Skip to main content
Course and syllabus guidance

University Physics III · unit UPIII-05

Physical Optics

Connect the ideas, make your working visible, and test the result. Use the hints when you need a starting point; open the full solution after your attempt.

Extra challenging questions

A selection from this pathway. Open a topic below for its complete practice and challenge set.

Extra challenging · 01

Coherence, phase & superposition of light: infer an input with uncertainty

Two light waves are coherent at a detector when their phase difference stays fixed for longer than the detector averages; their fields then add to make fringes, and the fringe visibility measures how completely they do so. Use the supplied topic model Y_out = 2*sqrt(ratio)/(1+ratio)*abs(sin(pi*max(path,0.01)*band/360)/(pi*max(path,0.01)*band/360)), where Y_out is VISIBILITY V (dimensionless). The output symbol Y_out is distinct from all input symbols. ^ denotes a power; π = 3.141592653589793; sqrt(x) means √x; abs(x) means |x|; max(a,b) selects the larger value; unmarked trigonometric functions use radians. ratio is Intensity ratio I₂/I₁, dimensionless. Keep path (Path difference Δ) = 4 μm; band (Source linewidth Δλ) = 20 nm fixed. For this exercise use only 0.10625 ≤ ratio ≤ 0.89375 on this continuous branch. A grid of test settings is an input restriction for this exercise, not by itself a claim of physical quantisation. This calculation retains the topic model's stated assumptions; it does not extend them to a different physical setup. A reading gives Y_out = 0.88892705, with a bounded reading uncertainty ±0.0045522. Treat the model and all fixed inputs as exact for this exercise; the bound is not a standard deviation. First estimate the unknown ratio by straight-line interpolation between the two endpoint predictions. Then solve the actual model on the stated branch to an absolute input tolerance of 0.00007875, using a numerical bracket if required. Find the full input interval consistent with the bounded reading uncertainty and compare it with a symmetric input-error assumption. Do not assume that the supplied calibration points prove monotonicity outside this branch.

Explore the question data

VISIBILITY V against ratio

Predictions from the supplied Coherence, phase & superposition of light model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law.

Vertical axis (y): VISIBILITY V

VISIBILITY V against ratioPredictions from the supplied Coherence, phase & superposition of light model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law. Horizontal axis: ratio: Intensity ratio I₂/I₁. Vertical axis: VISIBILITY V. Exact values are available in the data table below.0.52750.62920.73090.83260.93430.074750.28740.50.71260.9252xy

Horizontal axis (x): ratio: Intensity ratio I₂/I₁

Axes show the supplied calibration interval; the origin may lie outside the plot.

Reading 1ratio: Intensity ratio I₂/I₁: 0.1062VISIBILITY V: 0.5426
Read the exact data as a table
VISIBILITY V against ratio — supplied values
ratio: Intensity ratio I₂/I₁VISIBILITY V
0.106250.5425894174913162
0.3031250.7780095623023046
0.50.8680682592366252
0.69687499999999990.9059155713299115
0.89374999999999990.9192751387850172

These are the supplied values, not a worked answer. No fitted trend is drawn.

Show a hint

The model's endpoint predictions bracket the reading. Solve Y_out(ratio) = Y_measured and then solve again at Y_measured − u and Y_measured + u; a nonlinear inverse can give unequal input deviations.

Reveal the worked solution
  1. Endpoint predictions are Y_out(0.10625) = 0.542589 and Y_out(0.89375) = 0.919275. The target lies between them. On the selected branch the response is strictly increasing.
  2. Endpoint interpolation gives ratio_line = 0.10625 + (0.888927 − 0.542589)(0.89375 − 0.10625)/(0.919275 − 0.542589) = 0.830304. This estimates the inverse of the endpoint chord, rather than assuming that chord is the physical model.
  3. Use the actual equation, not the chord, and bracket its root. Evaluating the midpoint and retaining the sign-changing half-interval gives ratio = 0.586625; substituting back gives Y_out = 0.88892705.
  4. The interpolation error in the input is |ratio_line − ratio| = 0.243679. This is larger than the requested numerical tolerance.
  5. Invert both limits Y_out = 0.88437485 and 0.89347925. Sort the roots even if the response decreases: 0.564685 ≤ ratio ≤ 0.610992.
  6. The lower and upper input deviations are 0.0219396 and 0.0243665. They differ because the inverse response is nonlinear; a symmetric error bar would only be a local approximation. This interval includes reading uncertainty only, not model error or uncertainty in fixed inputs.

