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MYP Physics · unit 12

Electromagnetic spectrum

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

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Extra challenging · 01

Same light energy, different photon counts

Optional enrichment: this challenge may extend beyond the usual syllabus depth and assumes confidence with algebra and graph interpretation. A source emits monochromatic pulses of equal energy 6.626×10⁻⁶ J at two frequencies: 5.0×10¹⁴ Hz and 1.0×10¹⁵ Hz. Use h = 6.626×10⁻³⁴ J s and c = 3.0×10⁸ m s⁻¹. The graph provides photon energy as a function of frequency. Supplied model: Use photon energy E = hf, wavelength λ = c/f and photon count N = Epulse/Ephoton. Supplied data (Frequency / 10¹⁴ Hz; Photon energy / 10⁻¹⁹ J): (0, 0), (5, 3.313), (10, 6.626). (a) Calculate each wavelength, photon energy and photon count. Identify the approximate spectral region of each pulse. [3 marks] (b) Explain why interference supports a wave model while photon-counting detection needs a particle-like model. Evaluate the claim that all electromagnetic radiation has identical biological effects. [3 marks]

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Photon-energy model

Supplied question data. Read the labelled axes and use the observations to test the physical model.

Vertical axis (y): Photon energy / 10⁻¹⁹ J

Photon-energy modelSupplied question data. Read the labelled axes and use the observations to test the physical model. Horizontal axis: Frequency / 10¹⁴ Hz. Vertical axis: Photon energy / 10⁻¹⁹ J. Exact values are available in the data table below.01.6573.3134.976.62602.557.510xy

Horizontal axis (x): Frequency / 10¹⁴ Hz

Reading 1Frequency / 10¹⁴ Hz: 0Photon energy / 10⁻¹⁹ J: 0
Read the exact data as a table
Photon-energy model — supplied values
Frequency / 10¹⁴ HzPhoton energy / 10⁻¹⁹ J
00
53.313
106.626

These are the supplied values, not a worked answer. Lines join the supplied values; they are not a fitted model.

Show a hint

Begin with part (a): Calculate each wavelength, photon energy and photon count. Identify the approximate spectral region of each pulse.

Reveal the worked solution
  1. Use λ = c/f: the lower frequency has wavelength 6.0×10⁻⁷ m and the higher 3.0×10⁻⁷ m.
  2. Ephoton = hf gives 3.313×10⁻¹⁹ and 6.626×10⁻¹⁹ J. Dividing equal total pulse energy by these values gives 2.0×10¹³ and 1.0×10¹³ photons.
  3. 600 nm is visible light and 300 nm is ultraviolet. Both propagate at c in vacuum; the higher-frequency pulse contains fewer photons for the same total energy.
  4. Spatial interference patterns follow phase and superposition, which a simple stream of classical particles does not explain.
  5. Localized detector events with frequency-dependent energy are described by photons. These are complementary descriptions of quantum light rather than literal tiny balls riding classical waves.
  6. Absorption, penetration, dose and photon energy depend on wavelength and material. Ultraviolet can cause photochemical damage; exposure assessment cannot be inferred from vacuum speed alone.

Answer (a) 600 nm, 3.313×10⁻¹⁹ J, 2.0×10¹³ photons; 300 nm, 6.626×10⁻¹⁹ J, 1.0×10¹³ photons. (b) Different models describe different observations; common vacuum speed does not imply identical interaction or hazard.

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Extra challenging · 02

A prism separates colours but preserves frequencies

Optional enrichment: this challenge may extend beyond the usual syllabus depth and assumes confidence with algebra and graph interpretation. White light enters glass from air at 30° to the normal. The material's measured refractive indices at several vacuum wavelengths are supplied. Air has index 1.00 and c = 3.0×10⁸ m s⁻¹. Treat the colours independently and use Snell's law. Supplied data (Vacuum wavelength / nm; Refractive index): (400, 1.54), (550, 1.52), (700, 1.5). (a) Compare the refracted angles, glass speeds and glass wavelengths for 400 nm and 700 nm light. [3 marks] (b) Explain why recombining the spectrum can produce white light and distinguish this from mixing coloured paints. [3 marks]

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Glass dispersion

Supplied question data. Read the labelled axes and use the observations to test the physical model.

