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A Level H2 Physics Modern Physics Quiz

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Questions

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A-Level Physics H2 Quiz - Modern Physics

Name: __________________________
Class: __________________________
Date: __________________________
Score: ________ / 45

Duration: 45 minutes
Total Marks: 45

Instructions:

  1. Answer all questions.
  2. Write your answers in the spaces provided.
  3. The number of marks is given in brackets [ ] at the end of each question or part question.
  4. You may use a scientific calculator.
  5. Data and Formulae are provided on the separate data sheet (assume standard values: h=6.63×1034 J sh = 6.63 \times 10^{-34} \text{ J s}, c=3.00×108 m s1c = 3.00 \times 10^8 \text{ m s}^{-1}, e=1.60×1019 Ce = 1.60 \times 10^{-19} \text{ C}, 1 u=931.5 MeV1 \text{ u} = 931.5 \text{ MeV}).

Section A: Quantum Physics (Questions 1–7)

1. Define the term work function of a metal.
[1]



2. State Einstein’s photoelectric equation. Define all symbols used.
[2]




3. A monochromatic light source emits photons of wavelength 450 nm450 \text{ nm}.
(a) Calculate the energy of a single photon in Joules.
[2]

<br> <br> <br>

(b) Determine the energy of this photon in electron-volts (eV).
[1]

<br> <br>

4. The graph below shows the variation of maximum kinetic energy Ek,maxE_{k,max} of photoelectrons emitted from a metal surface with the frequency ff of the incident radiation.

(Imagine a graph with linear positive slope, crossing the x-axis at f0f_0 and y-axis at Φ-\Phi)

(a) Explain the physical significance of the x-intercept f0f_0.
[1]


(b) Explain why the graph does not pass through the origin.
[2]




5. In a photoelectric experiment, the intensity of the incident monochromatic light is doubled while the frequency remains constant.
(a) State and explain the effect on the maximum kinetic energy of the emitted photoelectrons.
[2]




(b) State and explain the effect on the photoelectric current.
[2]




6. An electron is accelerated from rest through a potential difference of 2.5 kV2.5 \text{ kV}.
(a) Calculate the kinetic energy of the electron in Joules.
[2]

<br> <br> <br>

(b) Calculate the de Broglie wavelength of this electron.
[3]

<br> <br> <br> <br>

7. Describe one piece of experimental evidence that supports the particle nature of light.
[2]






Section B: Nuclear Physics (Questions 8–14)

8. Define the term binding energy of a nucleus.
[2]




9. The unified atomic mass unit (u) is defined as one-twelfth of the mass of a carbon-12 atom.
(a) Show that 1 u1 \text{ u} is equivalent to approximately 931.5 MeV931.5 \text{ MeV}.
[2]

<br> <br> <br>

(b) Why is the mass of a stable nucleus always less than the sum of the masses of its constituent protons and neutrons?
[2]





10. Consider the following nuclear reaction representing the fusion of deuterium and tritium:
12H+13H24He+01n^2_1\text{H} + ^3_1\text{H} \rightarrow ^4_2\text{He} + ^1_0\text{n}
Given the following masses:
Mass of 12H=2.0141 u^2_1\text{H} = 2.0141 \text{ u}
Mass of 13H=3.0160 u^3_1\text{H} = 3.0160 \text{ u}
Mass of 24He=4.0026 u^4_2\text{He} = 4.0026 \text{ u}
Mass of 01n=1.0087 u^1_0\text{n} = 1.0087 \text{ u}

(a) Calculate the mass defect in u.
[2]

<br> <br> <br>

(b) Calculate the energy released in this reaction in MeV.
[2]

<br> <br> <br>

11. A radioactive isotope has a half-life of 12 hours12 \text{ hours}.
(a) Define half-life.
[1]


(b) If the initial activity of a sample is 800 Bq800 \text{ Bq}, calculate the activity after 2 days2 \text{ days}.
[2]

<br> <br> <br>

12. The graph of binding energy per nucleon against nucleon number AA shows a peak at Iron-56 (A=56A=56).
(a) Explain why energy is released during nuclear fusion of light nuclei.
[2]




