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Questions on refraction and Snell's law
Refractive index compares the speed of light in a vacuum with its speed in a material, and Snell's law uses that ratio to predict the angle of refraction. Frequency survives a boundary; speed and wavelength do not. Tracing a ray through a glass block at several angles and plotting sin θ₁ against sin θ₂ measures the index as the gradient.
21 original questions · 65 marks · the refraction and Snell's law notes · Waves
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These questions cover both lessons on refraction and total internal reflection: Refraction and Snell's law and Total internal reflection and optical fibres.
This topic is tagged for AQA, Edexcel, OCR A.
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Define the refractive index of a material in terms of the speed of light.
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Refractive index n = speed of light in a vacuum / speed of light in the material = c/v (1). It is always greater than or equal to 1 (1).Light travels at 2.0 × 108 m s−1 in a glass block. Calculate the refractive index of the glass.
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n = c/v = (3.0 × 108)/(2.0 × 108) (1)
n = 1.5 (1)State the two conditions required for total internal reflection to occur.
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The light must be travelling in the more optically dense medium (higher n) towards the boundary with a less dense one (1), and the angle of incidence must exceed the critical angle (1).A ray of light passes from air into a glass block. State what happens, if anything, to the speed, the frequency and the wavelength of the light.
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The speed decreases and the wavelength decreases in the same ratio (1). The frequency is unchanged (1).Explain why light travelling from air into glass can never be totally internally reflected at the boundary, however large the angle of incidence.
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Total internal reflection requires the light to be travelling towards a medium of lower refractive index (1). Air has a lower refractive index than glass, so this light is heading into the denser medium and no critical angle exists: sin θc = n2/n1 would be greater than 1 (1).A ray of light passes from air into glass of refractive index 1.5 at an angle of incidence of 40°. Calculate the angle of refraction.
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n1 sinθ1 = n2 sinθ2 (1)
sinθ2 = sin 40°/1.5 (1)
θ2 = 25.4° (1)Calculate the critical angle for a glass–air boundary where the glass has a refractive index of 1.5.
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sinθc = 1/n = 1/1.5 (1)
θc = 41.8° (1)Light of wavelength 600 nm in air enters glass of refractive index 1.5. Calculate its wavelength and speed in the glass.
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λglass = λ/n = 600/1.5 (1)
= 400 nm (1)
v = c/n = (3.0 × 108)/1.5 = 2.0 × 108 m s−1 (1)A ray of light travels from water (refractive index 1.33) into air, meeting the surface at an angle of incidence of 30° in the water. Calculate the angle of refraction in the air.
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n1 sinθ1 = n2 sinθ2 (1)
1.33 × sin 30° = 1 × sinθ2 (1)
θ2 = 41.7° (1)A ray of sunlight strikes the flat surface of a pond at 25° to the water surface. The refractive index of the water is 1.33. Calculate the angle of refraction in the water.
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The angle of incidence is measured from the normal: θ1 = 90° − 25° = 65° (1). sinθ2 = sin 65°/1.33 (1), so θ2 = 43.0° (1).A ray of light passes from crown glass of refractive index 1.52 into flint glass of refractive index 1.66. The angle of incidence at the boundary is 50°. Calculate the angle of refraction, and state which way the ray bends.
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n1 sinθ1 = n2 sinθ2: sinθ2 = 1.52 × sin 50°/1.66 (1), so θ2 = 44.5° (1). The ray bends towards the normal because it enters the optically denser medium, where light travels more slowly (1).State what is meant by modal dispersion in a step-index optical fibre, and give one design feature that reduces it.
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Rays reflecting along the fibre at different angles travel different total distances, so parts of a pulse arrive at different times and the pulse broadens (1). A very narrow core reduces it by forcing all rays onto nearly the same path (1).A student measures the refractive index of a glass block by tracing rays through it. For six angles of incidence she plots sin θ1, the sine of the angle in the air, against sin θ2, the sine of the angle in the glass. Her line of best fit passes through the origin and through the point at which sin θ2 = 0.41 and sin θ1 = 0.62. Determine the refractive index of the glass, and state what the line passing through the origin shows.
