← Unit 4: How have new ideas and ways of thinking developed our understanding of the physical world?
How has understanding of the physical world changed?
Explain polarisation of light as evidence for the transverse-wave nature of light, and apply Malus's law $I = I_0 \cos^2(\theta)$ to determine the intensity of light transmitted by an ideal polariser
A focused answer to the VCE Physics Unit 4 dot point on polarisation. Defines polarised and unpolarised light, explains why polarisation requires a transverse-wave nature, applies Malus's law $I = I_0 \\cos^2 \\theta$, and works through both the unpolarised-to-polariser and polariser-to-second-polariser cases.
Have a quick question? Jump to the Q&A page
What this dot point is asking
VCAA wants you to explain polarisation as evidence for the transverse-wave nature of light, apply Malus's law to compute the intensity of polarised light transmitted through a polariser, and handle both the unpolarised-then-polariser and polariser-then-polariser cases. Cross-link: see the Malus law calculator.
What is polarised light
Light is a transverse electromagnetic wave. The electric field oscillates perpendicular to the direction of propagation. The plane in which the electric field oscillates is the plane of polarisation.
Unpolarised light has electric field oscillations randomly distributed over all directions perpendicular to the propagation direction. A typical light source (incandescent bulb, sun) emits unpolarised light because the many radiating atoms are oriented randomly.
Polarised light has electric field oscillations confined to one specific direction. Polarised light can be produced by:
- Passing unpolarised light through a polarising filter. The filter transmits the component of along its transmission axis and absorbs the perpendicular component.
- Reflection. Light reflecting off non-metallic surfaces (water, glass) becomes partially or fully polarised, especially at Brewster's angle.
- Scattering. Light scattered through 90 degrees by atmospheric molecules is largely polarised (the blue sky has measurable polarisation).
- Specific sources. Lasers (depending on type), some LCDs.
Polarisation as evidence for transverse-wave nature
Only transverse waves can be polarised. A longitudinal wave (compression-rarefaction along the direction of travel) has no direction-of-oscillation choice perpendicular to the propagation direction; rotating a "longitudinal polariser" would have no effect.
The observation that light's intensity through a rotating polariser changes with angle is therefore direct evidence that light is a transverse wave. The first polariser-based experiments (early 1800s) established the transverse nature of light, supporting the wave model.
Malus's law
When polarised light of intensity passes through an ideal polariser whose transmission axis makes angle with the polarisation direction of the incoming light, the transmitted intensity is:
This is Malus's law.
Why ?
The electric field amplitude after the polariser is the projection of the incoming field onto the transmission axis: .
Intensity is proportional to the square of the field amplitude: .
So .
Limit cases
- IMATH_10 : , full transmission. The polariser's axis aligns with the light's polarisation.
- IMATH_12 : , no transmission. The axes are crossed.
- IMATH_14 : , half transmission.
Common values
| IMATH_16 | IMATH_17 | IMATH_18 |
|---|---|---|
| IMATH_19 | 1 | 1 |
| IMATH_20 | IMATH_21 | IMATH_22 |
| IMATH_23 | IMATH_24 | IMATH_25 |
| IMATH_26 | IMATH_27 | IMATH_28 |
| IMATH_29 | 0 | 0 |
The unpolarised-then-polariser rule
When unpolarised light passes through an ideal polariser, the transmitted intensity is half the incoming intensity:
This is because unpolarised light has equal contributions from all possible polarisation directions. The polariser transmits only the component along its axis, which averages to half over all orientations.
After the first polariser, the light is polarised along the polariser's axis. Subsequent polarisers behave according to Malus's law with measured from the previous polariser's axis.
Two-polariser problems
The standard Paper 2 polarisation problem involves an unpolarised source followed by two (or more) polarisers.
Procedure
- First polariser, unpolarised input. .
- Second polariser, polarised input. where is the angle between the first and second polarisers' axes.
- Third polariser, if present. where is between the second and third axes.
The angle in each Malus application is the angle between adjacent polarisers, not the cumulative angle from the source.
Worked example. Three polarisers
Unpolarised light of intensity passes through three polarisers oriented at , and .
After first polariser: .
After second polariser: , so .
After third polariser: (between 45 and 90), so .
Final intensity is .
Note: removing the middle polariser would give . A counter-intuitive result: inserting an extra polariser between two crossed polarisers actually increases the transmitted intensity. This is the classic three-polariser demonstration of the quantum nature of polarisation (each polariser projects, not filters; the second polariser "rotates" the polarisation toward its axis).
