Physics · Book 2 · Grades 10–12

High School Physics

High School Physics · Grades 10–12

3Refraction of Light

Dip a straw into a glass of water: it looks snapped at the waterline. Swimming pools are always deeper than they look, diamonds flash colored fire from a colorless stone, and the sentence you are reading probably crossed an ocean inside a glass thread thinner than a hair. One law explains all four — an equality between two sines, found by Snell in 1621 after fifteen centuries of physicists staring at tables of angles without seeing the pattern.

3.1 Reflection: a reminder

In a homogeneous transparent medium, light travels in straight lines — the rays of Chapter 2. At the boundary between two media, part of the light bounces back (reflection) and part crosses over (refraction). Both obey exact geometric laws, stated with one convention: angles are measured from the normal, never from the surface.

Definition 3.1 (Normal and angle of incidence)

At the point where a ray meets a surface, the normal is the line perpendicular to the surface at that point. The angle of incidence i1i_1 is the angle between the incoming ray and the normal; the angles of reflection and of refraction are measured from the normal in the same way.

Proposition 3.2 (Law of reflection)

The reflected ray lies in the plane containing the incident ray and the normal, on the other side of the normal, and the angle of reflection equals the angle of incidence:

i1=i1.i_1' = i_1 .

Proof. Admitted at this level.

Example 3.3 (Reading angles correctly)

A laser beam strikes a mirror “at 3535^\circ” — measured from the mirror’s surface, as beams are often described. The angle of incidence is 9035=5590^\circ - 35^\circ = 55^\circ, so the reflected ray also leaves at 5555^\circ from the normal, and the beam turns by 1802×55=70180^\circ - 2 \times 55^\circ = 70^\circ. Forgetting the normal convention is the most common error of this chapter; it costs 9090^\circ every time.

3.2 Refraction and the refractive index

Hold a pencil in a half-filled glass: it looks broken at the surface. Light from the underwater part changes direction as it leaves the water, so the eye — which assumes straight rays — reconstructs the tip somewhere it is not.

Definition 3.4 (Refraction)

Refraction is the change of direction of light as it crosses the boundary between two transparent media. The ray in the second medium is the refracted ray, and its angle from the normal is the angle of refraction i2i_2.

Refraction happens because light has different speeds in different media; each material is characterized by how much it slows light down.

Definition 3.5 (Refractive index)

The refractive index of a transparent medium is the ratio

n=cv,n = \frac{c}{v},

where c=3.00×108m/sc = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} is the speed of light in vacuum and vv its speed in the medium. Since vcv \leq c, the index satisfies n1n \geq 1; it has no unit. Some useful values:

mediumairwaterplexiglasglassdiamond
nn1.00031.00031.331.331.491.491.501.502.422.42

Example 3.6 (Speed of light in water)

In water, v=cn=3.00×108m/s1.33=2.26×108m/sv = \dfrac{c}{n} = \dfrac{3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}}{1.33} = 2.26 \times 10^{8}\,\mathrm{m}/\mathrm{s}. In diamond, light crawls at 3.00×108m/s/2.42=1.24×108m/s3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/2.42 = 1.24 \times 10^{8}\,\mathrm{m}/\mathrm{s} — less than half its vacuum speed. For air, n=1.0003n = 1.0003 changes the speed by 0.03%0.03\%: in this chapter we treat air as vacuum and take nair=1.00n_{\text{air}} = 1.00.

Theorem 3.7 (Snell’s law of refraction)

The refracted ray lies in the plane of the incident ray and the normal, on the other side of the normal, and the angles of incidence and refraction satisfy

n1sini1=n2sini2,n_1 \sin i_1 = n_2 \sin i_2 ,

where n1n_1 and n2n_2 are the refractive indices of the two media. The path is reversible: light traveling backwards along the refracted ray exits along the incident ray.

Proof. Admitted at this level.

Remark 3.8

The laws of reflection and refraction are stated here as experimental facts. They are honestly derived in the Year 1 volume, where light is treated as a wave: both laws — and the formula n=c/vn = c/v itself — then follow from the wave slowing down in the denser medium.

Incident (blue), reflected (gray) and refracted (red) rays. All angles are measured from the normal (dashed); entering the denser medium (n_2 > n_1), the ray bends toward the normal.
Incident (blue), reflected (gray) and refracted (red) rays. All angles are measured from the normal (dashed); entering the denser medium (n2>n1n_2 > n_1), the ray bends toward the normal.

Example 3.9 (Air to water)

A ray hits a calm pond at i1=30i_1 = 30^\circ. With n1=1.00n_1 = 1.00 and n2=1.33n_2 = 1.33:

sini2=n1sini1n2=sin301.33=0.5001.33=0.376,i2=22.1.\sin i_2 = \frac{n_1 \sin i_1}{n_2} = \frac{\sin 30^\circ}{1.33} = \frac{0.500}{1.33} = 0.376, \qquad i_2 = 22.1^\circ .

