Refraction and total internal reflection

Dip a straight stick into a pond and it looks bent at the waterline. Look up from underwater near sunset and the sky above shrinks into a bright circular window, ringed by a mirror-like darkness — beyond that ring the water surface reflects the pond bed back at you instead of showing the sky. Both are the same phenomenon at different angles: light changes direction whenever it crosses into a medium where it travels at a different speed, and past a certain steepness it stops crossing over at all. This article builds the two ideas the Class XII ray-optics syllabus asks for — Snell's law of refraction, worked through a glass slab, and total internal reflection (TIR), the complete return of light beyond a critical angle — and shows why TIR, not a mirror, is what steers light around a periscope prism and down an optical fibre.

The core insight

Light bends according to n21=sin⁡i/sin⁡rn_{21}=\sin i/\sin r when it crosses a boundary, and beyond a critical angle θc\theta_c (where sin⁡θc=1/n\sin\theta_c=1/n) light travelling from a denser to a rarer medium cannot cross the boundary at all and is completely reflected back.

The core idea

Refraction. When a ray of light passes from one transparent medium into another, its speed changes; if it strikes the boundary at an angle to the normal, this change of speed bends its path. The refractive index of medium 2 relative to medium 1 compares the angle of incidence ii in medium 1 with the angle of refraction rr in medium 2 (both measured from the normal to the surface):

n21=sin⁡isin⁡r=v1v2n_{21}=\frac{\sin i}{\sin r}=\frac{v_1}{v_2}

where: ii is the angle of incidence, rr is the angle of refraction, and v1,v2v_1,v_2 are the speeds of light in medium 1 and medium 2. This is Snell's law. The absolute refractive index of a single medium is n=c/vn=c/v, the ratio of the speed of light in vacuum to the speed in that medium — a denser medium (higher nn) always slows light down more.

Lateral displacement through a slab. A ray crossing a parallel-sided rectangular glass slab bends once entering and bends back by an equal amount leaving, so it emerges parallel to the original ray but shifted sideways. For a slab of thickness tt and refractive index nn, with ii the angle of incidence and rr the angle of refraction inside the slab:

d=tsin⁡(i−r)cos⁡rd=\frac{t\sin(i-r)}{\cos r}

where: dd is the perpendicular lateral shift between the incident ray's line and the emergent ray's line, tt is the slab thickness, and i−ri-r is the net bending the ray undergoes on entry (it undoes exactly that bend on exit, which is why the emergent ray is parallel to the incident one).

Total internal reflection. TIR happens only when light travels from a denser medium toward a rarer one (glass to air, water to air) and strikes the boundary steeply enough. As the angle of incidence in the denser medium increases, the refracted ray bends further away from the normal and grows dimmer while the reflected ray grows brighter. At one particular angle, the critical angle θc\theta_c, the refracted ray grazes along the boundary itself, at r=90°r=90°; past that angle no refracted ray exists at all, and essentially all the light is reflected back into the denser medium. Two conditions must both hold for TIR: light must be going from denser to rarer, and the angle of incidence must exceed θc\theta_c. The figure below shows the three regimes at a single boundary: a shallow ray that partly refracts and partly reflects, the critical ray whose refracted beam grazes the surface, and a steep ray beyond θc\theta_c that is totally reflected with no refracted beam at all.

Figure
A glass to air boundary showing three rays from the same point at increasing angles from the normal, a shallow ray that refracts out into the air with a weak reflection, the critical ray whose refracted beam grazes along the boundary at ninety degrees, and a steep ray beyond the critical angle that is totally reflected back into the glass with no refracted beam
Three angles at one boundary: refraction, the critical angle, and TIR air (rarer) glass (denser), refractive index n normal i = 25 degrees refracted (bright) i = critical angle θc refracted ray grazes surface (r = 90°) i greater than θc totally reflected, no refracted ray Reflected part grows brighter as i increases; beyond θc all the light returns into the glass.

Applications. A 45°–45°–90° right-angled prism turns light through 90° or 180° by TIR at its hypotenuse face, since 45° exceeds the critical angle (about 42° for ordinary glass); such totally reflecting prisms replace mirrors in periscopes and binoculars because TIR reflects essentially 100% of the light with no silvering to tarnish. Optical fibres guide light along a thin core of higher refractive index surrounded by cladding of lower refractive index; a ray entering within the fibre's acceptance cone strikes the core–cladding boundary beyond the critical angle every time, undergoes repeated TIR, and travels the full length of the fibre with very little loss.

Derivation AThe critical-angle relation sinθc = 1/n

The goal is to find the exact angle of incidence, measured in the denser medium, at which the refracted ray in the rarer medium grazes the boundary at 90°, since this single angle marks the onset of total internal reflection and is what "critical angle" means; the derivation needs nothing beyond applying Snell's law at that one special orientation.

Step 1. Set up the boundary. Light travels from a denser medium of absolute refractive index nn into a rarer medium, taken to be air with refractive index 1. Let the angle of incidence in the denser medium be θc\theta_c and the angle of refraction in air be rr.

Step 2. Apply Snell's law across this boundary, with the denser medium as the source: nsin⁡θc=1×sin⁡rn\sin\theta_c = 1\times\sin r.

