Physics
Quantum and nuclear processes
- 1.
Find energy in joules of a photon of frequency 5.00e14 Hz. Use h = 6.63e-34 J s. Explain why doubling beam intensity at fixed frequency does not double photon energy.
[3 marks]Answer explanation
Draft walkthroughs are based on marking guidance, not independently verified derivations.
- Multiply Planck's constant by frequency, retaining full precision until rounding.
- A brighter monochromatic beam supplies more photons, each with the same hf.
Marking points
- E = hf.
- E = 3.32e-19 J (3 significant figures).
- Intensity changes photon rate per unit area, not energy per photon at fixed frequency.
Examiner tip: Photon energy is set by frequency, not brightness.
- 2.
A stationary uranium-238 nucleus emits an alpha particle. State the daughter's mass and proton numbers and explain why it recoils. Neglect photon emission.
[3 marks] · no calculatorAnswer explanation
Draft walkthroughs are based on marking guidance, not independently verified derivations.
- Subtract alpha's nucleon and proton counts separately; the daughter is not another uranium isotope.
- Different masses mean equal momentum magnitudes do not imply equal recoil speeds.
Marking points
- Alpha has mass number 4 and proton number 2; uranium has proton number 92.
- Daughter has mass number 234 and proton number 90 (thorium).
- The daughter recoils with momentum equal and opposite to alpha momentum, conserving initial zero momentum.
Examiner tip: Conserve both nucleon number and charge in the decay equation.
- 3.
An atom emits a photon when its electron moves from -1.50 eV to -3.50 eV. Find wavelength using h = 6.63e-34 J s, c = 3.00e8 m s^-1 and 1 eV = 1.60e-19 J. Explain why the atom loses energy.
[3 marks]Answer explanation
Draft walkthroughs are based on marking guidance, not independently verified derivations.
- Use initial minus final level for positive emitted photon energy: -1.50 - (-3.50).
- Convert eV to joules before dividing hc; the negative level labels do not mean negative photon energy.
Marking points
- Photon energy is 2.00 eV = 3.20e-19 J.
- lambda = hc/E = 622 nm (3 significant figures).
- The final level is lower; energy difference leaves the atom as the photon.
Examiner tip: Use the difference between levels, not the magnitude of either individual level.
- 4.
A sample initially contains 2.00e12 radioactive nuclei and has half-life 6.00 hours. Find decay constant in s^-1 and activity after 12.0 hours. Assume no daughter contribution. Give 3 significant figures.
[3 marks]Answer explanation
Draft walkthroughs are based on marking guidance, not independently verified derivations.
- Activity counts decays per second, so convert the half-life to seconds before finding lambda.
- Use the remaining parent population and unrounded lambda; counting daughters would violate the stated model.
Marking points
- lambda = ln(2)/(6.00*3600) = 3.21e-5 s^-1.
- After two half-lives N = 5.00e11.
- Activity lambda N = 1.60e7 Bq (3 significant figures).
Examiner tip: Becquerels require seconds, even when elapsed times are stated in hours.
- 5.
An electron initially at rest is accelerated through 150 V in vacuum. Find its de Broglie wavelength using e = 1.60e-19 C, m = 9.11e-31 kg, h = 6.63e-34 J s. Use non-relativistic mechanics and justify that assumption from its speed with c = 3.00e8 m s^-1.
[3 marks]Answer explanation
Draft walkthroughs are based on marking guidance, not independently verified derivations.
- Electric potential energy supplies kinetic energy, and the classical momentum follows from KE = p^2/(2m).
- This is a matter-wave wavelength; hc/E is the photon formula and is not applicable to this electron.
Marking points
- KE = eV; momentum p = sqrt(2meV).
- lambda = h/p = 1.00e-10 m (3 significant figures).
- v = 7.26e6 m s^-1, about 0.0242c, so a non-relativistic approximation is reasonable.
Examiner tip: Use the magnitude of electron charge for energy gained through the accelerating voltage.
- 6.
A nucleus with mass number 4 has mass defect 0.0300 u relative to separated nucleons. Use 1 u = 1.66e-27 kg, c = 3.00e8 m s^-1 and 1 MeV = 1.60e-13 J. Find total binding energy and binding energy per nucleon. Explain the sign of energy needed to separate it.
[3 marks]Answer explanation
Draft walkthroughs are based on marking guidance, not independently verified derivations.
- Use nuclear masses consistently with the separated nucleons; the supplied defect already accounts for that comparison.
- The bound state has lower mass-energy. Separation reverses binding and therefore requires external energy, rather than releasing it.
Marking points
- Mass defect = 4.98e-29 kg; binding energy = delta m c^2.
- Total binding energy = 4.48e-12 J = 28.0 MeV (3 significant figures).
- Binding energy per nucleon = 7.00 MeV; positive energy must be supplied to separate the nucleus.
Examiner tip: Divide total binding energy by mass number, not proton number.
Marking points are indicative, not an official mark scheme. Accept equivalent valid methods and supported interpretations that address the task; award each mark once without requiring the model wording.