The photoelectric effect is one of the most beautiful phenomena in modern physics, bridging the gap between the wave and particle nature of light. In this problem, we are exploring how different wavelengths of incident light affect the kinetic energy—and consequently, the speed—of ejected electrons.
Decoding the Problem Statement
We are given a single metal surface, which means the work function (ϕ) remains constant throughout the experiment. The metal is illuminated by two different wavelengths:
1. λ1=350 nm
2. λ2=540 nm
The problem states that the maximum speeds of the photoelectrons in the two cases differ by a factor of 2.
Here is the critical logical deduction: Which electron is faster?
We know that the energy of a photon is inversely proportional to its wavelength (E=λhc). Since λ1<λ2, the photons in the first case pack a much stronger punch. Therefore, the electrons ejected in the first case will have a higher kinetic energy and a higher speed.
This allows us to confidently set our velocities as:
v1=2v
v2=v
The Master Equation
Einstein's photoelectric equation is our primary tool here. It elegantly states that the energy of the incident photon is split into two parts: overcoming the metal's binding energy (work function) and giving the electron kinetic energy.
Let's write this equation for both of our cases.
For Case 1 (λ1=350 nm):
350hc=ϕ+21m(2v)2
350hc=ϕ+4(21mv2)
For Case 2 (λ2=540 nm):
540hc=ϕ+21mv2
Algebraic Manipulation
We have a system of two equations. Our goal is to find the work function ϕ. The easiest way to do this is to eliminate the kinetic energy term (21mv2).
From the second equation, we can isolate the kinetic energy:
21mv2=540hc−ϕ
Now, we substitute this expression into our first equation:
350hc=ϕ+4(540hc−ϕ)
Let's expand the bracket and group the
ϕ terms together:
350hc=ϕ+5404hc−4ϕ
3ϕ=5404hc−350hc
ϕ=3hc(5404−3501)
The Final Calculation
The problem kindly provides the value of hc=1240 eV⋅nm. Let's plug this in and crunch the numbers.
ϕ=31240(540×3504×350−540)
ϕ=31240(1890001400−540)
ϕ=31240(189000860)
ϕ≈1.88 eV
Looking at our options, the closest value is 1.8 eV.
This problem beautifully demonstrates how a simple ratio in physical observables (like speed) can be traced back through conservation of energy to reveal fundamental properties of materials.