The beauty of Young's Double Slit Experiment (YDSE) lies in its delicate sensitivity to phase differences. Even the slightest change in the optical path of one of the interfering waves can dramatically alter the interference pattern observed on the screen. In this problem, we explore exactly such a scenario, where a thin mica sheet acts as the disruptor, and we use the resulting shift to deduce the wavelength of the light itself.
Analyzing the Setup
Imagine the standard YDSE setup. Two coherent light waves emerge from slits S1 and S2 and travel towards a screen at a distance D. When a transparent mica sheet of thickness t and refractive index μ is introduced in front of one of the slits, it forces the light wave to travel through a denser medium.
Because light travels slower in the mica sheet compared to air, it takes longer for that specific wave to reach the screen. This introduces an additional optical path length of (μ−1)t. To compensate for this "delay" and maintain a zero phase difference for the central maximum, the entire fringe pattern shifts towards the slit covered by the sheet.
The Master Equation
The physical distance by which the fringe pattern shifts on the screen is given by the well-known formula:
Here, d is the separation between the two slits. Notice that this shift is independent of the wavelength of the light! It only depends on the properties of the slab and the geometry of the setup.
Next, the problem introduces a twist. The mica sheet is removed, restoring the original symmetry, but the screen is moved twice as far away, to a new distance of 2D.
In this new configuration, the distance between successive maxima—which is simply the fringe width ω′—is given by:
Equating and Solving
The core of the problem lies in a single, elegant condition: the initial fringe shift Δy is exactly equal to the new fringe width ω′. Let's set them equal to each other:
Look at how beautifully the geometric factors D and d cancel out from both sides! This leaves us with a pure relationship between the optical properties:
Rearranging to solve for the unknown wavelength λ:
Final Calculation
Now, it's just a matter of plugging in the given values. We know the refractive index μ=1.6 and the thickness t=1.964×10−6 m.
To express this in a more standard unit for wavelength, we convert meters to Angstroms (A˚). Since 1 m=1010 A˚:
And there we have it! By simply observing the macroscopic shift of fringes on a screen, we have successfully measured the microscopic wavelength of the light.