Nuclear Radiation Flashcards

You may prefer our related Brainscape-certified flashcards:
1
Q

What happens to nuclei that are unstable

A

They break down to become more stable, making them radioactive.

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

What could instability within a nucleus be caused by

A

too many neutrons
too few neutrons
too many nucleons (nucleus is too heavy)
too much energy in the nucleus

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

What is radioactive/nuclear decay

A

The nucleus decays by releasing energy and/or particles, until it reaches a stable form

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

What is the nature of radioactive decay

A

It is random and spontaneous, it can’t be predicted

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

what is an alpha particle (α) made of

A

A helium nucleus, 2 protons, 2 neutrons & 2 electrons

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

What is the relative charge on an alpha particle

A

+2

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

What is the mass of an alpha particle

A

4 u (atomic units)

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

What is Beta-minus (β−), which is the normal Beta particle, and it’s properties

A

An electron, -1 charge, negligible mass

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

What is Beta-plus (β+) particle and it’s properties

A

A positron, +1 charge, negligible mass

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

What is gamma particle (γ) and it’s properties

A

Short-wavelength, high-frequency EM wave (gamma wave). Charge = 0, mass = 0

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

What can all waves, like gamma, act as

A

As a particle. You can have gamma photons

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

What are radioactive emissions known as and why

A

Ionising radiation because when radiation hits an atom, it can knock off electrons, creating an ion.

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

How are alpha, beta and gamma radiation tested to see if they penetrate

A

They are fired at a variety of objects with detectors placed on the other side. If they are detected, that means they have penetrated that object

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

What is the ionising ability of alpha, beta-minus and gamma radiation

A

alpha - strong
beta-minus - weak
gamma - very weak

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

What is the speed of alpha, beta-minus and gamma radiation

A

alpha - slow
beta-minus - fast
gamma - speed of light

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

What is the penetration/range of alpha, beta-minus and gamma radiation

A

alpha - very small, absorbed by paper or a few cm of air
beta-minus - small, absorbed by ~3 mm of aluminium
gamma - very large, absorbed by many cm of lead, or several meters of concrete

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

Is alpha, beta-minus and gamma radiation affected by magnetic field

A

Alpha and Beta-minus have a charge, so they are affected by a magnetic field. Gamma is not affected as it has a charge of 0.

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

Why does beta-plus radiation not have the properties of the others

A

It is annihilated by an electron, so it has virtually zero range.

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

How are ionising ability, charge and penetration range related

A

The more charge the radiation has, the more ionising ability it has. A particle with high ionising ability will have a low penetration range.

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

How are ionising ability, charge and penetration range related in alpha radiation

A

Alpha particles are strongly positive, +2 charge, so they can easily pull electrons off atoms, ionising them. Ionizing an atom transfers some of the energy from the alpha particle to the atom (you are pulling off an electron which takes energy). The alpha particle quickly ionises many atoms (about 10,000 ionizations per alpha particle) and loses its energy, meaning alpha particles don’t travel very far, they have low penetration.

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

How are ionising ability, charge and penetration range related in beta-minus radiation

A

Beta-minus particles have lower mass and charge than alpha particles, but a higher speed, so they also have a significant amount of energy. This means they can still knock off electrons from atoms. Each beta-particle will ionise about 100 atoms, losing energy at each ionisation. Since beta-minus has lower number of ionisations than alpha radiation , it travels further than alpha radiation, meaning it has higher penetration

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

How are ionising ability, charge and penetration range related in gamma radiation

A

Gamma radiation is even more weakly ionising than beta-minus as it has 0 charge and 0 mass. This means it has very high penetration, as it has a lot of energy for traveling/penetrating since it isn’t losing it by ionising a bunch of atoms

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

What must you do when you take a reading from a radioactive source (CORE PRAC ADVICE)

A

You need to measure the background radiation separately and subtract it from your measurement

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

What are the sources of background radiation

A

The air: Radioactive radon gas released from rocks. It emits alpha radiation. The concentration of this gas in the atmosphere varies a lot from place to place, but it’s usually the largest contributor to background radiation.