Step 3. Impose the defining condition of the critical angle: at θc\theta_c the refracted ray grazes exactly along the boundary, so r=90°r=90° and sin⁡r=sin⁡90°=1\sin r=\sin 90°=1.

Step 4. Substitute and solve. nsin⁡θc=1n\sin\theta_c=1, so sin⁡θc=1n\sin\theta_c=\dfrac{1}{n}. This gives the critical angle directly from the refractive index of the denser medium; a higher nn produces a smaller critical angle, so a denser medium confines light within a narrower cone before TIR takes over.

Check. For ordinary crown glass, n≈1.5n\approx1.5, so sin⁡θc=1/1.5=0.667\sin\theta_c=1/1.5=0.667 and θc≈41.8°\theta_c\approx41.8°, consistent with the commonly quoted value of about 42°.

Worked example

A ray of light is incident on a rectangular glass slab of refractive index 1.5 and thickness 6 cm at an angle of incidence of 60°.

Step 1. Find the angle of refraction inside the slab using Snell's law, n=sin⁡i/sin⁡rn=\sin i/\sin r, rearranged as sin⁡r=sin⁡i/n\sin r=\sin i/n.

sin⁡r=sin⁡60°1.5=0.8661.5=0.577⇒r≈35.3°\sin r=\frac{\sin 60°}{1.5}=\frac{0.866}{1.5}=0.577 \quad\Rightarrow\quad r\approx35.3°

Step 2. Substitute into the lateral displacement formula with t=6t=6 cm, i=60°i=60°, r=35.3°r=35.3°.

d=tsin⁡(i−r)cos⁡r=6×sin⁡(24.7°)cos⁡35.3°=6×0.4180.816≈3.07 cmd=\frac{t\sin(i-r)}{\cos r}=\frac{6\times\sin(24.7°)}{\cos 35.3°}=\frac{6\times0.418}{0.816}\approx3.07\ \text{cm}

Step 3. Check whether this same glass could support TIR. Its critical angle is θc=sin⁡−1(1/1.5)≈41.8°\theta_c=\sin^{-1}(1/1.5)\approx41.8°. Since this ray meets the far (glass-to-air) face of the slab travelling almost straight through (angle of incidence there equals r≈35.3°r\approx35.3°, well below θc\theta_c), it refracts out normally rather than reflecting — TIR is not triggered inside this slab at this geometry.

Answer. The ray refracts to about 35.3° inside the slab and emerges parallel to the incident ray but laterally shifted by about 3.1 cm.

Competitive stretch

The critical angle for a certain glass–air interface is 42°. A ray inside the glass strikes the surface at 50°. Since n=1/sin⁡42°≈1.495n=1/\sin42°\approx1.495 and the incidence angle (50°) exceeds θc\theta_c (42°) while travelling from the denser glass toward air, the ray cannot refract out at all — it undergoes total internal reflection, leaving the surface at 50° to the normal on the reflected side, obeying the ordinary law of reflection.

Common traps

  • Running TIR in the wrong direction. TIR only ever happens going from a denser medium into a rarer one; a ray travelling from air into glass never totally internally reflects, whatever the angle.
  • Treating the critical angle as "the angle of maximum bending." θc\theta_c is specifically the angle of incidence at which the refracted ray grazes the boundary at exactly 90°, not some vague largest-bend angle.
  • Forgetting the emergent ray from a slab is offset, not superimposed. It is parallel to the incident ray but shifted sideways by dd; it does not return to the same line.
  • Mixing up the direction of n21n_{21}. n21=sin⁡i/sin⁡rn_{21}=\sin i/\sin r is defined for light travelling from medium 1 into medium 2; reversing the direction gives n12=1/n21n_{12}=1/n_{21}.

Ask the tutor: want to see how the lateral-displacement formula is derived step by step from the slab geometry, or work through finding the maximum acceptance angle for light entering an optical fibre?

Why does a totally reflecting prism work better than an ordinary mirror?

An ordinary mirror relies on a thin silvered coating that can tarnish, scratch, or absorb a small fraction of the light at every reflection, gradually dimming and discolouring the image. A 45°–45°–90° glass prism instead uses total internal reflection at its hypotenuse face: since 45° comfortably exceeds the roughly 42° critical angle of ordinary glass, essentially all the light reflects with no coating required and no absorption loss, giving a brighter, cleaner image — which is why periscopes and binoculars favour prisms over mirrors.

Does total internal reflection ever happen with visible light going from air into water?

No. TIR requires travel from a denser medium into a rarer one, and air (refractive index about 1) is less dense optically than water (about 1.33). Light entering water from air only ever refracts, bending toward the normal, however steep the angle of incidence — it never totally reflects. TIR can only occur on the way back out, from water into air, and only beyond water's critical angle of about 48.6°.

How does TIR let an optical fibre carry light around bends without it leaking out?

The fibre's core has a higher refractive index than its surrounding cladding, so any light ray that enters within the fibre's acceptance cone always strikes the core–cladding boundary at an angle beyond that boundary's critical angle. Every single time the ray reaches the boundary, the TIR condition is satisfied and it reflects straight back into the core rather than escaping — even around a gentle bend, as long as the bend is not so sharp that it drives the angle of incidence below the critical angle. The ray effectively bounces down the length of the fibre with almost no light lost at each reflection.

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