The Magic of the Photoelectric Effect
Imagine a world where light isn't just a continuous wave, but a stream of tiny, energetic packets called photons. When these photons strike a photosensitive metal surface, they can knock electrons right out of the metal! This phenomenon, known as the photoelectric effect, was brilliantly explained by Albert Einstein, earning him the Nobel Prize.
But these ejected electrons don't just sit there; they fly off with kinetic energy. To measure this energy, physicists use a clever trick: they apply a reverse voltage, called the stopping potential (Vs), to a collector plate. This negative voltage repels the electrons. When the voltage is just strong enough to stop even the fastest electrons from reaching the collector, we know exactly how much kinetic energy they had.
Einstein's Master Equation
Einstein gave us a beautifully simple equation to describe this energy balance:
Here, e is the charge of an electron, Vs is the stopping potential, λhc is the energy of the incoming photon, and ϕ0 is the work function—the minimum energy required just to break the electron free from the metal's grip.
In our problem, we are dealing with the exact same metal surface, which means the work function ϕ0 is a constant. We are given two different scenarios with two different wavelengths of light.
The Art of Elimination
We don't know the work function ϕ0, and frankly, we don't need to! By subtracting the first equation from the second, the pesky ϕ0 completely vanishes, leaving us with a clean relationship between the two stopping potentials:
Dividing everything by e, we isolate our target variable, V2:
V2=V1+ehc(λ21−λ11)
Crunching the Numbers
Now comes the execution phase. We are given V1=0.48 V, λ1=670.5 nm, and λ2=474.6 nm.
First, let's evaluate the constant term ehc. Using standard values (h=6.63×10−34 J s, c=3×108 m/s, and e=1.6×10−19 C), we get:
(Note: Many students use the approximation 1240 eV nm or 1242 eV nm for speed, but using 1243 aligns perfectly with the exact constants provided in typical JEE problems).
Substituting this into our equation:
V2=0.48+1243(474.61−670.51)
Taking the common denominator inside the bracket:
V2=0.48+1243(474.6×670.5670.5−474.6)
V2=0.48+1243(318219.3195.9)
The Physical Intuition
Does this answer make sense? Absolutely! We decreased the wavelength of the incident light from 670.5 nm to 474.6 nm. Because photon energy is inversely proportional to wavelength (E=λhc), the new photons pack a much bigger punch.
With more incoming energy, the ejected electrons fly out with greater kinetic energy. Naturally, it requires a stronger (more negative) stopping potential to halt them. Our calculated stopping potential increased from 0.48 V to 1.25 V, perfectly aligning with the physics of the universe!