The ray bends toward the normal, as it always does when entering a slower medium (n2>n1n_2 > n_1). Leaving the water, the same computation runs backwards and the ray bends away from the normal.

Method 3.10 (Solving a refraction problem)

  1. Draw the surface, the normal, and the ray; identify n1n_1 (medium of the incident ray) and n2n_2.
  2. Check that the given angles are measured from the normal; convert if they are measured from the surface.
  3. Write n1sini1=n2sini2n_1 \sin i_1 = n_2 \sin i_2 and isolate the unknown sine; get the angle with the calculator’s inverse sine, as in the mathematics volume.
  4. Sanity check: the ray bends toward the normal if n2>n1n_2 > n_1, away from it if n2<n1n_2 < n_1, and sini2\sin i_2 must come out between 00 and 11.

The experiment behind the law fits on a desk: a half-disc of plexiglas, a protractor, a laser. Raw angle pairs (i1,i2)(i_1, i_2) look irregular — Ptolemy tabulated them around the year 150 and wrongly concluded that i2i_2 was proportional to i1i_1. Plot sine against sine instead, and the data straighten into a line through the origin of slope n1/n2n_1/n_2: that line is Snell’s law.

Air-to-water measurements for i_1 = 10 to 70: plotted sine against sine, the data align on a line through the origin of slope 1/1.33.
Air-to-water measurements for i1=10i_1 = 10^\circ to 7070^\circ: plotted sine against sine, the data align on a line through the origin of slope 1/1.331/1.33.

Proposition 3.11 (Apparent depth)

An object at depth dd under water, viewed from above at small angles, appears to be at the apparent depth

d=dn,d' = \frac{d}{n} ,

where nn is the index of water. A pool of depth 1.20m1.20\,\mathrm{m} looks only 1.20/1.33=0.90m1.20/1.33 = 0.90\,\mathrm{m} deep — a classic cause of imprudent dives.

Proof. Admitted at this level.

Remark 3.12

The formula follows from Snell’s law applied to the almost-vertical rays reaching the eye; the derivation is done in the Year 1 volume. The direction of the effect needs no formula: rays leaving the water bend away from the normal, so the eye traces them back to a point higher than the object.

3.3 Dispersion: one law per color

A prism turns white sunlight into a rainbow, as the spectra of Chapter 2 showed. Refraction explains why: the refractive index of a medium is not quite the same for every color.

Definition 3.13 (Dispersion)

A medium is dispersive when its refractive index depends on the wavelength of the light. In glass and water, nn is slightly larger for blue light (short wavelength) than for red light (long wavelength) — so blue bends more.

Example 3.14 (Two colors, one surface)

A beam of white light hits crown glass at i1=60i_1 = 60^\circ. For this glass nred=1.51n_{\text{red}} = 1.51 and nblue=1.53n_{\text{blue}} = 1.53. Snell’s law, once per color:

sinired=sin601.51=0.574,ired=35.0;siniblue=sin601.53=0.566,iblue=34.5.\sin i_{\text{red}} = \frac{\sin 60^\circ}{1.51} = 0.574, \quad i_{\text{red}} = 35.0^\circ ; \qquad \sin i_{\text{blue}} = \frac{\sin 60^\circ}{1.53} = 0.566, \quad i_{\text{blue}} = 34.5^\circ .

A single surface splits white light by half a degree — invisible on a window pane, but a prism refracts twice in the same rotational sense, widens the fan, and a few meters away the colors are centimeters apart.

Remark 3.15

The rainbow is the same computation run inside a raindrop: sunlight refracts entering the drop, reflects on its back wall, and refracts again on the way out. Water’s index runs from 1.3311.331 (red) to 1.3431.343 (blue), so each color exits at its own angle — and no two observers see the same rainbow.

3.4 Total internal reflection

Snell’s law contains a trap. Going from water toward air, the refracted ray bends away from the normal: sini2=1.33sini1>sini1\sin i_2 = 1.33 \sin i_1 > \sin i_1. Increase i1i_1, and the formula soon demands sini2>1\sin i_2 > 1, which no angle can deliver. Refraction then simply stops happening.

Definition 3.16 (Critical angle and total internal reflection)

Let light travel in a medium of index n1n_1 toward a medium of smaller index n2<n1n_2 < n_1. The critical angle ici_c is the angle of incidence for which the refracted ray grazes the surface (i2=90i_2 = 90^\circ). For i1>ici_1 > i_c no refracted ray exists: the surface reflects all the light back into the first medium, following the law of reflection. This is total internal reflection.

Proposition 3.17 (Critical angle formula)

For n1>n2n_1 > n_2,

sinic=n2n1.\sin i_c = \frac{n_2}{n_1} .

Proof. Set i2=90i_2 = 90^\circ in Snell’s law: n1sinic=n2sin90=n2n_1 \sin i_c = n_2 \sin 90^\circ = n_2. For i1>ici_1 > i_c, Snell’s law would require sini2=n1n2sini1>1\sin i_2 = \frac{n_1}{n_2}\sin i_1 > 1: no refracted direction exists. (That the light is then entirely reflected — not absorbed — is an experimental fact, confirmed by the wave theory of the Year 1 volume.)

