Refraction and total internal reflection · Physics… | StemPy Lab
Course 23.1·Lesson 2 of 3
Refraction and total internal reflection
Light bends when it passes from one material to another, and Snell's law n1sinθ1=n2sinθ2
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A spoon that bends in water
Put a spoon in a glass of water and look from the side. The spoon seems to break at the surface. A swimming pool looks shallower than it is. A diamond flashes brighter than a piece of glass of the same shape. In each case light changes direction at a boundary between two materials. This lesson explains how, and why a diamond is special.
Refraction
When a ray of light goes from one material into another, it usually changes direction at the boundary. This is refraction. The cause is the speed. Light travels at c=3.00×108m/s in a vacuum, and more slowly in a material.
The refractive indexn of a material tells us how much it slows light:
n=vc
Here v is the speed of light in the material. The index has no unit, and it is never less than 1. Some typical values for yellow light follow.
Material
Refractive index n
Speed of light in it
Air
1.00
3.00×108m/s
Ice
1.31
2.29×108m/s
Water
1.33
2.26×108m/s
Crown glass
1.50
2.00×108m/s
Flint glass
1.62
1.85×108m/s
Diamond
2.42
1.24×108m/s
These are standard values. Glass varies from one kind to another between about 1.5 and 1.9, and the index of every material changes a little with the colour of the light. Some books write the Greek letter μ for the refractive index. A-Level, IB, AP and the newer NCERT books write n, and so do we.
A material with a larger n is called optically denser. This has nothing to do with its mass density. Some oils are optically denser than water and yet float on it.
What changes and what does not. The wave goes from medium 1 into medium 2. The frequencyf does not change, because the wave crests arrive at the boundary at a fixed rate and must leave at the same rate. The speed changes from v1 to v2. Since v=fλ, the wavelength changes in the same ratio. In a material of index n the wavelength is λ=nλ0, where λ0 is the wavelength in a vacuum.
Example 1: sodium light in water. Sodium light has a wavelength of 589nm in air. In water (n=1.33) its wavelength is 1.33589nm=443nm. Its speed is 1.333.00×108m/s=2.26×108m/s. The frequency stays at 589×10−9m3.00×108m/s=5.09×1014Hz. The colour you see depends on the frequency, so the light is still yellow under water.
Snell's law
Think of a ray that meets a boundary at an angle. We measure the angle of incidenceθ1 and the angle of refractionθ2 from the normal. Snell's law says:
n1sinθ1=n2sinθ2
The incident ray, the refracted ray and the normal lie in one plane. When light goes into a denser material (n2>n1), sinθ2 is smaller than sinθ1, so the ray bends toward the normal. When it goes into a rarer material, it bends away from the normal.
A horizontal line is the surface between air above, medium 1 with refractive index 1.00, and glass below in light blue, medium 2 with refractive index 1.50. A dashed vertical line is the normal. An orange incident ray comes down from the upper left and meets the surface at the foot of the normal. It makes an angle theta 1 of 50 degrees with the normal. A grey dashed reflected ray leaves to the upper right at the same angle. The orange refracted ray goes on into the glass, bent toward the normal, at an angle theta 2 of 30.7 degrees. Coloured arcs mark the two angles. The law n1 sine theta 1 equals n2 sine theta 2 is written at the bottom.
The ratio n1n2 is the refractive index of medium 2 with respect to medium 1, also written n21. It is also equal to v2v1, because n=vc.
Example 2: air into glass. A ray in air meets crown glass (n=1.50) at an angle of incidence of 50°.
We want θ2, so sinθ2=n2n1sinθ1=1.501.00×sin50°=1.500.766=0.511.
So θ2=30.7°.
The ray turned toward the normal. Check. A ray along the normal has θ1=0°, so sinθ2=0 and it goes straight on. This agrees with the picture that a ray at right angles to a boundary does not bend.
Apparent depth
A pool of depth D looks shallower when you look straight down. A ray from a coin at the bottom bends away from the normal as it leaves the water. Your eye follows it back in a straight line and puts the coin higher than it is.
