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A Level H2 Physics Modern Physics Quiz

Free A Level H2 Physics Modern Physics quiz, Qwen3.6 Exam version, with questions, answers, and A Level-style practice for Singapore students.

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A Level H2 Physics From Real Exams Generated by Qwen3.6 Plus Updated 2026-08-17

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Answers

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.
Energy of incident photon E=hcλE = \frac{hc}{\lambda}
E=6.63×1034×3.00×108250×109=7.956×1019 JE = \frac{6.63 \times 10^{-34} \times 3.00 \times 10^8}{250 \times 10^{-9}} = 7.956 \times 10^{-19} \text{ J} [1]
Work function Φ=4.3 eV=4.3×1.60×1019=6.88×1019 J\Phi = 4.3 \text{ eV} = 4.3 \times 1.60 \times 10^{-19} = 6.88 \times 10^{-19} \text{ J} [1]
Max KE =EΦ=7.956×10196.88×1019=1.076×1019 J= E - \Phi = 7.956 \times 10^{-19} - 6.88 \times 10^{-19} = 1.076 \times 10^{-19} \text{ J}
Answer: 1.1×1019 J1.1 \times 10^{-19} \text{ J} [1]

3.
(a) No change. [1]
Max KE depends only on the frequency (energy) of individual photons and the work function (KEmax=hfΦKE_{max} = hf - \Phi). Intensity does not change photon energy. [1]
(b) Increases. [1]
Intensity is proportional to the number of photons incident per unit time. More photons cause more photoelectrons to be emitted per second, increasing the current. [1]

4.
Wave theory predicts that energy accumulates over time, so emission should occur at any frequency given enough intensity/time. [1]
Particle theory states energy is quantized in packets (E=hfE=hf). [1]
If hf<Φhf < \Phi, no single photon has enough energy to eject an electron, regardless of intensity. This explains the threshold frequency. [1]

5.
(a) Planck constant hh (or h/eh/e if plotting VsV_s vs ff, since eVs=hfΦVs=hefΦeeV_s = hf - \Phi \Rightarrow V_s = \frac{h}{e}f - \frac{\Phi}{e}). Note: Standard syllabus accepts h/eh/e for gradient of VsV_s vs ff. [1]
(b) Threshold frequency f0f_0. [1]

6. The minimum energy required to remove an electron from the ground state of an atom to infinity (where it is free from the nucleus). [1]

7.
Energy difference ΔE=E3E2=1.51(3.40)=1.89 eV\Delta E = E_3 - E_2 = -1.51 - (-3.40) = 1.89 \text{ eV} [1]
Convert to Joules: 1.89×1.60×1019=3.024×1019 J1.89 \times 1.60 \times 10^{-19} = 3.024 \times 10^{-19} \text{ J}
λ=hcΔE=6.63×1034×3.00×1083.024×1019\lambda = \frac{hc}{\Delta E} = \frac{6.63 \times 10^{-34} \times 3.00 \times 10^8}{3.024 \times 10^{-19}} [1]
λ=6.59×107 m\lambda = 6.59 \times 10^{-7} \text{ m} (or 659 nm) [1]

8.
Electrons in atoms occupy discrete/quantized energy levels. [1]
Transitions occur only between these specific levels, emitting photons of specific energies (and thus specific wavelengths/frequencies). [1]

9.
(a) Energy required for transition n=1n=2n=1 \to n=2:
ΔE=E2E1=3.40(13.6)=10.2 eV\Delta E = E_2 - E_1 = -3.40 - (-13.6) = 10.2 \text{ eV} [1]
Since incident electron KE (12.0 eV) > 10.2 eV, excitation can occur. [1]
(b) The remaining kinetic energy (12.010.2=1.8 eV12.0 - 10.2 = 1.8 \text{ eV}) is retained by the incident electron as kinetic energy. [1]