From water toward air, at increasing incidence: refraction away from the normal, then a refracted ray grazing the surface at the critical angle, then total internal reflection — the surface has become a perfect mirror.
From water toward air, at increasing incidence: refraction away from the normal, then a refracted ray grazing the surface at the critical angle, then total internal reflection — the surface has become a perfect mirror.

Example 3.18 (Three critical angles)

Toward air: for water, sinic=1/1.33=0.752\sin i_c = 1/1.33 = 0.752, so ic=48.8i_c = 48.8^\circ; for glass, sinic=1/1.50\sin i_c = 1/1.50, so ic=41.8i_c = 41.8^\circ; for diamond, sinic=1/2.42=0.413\sin i_c = 1/2.42 = 0.413, so ic=24.4i_c = 24.4^\circ. The higher the index, the narrower the escape cone: in diamond, any ray more than 24.424.4^\circ off a facet’s normal is trapped — the secret of its sparkle, dissected in Problem 3.1.

3.5 Optical fibers

Total internal reflection turns a glass thread into a pipe for light: a ray entering nearly parallel to the axis strikes the wall far beyond the critical angle, reflects without loss, and does so millions of times per kilometer without leaking.

Definition 3.19 (Optical fiber)

An optical fiber is a thin glass thread made of a core of index n1n_1 wrapped in a cladding of slightly smaller index n2<n1n_2 < n_1. Light injected at one end travels along the core by repeated total internal reflection on the core–cladding boundary.

Light guided along the core of a fiber by total internal reflection (bounce angles greatly exaggerated: real rays graze the wall at more than 80 from the normal).
Light guided along the core of a fiber by total internal reflection (bounce angles greatly exaggerated: real rays graze the wall at more than 8080^\circ from the normal).

Example 3.20 (A fiber by the numbers)

With n1=1.48n_1 = 1.48 and n2=1.46n_2 = 1.46,

sinic=1.461.48=0.986,ic=80.6:\sin i_c = \frac{1.46}{1.48} = 0.986, \qquad i_c = 80.6^\circ :

only rays within about 99^\circ of the axis are guided — which is fine, since that is exactly how laser light is injected. Inside the core the light travels at v=c/1.48=2.03×108m/sv = c/1.48 = 2.03 \times 10^{8}\,\mathrm{m}/\mathrm{s}: a pulse crosses a 100km100\,\mathrm{km} fiber in about half a millisecond.

Remark 3.21 (Order of magnitude of data links)

Submarine cables — bundles of a few dozen fibers on the ocean floor — carry almost all intercontinental traffic. A single modern fiber transports on the order of 101310^{13} bits per second by sending many wavelengths at once; a whole cable reaches 101410^{14} bits per second, with an amplifier every 80km80\,\mathrm{km} or so. Satellites, for comparison, handle a small fraction of a percent of the traffic.

3.6 Exercises

Exercise 3.1

A laser beam strikes a flat mirror at 2525^\circ from the mirror’s surface. Give the angle of incidence, the angle of reflection, and the angle between the incident and reflected beams.

Solution

Solution of Exercise 3.1.

Angles are measured from the normal: the angle of incidence is 9025=6590^\circ - 25^\circ = 65^\circ, so the angle of reflection is also 6565^\circ. The incident and reflected beams make an angle of 2×65=1302 \times 65^\circ = 130^\circ with each other.

Exercise 3.2

  1. Compute the speed of light in water (n=1.33n = 1.33) and in diamond (n=2.42n = 2.42).
  2. In a certain solid, light travels at 1.97×108m/s1.97 \times 10^{8}\,\mathrm{m}/\mathrm{s}. Compute its refractive index and identify the material.
Solution

Solution of Exercise 3.2.

1. v=c/nv = c/n: in water v=3.00×108m/s/1.33=2.26×108m/sv = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/1.33 = 2.26 \times 10^{8}\,\mathrm{m}/\mathrm{s}; in diamond v=3.00×108m/s/2.42=1.24×108m/sv = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/2.42 = 1.24 \times 10^{8}\,\mathrm{m}/\mathrm{s}.

2. n=cv=3.00×108m/s1.97×108m/s=1.52n = \dfrac{c}{v} = \dfrac{3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}} {1.97 \times 10^{8}\,\mathrm{m}/\mathrm{s}} = 1.52: glass.

Exercise 3.3

A ray in air strikes a glass block (n=1.50n = 1.50) at i1=40i_1 = 40^\circ. Compute the angle of refraction. At what angle would a ray traveling inside the glass have to hit the surface to exit into the air at 4040^\circ?