The ground and buildings: all rock contains radioactive isotopes

Cosmic radiation: Cosmic rays are particles (mostly high-energy protons) from space. When they collide with particles in the upper atmosphere, they produce nuclear radiation

Living things: All plants and animals contain carbon, and some of this will be the radioactive isotope carbon-14

Man-made radiation: In most areas, radiation from medical or industrial sources make up a tiny, tiny fraction of the background radiation.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
25
Q

How do you write nuclear decay equations

A

In standard chemistry style notation. You write the proton number on the bottom and the nucleon number on top

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
26
Q

What must be conserved in decay equations

A

Charge and Nucleon number. Decay equations need to be balanced, in every nuclear reaction, including fission and fusion, charge, and nucleon number must be conserved.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
27
Q

How do you check that charge is conserved in a nuclear decay equation

A

The total proton number before and after an interaction must be the same. This will tell you whether charge is conserved

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
28
Q

How are beta-minus particles written in nuclear decay equations

A

0
β
-1

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
29
Q

What else, other than nucleon number and charge, must be conserved in all nuclear reactions

A

Energy and momentum

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
30
Q

Why does mass not have to be conserved in nuclear reactions

A

The mass of an alpha particle is less than the individual masses of 2 protons and 2 neutrons due to the mass deficit. The energy is released when nucleons bind together to form alpha particles, and this accounts for the missing mass

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
31
Q

What is the concept of mass deficit in nuclear physics

A

Making bonds is exothermic, so it releases energy. This means that particles together in a nucleus have less energy, and therefore less mass than the same particles separated. 2 protons and 2 neutrons weigh 100g, but a nucleus with 2 protons and 2 neutrons weighs 70g. Because when the bonds are formed, energy is released in the form of mass, which is what the difference in mass is. This is the mass deficit. When you want to split the nucleons apart, you have to put energy in.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
32
Q

Where does alpha emission only happen and why

A

Alpha emission only happens in the nuclei of very heavy atoms like uranium and radium. This is because the nuclei of these atoms are too massive to be stable.

Uranium Atomic mass: 238
Radium Atomic mass: 226

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
33
Q

How do proton number and nucleon number of the atom change when an alpha particle is emitted

A

Proton number decreases by 2, nucleon number decreases by 4

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
34
Q

What does beta-minus decay involve

A

The emission of an electron from the nucleus along with an antineutrino

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
35
Q

Where does beta-minus decay happen

A

In isotopes that are neutron rich, meaning they have many more neutrons than protons in their nucleus

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
36
Q

What happens in beta-minus decay

A

One of the neutrons in the nucleus decays into a proton and ejects a beta-minus particle (an electron) and an antineutrino

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
37
Q

How do proton number and nucleon number of the atom change when a beta-minus particle and an antineutrino is emitted

A

Proton number increases by 1. Nucleon number stays the same.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
38
Q

What happens in beta-plus emission

A

A proton gets changed into a neutron, releasing a positron and a neutrino.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
39
Q

How do proton number and nucleon number of the atom change in beta-plus emission

A

Proton number decreases by 1. Nucleon number stays the same

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
40
Q

When does gamma radiation occur

A

This often happens after an alpha or beta decay has occurred.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
41
Q

How do proton number and nucleon number of the atom change in gamma emission and why

A

During gamma emission, there is no change to nuclear constituents. The nucleus just loses excess energy

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
42
Q

What happens in gamma radiation

A

An excited nucleus, nucleus with excess energy, loses this energy by emitting a gamma ray. Gamma rays can be emitted from a nucleus with excess, too much energy.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
43
Q

What is the general overview of the absorption of gamma radiation by lead experiment

A
  1. Choose radioactive source, use micrometer to verify all lead sheets are same thickness, check background radiation with Geiger counter, place radioactive source 15cm from Geiger counter.
  2. Place lead into clamp perpendicularly so it completely blocks off straight line between source and counter. Record count rate, then add another lead sheet to clamp to increase combined thickness of lead sheets. Continue the experiment for up to 10 lead sheets.
  3. Subtract background count rate from results and plot the graph of corrected count rate (y-axis) vs thickness of lead (x-axis). Reduction in count rate means increase in absorption.
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
44
Q