Answer ratio ≈ 0.586625; compatible interval [0.564685, 0.610992]. Endpoint interpolation gives 0.830304.

Compare the assumptions, method and units with your attempt. Explain any correction before trying another question.

Extra challenging · 02

Two-source interference & double-slit intensity: infer an input with uncertainty

Two-source interference is the far-field pattern of two equal, in-phase point sources: a screen intensity I = 4I₀ cos²(φ/2) whose phase difference φ = 2πd sinθ/λ is set by the slit separation, the angle and the wavelength. Use the supplied topic model Y_out = 0.002*lam/d, where Y_out is FRINGE SPACING λL/d (mm). The output symbol Y_out is distinct from all input symbols. ^ denotes a power; π = 3.141592653589793. d is Slit separation d, measured in mm. Keep lam (Wavelength λ) = 633 nm; y (Probe position y on the screen) = 1.25 mm fixed. For this exercise use only 0.131875 mm ≤ d ≤ 0.368125 mm on this continuous branch. A grid of test settings is an input restriction for this exercise, not by itself a claim of physical quantisation. This calculation retains the topic model's stated assumptions; it does not extend them to a different physical setup. A reading gives Y_out = 4.5871643 mm, with a bounded reading uncertainty ±0.17222 mm. Treat the model and all fixed inputs as exact for this exercise; the bound is not a standard deviation. First estimate the unknown d by straight-line interpolation between the two endpoint predictions. Then solve the actual model on the stated branch to an absolute input tolerance of 0.000023625 mm, using a numerical bracket if required. Find the full input interval consistent with the bounded reading uncertainty and compare it with a symmetric input-error assumption. Do not assume that the supplied calibration points prove monotonicity outside this branch.

Explore the question data

FRINGE SPACING λL/d against d

Predictions from the supplied Two-source interference & double-slit intensity model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law.

Vertical axis (y): FRINGE SPACING λL/d / mm

FRINGE SPACING λL/d against dPredictions from the supplied Two-source interference & double-slit intensity model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law. Horizontal axis: d: Slit separation d / mm. Vertical axis: FRINGE SPACING λL/d / mm. Exact values are available in the data table below.3.1934.8566.528.1839.8460.12240.18620.250.31380.3776xy

Horizontal axis (x): d: Slit separation d / mm

Axes show the supplied calibration interval; the origin may lie outside the plot.

Reading 1d: Slit separation d / mm: 0.1319FRINGE SPACING λL/d / mm: 9.6
Read the exact data as a table
FRINGE SPACING λL/d against d — supplied values
d: Slit separation d / mmFRINGE SPACING λL/d / mm
0.131875000000000029.599999999999998
0.190937500000000046.630441898527003
0.255.064
0.30906254.0962588473205255
0.368125000000000043.4390492359932083

These are the supplied values, not a worked answer. No fitted trend is drawn.

Show a hint

The model's endpoint predictions bracket the reading. Solve Y_out(d) = Y_measured and then solve again at Y_measured − u and Y_measured + u; a nonlinear inverse can give unequal input deviations.

Reveal the worked solution
  1. Endpoint predictions are Y_out(0.131875) = 9.6 mm and Y_out(0.368125) = 3.43905 mm. The target lies between them. On the selected branch the response is strictly decreasing.
  2. Endpoint interpolation gives d_line = 0.131875 + (4.58716 − 9.6)(0.368125 − 0.131875)/(3.43905 − 9.6) = 0.324099 mm. This estimates the inverse of the endpoint chord, rather than assuming that chord is the physical model.
  3. Use the actual equation, not the chord, and bracket its root. Evaluating the midpoint and retaining the sign-changing half-interval gives d = 0.275987 mm; substituting back gives Y_out = 4.5871643 mm.
  4. The interpolation error in the input is |d_line − d| = 0.0481115 mm. This is larger than the requested numerical tolerance.
  5. Invert both limits Y_out = 4.4149443 mm and 4.7593843 mm. Sort the roots even if the response decreases: 0.266001 mm ≤ d ≤ 0.286753 mm.
  6. The lower and upper input deviations are 0.0099867 mm and 0.0107658 mm. They differ because the inverse response is nonlinear; a symmetric error bar would only be a local approximation. This interval includes reading uncertainty only, not model error or uncertainty in fixed inputs.

Answer d ≈ 0.275987 mm; compatible interval [0.266001, 0.286753] mm. Endpoint interpolation gives 0.324099 mm.

Compare the assumptions, method and units with your attempt. Explain any correction before trying another question.