Vertical axis (y): Refractive index

Glass dispersionSupplied question data. Read the labelled axes and use the observations to test the physical model. Horizontal axis: Vacuum wavelength / nm. Vertical axis: Refractive index. Exact values are available in the data table below.00.3850.771.1551.540175350525700xy

Horizontal axis (x): Vacuum wavelength / nm

Reading 1Vacuum wavelength / nm: 400Refractive index: 1.54
Read the exact data as a table
Glass dispersion — supplied values
Vacuum wavelength / nmRefractive index
4001.54
5501.52
7001.5

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

Show a hint

Begin with part (a): Compare the refracted angles, glass speeds and glass wavelengths for 400 nm and 700 nm light.

Reveal the worked solution
  1. Snell's law gives sin r = sin30°/n. The blue/violet value is asin(0.5/1.54)≈18.9° and the red value is asin(0.5/1.50)≈19.5°.
  2. Speeds are c/n, about 1.95×10⁸ and 2.0×10⁸ m s⁻¹. Higher index gives greater bending toward the normal on entry.
  3. Frequency is unchanged at entry, so λglass = λvacuum/n, giving about 260 and 467 nm. Dispersion separates directions because n depends on wavelength.
  4. A second appropriately oriented prism or lens arrangement can recombine the separated spectral components into the original white-light mixture.
  5. The first prism separates pre-existing frequencies; it does not manufacture colours or convert red photons into blue ones.
  6. Coloured pigments absorb and scatter different bands, so pigment mixing is subtractive and does not follow the same colour rules as adding light beams.

Answer (a) 400 nm: r≈18.9°, v≈1.95×10⁸ m s⁻¹, λglass≈260 nm; 700 nm: r≈19.5°, v=2.0×10⁸ m s⁻¹, λglass≈467 nm. (b) Light addition combines spectral components; paints remove selected components through absorption.

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Extra challenging · 03

Finding a hidden polariser axis

Optional enrichment: this challenge may extend beyond the usual syllabus depth and assumes confidence with algebra and graph interpretation. Unpolarised light of intensity 80 W m⁻² passes through an ideal first polariser and then an ideal analyser. The analyser data are supplied for angles relative to the first axis. Use I = I0 cos²θ for linearly polarised light at an analyser. Supplied data (Relative angle / °; Transmitted intensity / W m⁻²): (0, 40), (30, 30), (45, 20), (60, 10), (90, 0). (a) Explain the first intensity reduction and predict the intensity when a third polariser at 45° is inserted between crossed first and last polarisers. [3 marks] (b) Explain what the extinction supports about light and give one limitation when using this model to reduce glare. [3 marks]

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Analyser transmission

Supplied question data. Read the labelled axes and use the observations to test the physical model.

Vertical axis (y): Transmitted intensity / W m⁻²

Analyser transmissionSupplied question data. Read the labelled axes and use the observations to test the physical model. Horizontal axis: Relative angle / °. Vertical axis: Transmitted intensity / W m⁻². Exact values are available in the data table below.010203040022.54567.590xy

Horizontal axis (x): Relative angle / °

Reading 1Relative angle / °: 0Transmitted intensity / W m⁻²: 40
Read the exact data as a table
Analyser transmission — supplied values
Relative angle / °Transmitted intensity / W m⁻²
040
3030
4520
6010
900

These are the supplied values, not a worked answer. Lines join the supplied values; they are not a fitted model.

Show a hint

Begin with part (a): Explain the first intensity reduction and predict the intensity when a third polariser at 45° is inserted between crossed first and last polarisers.