In the absorption of gamma radiation by lead experiment, what should you check the lead sheets for and how

A

Your lead sheets should all be the same thickness. Use a micrometer to measure their thickness and verify this.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
45
Q

In the absorption of gamma radiation by lead experiment, how do you check for background radiation, and why do you need to do this

A

Turn on the Geiger counter and take a reading of the background count rate (in counts per sec). Do this 3 times and take an average. You’ll need to subtract this from your count rate measurements to get the corrected count rate.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
46
Q

In the absorption of gamma radiation by lead experiment, how should you position your lead sheets in relation to the radiation source

A

When placing the piece of lead in the clamp, make sure it is perpendicular to the Geiger counter source so it completely blocks the straight line between the source and the counter.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
47
Q

In the absorption of gamma radiation by lead experiment, when measuring the count rate for each thickness of lead used, what should you do

A

Measure the count rate 3 times then take an average for each thickness

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
48
Q

In the absorption of gamma radiation by lead experiment, how many lead sheets should you test up to

A

10 lead sheets is a good amount

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
49
Q

In the absorption of gamma radiation by lead experiment, what must you do once the experiment is finished for safety reasons and why

A

Once the experiment is finished, put away the gamma source immediately. You don’t want to be exposed to more radiation than you need to be.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
50
Q

In the absorption of gamma radiation by lead experiment, what must you do to your recorded values before plotting them on a graph

A

Correct your data by subtracting the background radiation from your results.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
51
Q

In the absorption of gamma radiation by lead experiment, once you initially position the radioactive source, what must you not do and why

A

Once you’ve placed the radioactive source at about a 15cm distance from the tube, don’t move it again or it could impact the count rate on the Geiger counter.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
52
Q

In the absorption of gamma radiation by lead experiment, what is an example of a radioactive source you can use

A

Cobalt-60

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
53
Q

In the absorption of gamma radiation by lead experiment, how should you set up the apparatus

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
54
Q

In the absorption of gamma radiation by lead experiment, what graph should you plot, and what results do you expect to see

A

Then plot a graph of corrected count rate against thickness of lead. We should see that the count rate reduces with each sheet of lead. This means the absorption increases.

55
Q

In the absorption of gamma radiation by lead experiment, what is the count rate

A

The count rate is the number of counts detected per second

56
Q

Define Mass Defect

A

The difference in mass between a nucleus and it’s constituent parts

57
Q

Define binding energy

A

Energy equivalent to the mass deficit/difference when nucleons bind together to form an atomic nucleus

58
Q

What is rate of radioactive decay measured by

A

The decay constant

59
Q

How can you predict how many nuclei will decay in a given amount of time

A

Using the equation for nuclear activity

60
Q

What is activity (A) measured in

A

Activity is measured in becquerels (Bq).

61
Q

What is activity (A) in nuclear radiation

A

The number of nuclei that decay each second

62
Q

What is activity in nuclear radiation proportional to

A

Activity is proportional to the size of the sample

63
Q

What does a value of 1 Bq mean

A

1 Bq means that 1 nucleus decays per second (s^-1).

64
Q

What is the decay constant (λ)

A

The probability that a given nucleus will decay each second

65
Q

What does a larger value of decay constant (λ) mean

A

The bigger the value of λ, the faster the rate of decay. Its unit is s^-1.

66
Q

What are the units for decay constant (λ)

A

Its unit is s^-1.

67
Q

What is the equation linking nuclear activity and decay constant

A

A = λN

activity = decay constant x number of undecayed nuclei

68
Q

How else can you write represent activity and why can you do it this way

A

Since it is the rate of nuclei decay, it can be represented as a derivative. It will be a negative derivative as the number of decayed nuclei will be decreasing, so we write it as.

Because activity, A, is number of nuclei that decay each second, it is equal to minus the rate of change in the number of undecayed nuclei, which is dN/dt

-dN/dt

A = -dN/dt = λN

69
Q

Why is there a negative sign in front of dN/dt

A

The number of undecayed nuclei (N) is decreasing, so dN/dt is negative. A negative sign must be put in front of it to make sure A is positive.