For rays close to the vertical, the angles are small, so sinθ≈tanθ. Call the horizontal distance from the coin to the point where the ray leaves the water x. Then x=Dtanr, and x=D′tani for the apparent depth D′. With sini=nsinr we get
apparent depth=nreal depth
Example 3. A pool is 1.60m deep, so D=1.60m. Its apparent depth is 1.331.60m=1.20m. A swimmer looking up sees the opposite: a bird above the pool seems higher than it is, by the factor n.
Light through a glass slab
A ray goes into a parallel-sided slab and comes out again.
A horizontal glass slab, light blue, 4.0 cm thick with refractive index 1.50, in air. An orange ray comes down from the upper left at 45 degrees to the vertical normal and enters the top face. Inside the glass it bends toward the normal and makes an angle r of 28.1 degrees. It leaves through the bottom face and continues down and to the right at 45 degrees, parallel to the incident ray. A grey dashed line shows the path the ray would have taken with no slab. A short red segment at right angles to the rays, labelled d equals 1.32 cm, shows the sideways shift between the two parallel paths. A 4 cm scale bar is drawn at the lower left.
At the first face the ray bends toward the normal. At the second face it bends away by exactly the same angle. The emergent ray is parallel to the incident ray, but it is shifted sideways. The shift for a slab of thickness t is
d=cosrtsin(i−r)
Example 4. A glass block of thickness t=4.0cm and n=1.50 has a ray at i=45°. Then sinr=1.50sin45°=0.471, so r=28.1°. The shift is d=cos28.1°4.0cm×sin16.9°=1.32cm.
If you look straight through the slab at a mark, the mark seems to rise by t(1−n1). For this block, 4.0cm×31=1.33cm.
Begin with glass above and air below, and an angle of 30°. Slowly raise the angle of incidence. At what angle does the refracted ray vanish? Compare this angle with the critical angle in the readouts.
Total internal reflection
Now send light from a denser material to a rarer one, from glass to air. The ray bends away from the normal, so the angle of refraction is larger than the angle of incidence. Raise the angle of incidence. At one value, the angle of refraction becomes 90° and the refracted ray goes along the surface. This angle is the critical angleC. Put θ2=90° in Snell's law: n1sinC=n2, so
sinC=n1n2
For a material in air, sinC=n1.
A horizontal surface between glass below, in light blue, and air above. A point source S inside the glass sends three rays to the surface. The orange ray meets the surface at 25 degrees to the normal. It passes into the air at 39.3 degrees from the normal and a weak reflected ray, dashed, goes back down. The green ray meets the surface at 41.8 degrees, the critical angle, and the refracted ray grazes along the surface. The purple ray meets the surface at 55 degrees and is totally reflected back into the glass. Dashed vertical normals are drawn at the three points. The labels give the glass as refractive index 1.50, air as 1.00 and the critical angle as 41.8 degrees.
For an angle of incidence larger than C, there is no refracted ray at all. All the light is reflected back into the denser material. This is total internal reflection. It needs two things.
The light must travel from a denser material to a rarer one.
The angle of incidence must be larger than the critical angle.
Critical angles in air: water 48.8°, crown glass 41.8°, flint glass 38.1° and diamond 24.4°. A material with a larger n has a smaller critical angle.
Total internal reflection at work
The diamond. The critical angle of diamond is only 24.4°. Light that enters a cut diamond meets the inside faces at angles larger than this, and it is reflected again and again. It leaves through the top. The jeweller cuts the faces to send as much light as possible back up to the eye. A piece of glass has a larger critical angle, so more light leaks out of the back, and it looks dull.
The optical fibre. A glass fibre as thin as a hair has a core of index n1 inside a cladding of a slightly smaller index n2. Light that meets the boundary of the two at more than the critical angle is totally reflected and travels along the fibre, even when the fibre bends.
A straight optical fibre drawn from left to right. A blue core, refractive index 1.50, is surrounded by a thin grey cladding of refractive index 1.45. A dashed grey line shows the axis outside the fibre at the left. An orange ray enters the flat end face from the lower left at 22.6 degrees to the axis, the acceptance angle, and is refracted into the core. It then zigzags along the fibre, totally reflected each time it meets the core and cladding boundary. A purple ray enters at 30 degrees, which is larger, meets the boundary at a smaller angle than the critical angle and leaks out into the cladding. The text gives the formula sine theta a equals the square root of n1 squared minus n2 squared, which equals 0.384.