(b) Explain why energy is released during nuclear fission of heavy nuclei.
[2]




13. Write the nuclear equation for the β\beta^- decay of Carbon-14 (614C^{14}_6\text{C}) into Nitrogen. Include the antineutrino.
[2]

<br> <br> <br>

14. In β\beta^- decay, the emitted electrons have a continuous spectrum of energies up to a maximum value, rather than a single discrete energy.
(a) Explain why this observation led to the postulation of the neutrino (or antineutrino).
[2]




(b) State two properties of the neutrino.
[2]




Section C: Applications & Synthesis (Questions 15–20)

15. X-rays are produced in an X-ray tube when high-speed electrons strike a metal target.
(a) Explain the origin of the continuous spectrum of X-rays (Bremsstrahlung).
[2]




(b) Explain the origin of the characteristic line spectrum of X-rays.
[2]




16. The minimum wavelength λmin\lambda_{min} of the X-rays produced depends on the accelerating voltage VV.
(a) Derive the expression λmin=hceV\lambda_{min} = \frac{hc}{eV}.
[2]

<br> <br> <br> <br>

(b) If the accelerating voltage is doubled, state the effect on λmin\lambda_{min}.
[1]


17. A laser emits light of wavelength 633 nm633 \text{ nm} with a power output of 2.0 mW2.0 \text{ mW}.
(a) Calculate the number of photons emitted per second.
[3]

<br> <br> <br> <br> <br>

(b) State two properties of laser light that distinguish it from ordinary light.
[2]



18. In a semiconductor, the conductivity increases with temperature.
(a) Explain this phenomenon in terms of charge carriers.
[2]




(b) Distinguish between intrinsic and extrinsic semiconductors.
[2]




19. A student investigates the photoelectric effect using a zinc plate and an electroscope. The zinc plate is negatively charged.
(a) Explain why the leaf of the electroscope collapses when UV light is shone on the plate.
[2]




(b) Explain why the leaf does not collapse if visible light is used, regardless of intensity.
[2]




20. Compare and contrast nuclear fusion and nuclear fission by stating:
(a) One similarity in terms of energy release.
[1]


(b) One difference in terms of the conditions required for the reaction to occur.
[1]


(c) One advantage of fusion over fission for power generation.
[1]



End of Quiz

Answers

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A-Level Physics H2 Quiz - Modern Physics (Answer Key)

1.
The minimum energy required to remove an electron from the surface of a metal. [1]

2.
hf=Φ+Ek,maxhf = \Phi + E_{k,max} [1]
Where:
hh is Planck’s constant,
ff is the frequency of incident radiation,
Φ\Phi is the work function of the metal,
Ek,maxE_{k,max} is the maximum kinetic energy of the emitted photoelectron. [1]
(1 mark for correct equation, 1 mark for defining at least 2 symbols correctly)

3.
(a) E=hcλE = \frac{hc}{\lambda} [1]
E=6.63×1034×3.00×108450×109E = \frac{6.63 \times 10^{-34} \times 3.00 \times 10^8}{450 \times 10^{-9}}
E=4.42×1019 JE = 4.42 \times 10^{-19} \text{ J} [1]

(b) E(eV)=4.42×10191.60×1019E (\text{eV}) = \frac{4.42 \times 10^{-19}}{1.60 \times 10^{-19}} [1]
E=2.76 eVE = 2.76 \text{ eV}

4.
(a) f0f_0 is the threshold frequency. It is the minimum frequency of incident radiation required to emit photoelectrons from the metal surface. [1]

(b) The graph intersects the y-axis at Φ-\Phi because energy is required to overcome the work function. If f<f0f < f_0, the photon energy hfhf is less than the work function Φ\Phi, so no electrons are emitted (kinetic energy cannot be negative). The equation Ek,max=hfΦE_{k,max} = hf - \Phi shows a negative intercept. [2]

5.
(a) No change. [1]
The maximum kinetic energy depends only on the frequency of the incident photons and the work function of the metal (Ek,max=hfΦE_{k,max} = hf - \Phi). Intensity affects the number of photons, not their individual energy. [1]