70
Q

How can you model radioactive decay using a spreadsheet

A
  1. Set up spreadsheet columns for t, ΔN, N, Δt and λ.
  2. Decide on Δt interval to use depending on λ.
  3. Enter formulas into spreadsheet to calculate N in sample after each interval. Use ΔN = -λ xNx t
  4. Plot graph of N over t, changing Δt slightly to get a nice exponential shape if needed.

TABLE AND GRAPH FROM PG 152

71
Q

What is Δt in the experiment with setting up a spreadsheet to model -ΔN/Δt = λN

A

This is the time interval between the values of N that the spreadsheet will calculate. The most sensible time interval will depends on your decay constant.

72
Q

When setting up a spreadsheet to model -ΔN/Δt = λN, how should your columns be set up

A

Set up a spreadsheet with column headings for total time (t), change in number of number of undecayed nuclei (ΔN), and number of undecayed nuclei (N), and data input cells for Δt and λ

73
Q

What do you need to model how an isotope sample will decay on a spreadsheet

A

ΔN, Δt λ, N_0.

You need these values to model -ΔN/Δt = λN.

74
Q

How can you model the rate of radioactive decay and why

A

The rate of change of N, dN/dt, is close to the change in N, ΔN, divided by the change in t, Δt, provided that Δt is small. So you can model radioactive decay as: -ΔN/Δt = λN.

75
Q

What kind of process is radioactive decay

A

Radioactive decay is an iterative process (the number of nuclei that decay in one time period controls the number that are available to decay in the next)

76
Q

What is the equation to work out the number of undecayed nuclei remaining, N

A

N = N_0 e^-(λt)

N_0, initial number of undecayed nuclei
t, time, is measured in seconds
This is the equation of the exponential graph generated by the spreadsheet.

77
Q

What does the value of N depend on and why

A

N, number of undecayed nuclei, depends on N_0, number of undecayed nuclei originally present, because radioactive decay is an iterative process.

78
Q

What is the equation for how a radioactive sample’s activity goes down as it decays

A

A = A_0 e^(-λt)

A: Activity
A_0: Initial activity at t=0

Both A and A_0 are measured in Bq.

79
Q

What is the half-life of an isotope, and which isotopes have it

A

The half life, t_(1/2), is the average time it takes for the number of undecayed nuclei to halve. All radioactive isotopes have a half-life

80
Q

How is half-life measured

A

By measuring the time it takes the activity or count rate to half. We do it this way because measuring the number of undecayed nuclei is difficult.

81
Q

What does a longer half-life mean

A

The longer the half-life of an isotope, the longer it stays radioactive.

82
Q

What is the count rate

A

The number of decays detected per second (this is lower than activity)

83
Q

How do you use the graph of N against t, number of undecayed nuclei against time, to find the half-life

A

Read off the value of N when t=0 (this is N_0). Go to half the original value of N (half of N_0). Draw a horizontal line to the curve, then a vertical line to the x-axis. Half-life is where this line meets the x-axis. Check your answer by checking the value for 1/4 of N_0 and 3/4 of N_0

84
Q

Does half life change as the number of undecayed nuclei decreases

A

No, half life stays the same. It takes the same amount of time for half the nuclei to decay regardless of the number of nuclei you start with.

85
Q

How to measure half-life of a radioactive material

A

Using a proctactinium generator, a bottle containing a uranium salt, the decay products of uranium (including protactinium-234) and two solvents, which separate out the two layers.

86
Q

In a nutshell, how to do protactinium generator experiment

A
  1. Shake bottle to activate generator
  2. Wait for layer separation, p-234 in top layer. Uranium salt in bottom. Point geiger-muller tube at top layer to measure activity of p-234
  3. When layers separate, measure count rate asap. How many counts you get in 10 seconds of measuring, do this every 30 seconds
  4. Record all data, leave bottle for 10 mins, then take count rate again. This gives you background radiation.
  5. Subtract background from count rate, then plot graph of count rate against time. Should be negative exponential.
87
Q

How do you start activate the protactinium generator so you can measure the count rate

A

Shake the bottle to mix the solvents, then add it to the equipment shown

Wait for the liquids to separate. Protactinium-234 will be in top layer of solution, the uranium salt in the bottom layer. Point the Geiger-Muller tube at the top layer to measure activity of the protactinium-234.

