Before you tackle the traps, look at the boundary itself — because almost every trap below is really a misreading of this one picture.
Read the figure left to right. In the leftmost panel the incidence angle θ1 is small: the light crosses into the rarer medium and bends away from the normal, so θ2>θ1. As you slide θ1 up (middle panel), the refracted ray tips further and further toward the surface. In the right panel θ1 has reached the exact value where the refracted ray lies flat along the boundary — that is θ2=90°, and that incidence angle is θc.
Where the formula comes from — a wavefront argument, not a memorised rule. Snell's law n1sinθ1=n2sinθ2 is just the statement that wavefronts stay continuous along the boundary (see Snell's Law). Plug in the grazing condition θ2=90°, for which sin90°=1:
n1sinθc=n2⋅1⟹sinθc=n1n2
So the formula is nothing more than "the refracted ray has run out of room to bend." Since we need n1>n2 (dense→rare), the right side is always less than 1, which is exactly why a valid angle exists. Keep this panel in mind — the "flat refracted ray" picture is the anchor for every item below.
TIR can occur when light travels from a rarer medium into a denser medium.
False — with n1<n2 we get sinθ2=n2n1sinθ1<1 for every θ1, so a real refracted ray always exists and refraction never ceases.
At exactly θ1=θc, all the light is already totally internally reflected.
False — at exactly θc the refracted ray still exists but grazes the surface at θ2=90°; TIR (100% reflection) begins only for θ1strictly greater than θc.
A larger refractive index of the denser medium gives a larger critical angle.
False — sinθc=n2/n1, so raising n1 shrinks the fraction and hence θc; that is why diamond (n=2.42, θc≈24°) traps light far more easily than glass.
The critical angle depends only on the denser medium's index.
False — it depends on the ration2/n1; the same glass has one θc against air and a completely different one against water.
Below the critical angle, no light reflects at the boundary at all.
False — some light always reflects (partial reflection happens at every boundary); below θc most energy is transmitted, and the reflected fraction merely grows as θ1 approaches θc.
If two media have equal refractive indices, there is no critical angle.
True — with n1=n2, sinθc=1 so θc=90°; light never bends and can never be trapped, so TIR effectively cannot occur.
TIR only reflects part of the light; some always leaks through.
False — beyond θc100% of the energy is reflected (ideally); no ordinary refracted ray carries away time-averaged energy, which is exactly what "total" means.
Beyond the critical angle the electromagnetic field is exactly zero on the far side of the boundary.
False — a non-propagating evanescent field exists just past the surface, decaying exponentially over a fraction of a wavelength; it carries no net energy across, so reflection is still total (see the edge-case section).
Total internal reflection is the same phenomenon as the reflection off a metal mirror.
False — a metal mirror absorbs a few percent each bounce, while TIR is essentially lossless; this is why fibre optics and prisms use TIR rather than metallic coatings.
"sinθc=n1/n2, since the incident medium is written first."
The ratio is flipped. Setting θ2=90° in n1sinθc=n2sin90° gives sinθc=n2/n1 — rarer over denser, which is correctly less than 1.
"Light going from air into glass can undergo TIR if the angle is steep enough."
Backwards direction. Air→glass is rarer→denser, so no critical angle exists on that side; TIR needs the light to be inside the denser medium hitting the boundary.
"The critical angle is where the reflected ray is exactly 90° from the incident ray."
That describes Brewster's condition — at θB the reflected and refracted rays are perpendicular (θB+θ2=90°), which polarizes the reflection. The critical angle is different: it is defined by the refracted ray grazing at θ2=90°, a statement about refraction ceasing, not about polarization (see Brewster's Angle).
"Since sinθc=n2/n1, a fibre core with n=1.0 against air would trap light perfectly."
With n1=1.0=n2 the fraction is 1 and θc=90°; nothing is trapped. A working fibre needs a core denser than its cladding (see Optical Fibres).
"θc=sin−1(1.4/1.2) for light going from n1=1.2 to n2=1.4."
The argument 1.4/1.2>1 has no valid arcsine — the tell that this direction (rarer→denser) admits no critical angle at all, so the setup is invalid.
"Refraction still happens beyond θc, it just bends more than 90°."
There is no such thing as bending "more than 90°" for a transmitted ray — that would put it back on the incident side. Snell demands sinθ2>1, which is impossible, so refraction genuinely stops (see Refraction of Light).
Why does the refracted ray reach 90°before the incident ray does, as θ1 grows?
Because dense→rare gives sinθ2=n2n1sinθ1 with n1/n2>1, so θ2>θ1 always; θ2 races ahead and hits its ceiling of 90° while θ1 is still smaller.
Why is θ2=90° chosen as the defining condition for θc?
Because 90° is the largest possible refraction angle — the ray lying flat along the surface (rightmost panel of the figure). Any demand for a larger θ2 is geometrically impossible, so this is the exact tipping point where refraction can no longer exist.
Why do diamonds sparkle more than glass gems of the same cut?
Diamond's high index (2.42) gives a small θc≈24°, so most internal rays exceed it and bounce many times inside before escaping, concentrating and delaying the light before release.
Why must sinθc always come out less than 1 for a valid critical angle?
Because sinθc=n2/n1 and TIR requires n1>n2 (denser to rarer); a value ≥1 signals you either flipped the ratio or chose the wrong direction (see Refractive Index).
Why is TIR preferred over silvered mirrors inside binoculars and periscopes?
TIR reflects essentially 100% of the light with no metallic absorption, so images stay bright; a 45° prism angle comfortably exceeds glass's θc≈42° (see Prisms and Total Internal Reflection).
Why does a road on a hot day look like a wet, reflective surface from far away?
The air near the hot road forms a continuous index gradient (rarest right at the surface); each thin layer refracts the sky-light a little more until a ray is bent back upward. It is not a single sharp interface, so strictly it is gradient refraction, not textbook TIR — though the trapping effect looks similar (see Mirage and Atmospheric Refraction).
What is θc when the two media are identical (n1=n2)?
sinθc=1, so θc=90°; light travels straight through with no bending and can never be trapped — TIR is impossible.
As n2→n1 from below, what happens to the critical angle?
n2/n1→1, so θc→90°; the "trapping window" (θc,90°) shrinks to nothing, meaning it becomes ever harder to achieve TIR as the indices approach each other.
As n1 becomes enormous compared to n2, what does θc approach?
n2/n1→0, so θc→0°; almost any angle of incidence traps the light, which is the ideal limit for lossless light-piping.
What happens exactly at θ1=θc — is the boundary a mirror or a window?
Neither fully — the refracted ray exists but skims along the surface (θ2=90°), a knife-edge case; the true mirror behaviour switches on only just past this angle.
If light hits the boundary at θ1=0° (straight on) in a dense→rare setup, does TIR occur?
No — a normally-incident ray passes straight through with θ2=0°; since 0°<θc, refraction happens freely and no trapping occurs.
Can TIR occur if the incident medium is a vacuum?
No — vacuum has the lowest possible index (n=1), so there is no rarer medium to send light into; TIR requires starting in something denser than the destination.
Beyond θc, can any energy cross into the rarer medium?
Not through the flat boundary alone — the field there is evanescent, decaying exponentially with penetration depth ∼λ/(2π) and carrying no net energy across. But if a second dense medium is brought within that decay distance, light can "tunnel" across the gap (frustrated TIR) — the wave equivalent of quantum tunnelling.
How deep does the evanescent field reach past the surface at θ1>θc?
Only a fraction of a wavelength — its amplitude falls to 1/e within roughly λ/(2π) of the boundary, which is why "total" reflection is genuinely total unless another medium is placed right up against the surface.