10.
High-speed electrons from the cathode collide with target atoms. [1]
They knock out inner-shell (e.g., K-shell) electrons, creating a vacancy. [1]
Outer-shell electrons drop down to fill the vacancy, emitting X-ray photons with specific energies corresponding to the difference in binding energies of the shells. [1]

11.
The energy required to completely separate a nucleus into its constituent protons and neutrons. [1]
(Or: The energy released when protons and neutrons combine to form a nucleus). [1]

12.
Mass of constituents: 2(1.00728)+2(1.00867)=2.01456+2.01734=4.03190 u2(1.00728) + 2(1.00867) = 2.01456 + 2.01734 = 4.03190 \text{ u} [1]
Mass defect Δm=4.031904.00151=0.03039 u\Delta m = 4.03190 - 4.00151 = 0.03039 \text{ u}
Binding Energy BE=0.03039×931.5=28.308 MeVBE = 0.03039 \times 931.5 = 28.308 \text{ MeV} [1]
BE per nucleon =28.308/4=7.08 MeV= 28.308 / 4 = 7.08 \text{ MeV} [1]

13.

  1. β\beta^- involves emission of an electron (and antineutrino); γ\gamma is electromagnetic radiation (photon). [1]
  2. β\beta^- changes the proton/neutron number (transmutation); γ\gamma does not change the composition of the nucleus. [1]
    (Other valid answers: Charge, Mass, Penetrating power)

14.
Number of half-lives n=60/15=4n = 60 / 15 = 4 [1]
Activity A=A0(1/2)n=8.0×104×(1/2)4A = A_0 (1/2)^n = 8.0 \times 10^4 \times (1/2)^4
A=8.0×104/16=5.0×103 BqA = 8.0 \times 10^4 / 16 = 5.0 \times 10^3 \text{ Bq} [1]

15.
When nucleons combine, energy is released (binding energy). [1]
By mass-energy equivalence (E=mc2E=mc^2), this loss of energy corresponds to a loss of mass. [1]

16.
(a) A56A \approx 56 (Iron/Fe). [1]
(b) Light nuclei have lower BE per nucleon than the product nucleus formed after fusion. [1]
The product nucleus is more tightly bound (higher BE per nucleon). [1]
The increase in total binding energy corresponds to energy released to the surroundings. [1]

17.
Kinetic Energy KE=eV=1.60×1019×150=2.40×1017 JKE = eV = 1.60 \times 10^{-19} \times 150 = 2.40 \times 10^{-17} \text{ J}
Momentum p=2meKE=2×9.11×1031×2.40×1017p = \sqrt{2m_e KE} = \sqrt{2 \times 9.11 \times 10^{-31} \times 2.40 \times 10^{-17}} [1]
p=4.3728×1047=6.61×1024 kg m s1p = \sqrt{4.3728 \times 10^{-47}} = 6.61 \times 10^{-24} \text{ kg m s}^{-1}
λ=h/p=6.63×10346.61×1024\lambda = h/p = \frac{6.63 \times 10^{-34}}{6.61 \times 10^{-24}} [1]
λ=1.00×1010 m\lambda = 1.00 \times 10^{-10} \text{ m} [1]

18.
(a) Wave nature (or wave-particle duality). [1]
(b) Diameter decreases. [1]
Higher voltage \rightarrow higher momentum \rightarrow shorter de Broglie wavelength. Shorter wavelength diffracts less, resulting in smaller ring diameters. [1]

19.
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}
Number of photons N=PE=2.0×1033.14×1019N = \frac{P}{E} = \frac{2.0 \times 10^{-3}}{3.14 \times 10^{-19}} [1]
N=6.37×1015 s1N = 6.37 \times 10^{15} \text{ s}^{-1} [1]

20.
An incident photon of specific energy interacts with an excited atom, causing it to drop to a lower energy level and emit a second photon. [1]
The emitted photon is identical to the incident photon in frequency, phase, direction, and polarization. [1]
Condition: Population Inversion (more atoms in excited state than ground state). [1]