88
Q

How does the graph of count rate against time from a protactinium generator look like, and what does it help you find

A

Negative exponential. You can use this graph to find the half-life. In this case the half-life is the time taken for the count rate to halve.

89
Q

In the protactinium generator, what how do you account for background radiation

A

First measure count rate of generator and count rate of background. Subtract value of background from your measured count rates, then plot a graph of count rate against time. It should look like the graph on the right. You can use this graph to find the half-life in exactly the same way as above. In this case the half-life is the time taken for the count rate to halve.

90
Q

In the protactinium generator, what should you do once you have recorded the count rate

A

Once you’ve collected your data, leave the bottle to stand for at least 10 minutes, then take the count rate again. This is the background count rate corresponding to the background radiation (You could also do this at the beginning of the experiment before shaking the bottle).

91
Q

What does the protactinium generator look like

A

Bottle contains uranium salt, decay products of uranium, including protactinium-234, and 2 solvents that separate into layers

92
Q

In the protactinium generator, when should you record the count rate

A

As soon as the liquids separate, record the count rate (e.g how many counts you get in 10 seconds). Re-measure the count rate at sensible intervals (e.g every 30 seconds)

93
Q

What is the equation to calculate decay constant (λ), from half-life (t_1/2)

A

λ = ln2 / t_1/2

λ units are s^-1
t_1/2 units are seconds

You can rearrange this to find half life from decay constant as well

94
Q

How to take logs of exponential decay equations

A

REMEMBER to subtract the background activity from any measurement first.

The gradient of the line is -λ (decay constant). From this you can calculate the half-life, t_1/2, of the sample. This works for graphs of activity against time too.
A = A_0 e^-λt —> ln (A) = -λt + ln(A_0).

95
Q

Define binding energy

A

The energy needed to separate all of the nucleons in a nucleus. This is equivalent to the mass deficit.

96
Q

What is binding energy measured in

A

MeV

97
Q

How do you convert from atomic mass, u, to kg

A

Multiply the u value by 1.66 x 10^-27. To go the other way, divide the mass in kg by 1.66 x 10^-27

98
Q

How do you convert from Joules to MeV

A

1MeV = 1.60 x 10^-13 J

Divide the value in joules by 1.60 x 10^-13. If you want to go from MeV to Joules, multiply the value in joules by 1.60 x 10^-13.

99
Q

What is the principle of mass deficit

A

The mass of a nucleus is less than the mass of its constituent parts. The difference in mass between the nucleus and the nucleons separated is called the mass deficit.

100
Q

What happens when nucleons join together

A

Total mass decreases, this lost mass is converted into energy and released. The amount of energy released is equivalent to the mass deficit.

101
Q

How do you calculate the energy released when nucleons join together to make a nucleus

A

Use E=mc² and take the value for m as the mass deficit.

102
Q

What are the units for E=mc²

A

m is in kg
E is in joules
c is in ms^-1

103
Q

How much energy would you have to use to split the nucleons in a nucleus completely apart

A

If you pulled the nucleus completely apart, the energy you’d have to use to do it would be the same as the energy released when the nucleus is formed.

104
Q

How do you caluclate the binding energy per unit of mass deficit, and what are the units

A

binding energy / mass deficit
Units, MeV u^-1

105
Q

What does binding energy per unit of mass deficit of 930 MeV u^-1 mean

A

This means that a mass deficit of 1u is equivalent to about 930 MeV of binding energy. You can use this approximation to check your answer.

106
Q

What is the equation and units for binding energy per nucleon

A

binding energy (B) / Nucleon Number (A)
Measured in MeV

107
Q

What does a high binding energy per nucleon mean

A

More energy is needed to remove nucleons from the nucleus

108
Q

Where do the most stable nuclei occur

A

Around the maximum point on the graph of binding energy per nucleon against nucleon number, which is at nucleon number 56, Fe - Iron.

109
Q

How does nuclear fusion affect binding energy per nucleon

A

Nuclear fusion is when you combine nuclei. This increases the binding energy per nucleon dramatically, which means a lot of energy is released during nuclear fusion.