(b) Current doubles (increases proportionally). [1]
Intensity is proportional to the number of photons incident per unit time. Doubling intensity doubles the number of photons, which doubles the number of photoelectrons emitted per second, hence doubling the current. [1]

6.
(a) Ek=eVE_k = eV [1]
Ek=1.60×1019×2500E_k = 1.60 \times 10^{-19} \times 2500
Ek=4.00×1016 JE_k = 4.00 \times 10^{-16} \text{ J} [1]

(b) λ=hp=h2mEk\lambda = \frac{h}{p} = \frac{h}{\sqrt{2mE_k}} [1]
λ=6.63×10342×9.11×1031×4.00×1016\lambda = \frac{6.63 \times 10^{-34}}{\sqrt{2 \times 9.11 \times 10^{-31} \times 4.00 \times 10^{-16}}} [1]
λ=6.63×10347.288×1046\lambda = \frac{6.63 \times 10^{-34}}{\sqrt{7.288 \times 10^{-46}}}
λ=6.63×10342.70×1023\lambda = \frac{6.63 \times 10^{-34}}{2.70 \times 10^{-23}}
λ=2.46×1011 m\lambda = 2.46 \times 10^{-11} \text{ m} [1]

7.
The photoelectric effect. [1]
Wave theory predicts that energy accumulates over time, so low-intensity light should eventually eject electrons. However, experiments show that emission is instantaneous and only occurs if frequency exceeds a threshold, supporting the particle (photon) model where energy is quantized in packets E=hfE=hf. [1]

8.
The energy required to completely separate a nucleus into its constituent protons and neutrons (nucleons). [1]
Alternatively: The energy released when constituent nucleons combine to form a nucleus. [1]

9.
(a) E=mc2E = mc^2
1 u=1.6605×1027 kg1 \text{ u} = 1.6605 \times 10^{-27} \text{ kg}
E=1.6605×1027×(3.00×108)2=1.494×1010 JE = 1.6605 \times 10^{-27} \times (3.00 \times 10^8)^2 = 1.494 \times 10^{-10} \text{ J} [1]
1 eV=1.60×1019 J1 \text{ eV} = 1.60 \times 10^{-19} \text{ J}
E(MeV)=1.494×10101.60×1013934 MeVE (\text{MeV}) = \frac{1.494 \times 10^{-10}}{1.60 \times 10^{-13}} \approx 934 \text{ MeV} (Accept 931.5 based on precise constants) [1]

(b) The mass difference (mass defect) is converted into binding energy according to E=mc2E=mc^2. This energy is released when the nucleus forms, making the bound system more stable (lower energy state) than the separated nucleons. [2]

10.
(a) Mass of reactants =2.0141+3.0160=5.0301 u= 2.0141 + 3.0160 = 5.0301 \text{ u}
Mass of products =4.0026+1.0087=5.0113 u= 4.0026 + 1.0087 = 5.0113 \text{ u}
Mass defect Δm=5.03015.0113=0.0188 u\Delta m = 5.0301 - 5.0113 = 0.0188 \text{ u} [2]

(b) Energy =0.0188×931.5= 0.0188 \times 931.5 [1]
Energy =17.51 MeV= 17.51 \text{ MeV} [1]

11.
(a) The time taken for half the number of radioactive nuclei in a sample to decay (or for the activity to fall to half its initial value). [1]

(b) Time elapsed =2 days=48 hours= 2 \text{ days} = 48 \text{ hours}.
Number of half-lives n=4812=4n = \frac{48}{12} = 4. [1]
A=A0(12)n=800×(12)4=800×116=50 BqA = A_0 \left(\frac{1}{2}\right)^n = 800 \times \left(\frac{1}{2}\right)^4 = 800 \times \frac{1}{16} = 50 \text{ Bq}. [1]

12.
(a) In fusion, light nuclei combine to form a heavier nucleus with a higher binding energy per nucleon. [1]
This increase in binding energy per nucleon means the final nucleus is more tightly bound, and the difference in binding energy is released as kinetic energy/radiation. [1]

