Electromagnetic Waves in Matter
Electromagnetic waves propagate through matter as well as vacuum, but with a modified speed $v=c/n$ where $n=\sqrt{\varepsilon_r\mu_r}$ is the index of refraction. At boundaries between media, waves are partially reflected and partially transmitted according to the Fresnel equations. Dispersion — the frequency-dependence of $n$ — is the origin of rainbows.
Key Concepts
Key Equations
Reflection at Glass-Air Interface
Light travels from glass () to air () at normal incidence. Find the reflectance and the critical angle .
Exercises
7 problemsDrag the slider — the wave on the right slows down and its wavelength shrinks by factor $n$. Find the speed v = c/n in glass ($n = 1.50$) in m/s (enter 2e8).
Drag n — the wave on the right slows AND its wavelength shrinks by factor n. Frequency stays the same.
Enter 2e8 or 200000000 (m/s)
Drag $n_2$ and watch the reflected ray grow brighter. At air→glass ($n_1=1.0$, $n_2=1.5$), find the reflectance R = ((n₁−n₂)/(n₁+n₂))² (enter as decimal, e.g. 0.04).
Drag n₂ — as the contrast increases, more light reflects. At n₁=1.0 (air) to n₂=1.5 (glass), only 4% reflects.
R = ((1.0−1.5)/(1.0+1.5))² = ? Enter as decimal (e.g. 0.04)
Critical angle for total internal reflection from glass () to air (). (in degrees).
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Upgrade to Pro →A light wave in vacuum has nm. In glass (), find (in nm).
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Upgrade to Pro →Snell's law: light goes from water () to glass () at . Find (in degrees). .
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Upgrade to Pro →Brewster's angle for air-glass (): . Find (in degrees).
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Upgrade to Pro →An optical fiber has core and cladding . Find the numerical aperture .
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Upgrade to Pro →Key Takeaways
- EM waves travel at in a medium; frequency is unchanged, wavelength is .
- Fresnel equations give reflection and transmission at interfaces; (for energy).
- Total internal reflection occurs when with .
- Brewster's angle: at , reflected light is perfectly -polarized.