Solution

Solution of Exercise 3.3.

sini2=sin401.50=0.6431.50=0.429\sin i_2 = \dfrac{\sin 40^\circ}{1.50} = \dfrac{0.643}{1.50} = 0.429, so i2=25.4i_2 = 25.4^\circ. By reversibility of light paths, a ray inside the glass hitting the surface at 25.425.4^\circ exits into the air at exactly 4040^\circ.

Exercise 3.4

Sunlight reaches the surface of a lake at 5555^\circ from the vertical. Compute the angle of the refracted ray, and state whether the ray bends toward or away from the normal — with the one-word reason.

Solution

Solution of Exercise 3.4.

sini2=sin551.33=0.8191.33=0.616\sin i_2 = \dfrac{\sin 55^\circ}{1.33} = \dfrac{0.819}{1.33} = 0.616, so i2=38.0i_2 = 38.0^\circ. The ray bends toward the normal, because water is the slower medium (n2>n1n_2 > n_1).

Exercise 3.5

To identify a clear liquid, a ray is sent onto its surface at i1=45i_1 = 45^\circ; the refracted ray is measured at i2=32i_2 = 32^\circ. Compute the refractive index and identify the liquid from the table of Definition 3.5.

Solution

Solution of Exercise 3.5.

n=sin45sin32=0.7070.530=1.33n = \dfrac{\sin 45^\circ}{\sin 32^\circ} = \dfrac{0.707}{0.530} = 1.33: the liquid is water.

Exercise 3.6 ★★

A half-disc of a transparent plastic gives the following measurements:

i1i_12020^\circ3030^\circ4040^\circ5050^\circ6060^\circ
i2i_213.513.5^\circ19.519.5^\circ25.525.5^\circ31.031.0^\circ35.535.5^\circ
  1. Compute sini1sini2\dfrac{\sin i_1}{\sin i_2} for each pair. What do you observe?
  2. Deduce the refractive index of the plastic and identify it.
  3. Why is plotting sini2\sin i_2 against sini1\sin i_1 a better test of Snell’s law than plotting i2i_2 against i1i_1?
Solution

Solution of Exercise 3.6.

1. The five ratios are

0.3420.233=1.47,0.5000.334=1.50,0.6430.431=1.49,0.7660.515=1.49,0.8660.581=1.49:\frac{0.342}{0.233} = 1.47,\quad \frac{0.500}{0.334} = 1.50,\quad \frac{0.643}{0.431} = 1.49,\quad \frac{0.766}{0.515} = 1.49,\quad \frac{0.866}{0.581} = 1.49 :

constant within measurement error — Snell’s law.

2. n1.49n \approx 1.49: plexiglas.

3. Snell’s law predicts sini2=sini1/n\sin i_2 = \sin i_1 / n: sine against sine, the data must align on a straight line through the origin, which a ruler checks at a glance. Plotted angle against angle, the data lie on a curve; at small angles the curve is deceptively close to a straight line, which is exactly what fooled Ptolemy.

Exercise 3.7 ★★

Compute the critical angle toward air for water, glass (n=1.50n = 1.50) and diamond. Then explain, with Snell’s law, why there is no critical angle for light going from air into water.

Solution

Solution of Exercise 3.7.

sinic=n2/n1\sin i_c = n_2/n_1 with n2=1.00n_2 = 1.00: water sinic=1/1.33=0.752\sin i_c = 1/1.33 = 0.752, ic=48.8i_c = 48.8^\circ; glass sinic=1/1.50=0.667\sin i_c = 1/1.50 = 0.667, ic=41.8i_c = 41.8^\circ; diamond sinic=1/2.42=0.413\sin i_c = 1/2.42 = 0.413, ic=24.4i_c = 24.4^\circ.

From air into water, sini2=sini1/1.331/1.33<1\sin i_2 = \sin i_1/1.33 \leq 1/1.33 < 1 for every incidence: a refracted angle always exists, so nothing special ever happens — total internal reflection needs n1>n2n_1 > n_2.

Exercise 3.8 ★★

  1. A pool is 2.0m2.0\,\mathrm{m} deep. What depth does a swimmer standing at the edge perceive?
  2. A heron eyes a fish swimming 40cm40\,\mathrm{cm} below the surface. At what depth does the fish appear, and should the heron strike above, at, or below the image it sees?
Solution

Solution of Exercise 3.8.

1. d=dn=2.0m1.33=1.5md' = \dfrac{d}{n} = \dfrac{2.0\,\mathrm{m}}{1.33} = 1.5\,\mathrm{m}.

2. The fish appears at 40cm/1.33=30cm40\,\mathrm{cm}/1.33 = 30\,\mathrm{cm}: the image is above the fish, so the heron must strike below the image it sees. Herons, unburdened by Snell’s law, learn this by trial and error.

Exercise 3.9 ★★

A ray hits a window pane (n=1.50n = 1.50, parallel faces) at 5050^\circ.

  1. Compute the angle of refraction at the first face.
  2. The refracted ray hits the second face from inside, at the same angle. Compute the exit angle and compare it with 5050^\circ.
  3. What, then, does a thick window do to the direction and to the position of a ray crossing it?
Solution

Solution of Exercise 3.9.

