:
Substituting the values we calculated:
The work function of the metal is approximately 1.1 eV.