Extra challenging · 03

Thin Films, Wedges & Newton's Rings: infer an input with uncertainty

Thin-film interference is the superposition of the light reflected from a film's two faces, whose phase difference is the optical path 2nt cos θ_t counted in wavelengths, plus a half-cycle for each reflection off a denser medium. Use the supplied topic model Y_out = 100*(((1-nf)/(1+nf))^2+((1-((1-nf)/(1+nf))^2)*(nf-ns)/(nf+ns))^2+2*((1-nf)/(1+nf))*(1-((1-nf)/(1+nf))^2)*(nf-ns)/(nf+ns)*cos(4*pi*nf*t/550)), where Y_out is R AT 550 nm (%). The output symbol Y_out is distinct from all input symbols. ^ denotes a power; π = 3.141592653589793; unmarked trigonometric functions use radians. t is Film thickness t, measured in nm. Keep nf (Film index n_f) = 1.38; ns (Substrate index n_s) = 1.52 fixed. For this exercise use only 310.325 nm ≤ t ≤ 363.875 nm on this continuous branch. A grid of test settings is an input restriction for this exercise, not by itself a claim of physical quantisation. This calculation retains the topic model's stated assumptions; it does not extend them to a different physical setup. A reading gives Y_out = 2.5001094 %, with a bounded reading uncertainty ±0.14412 %. Treat the model and all fixed inputs as exact for this exercise; the bound is not a standard deviation. First estimate the unknown t by straight-line interpolation between the two endpoint predictions. Then solve the actual model on the stated branch to an absolute input tolerance of 0.005355 nm, using a numerical bracket if required. Find the full input interval consistent with the bounded reading uncertainty and compare it with a symmetric input-error assumption. Do not assume that the supplied calibration points prove monotonicity outside this branch.

Explore the question data

R AT 550 nm against t

Predictions from the supplied Thin Films, Wedges & Newton's Rings model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law.

Vertical axis (y): R AT 550 nm / %

R AT 550 nm against tPredictions from the supplied Thin Films, Wedges & Newton's Rings model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law. Horizontal axis: t: Film thickness t / nm. Vertical axis: R AT 550 nm / %. Exact values are available in the data table below.1.2811.8472.4132.9793.545308.2322.6337.1351.6366xy

Horizontal axis (x): t: Film thickness t / nm

Axes show the supplied calibration interval; the origin may lie outside the plot.

Reading 1t: Film thickness t / nm: 310.3R AT 550 nm / %: 1.365
Read the exact data as a table
R AT 550 nm against t — supplied values
t: Film thickness t / nmR AT 550 nm / %
310.3251.3645030338248338
323.71251.7046285577859859
337.12.231878668679646
350.48752.8536961833453516
363.8753.460922893167949

These are the supplied values, not a worked answer. No fitted trend is drawn.

Show a hint

The model's endpoint predictions bracket the reading. Solve Y_out(t) = Y_measured and then solve again at Y_measured − u and Y_measured + u; a nonlinear inverse can give unequal input deviations.

Reveal the worked solution
  1. Endpoint predictions are Y_out(310.325) = 1.3645 % and Y_out(363.875) = 3.46092 %. The target lies between them. On the selected branch the response is strictly increasing.
  2. Endpoint interpolation gives t_line = 310.325 + (2.50011 − 1.3645)(363.875 − 310.325)/(3.46092 − 1.3645) = 339.332 nm. This estimates the inverse of the endpoint chord, rather than assuming that chord is the physical model.
  3. Use the actual equation, not the chord, and bracket its root. Evaluating the midpoint and retaining the sign-changing half-interval gives t = 342.991 nm; substituting back gives Y_out = 2.5001094 %.
  4. The interpolation error in the input is |t_line − t| = 3.65809 nm. This is larger than the requested numerical tolerance.
  5. Invert both limits Y_out = 2.3559894 % and 2.6442294 %. Sort the roots even if the response decreases: 339.864 nm ≤ t ≤ 346.061 nm.
  6. The lower and upper input deviations are 3.12639 nm and 3.07076 nm. They differ because the inverse response is nonlinear; a symmetric error bar would only be a local approximation. This interval includes reading uncertainty only, not model error or uncertainty in fixed inputs.

Answer t ≈ 342.991 nm; compatible interval [339.864, 346.061] nm. Endpoint interpolation gives 339.332 nm.

Compare the assumptions, method and units with your attempt. Explain any correction before trying another question.