1. sinr=sin501.50=0.7661.50=0.511\sin r = \dfrac{\sin 50^\circ}{1.50} = \dfrac{0.766}{1.50} = 0.511, so r=30.7r = 30.7^\circ.

2. Glass to air at 30.730.7^\circ: sini2=1.50×0.511=0.766\sin i_2 = 1.50 \times 0.511 = 0.766, so i2=50i_2 = 50^\circ — the exit angle equals the entry angle.

3. The two refractions undo each other: the ray leaves parallel to its original direction, merely shifted sideways. That is why a window does not distort the scene, only (imperceptibly) translates it.

Exercise 3.10 ★★

White light strikes a block of flint glass at 5555^\circ. For this glass, nred=1.61n_{\text{red}} = 1.61 and nblue=1.66n_{\text{blue}} = 1.66. Compute the refraction angles of the red and blue rays and the angle between them. Which color ends up closer to the normal?

Solution

Solution of Exercise 3.10.

sin55=0.819\sin 55^\circ = 0.819. Red: sini2=0.819/1.61=0.509\sin i_2 = 0.819/1.61 = 0.509, i2=30.6i_2 = 30.6^\circ. Blue: sini2=0.819/1.66=0.493\sin i_2 = 0.819/1.66 = 0.493, i2=29.6i_2 = 29.6^\circ. The two colors are separated by 1.01.0^\circ; blue, with the larger index, bends more and ends up closer to the normal.

Exercise 3.11 ★★

An optical fiber has a core of index 1.481.48 and a cladding of index 1.461.46.

  1. Compute the critical angle on the core–cladding boundary.
  2. A guided ray bounces along at exactly the critical angle. Show that over 1.0km1.0\,\mathrm{km} of straight fiber it travels about 14m14\,\mathrm{m} more than a ray going straight down the axis.
Solution

Solution of Exercise 3.11.

1. sinic=1.461.48=0.986\sin i_c = \dfrac{1.46}{1.48} = 0.986, so ic=80.6i_c = 80.6^\circ.

2. A ray at ici_c from the normal makes 90ic90^\circ - i_c with the axis, so its path along an axis length LL is Lsinic\dfrac{L}{\sin i_c}:

1000m×1.481.46=1013.7m,1000\,\mathrm{m} \times \frac{1.48}{1.46} = 1013.7\,\mathrm{m},

about 14m14\,\mathrm{m} more than the axial ray.

Exercise 3.12 ★★★

A diver’s eye is 2.0m2.0\,\mathrm{m} below a perfectly calm surface. Because of refraction, the diver sees the entire sky compressed into a bright disc directly overhead — Snell’s window.

  1. Explain why light from the horizon reaches the diver’s eye at the critical angle of water, 48.848.8^\circ from the vertical.
  2. Compute the radius of the bright disc on the surface, using the tangent in the right triangle eye–vertical–disc edge.
  3. What does the diver see on the surface outside the disc?
Solution

Solution of Exercise 3.12.

1. Light grazing from the horizon arrives at i1i_1 close to 9090^\circ; it refracts to sini2=sin90/1.33=0.752\sin i_2 = \sin 90^\circ / 1.33 = 0.752, i.e. i2=48.8i_2 = 48.8^\circ — the critical angle, as reversibility demands. Rays from the whole sky therefore reach the eye within a cone of half-angle 48.848.8^\circ.

2. The disc’s edge is where that cone meets the surface:

r=dtanic=2.0m×tan48.8=2.0m×1.14=2.3m.r = d \tan i_c = 2.0\,\mathrm{m} \times \tan 48.8^\circ = 2.0\,\mathrm{m} \times 1.14 = 2.3\,\mathrm{m}.

3. Outside the disc, light from below hits the surface beyond the critical angle and is totally reflected: the diver sees a silvery mirror showing the bottom of the pool.

Exercise 3.13 ★★★

A prism has angles 3030^\circ, 6060^\circ, 9090^\circ. A thin beam of white light enters perpendicular to one of the sides adjacent to the right angle, crosses undeviated, and strikes the long face from inside at i1=30i_1 = 30^\circ. For this glass, nred=1.51n_{\text{red}} = 1.51 and nblue=1.53n_{\text{blue}} = 1.53.

  1. Compute the exit angles of the red and blue rays and the angular width of the fan between them.
  2. The prism is replaced by a 4545^\circ4545^\circ9090^\circ prism, so the internal angle of incidence becomes 4545^\circ. Show that no light exits through the long face at all.
Solution

Solution of Exercise 3.13.

1. Red: sini2=1.51×sin30=0.755\sin i_2 = 1.51 \times \sin 30^\circ = 0.755, so i2=49.0i_2 = 49.0^\circ. Blue: sini2=1.53×0.500=0.765\sin i_2 = 1.53 \times 0.500 = 0.765, so i2=49.9i_2 = 49.9^\circ. The white beam fans out over 49.949.0=0.949.9^\circ - 49.0^\circ = 0.9^\circ — a prism spectrum from a single refraction.

