Nuclear Fusion & Fission (Edexcel International A Level (IAL) Physics): Exam Questions

Exam code: YPH11

1 hour9 questions
1a
2 marks

Experiments with muons are taking place at Fermilab in the USA to improve our understanding of the standard model.

The muon belongs to the same family of particles as the electron.

State how the muon is classified in the standard model.

1b
2 marks

A muon (μ) can be produced by the decay shown in this nuclear equation.

         π  μ + ν μ

State the names of the two other particles involved.

1c
3 marks

A website states: “The rest mass of a muon is 106 MeV / c2, which is a little over 200 times that of an electron.”

Deduce whether this statement is correct.

1d
7 marks

Muons are stored in a ‘storage ring’ at Fermilab. The website describes the ring as having a circumference of 44.7 m and using a magnetic field of flux density 1.45 T.

The website claims that this enables the storage ring to confine muons with a momentum of 3.10 GeV / c.

i) Explain why the unit GeV / c is a valid unit for momentum.

(2)

ii) Deduce whether the website’s claim is correct.

muon charge = −1.6 × 10−19 C

3.10 GeV / c = 1.65 × 10–18 N s

(3)

iii) Stationary muons are unstable and have a mean lifetime of a few microseconds.

Explain why muons in the ring are observed to have a much greater mean lifetime.

(2)

2a
4 marks

Thorium is an unstable isotope that decays into radium as shown in the nuclear equation.

Th90228  Ra88224 + α24

The table below gives the masses of the nuclei.

Nucleus

Mass/u

228Th

228.02873

224Ra

224.02021

4α

4.00260

Show that the energy released in the decay is about 5.5 MeV

2b
4 marks

A textbook states that the kinetic energy gained by the alpha particle when a nucleus of thorium‐228 decays is equal to 5.4 Me V.

Comment on this statement. Your answer should include a calculation.

3
6 marks

Nuclear fusion in the core of a star is the source of the star’s power output.

Explain the conditions required to bring about and maintain nuclear fusion in stars.

4a
1 mark

Many countries use nuclear power stations to provide electrical power. Energy is released when nuclei undergo fission in the core of the reactor.

State what is meant by nuclear fission.

4b
3 marks

i) Sketch a graph to show how the binding energy per nucleon varies with nucleon number, for a wide range of isotopes.

q18bi-wph15-05-june-2021-edexcel-int-as-and-a-level-phy

(2)

ii) Mark the position of iron-56 on your graph.

(1)

4c
2 marks

Complete the nuclear equation below.

U92236  Sr38 + Xe141 + 2 × n

4d
2 marks

Calculate, in MeV, the binding energy per nucleon for a nucleus of U92236.

Mass/GeV/c2

U92236

219.8750

n

0.93956

p

0.93827

Binding energy per nucleon = ............................................ MeV

4e
6 marks

Ultraviolet radiation (UV) is produced when alpha particles interact with air.

This can be used to detect alpha particles when a nuclear reactor is decommissioned.

Explain how UV is produced by alpha particles in the air, and why detecting UV has advantages compared with detecting alpha particles directly.

1a
2 marks

Actinium‐225 is a radioactive isotope. It decays to francium by emitting alpha particles.

Actinium‐225 has a short half-life, which makes it suitable for medical applications.

Complete the nuclear equation for this decay.

Ac89225   Fr + α

1b
4 marks

In a radioactive decay, energy is released and the total mass decreases.

Show that the energy released if the mass decreases by 1 u is about 930 MeV.

1c
4 marks

The francium nucleus and the alpha particle move away from each other after the decay.

Explain why the kinetic energy given to the alpha particle is just less than 5.9 MeV.

mass decrease for the decay = 6.35 × 10–3 u

1d
4 marks

The activity of a sample of actinium‐225 is 7.4 × 107 Bq when it is prepared.

Calculate the number of actinium atoms in the sample 7.0 days later.

half‐life of actinium-225 = 9.9 days

Number of actinium atoms after 7.0 days = ...........................