Reveal the worked solution
  1. An ideal polariser transmits half the average intensity of unpolarised light, giving 80/2 = 40 W m⁻².
  2. The middle axis at 45° transmits 40cos²45° = 20 W m⁻² and defines a new output polarisation direction.
  3. The last axis is another 45° from the middle, so it transmits 20cos²45° = 10 W m⁻². Without the middle element, the crossed pair transmits zero in the ideal model.
  4. A transverse oscillation has a selectable direction perpendicular to propagation. A simple longitudinal wave has no equivalent independent transverse axis to filter.
  5. The evidence supports the transverse nature of light, not every microscopic detail of a classical-wave picture.
  6. Reflected glare may be only partially polarised, and real filters leak light and absorb other components. Measured minima therefore need not be exactly zero.

Answer (a) First output = 40 W m⁻²; with the middle polariser, final output = 10 W m⁻². (b) Polarisation supports transverse electric-field oscillations; real glare and real filters need not reach complete extinction.

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

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Extra challenging · 04

A sharper X-ray image with a dose trade-off

Optional enrichment: this challenge may extend beyond the usual syllabus depth and assumes confidence with algebra and graph interpretation. An X-ray beam passes through a uniform absorber. Measured transmitted intensity fractions are supplied. Assume exponential attenuation I/I0 = exp(−μx), ignore scatter, and use h = 6.63×10⁻³⁴ J s, c = 3.0×10⁸ m s⁻¹ and electron charge e = 1.60×10⁻¹⁹ C. The tube voltage is 60 kV. Supplied model: For the shortest X-ray wavelength use eV = hc/λmin. Supplied data (Thickness / cm; I/I₀): (0, 1), (1, 0.5), (2, 0.25), (3, 0.125). (a) Determine attenuation coefficient, transmission through 4 cm and the shortest possible tube-emission wavelength. [3 marks] (b) Explain the image contrast and evaluate raising beam intensity to improve a weak image. [3 marks]

Explore the question data

Measured X-ray attenuation

Supplied question data. Read the labelled axes and use the observations to test the physical model.

Vertical axis (y): I/I₀

Measured X-ray attenuationSupplied question data. Read the labelled axes and use the observations to test the physical model. Horizontal axis: Thickness / cm. Vertical axis: I/I₀. Exact values are available in the data table below.00.250.50.75100.751.52.253xy

Horizontal axis (x): Thickness / cm

Reading 1Thickness / cm: 0I/I₀: 1
Read the exact data as a table
Measured X-ray attenuation — supplied values
Thickness / cmI/I₀
01
10.5
20.25
30.125

These are the supplied values, not a worked answer. Lines join the supplied values; they are not a fitted model.

Show a hint

Begin with part (a): Determine attenuation coefficient, transmission through 4 cm and the shortest possible tube-emission wavelength.

Reveal the worked solution
  1. The half-value thickness is 0.01 m, so μ = ln2/0.01 ≈69.3 m⁻¹. Four such thicknesses transmit (1/2)⁴ = 1/16.
  2. The greatest photon energy is the full electron energy eV = (1.60×10⁻¹⁹)(60000) = 9.60×10⁻¹⁵ J.
  3. Using E = hc/λ gives λmin = hc/(eV) ≈2.07×10⁻¹¹ m. Most emitted photons need not have this maximum energy.
  4. Different tissue thicknesses and attenuation coefficients give different transmitted intensities at the detector, creating contrast.
  5. If detected photons are independently counted, relative random counting uncertainty scales approximately as 1/√N; increasing N can improve statistical image quality.
  6. X-rays are ionising, so increased photon fluence can increase patient dose. The exposure should be justified by the diagnostic task, with collimation, shielding and detector efficiency considered; ultrasound may answer some questions without ionising radiation.

Answer (a) μ≈69.3 m⁻¹; transmission at 4 cm = 1/16 = 6.25%; λmin≈2.07×10⁻¹¹ m. (b) Different attenuation gives contrast; more incident photons can reduce relative counting noise but also increases exposure.

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

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