Module 6 Fission and Fusion Flashcards

1
Q

Why is there a slight increase in mass when water at 100º is boiled to steam?

A

Gain in potential energy to separate particles. This is latent heat.

Plug into E=mc^2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Why is there a gain in mass during ionisation?

A

Energy is gained as electrostatic potential energy to separate opposite charges. Energy is converted to mass by E=mc^2.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Why can the mass gained during ionisation be ignored?

A

Negligible when compared to the original mass.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

What can be said about the masses of particles during radioactive decay?

A

Total final mass is less than total initial mass.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

What happens to the mass lost during nuclear decay?

A

Increases binding energy and gained as kinetic energy in products.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

What is the symbol for a mass defect?

A

Δ m.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Why does a proton plus a neutron have higher mass than a deuterium nucleus?

A

There is a mass defect due to energy put in, to overcome the strong nuclear force.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

What can you do when showing a diagram with three forces where RF=0?

A

Put it into a closed vector triangle.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

How do you calculate the nuclear binding energy?

A

Find mass of original nucleus, find mass of separate protons and neutrons, find change in mass, plug into E=mc^2.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Define binding energy.

A

Minimum energy required to split a nucleus completely into its separate protons and neutrons.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Define mass defect.

A

[mass of protons + mass of neutrons] – mass of nucleus.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

What is used to measure nuclear stability?

A

Binding energy per nucleon.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

How do you calculate binding energy per nucleon?

A

Calculate binding energy, divide by A

(A is nucleon number)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

What is the nucleon number of iron?

A

56.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

What is the proton number of iron?

A

26.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

What is the approximate value for the binding energy per nucleon of iron?

A

8.72 MeV.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

What is the most stable nucleus?

A

Iron-56.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

On binding energy per nucleon (y axis) against nucleon numer (x axis)

To what side of iron does fusion happen?

A

To the left side.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

What happens during fusion?

A

Two nuclei fuse to form a larger one.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

Explain, using binding energies, why fusion releases energy.

A

Two small nuclei join to form a larger one. Total binding energy increases. E=mc^2. Higher mass defect and so energy is released.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

When is energy released during nuclear reactions?

A

Total final mass is less than initial mass. Mass defect (mass is lost). Energy is released according to E=mc^2 as kinetic energy of the products.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

What must be done to calculate the energy released when two protons combine to form a hydrogen-2 atom?

A

Write out an equation. Find mass defect (mass of two protons) - (mass of hydrogen-2 and positron).

Find E using E=mc^2.

Positron will annihilate with an electron. Double mass of one electron and plug into equation E=mc^2.

23
Q

Why is usually a very high temperature required for fusion?

A

High temperature to provide the high kinetic energy to overcome electrostatic repulsion so closest approach can be less than 3 fm and the strong nuclear force can come into play and bind nucleons.

24
Q

Why is a high density required for nuclear fusion?

A

So there is a high probability of a head-on collision so maximum kinetic energy is transferred to electrostatic potential energy.

25
Q

How to find the gain in potential energy of colliding particles during fusion when a temperature is given?

A

Calculate average kinetic energy using KE=3/2kT.

Gain in potential energy = Loss of kinetic energy + Loss of kinetic energy

(both particles lose all their kinetic energy in a head-on collision). So multiply kinetic energy by 2.

26
Q

Describe how you find out the temperature at which fusion of two particles can happen?

A

Find the electrostatic potential energy which is required for r to be 3 fm using the Coulomb equation for energy.

Divide value by 2 to get the kinetic energy of one of the original particles in the collision.

Plug into KE=3/2kT and rearrange for T (in Kelvin).

27
Q

Given the temperature of the core in the sun is 1.5x10^7K, explain why it has a long life.

A

Find the potential energy and thus kinetic energy and temperature required for fusion (r=3 fm).

Value will be greater than temperature.

Plasma of the sun has a Maxwell-Boltzmann distribution.

Very few protons have higher kinetic energy and can fuse. Chance of protons fusing is therefore low and has a longer lifetime.

28
Q

Explain why helium nuclei are much more difficult to fuse when compared to hydrogen nuclei.