2. At 4545^\circ: sini2=1.51×0.707=1.07>1\sin i_2 = 1.51 \times 0.707 = 1.07 > 1 (and 1.53×0.707=1.081.53 \times 0.707 = 1.08 for blue). No refracted angle exists for either color: the critical angle is arcsin(1/1.51)=41.5<45\arcsin(1/1.51) = 41.5^\circ < 45^\circ, so the long face totally reflects the whole beam.

Exercise 3.14 ★★★

Periscopes fold light with 4545^\circ4545^\circ9090^\circ glass prisms (n=1.50n = 1.50): the beam enters one short face perpendicularly and hits the long face from inside at 4545^\circ.

  1. Show that the long face acts as a perfect mirror. Why is this better than a metallic mirror, which absorbs a few percent at each reflection?
  2. The periscope floods and the long face is now in contact with water. Compute the new critical angle of the glass–water boundary and show the mirror fails.
  3. At what angle does the light of question 2 leave the prism into the water?
Solution

Solution of Exercise 3.14.

1. Critical angle glass–air: sinic=1/1.50\sin i_c = 1/1.50, so ic=41.8<45i_c = 41.8^\circ < 45^\circ: the beam is totally reflected — 100%100\% of the light, with no coating to tarnish. A metallic mirror loses a few percent at each bounce, and a periscope needs two.

2. Glass–water: sinic=1.331.50=0.887\sin i_c = \dfrac{1.33}{1.50} = 0.887, so ic=62.5i_c = 62.5^\circ. Now 45<ic45^\circ < i_c: the incidence is below critical, most of the light refracts out into the water, and the mirror — hence the image — fails.

3. sini2=1.501.33×sin45=1.128×0.707=0.798\sin i_2 = \dfrac{1.50}{1.33} \times \sin 45^\circ = 1.128 \times 0.707 = 0.798, so i2=52.9i_2 = 52.9^\circ into the water.

Exercise 3.15 ★★★

A transatlantic cable runs 6200km6200\,\mathrm{km} of fiber (core index 1.471.47) between London and New York.

  1. Compute the speed of light in the core and the one-way travel time of a pulse.
  2. A radio wave travels at cc. How long would it need over the same distance, and how much round-trip time does the fiber’s glass cost compared with radio?
  3. Some financial firms pay fortunes to shave milliseconds off this link. Propose two distinct physical ways to make the light arrive earlier.
Solution

Solution of Exercise 3.15.

1. v=3.00×108m/s1.47=2.04×108m/sv = \dfrac{3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}}{1.47} = 2.04 \times 10^{8}\,\mathrm{m}/\mathrm{s}, so

t=6.2×106m2.04×108m/s=30.4ms30ms.t = \frac{6.2 \times 10^{6}\,\mathrm{m}}{2.04 \times 10^{8}\,\mathrm{m}/\mathrm{s}} = 30.4\,\mathrm{ms} \approx 30\,\mathrm{ms}.

2. Radio: t=6.2×106m/3.00×108m/s=20.7mst = 6.2 \times 10^{6}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} = 20.7\,\mathrm{ms}. The glass costs 30.420.7=9.7ms30.4 - 20.7 = 9.7\,\mathrm{ms} each way, about 19ms19\,\mathrm{ms} per round trip.

3. Lower the index — hollow-core fibers guide light through air (n1.00n \approx 1.00), and microwave links through the atmosphere do the same — or shorten the path: a cable laid closer to the great-circle route between the two cities. Both are actually sold, at prices per millisecond.

3.7 Problem: The diamond, the pool and the fiber

Problem 3.1

Weekend problem — three lives of Snell’s law: a pool that lies about its depth, a stone cut so that light cannot leave, and the sixty-millisecond ocean under the internet

One equality of two sines, three careers. In a swimming pool it cheats your eyes about depth and squeezes the whole sky into a circle. In a diamond, pushed to its breaking point, it refuses to let light out — and jewelers have cut stones around that refusal for centuries. Under the Atlantic it guides laser pulses inside a strand of glass, and sets the speed limit of the global internet. This problem works through the three lives in order, with the same law each time.

Part I — Warming up.

  1. Compute the speed of light in water (n=1.33n = 1.33) and in diamond (n=2.42n = 2.42). By what factor does diamond slow light down?
  2. A ray in air strikes a pond at i1=40i_1 = 40^\circ. Compute the angle of refraction.
  3. A ray in the water hits the surface from below at 28.928.9^\circ. At what angle does it exit into the air? State the principle this illustrates.
  4. Compute the critical angle of the water–air boundary, and describe what happens to an underwater ray hitting the surface at 6060^\circ.
  5. The index of air is 1.00031.0003. Compute the speed of light in air and justify the approximation nair=1.00n_{\text{air}} = 1.00 used throughout.

Part II — The pool.

