35-4 Interference from Thin Films#
Prompts
Sketch the thin-film setup: incident ray, reflected rays \(r_1\) and \(r_2\), thickness \(L\), indices \(n_1\), \(n_2\), \(n_3\). When does reflection cause a phase shift of \(\pi\) (half-wavelength)?
For a film in air (\(n_1 = n_3 = 1 < n_2\)): which reflected ray(s) get a phase shift? Why is a very thin film (\(L \ll \lambda\)) always dark in reflected light?
What are the three factors that determine the interference of reflected waves? Write the conditions for bright and dark reflected light for a film in air.
How does an anti-reflection coating (e.g., MgF\(_2\) on glass) work? Why is the optimal thickness \(L = \lambda/(4n)\)?
For a wedge of varying thickness: how do you count bright and dark fringes? What determines the number of bands?
Lecture Notes#
Overview#
Thin-film interference causes the colors on soap bubbles, oil slicks, and anti-reflection coatings. Light reflected from the front and back surfaces of a thin transparent film interferes.
The phase difference between the two reflected waves depends on three factors: (1) reflection phase shifts at each interface, (2) path length difference \(2L\) (ray \(r_2\) travels through the film twice), and (3) the internal wavelength \(\lambda_n = \lambda/n\) in the film.
Reflection can add a phase shift of \(\pi\) (half-wavelength); refraction never does.
Setup#
Light is incident on a thin film of thickness \(L\) and index \(n_2\), with media \(n_1\) and \(n_3\) on either side. Ray \(r_1\) reflects from the front surface; ray \(r_2\) reflects from the back surface and emerges. Both reach the observer. For near-normal incidence, the path length difference is \(2L\) (the extra distance \(r_2\) travels in the film).
Reflection phase shifts#
Rule: Reflection causes a phase shift of \(\pi\) rad (equivalent to half-wavelength) only when the incident light is in the medium with the smaller index of refraction (i.e., reflecting off a “denser” medium).
Incident side |
Reflected side |
Phase shift |
|---|---|---|
Lower \(n\) |
Higher \(n\) |
\(\pi\) (0.5\(\lambda\)) |
Higher \(n\) |
Lower \(n\) |
0 |
Refraction never causes a phase shift.
String analogy
A pulse on a light string reflecting from a dense string inverts (phase shift \(\pi\)); a pulse on a dense string reflecting from a light string does not invert.
Film in air#
For a film in air: \(n_1 = n_3 = 1\), \(n_2 = n > 1\).
\(r_1\) (front surface): air \(\to\) film, \(n_1 < n_2\) \(\Rightarrow\) phase shift 0.5\(\lambda\).
\(r_2\) (back surface): film \(\to\) air, \(n_2 > n_3\) \(\Rightarrow\) no phase shift.
So the reflection shifts contribute 0.5\(\lambda\) to the phase difference between \(r_1\) and \(r_2\). The path adds \(2L\) in the film, i.e., \(2L/\lambda_n = 2nL/\lambda\) wavelengths.
Total phase difference (in wavelengths) \(= 0.5 + 2nL/\lambda\).
Result |
Condition |
Equation |
|---|---|---|
Bright (constructive) |
\(0.5 + 2nL/\lambda = m\) |
\(2nL = (m + \frac{1}{2})\lambda\) |
Dark (destructive) |
\(0.5 + 2nL/\lambda = m + 0.5\) |
\(2nL = m\lambda\) |
Very thin film (\(L \ll \lambda\)): \(2nL/\lambda \approx 0\), so total phase \(\approx 0.5\) \(\Rightarrow\) destructive \(\Rightarrow\) film appears dark in reflected light.
Films between other media#
When \(n_1\), \(n_2\), \(n_3\) differ (e.g., coating on glass), the bright and dark equations may interchange. Use an organizing table:
For \(r_1\): does reflection at the front interface cause a phase shift? (Yes if \(n_1 < n_2\).)
For \(r_2\): does reflection at the back interface cause a phase shift? (Yes if \(n_2 < n_3\).)
If the reflection shifts differ (one yes, one no): use the film-in-air formulas above.
If the reflection shifts are the same (both yes or both no): the path alone determines relative phase; bright and dark conditions swap.
Anti-reflection coating#
A thin layer (e.g., MgF\(_2\), \(n_2 = 1.38\)) on glass (\(n_3 = 1.50\)) can eliminate reflection at a chosen wavelength. Both interfaces give a phase shift (air\(\to\)MgF\(_2\) and MgF\(_2\)\(\to\)glass: \(n_2 < n_3\)). For destructive interference of reflected light:
Minimum thickness (\(m = 0\)): \(L = \lambda/(4n_2)\). For \(\lambda = 550\) nm: \(L \approx 100\) nm.
Wedge-shaped films#
For a wedge (thickness varies from \(L_L\) to \(L_R\)), the brightness varies along the film. Apply the same equations at each point; \(L\) changes, so different regions satisfy bright or dark conditions.
At each end, determine whether that thickness gives bright or dark.
Count how many times \(2nL/\lambda\) increases by \(\frac{1}{2}\) (or 1) between the ends to find the number of fringes.
Example: Water film in air
Water film (\(n = 1.33\), \(L = 320\) nm) in air. Bright reflected: \(2nL = (m+\frac{1}{2})\lambda\) \(\Rightarrow\) \(\lambda = 2nL/(m+\frac{1}{2})\). For \(m=1\): \(\lambda \approx 567\) nm (yellow-green). For \(m=0\): \(\lambda \approx 1700\) nm (IR).
Example: Wedge
Air wedge: six dark and five bright fringes. Dark at both ends \(\Rightarrow\) \(2L_L = m\lambda\) and \(2L_R = (m+5)\lambda\) (for air, \(n\approx 1\)). So \(\Delta L = L_R - L_L = 2.5\lambda\).
Summary#
Reflection phase shift: \(\pi\) when incident from lower \(n\) to higher \(n\); otherwise 0.
Film in air: Bright \(2nL = (m+\frac{1}{2})\lambda\); dark \(2nL = m\lambda\). Very thin \(\Rightarrow\) dark.
Other configurations: Use reflection rules; bright/dark may swap.
Anti-reflection: \(L = \lambda/(4n)\) for destructive reflection.
Wedge: Thickness varies; count fringes by applying conditions along the film.