Extra challenging · 04

The Michelson Interferometer & Optical Metrology: infer an input with uncertainty

A Michelson interferometer divides a beam's amplitude at a beam splitter, returns the two halves from separate mirrors and reads the path difference 2d between the arms as a fringe pattern that shifts by one fringe for every λ/2 of mirror travel. Use the supplied topic model Y_out = lam^2/(1000*dl), where Y_out is COHERENCE LENGTH λ²/Δλ (μm). The output symbol Y_out is distinct from all input symbols. ^ denotes a power; π = 3.141592653589793. dl is Spectral width Δλ, measured in nm. Keep lam (Centre wavelength λ) = 633 nm; d (Mirror displacement d) = 0.95 μm fixed. For this exercise use only 32.7687 nm ≤ dl ≤ 268.231 nm on this continuous branch. A grid of test settings is an input restriction for this exercise, not by itself a claim of physical quantisation. This calculation retains the topic model's stated assumptions; it does not extend them to a different physical setup. A reading gives Y_out = 2.2714683 μm, with a bounded reading uncertainty ±0.11665 μm. Treat the model and all fixed inputs as exact for this exercise; the bound is not a standard deviation. First estimate the unknown dl by straight-line interpolation between the two endpoint predictions. Then solve the actual model on the stated branch to an absolute input tolerance of 0.0235462 nm, using a numerical bracket if required. Find the full input interval consistent with the bounded reading uncertainty and compare it with a symmetric input-error assumption. Do not assume that the supplied calibration points prove monotonicity outside this branch.

Explore the question data

COHERENCE LENGTH λ²/Δλ against dl

Predictions from the supplied The Michelson Interferometer & Optical Metrology model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law.

Vertical axis (y): COHERENCE LENGTH λ²/Δλ / μm

COHERENCE LENGTH λ²/Δλ against dlPredictions from the supplied The Michelson Interferometer & Optical Metrology model, with all other inputs fixed as stated in the question. 5 calibration points support a trend comparison; they are not measured data or a straight-line law. Horizontal axis: dl: Spectral width Δλ / nm. Vertical axis: COHERENCE LENGTH λ²/Δλ / μm. Exact values are available in the data table below.1.0643.9636.8619.75912.6623.3586.93150.5214.1277.6xy

Horizontal axis (x): dl: Spectral width Δλ / nm

Axes show the supplied calibration interval; the origin may lie outside the plot.

Reading 1dl: Spectral width Δλ / nm: 32.77COHERENCE LENGTH λ²/Δλ / μm: 12.23
Read the exact data as a table
COHERENCE LENGTH λ²/Δλ against dl — supplied values
dl: Spectral width Δλ / nmCOHERENCE LENGTH λ²/Δλ / μm
32.7687512.227777989700552
91.634374999999994.372693107799339
150.52.6623853820598007
209.365624999999971.9138242010836308
268.231251.4938192324719808

These are the supplied values, not a worked answer. No fitted trend is drawn.

Show a hint

The model's endpoint predictions bracket the reading. Solve Y_out(dl) = Y_measured and then solve again at Y_measured − u and Y_measured + u; a nonlinear inverse can give unequal input deviations.

Reveal the worked solution
  1. Endpoint predictions are Y_out(32.7687) = 12.2278 μm and Y_out(268.231) = 1.49382 μm. The target lies between them. On the selected branch the response is strictly decreasing.
  2. Endpoint interpolation gives dl_line = 32.7687 + (2.27147 − 12.2278)(268.231 − 32.7687)/(1.49382 − 12.2278) = 251.173 nm. This estimates the inverse of the endpoint chord, rather than assuming that chord is the physical model.
  3. Use the actual equation, not the chord, and bracket its root. Evaluating the midpoint and retaining the sign-changing half-interval gives dl = 176.401 nm; substituting back gives Y_out = 2.2714683 μm.
  4. The interpolation error in the input is |dl_line − dl| = 74.7717 nm. This is larger than the requested numerical tolerance.
  5. Invert both limits Y_out = 2.1548183 μm and 2.3881183 μm. Sort the roots even if the response decreases: 167.784 nm ≤ dl ≤ 185.95 nm.
  6. The lower and upper input deviations are 8.61648 nm and 9.54937 nm. They differ because the inverse response is nonlinear; a symmetric error bar would only be a local approximation. This interval includes reading uncertainty only, not model error or uncertainty in fixed inputs.

Answer dl ≈ 176.401 nm; compatible interval [167.784, 185.95] nm. Endpoint interpolation gives 251.173 nm.

Compare the assumptions, method and units with your attempt. Explain any correction before trying another question.

Choose a topic