110
Q

How does nuclear fission affect binding energy per nucleon

A

Fission is when nuclei are split in two. The nucleon numbers of the two new nuclei are smaller than the original nucleus, which means there is an increase in the binding energy per nucleon. So energy is also released during nuclear fission, but not as much energy as fusion.

111
Q

Why are elements with the highest binding energy per nucleon the most stable, like Fe

A

Highest binding energy per nucleon means it takes that the bond between nucleons has the most energy out of any element. To split up the nucleons and separate the bonds, a lot of energy is needed. Since it is difficult to do, it is the most stable element, as not many things can cause the nucleons to split up.

112
Q

What does the graph of binding energy per nucleon, in MeV, against Nucleon Number, no units, look like

A
113
Q

How do you use the binding energy per nucleon graph to estimate the energy released from nuclear fusion

A
114
Q

How do you use the binding energy per nucleon graph to estimate the energy released from nuclear fission

A
115
Q

Why does fission happen

A

Because heavy nuclei are unstable. This means some can randomly split into 2 smaller nuclei (and sometimes several neutrons)

116
Q

Which gives you more energy generally, fusion or fission

A

Fusion gives you more energy per nucleon, but fission generally gives you more energy per reaction.

117
Q

What is the difference between spontaneous and induced fission

A

Spontaneous is when it happens by itself, induced is if we encourage it to happen

118
Q

Why is energy released during nuclear fission

A

Because the new, smaller nuclei have a higher binding energy per nucleon and a lower total mass, { so some energy is released due to conservation of mass energy } - idk if this part is right though, ask chris or paulio

119
Q

What relationship does the size of the nucleus have to fission

A

The larger the nucleus, the more unstable it will be, so the large nuclei are more likely to spontaneously fission.

120
Q

What does spontaneous fission limit

A

Limits the number of nucleons that a nucleus can contain, in other words, it limits the number of possible elements, because if we try to get an even larger nucleus than we have already discovered, the element is very likely to have spontaneous fission occur.

121
Q

What is an example of fission

A

Fission can be induced by making a neutron enter a U-235 nucleus, causing it to become very unstable.

Only low energy neutrons can be captured this way. A low energy neutron is called a thermal neutron.

122
Q

Which nuclear process do nuclear power stations use

A

Nuclear power stations generate electricity from nuclear fission reactions

123
Q

What is nuclear fusion

A

Nuclei can fuse together, increasing the binding energy per nucleon and releasing a lot of energy.

124
Q

What force exists between nuclei that we must overcome to do fusion

A

All nuclei are positively charged, so there will be an electrostatic (otherwise known as Coulomb) force of repulsion between them

125
Q

How can fusion happen if there is a repulsive force between nuclei

A

Nuclei can only fuse if they overcome this electrostatic force and get close enough for an attractive force called the strong interaction force to hold them together.

126
Q

What is the force which holds nucleons together

A

Strong interaction force

127
Q

Which conditions does fusion require for it to happen

A

Very high temperatures, and a high density of matter.

128
Q

Why does fusion require very high temperatures to occur

A

Typically fusion reactions need about 1 MeV of kinetic energy. That is a very large amount of energy relatively. So very high temperatures are required

129
Q

Why does fusion require a high density of matter to occur

A

Higher densities increases the likelihood of collisions between nuclei.

130
Q

Where does fusion occur

A

In the core of stars

131
Q

Where does the energy emitted from stars come from

A

Nuclear fusion reactions. This includes the energy from the Sun

132
Q

Why is fusion able to happen in stars

A

Because the temperature in the core of stars is so high, the core of the sun is about 10^7 Kelvin.

133
Q

What happens with the atoms in the core of a star

A

Because of the extremely high temperatures, atoms don’t exist. The negatively charged electrons are stripped away, leaving positively charged nuclei and free electrons. The resulting mixture is called plasma

134
Q

How does is nuclear fusion maintained in stars

A

A lot of energy is released during nuclear fusion because the new, heavier nuclei have much higher binding energy per nucleon. This helps to maintain the temperatures for further fusion reactions to happen.