A

Each He nucleus has double the charge. When plugged into the Coulomb energy equation, potential energy increases by a factor of 4. Therefore average temperature required increases by a factor of 4.

29
Q

Why does fission have a lower final mass when compared to initial?

A

Mass defect due to neutrons being un-bonded which requires the input of energy, which is converted to an extra mass. Therefore there is a decrease in mass (mass of initial particles - final). Energy is produced during the reaction and is converted to kinetic energy of particles.

30
Q

What is spontaneous fission?

A

A large nucleus splits into two smaller nuclei plus several neutrons and releases energy.

31
Q

What is induced fission?

A

Where a large nucleus absorbs a neutron and splits into two smaller nuclei and several neutrons and releases energy.

32
Q

What is the basic principle of chain reactions?

A

Fission produces neutrons which can induce further fission.

33
Q

Explain what must be done so fission reactions can be controlled.

A

Fission reactions must only produce one neutron so that only one further fission reaction is induced.

34
Q

What are fuel rods?

A

Rods which are enriched with a higher percentage of U-235 which can undergo induced fission.

35
Q

What is the fuel usually used in nuclear reactors?

A

Uranium-235.

36
Q

What does uranium-235 turn into once it undergoes fission?

A

Two smaller nuclei plus on average two neutrons.

37
Q

What is a moderator rod usually made of?

A

Solid carbon graphite (can also be of water).

38
Q

What is the function of a moderator rod?

A

Absorb neutrons from fission and causes them to lose kinetic energy through many collisions, forming thermal neutrons with low kinetic energy which can be absorbed by U-235 inducing fission.

39
Q

Why must moderator rods be used?

A

To decrease kinetic energy of neutrons forming thermal neutrons.

40
Q

Why must thermal neutrons be used for fission?

A

Fast moving ones will rebound and not join nuclei.

41
Q

What are control rods made of?

A

Boron, Cadmium.

42
Q

What is the function of control rods?

A

Absorbs excess neutrons so that on average each fission will induce one further fission reaction.

43
Q

How can a stable temperature of a nuclear reactor be maintained?

A

Lowering or raising control rods.

44
Q

How can the rate of fission be controlled in a nuclear reactor?

A

Lowering or raising control rods.

45
Q

What is nuclear waste?

A

Radioactive byproducts of fission reactions.

46
Q

Why does some nuclear waste need storing?

A

Products are radioactive isotopes with long half-lives so will remain radioactive and potentially dangerous for years.

47
Q

What is a percentage mass conversion of a sample?

A

Mass defect (energy converted) over original mass.

48
Q

Compare the reactions (in practice) of fission and fusion.

A

Fission is a self-sustaining chain reaction that’s easy to start and control. Fusion requires very high temperatures and densities to start; therefore, a high input energy is required to start.

49
Q

Why would a fission reactor require a large input energy?

A

Requires high temperatures and pressures/densities. Strong magnetic fields are needed to contain plasma.

50
Q

Why are fission reactors not used commercially?

A

Have only been shown to be used experimentally and have not been shown to operate continuously.

51
Q

Using the idea of fuel, explain why fusion may be advantageous over fission reactors.

A

Fission reactors require uranium-235 or other elements and isotopes which must be mined and enriched. Thus a finite resource. Fusion reactors only require isotopes of hydrogen which are plentiful in seawater.

52
Q

Using the idea of nuclear waste, explain why fusion may be advantageous when compared to fission.

A

Fission reactors produce large amounts of radioactive waste which must be treated and stored for potentially thousands of years. Fusion reactors produce minimal radioactive waste.

53
Q

Why are fusion reactors considered safer?

A

Fusion reactors may produce a lot of radioactive contamination if shielding is damaged. If control systems fail, a nuclear meltdown may happen. Fusion reactors will shut down if the plasma is not confined and will cool down immediately so fusion stops. Minimal danger.

54
Q

Explain how you show the energy of each photon during an annihilation between a positron and an electron.

A

Find total energy using E=mc^2 (add individual energies). Divide final value by 2.