Imagine a light wave traveling through the emptiness of a vacuum and suddenly hitting a denser medium, like a block of glass. What happens to its properties? This is a classic scenario in optics that tests our understanding of the fundamental nature of waves.
The Wavelength Compression
When light enters a denser medium, it slows down. This is a direct consequence of the medium's optical density, quantified by its refractive index, μ. However, the frequency of the light—the number of wave cycles passing a point per second—is a fundamental property of the source emitting the light. It acts like the heartbeat of the wave and does not change when crossing boundaries.
Because the speed decreases but the frequency remains constant, the waves get "bunched up" or compressed. The new wavelength in the medium is simply the original wavelength in a vacuum divided by the refractive index:
Let's plug in the numbers from our problem. The original wavelength is 6000 A˚, and the refractive index is 1.5:
λmedium=1.56000=4000 A˚
So, the wavelength in the medium is compressed to 4000 A˚.
The Unchanging Frequency
Now, what about the frequency? As we discussed, frequency remains constant across boundaries. We can calculate it using the speed of light in a vacuum (c) and the original wavelength in a vacuum (λvacuum), using the universal wave equation c=fλ:
The speed of light is 3.0×108 m/s. The wavelength is 6000 A˚, which we must convert to meters. Since 1 A˚=10−10 m, the wavelength is 6000×10−10 m, or 6.0×10−7 m.
Dividing the numbers gives us:
f=0.5×1015 Hz=5.0×1014 Hz
The Core Takeaway
Always remember this golden rule of wave mechanics: Frequency is the heartbeat of the wave, set by the source. It never changes when crossing boundaries. However, the speed and wavelength are properties dictated by the medium, and they will change proportionally to keep the frequency constant.