Applications
- Polarising sunglasses reduce glare from horizontal surfaces (water, roads). The glare is largely horizontally polarised by reflection at grazing angles, so vertical-axis polarising lenses block it.
- LCD displays use crossed polarisers with liquid-crystal rotators in between. Applying voltage to a pixel rotates the polarisation, changing transmitted intensity.
- Stress analysis. Stressed transparent plastics become birefringent and show coloured patterns under polarised light, revealing stress concentrations.
- 3D cinema. Some 3D systems use orthogonal circular polarisations for the two eyes.
Common errors
Applying Malus's law to unpolarised input. Malus's law requires polarised input. For unpolarised input use the half-rule.
Cumulative angle instead of adjacent angle. The angle in Malus's law is between consecutive polarisers, not from some absolute reference.
Forgetting to square the cosine. is wrong. The intensity depends on the square of the amplitude, so .
Cross polarisers thought to give half intensity. With , . Crossed polarisers transmit zero intensity.
Mixing radians and degrees. , not radians. Use the correct angle unit.
In one sentence
Polarised light has its electric field confined to one direction perpendicular to propagation; an ideal polariser transmits unpolarised light at half intensity and polarised light according to Malus's law (where is the angle between the polarisation direction and the transmission axis), and the existence of polarisation effects is direct evidence that light is a transverse wave.
Past exam questions, worked
Real questions from past VCAA papers on this dot point, with our answer explainer.
2024 VCAA4 marksUnpolarised light of intensity $I_0$ passes through a vertical polariser. The transmitted light then passes through a second polariser whose axis is at $30^\circ$ to the first. (a) State the intensity after the first polariser. (b) Calculate the intensity after the second polariser, in terms of $I_0$.Show worked answer →
(a) After the first polariser. An ideal polariser transmits half the intensity of unpolarised light (averaged over all orientations of the incoming electric field).
Intensity after first polariser: .
(b) After the second polariser. Now the light entering the second polariser is polarised. Apply Malus's law with .
.
So the final intensity is .
Markers reward the half-intensity rule for unpolarised-through-first-polariser, the correct form of Malus's law, exact-value handling, and a clean fraction or decimal of .
2023 VCAA3 marksPolarised light of intensity $200$ W m$^{-2}$ is incident on a polariser whose transmission axis is at $60^\circ$ to the polarisation direction. (a) Calculate the intensity of the transmitted light. (b) Explain what polarisation observation reveals about the nature of light.Show worked answer →
(a) Transmitted intensity. Apply Malus's law.
W m.
(b) Polarisation and the nature of light. Polarisation effects (the dependence of transmitted intensity on the orientation of a polariser) require light's electric field oscillation to have a transverse direction (perpendicular to the propagation direction). A purely longitudinal wave could not be polarised. Therefore polarisation observations confirm that light is a transverse wave.
Markers reward correct application of Malus's law with exact-value handling, and an explicit statement linking polarisation to transverse-wave behaviour (longitudinal waves, like sound, cannot be polarised).
Related dot points
- Investigate the wave model of light, including diffraction and constructive and destructive interference (Young's double-slit experiment), and apply $\Delta x = \lambda L / d$ for fringe spacing in the small-angle limit
A focused answer to the VCE Physics Unit 4 dot point on the wave model of light. Covers Young's double-slit experiment, the path-difference condition for constructive and destructive interference, the fringe-spacing formula $\\Delta x = \\lambda L / d$ in the small-angle limit, and single-slit diffraction.
- Describe electromagnetic waves as transverse waves of oscillating electric and magnetic fields propagating at the speed of light, and identify the regions of the electromagnetic spectrum with their characteristic frequencies, wavelengths and applications
A focused answer to the VCE Physics Unit 4 dot point on electromagnetic waves and the EM spectrum. Describes EM waves as transverse oscillations of E and B fields, gives the order-of-magnitude regions of the spectrum (radio, microwave, IR, visible, UV, X-ray, gamma), and applies $c = f \\lambda$ across regions.
- Apply the photon model of light to the photoelectric effect using $E_{\text{photon}} = h f$ and $E_{k,\max} = h f - \phi$, where $\phi$ is the work function of the metal, and interpret the stopping voltage $V_0$ as $e V_0 = E_{k,\max}$
A focused answer to the VCE Physics Unit 4 dot point on the photoelectric effect. Sets out the photon energy $E = hf$, the photoelectric equation $E_{k,\\max} = hf - \\phi$, the role of the work function, the stopping voltage, and the four observations that the classical wave model cannot explain.