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Air has n = 1.00, so for a ray going from air into the solid Snell's law reduces to n = sin θ1/sin θ2 (1). The gradient of the graph is therefore n, and it must be read from the line of best fit rather than from any single plotted point (1). n = 0.62/0.41 = 1.5 (1). A straight line through the origin shows that sin θ1 is proportional to sin θ2, which is Snell's law itself (1).An optical fibre has a core of refractive index 1.50 and a cladding of refractive index 1.40. Calculate the critical angle at the core–cladding boundary.
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sinθc = ncladding/ncore (1)
= 1.40/1.50 (1)
θc = 69.0° (1)A ray inside a glass block (refractive index 1.5) strikes a face at an angle of incidence of 45°. Deduce whether the ray is totally internally reflected or refracted out of the block.
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sinθc = 1/n = 1/1.5 (1)
θc = 41.8° (1)
45° is greater than the critical angle, so the ray undergoes total internal reflection and does not leave the block (1)Describe the structure of a step-index optical fibre and state the purpose of the cladding.
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It has a central core of high refractive index surrounded by a cladding of slightly lower refractive index (1). The cladding gives a well-defined boundary for total internal reflection (1), protects the core, and reduces signal loss and crossover between fibres (1).A manufacturer is designing a step-index optical fibre with a core of refractive index 1.52. To limit modal dispersion, the critical angle at the core–cladding boundary must be at least 80°. Three cladding glasses are available: P (refractive index 1.38), Q (refractive index 1.45) and R (refractive index 1.50). Deduce which cladding the manufacturer should choose.
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sinθc = ncladding/ncore (1). For P: θc = 65.2°; for Q: θc = 72.5° (1); for R: θc = 80.7° (1). Only R gives a critical angle of at least 80°, so the manufacturer should choose cladding R (1).A straight optical fibre is 15 km long and its core has a refractive index of 1.48. The speed of light in a vacuum is 3.0 × 108 m s−1. Show that light travels along the core at about 2 × 108 m s−1. Go on to calculate the minimum time for a light pulse to travel the length of the fibre.
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v = c/n = (3.0 × 108)/1.48 (1) = 2.03 × 108 m s−1, which is about 2 × 108 m s−1 (1). t = d/v = (15 × 103)/(2.03 × 108) (1) = 7.4 × 10−5 s (1).A step-index optical fibre carries digital data as short pulses of light. Explain the two causes of pulse broadening in the fibre, state how the design of the fibre and the choice of light source reduce each one, and explain why pulse broadening limits the rate at which data can be sent.
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Modal dispersion: rays reflecting at different angles travel different total path lengths along the fibre (1), so parts of the same pulse arrive at different times and the pulse spreads out (1). A very narrow core reduces this by forcing every ray onto nearly the same path (1). Material dispersion: different wavelengths travel at slightly different speeds in the glass, so a pulse of non-monochromatic light spreads in time (1); using monochromatic light (a single wavelength, for example from a laser) removes this spread (1). Broadened pulses can overlap their neighbours so that individual pulses can no longer be distinguished; pulses must therefore be sent less often, limiting the data rate (1).A student is given a rectangular glass block, a sheet of paper, four optical pins and a protractor. Describe how she obtains one pair of values of θ1 and θ2, the angles the ray makes with the normal in the air and in the glass, and explain why she repeats the measurement at several different angles of incidence.
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Lay the block on the paper, draw round its outline, mark a point on one long face and rule the normal at that point (1). Push two pins into the paper in line with a ray entering at that point, mark the incident ray, and measure θ1 between it and the normal (1). Look through the block from the far side and push in two more pins so that all four appear in a line through the glass, then mark the emergent ray (1). Lift the block off and join the entry point to the exit point: that line is the path the light took inside the block, which could not be watched directly, and θ2 is measured between it and the normal (1). One tracing gives one value of n, and a poor one; taking six angles spread between about 20° and 70° and plotting them lets a line of best fit average the readings, and the graph tests Snell's law at the same time (1).A step-index optical fibre has a core of refractive index 1.50 and cladding of refractive index 1.47. A ray travelling inside the core meets the core-cladding boundary while travelling at 8.0° to the axis of the fibre. Deduce whether this ray is totally internally reflected at the boundary.
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The normal to the boundary is at right angles to the axis, so the angle of incidence at the wall is 90° − 8.0° = 82.0° (1). sinθc = ncladding/ncore = 1.47/1.50 (1), so θc = 78.5° (1). The angle of incidence 82.0° is greater than the critical angle, so the ray is totally internally reflected and stays in the core (1).
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