Light must enter the end of the fibre at a small enough angle θ to the axis. A ray refracts at the end face, so sinθ=n1sinr. It meets the side wall at the angle 90°−r, and it is trapped when sin(90°−r)≥n1n2. Put these together, and the largest angle, the acceptance angleθa, satisfies
sinθa=n12−n22
For a core of 1.50 and a cladding of 1.45 the right side is 1.502−1.452=0.384, so θa=22.6°. Fibres carry telephone calls, the internet and television, and doctors use them in endoscopes to look inside the body.
The mirage. On a hot day the air close to a road is hotter and thinner than the air above it, so its refractive index is a little smaller. A ray from the sky going down meets layers of smaller and smaller n. It bends away from the normal each time, until at some layer the angle of incidence is larger than the critical angle. The ray turns upward and reaches your eye. You follow it back in a straight line, and you seem to see the sky on the road, like a pool of water.
The totally reflecting prism. A prism with angles 45°, 45° and 90° and made of glass with n=1.50 has a critical angle of 41.8°. A ray that goes into one short face at right angles meets the long face at 45°, which is larger than C, and it is totally reflected.
Two glass prisms in the shape of an isosceles right-angled triangle, light blue, refractive index 1.50, in air. In the left prism the right angle is at the lower left. An orange ray enters the vertical face at right angles, travels to the sloping face, meets it at 45 degrees, which is greater than the critical angle 41.8 degrees, is totally reflected, and leaves the lower face downward at right angles: it is turned through 90 degrees. In the right prism the sloping face is at the bottom. A purple ray enters it from below at right angles, meets the left slanting face at 45 degrees, is reflected horizontally, meets the right slanting face, is reflected again, and leaves downward through the bottom face parallel to its entering path: it is turned through 180 degrees. A 5 cm scale bar is drawn at the top right.
The ray is turned through 90° (left) or, if it goes in through the long face, through 180° (right). Periscopes and binoculars use such prisms, because a prism reflects all the light and a silvered mirror does not. The glass must have n>2=1.41, so that C<45°.
Practise with new numbers
Try it in Python
The program sends a ray at 30° from air into four materials, and finds the critical angle for light that tries to leave each of them for air.
Common mistakes
Measuring angles from the surface. In Snell's law every angle is from the normal.
Taking the sine of the wrong angle. The index n1 goes with the angle in medium 1, and n2 with the angle in medium 2.
Looking for total internal reflection when light goes from air to glass. It happens only from a denser to a rarer material.
Dividing the angle, not its sine, by n. Snell's law is about sines.
Forgetting that the apparent depth is real depth divided by n. An object in a denser material looks nearer than it is.
Saying that the frequency of light changes in glass. The speed and the wavelength change. The frequency does not.
Remember these
Refractive index: n=vc. In a material the wavelength is nλ0 and the frequency does not change.
Snell's law: n1sinθ1=n2sinθ2.
Apparent depth for a view straight down: real depth divided by n. A slab shifts a ray sideways by d=cosrtsin(i−r).
Critical angle: sinC=n1n2. Total internal reflection needs a denser to a rarer material and i>C.
Uses: the sparkle of a diamond, the optical fibre with sinθa=n12−n22, the mirage, and the totally reflecting prism.
Check yourself
Try each one on your own first. If you are stuck, open a hint. Then check with Show the answer.
Find the speed of light in diamond, which has n=2.42.
A ray in air meets water (n=1.33) at 45° to the normal. Find the angle of refraction.
Why does a fish in a pond see a bird above the water higher than the bird really is?
Can light going from water into air at an angle of incidence of 60° be totally reflected? Can light going from air into water at 60°?
Why does a diamond sparkle more than a glass imitation of the same shape?
References
NCERT Physics Part II (Class 12), Chapter 9, the sections on refraction and total internal reflection. Some books round the index of crown glass to 1.5, and others print 1.52.
OpenStax University Physics Volume 3, Chapter 1, the sections on refraction and total internal reflection.
OpenStax College Physics 2e, Chapter 25, the sections on the law of refraction and total internal reflection.
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