  1. A pool is 3.0m3.0\,\mathrm{m} deep. Using the apparent-depth formula (Proposition 3.11), compute the depth a person standing above perceives.
  2. Explain with a two-ray sketch (described in words) why a coin on the bottom seems to rise: what do rays leaving the water do, and where does the eye place their intersection?
  3. A diver’s eye is at 3.0m3.0\,\mathrm{m}. Compute the radius of Snell’s window — the bright disc through which the diver sees the whole sky (Exercise 3.12).
  4. A lamp on the bottom sends rays upward at 3030^\circ, 4545^\circ and 5050^\circ from the vertical. For each ray, say whether it escapes and at what angle, or what happens instead.
  5. A spear-fisher on the bank aims at a fish. Should the strike be aimed above, at, or below the fish’s image — and does the fish, looking back, see the fisher displaced too?

Part III — The diamond.

  1. Compute the critical angle of diamond (n=2.42n = 2.42) toward air, and compare it with that of glass (n=1.52n = 1.52), which is 41.141.1^\circ.
  2. A ray inside the stone hits a facet at 3030^\circ from its normal. What happens in the diamond? In the glass imitation? Explain in one sentence why the cut of a diamond, combined with its tiny critical angle, produces the sparkle.
  3. Diamond is also strongly dispersive: nred=2.41n_{\text{red}} = 2.41, nblue=2.45n_{\text{blue}} = 2.45. White light enters a facet at 4545^\circ; compute the refraction angle for each color and the angular split.
  4. Later, red and blue rays both reach an exit facet from inside at 17.017.0^\circ. Compute the two exit angles and the split of the emerging fan. Compare with the split at entry: what happens to dispersion near the critical angle?
  5. A drop of water (n=1.33n = 1.33) coats a facet. Compute the new critical angle of the diamond–water boundary, decide the fate of the 3030^\circ ray of question 12, and explain why jewelers keep diamonds scrupulously clean.

Part IV — The fiber.

  1. A fiber has a core of index 1.481.48 and a cladding of index 1.461.46. Compute the critical angle on the core–cladding boundary.
  2. A bare glass thread in air would have a critical angle of 42.542.5^\circ — seemingly far better. Give two reasons the cladding is used anyway. (Think about dust, scratches, and what touching the surface would do to total internal reflection.)
  3. Compute the speed of light in the core, then the one-way travel time of a pulse along 6000km6000\,\mathrm{km} of fiber.
  4. A ray bouncing at exactly the critical angle travels 1/sinic1/\sin i_c times the length of the axis. Compute the extra distance over the 6000km6000\,\mathrm{km} and the extra time it costs.
  5. The punchline. A modern fiber pair carries about 101310^{13} bits per second, and this book is about 2.4×1082.4 \times 10^8 bits. Compute the round-trip (“ping”) time across the ocean and the number of copies of this book the fiber moves per second — then state, in one sentence, what Snell’s law does for the internet.
Solution

Solution of Problem 3.1.

1. vwater=3.00×108m/s/1.33=2.26×108m/sv_{\text{water}} = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/1.33 = 2.26 \times 10^{8}\,\mathrm{m}/\mathrm{s}; vdiamond=3.00×108m/s/2.42=1.24×108m/sv_{\text{diamond}} = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/2.42 = 1.24 \times 10^{8}\,\mathrm{m}/\mathrm{s} — diamond slows light by the factor n=2.42n = 2.42.

2. sini2=sin40/1.33=0.643/1.33=0.483\sin i_2 = \sin 40^\circ / 1.33 = 0.643/1.33 = 0.483, so i2=28.9i_2 = 28.9^\circ.

3. sini2=1.33×sin28.9=1.33×0.483=0.643\sin i_2 = 1.33 \times \sin 28.9^\circ = 1.33 \times 0.483 = 0.643, so i2=40i_2 = 40^\circ: light retraces its path — reversibility of light rays.

4. sinic=1/1.33=0.752\sin i_c = 1/1.33 = 0.752, so ic=48.8i_c = 48.8^\circ. At 60>ic60^\circ > i_c, Snell’s law would need sini2=1.33sin60=1.15>1\sin i_2 = 1.33 \sin 60^\circ = 1.15 > 1: no refracted ray; the surface totally reflects the light back down.

5. v=3.00×108m/s/1.0003=2.999×108m/sv = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/1.0003 = 2.999 \times 10^{8}\,\mathrm{m}/\mathrm{s}: light in air is slower than in vacuum by 0.03%0.03\%, far below the precision of our angle measurements, so nair=1.00n_{\text{air}} = 1.00 is harmless.

6. d=3.0m/1.33=2.3md' = 3.0\,\mathrm{m}/1.33 = 2.3\,\mathrm{m}: the pool hides 70cm70\,\mathrm{cm} of itself.

7. Two rays leaving the coin refract at the surface, bending away from the normal, so they diverge more steeply above the water than below. The eye prolongs the two exiting rays backwards in straight lines; they cross above the coin, and that crossing is where the eye places the image.