(b) In fission, a heavy nucleus splits into lighter nuclei which have a higher binding energy per nucleon (closer to the peak at Fe-56). [1]
The increase in binding energy per nucleon results in a release of energy. [1]

13.
614C714N+10β+νˉe^{14}_6\text{C} \rightarrow ^{14}_7\text{N} + ^0_{-1}\beta + \bar{\nu}_e [2]
(1 mark for correct Nucleus, 1 mark for electron and antineutrino)

14.
(a) If only two particles (nucleus and electron) were involved, conservation of energy and momentum would require the electron to have a fixed discrete energy. The continuous spectrum implies a third particle (antineutrino) shares the energy and momentum variably. [2]

(b) Any two from:

  1. Zero charge. [1]
  2. Very small/negligible mass. [1]
  3. Weakly interacting (low interaction cross-section). [1]

15.
(a) Incident electrons are decelerated by the electric fields of the target nuclei. [1]
The loss in kinetic energy is converted into a photon. Since electrons lose varying amounts of energy (from zero to maximum), a continuous range of photon energies (wavelengths) is produced. [1]

(b) Incident electrons collide with and eject inner-shell electrons from the target atoms. [1]
Outer-shell electrons drop down to fill the vacancies, emitting photons with specific energies corresponding to the difference between discrete atomic energy levels. [1]

16.
(a) Maximum photon energy corresponds to an electron losing all its kinetic energy in a single collision.
Emax=hfmax=hcλminE_{max} = hf_{max} = \frac{hc}{\lambda_{min}} [1]
Kinetic energy of electron K=eVK = eV.
Equating energies: eV=hcλminλmin=hceVeV = \frac{hc}{\lambda_{min}} \Rightarrow \lambda_{min} = \frac{hc}{eV}. [1]

(b) λmin\lambda_{min} is halved. [1]

17.
(a) Energy of one photon E=hcλ=6.63×1034×3.00×108633×109=3.14×1019 JE = \frac{hc}{\lambda} = \frac{6.63 \times 10^{-34} \times 3.00 \times 10^8}{633 \times 10^{-9}} = 3.14 \times 10^{-19} \text{ J}. [1]
Power P=2.0 mW=2.0×103 J s1P = 2.0 \text{ mW} = 2.0 \times 10^{-3} \text{ J s}^{-1}. [1]
Number of photons N=PE=2.0×1033.14×1019=6.37×1015 s1N = \frac{P}{E} = \frac{2.0 \times 10^{-3}}{3.14 \times 10^{-19}} = 6.37 \times 10^{15} \text{ s}^{-1}. [1]

(b) Any two from:

  1. Monochromatic (single wavelength/frequency). [1]
  2. Coherent (constant phase difference). [1]
  3. Collimated (low divergence/parallel beam). [1]
  4. High intensity. [1]

18.
(a) As temperature increases, more covalent bonds are broken, releasing more electron-hole pairs. [1]
This increases the number density of charge carriers, thereby increasing conductivity. [1]

(b) Intrinsic: Pure semiconductor where charge carriers are generated only by thermal excitation across the band gap. [1]
Extrinsic: Semiconductor doped with impurities (Group 3 or 5) to increase the number of majority charge carriers (holes or electrons). [1]

19.
(a) UV photons have energy greater than the work function of zinc. [1]
Photoelectrons are emitted, removing negative charge from the plate. The electroscope discharges, causing the leaf to collapse. [1]

(b) Visible light photons have frequency lower than the threshold frequency of zinc (f<f0f < f_0). [1]
Individual photon energy hfhf is less than the work function Φ\Phi, so no electrons are emitted regardless of how many photons (intensity) strike the surface. [1]

20.
(a) Both involve a mass defect which is converted into energy according to E=mc2E=mc^2. [1]
(b) Fusion requires extremely high temperatures and pressures to overcome electrostatic repulsion between nuclei; Fission can occur at lower temperatures (often initiated by neutron absorption). [1]
(c) Fusion fuel (isotopes of hydrogen) is more abundant / Fusion produces no long-lived high-level radioactive waste / Fusion has higher energy yield per unit mass. [1]