8. r=dtanic=3.0m×tan48.8=3.0m×1.14=3.4mr = d \tan i_c = 3.0\,\mathrm{m} \times \tan 48.8^\circ = 3.0\,\mathrm{m} \times 1.14 = 3.4\,\mathrm{m}: a disc about 6.9m6.9\,\mathrm{m} across holds the entire sky.

9. At 3030^\circ: sini2=1.33×0.500=0.665\sin i_2 = 1.33 \times 0.500 = 0.665, the ray exits at 41.741.7^\circ. At 4545^\circ: sini2=1.33×0.707=0.940\sin i_2 = 1.33 \times 0.707 = 0.940, it exits at 70.170.1^\circ, nearly grazing. At 5050^\circ: 1.33×0.766=1.02>11.33 \times 0.766 = 1.02 > 1total internal reflection, the ray dives back into the pool.

10. The image is above the real fish (Proposition 3.11), so aim below it. And yes: the fish sees the fisher displaced too, squeezed toward the vertical inside Snell’s window — each sees the other where the other is not.

11. Diamond: sinic=1/2.42=0.413\sin i_c = 1/2.42 = 0.413, so ic=24.4i_c = 24.4^\circ, against 41.141.1^\circ for glass: diamond’s escape cone is not even half as wide.

12. In diamond, 30>24.430^\circ > 24.4^\circ: total internal reflection, the ray stays in the stone. In glass, 30<41.130^\circ < 41.1^\circ: the ray leaks out the back. The facets of a brilliant cut are angled so that entering light almost always strikes them beyond 24.424.4^\circ and bounces until it exits upward toward the eye — a glass imitation, with its wide escape cone, simply lets the light fall through.

13. sin45=0.707\sin 45^\circ = 0.707. Red: 0.707/2.41=0.2930.707/2.41 = 0.293, so i2=17.1i_2 = 17.1^\circ. Blue: 0.707/2.45=0.2890.707/2.45 = 0.289, so i2=16.8i_2 = 16.8^\circ. Split at entry: about 0.30.3^\circ.

14. sin17.0=0.292\sin 17.0^\circ = 0.292. Red: sini2=2.41×0.292=0.705\sin i_2 = 2.41 \times 0.292 = 0.705, so i2=44.8i_2 = 44.8^\circ. Blue: sini2=2.45×0.292=0.716\sin i_2 = 2.45 \times 0.292 = 0.716, so i2=45.8i_2 = 45.8^\circ. The fan is now 1.01.0^\circ wide: the exit refraction, working near the critical angle, stretched the 0.30.3^\circ entry split threefold. That stretched spray of colors is the diamond’s fire.

15. Diamond–water: sinic=1.33/2.42=0.550\sin i_c = 1.33/2.42 = 0.550, so ic=33.3i_c = 33.3^\circ. The 3030^\circ ray, trapped when the facet faced air, now escapes (30<33.330^\circ < 33.3^\circ) into the water film: every drop, fingerprint or film of grease raises the outside index, widens the escape cone and drains the sparkle — hence the jeweler’s cloth.

16. sinic=1.461.48=0.986\sin i_c = \dfrac{1.46}{1.48} = 0.986, so ic=80.6i_c = 80.6^\circ.

17. Total internal reflection happens at the surface, so the surface must stay perfect: on a bare thread, every speck of dust, scratch, water drop or touching finger raises the outside index at that point and bleeds light out. The cladding buries the mirror inside clean glass where nothing can reach it — and, as a bonus, protects the hair-thin core mechanically.

18. v=3.00×108m/s/1.48=2.03×108m/sv = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}/1.48 = 2.03 \times 10^{8}\,\mathrm{m}/\mathrm{s}, so

t=6.0×106m2.03×108m/s=29.6ms30ms.t = \frac{6.0 \times 10^{6}\,\mathrm{m}}{2.03 \times 10^{8}\,\mathrm{m}/\mathrm{s}} = 29.6\,\mathrm{ms} \approx 30\,\mathrm{ms}.

19. Path factor 1/sinic=1.48/1.46=1.01371/\sin i_c = 1.48/1.46 = 1.0137: at worst 6000km×0.013782km6000\,\mathrm{km} \times 0.0137 \approx 82\,\mathrm{km} of extra glass, costing 8.2×104m/2.03×108m/s0.4ms8.2 \times 10^{4}\,\mathrm{m} / 2.03 \times 10^{8}\,\mathrm{m}/\mathrm{s} \approx 0.4\,\mathrm{ms} — the zigzag is nearly free.

20. Ping: 2×(29.6+0.4)60ms2 \times (29.6 + 0.4) \approx 60\,\mathrm{ms}. Throughput: 10132.4×10840000\dfrac{10^{13}}{2.4 \times 10^8} \approx 40\,000 copies of this book per second. In one sentence: by trapping light inside glass through total internal reflection, Snell’s law carries a library across the ocean every second, sixty milliseconds there and back.