Topic 11: Nuclear Radiation Flashcards

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1
Q

What is the definition of binding energy?

A

Binding energy is the energy required to separate a nucleus into individual constituents (protons and neutrons).

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2
Q

How does binding energy change in either fission and fusion?

A

Total binding energy always increases as energy is always released during reaction.

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3
Q

Why is the mass of a nucleus always lower than the mass of the mass of its constituents?

A

The mass ‘lost’ is converted into energy and released. Known as mass deficit.

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4
Q

What is atomic mass unit?

A

Atomic mass unit is defined as 1/12 of the mass of a carbon-12 atom (1u = 1.661x10^27).

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5
Q

What is a mass defect?

A

When the mass of the constituents is greater than the mass of the nucleus.

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6
Q

Why does a mass defect occur?

A

A mass defect occurs because energy is required for nucleons to join together so the lost mass is converted into energy and released

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7
Q

What is nuclear fission?

A

Nuclear fission is the splitting of a large nucleus into 2 daughter nuclei.

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8
Q

When does nuclear fission usually occur?

A

In very large nuclei, which are unstable.

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9
Q

Why is energy released during fission?

A

because the Smaller daughter nuclei have a higher binding energy per nucleon.

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10
Q

What is nuclear fusion?

A

When two smaller nuclei join together forming one larger nucleus.

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11
Q

Why is enegy released during fusion?

A

Because the larger nucleus has a much higher binding energy per nucleon.

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12
Q

What is the binding energy per nucleon?

A

It is the binding energy of a nucleus divided by the number of nucleons in the nucleus.

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13
Q

How can you tell whether an element undergoes fission or fusion?

A

On the graph of Binding energy/nucleon over no of nucleons,
- the elements that undergo fusion have less nucleons than iron
- the elements that undergo fission have more nucleons than iron

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14
Q

What are the 2 conditions of nuclear fusion?

A

High Temperature
- Needed to overcome electrostatic repulsion between positively charged nuclei
High Density/Pressure
- Ensure nuclei are close together so increased rate of collision to maintain fusion reaction.

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15
Q

What is background radiation?

A

Background radiation is the level of ionising radiation present in the environment.

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16
Q

What is count rate?

A

No of decays recorded each second by GM tube

17
Q

How to calculate corrected count rate?

A
  • Calculate background radiation count
  • Calculate total count
  • Take away background count from total count
18
Q

What is radiation?

A

Radiation is when an unstable nucleus emits energy in the form of EM waves or subatomic particles in order to become more stable.

19
Q

What can cause a nucleus to become unstable?

A

Unstable nuclei can be caused by
- too many neutrons
- too few neutrons
- too many nucleons (heavy)
- too much energy in the nucleus

20
Q

How does a nucleus decay?

A

By radioactive decay.
This is when a nucleus decays by releasing energy/particles until it is in a stable form.

21
Q

What are the 4 types of radiation?

A

Alpha - α - helium nucleus - 2 protons, 2 neutrons, +2 charge
Beta-minus - β, β- - electron
Beta-plus - β+ - positron
Gamma- Γ - short wavelength, high frequency EM wave

22
Q

What are the properties of alpha radiation?

A

Alpha has a:
- strong ionising ability
- slow speed
- Absorbed by paper or few cm of air

23
Q

What are the properties of a beta-minus?

A

Beta minus has a:
- Weak ionising ability
- Fast speed
- Absorbed by thin sheet of aluminium

24
Q

What are the properties of a gamma?

A

Gamma particles are:
- EM wave
- Infinte range; follows inverse square law
- Weak ionising ability
- Absorbed by metrrs of concrete or inches of lead

25
Q

List types of radiation from most ionising to least

A

Alpha
Beta
Gamma

26
Q

List types of radiation from most penetrative to least

A

Gamm
Beta
Alpha

27
Q

What is the nature of radioactive decay?

A

Random
-
Spontaneous
- Cannot influence when a nucleus will decay

28
Q

What is the decay constant?

A

Probability of a nucleus decaying per unit time
ΔN/Δt = -λN

29
Q

What is the half-life?

A

Time taken for the number of nuclei to halve

30
Q

How can you determine half-life from graph?

A
  • Measure t for sample size to half.
  • Complete multiple times
  • Work out average half life

Plot lnN₀ against time; straight line
Gradient is decay constant λ
Use λ to calculate half life

31
Q

What is activity?

A

Activity is the number of nuclei that decay per second
A =λN

32
Q

What is ionising radiation?

A

Ionising radiation removes electrons from atoms/molecules

33
Q

What is not directly ionising but may still cause ionisation?

A

Presence of neutrons
Uncharged particles may not be directly ionising

34
Q

Why is radioactive count repeated?

A

Radioactive is random process so count for fixed time will vary
Repeated measurements allow for mean to be calculated

35
Q

What is the process of nuclear fusion? (2)

A
  • Smaller mass nuclei come very close together
  • So nuclei join and form a larger nucleus
36
Q

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

A

Very high temperature
- as nuclei have positive charge leading to electrostatic force of repulsion
- High temp increases KE to help overcome electrostatic force of repulsion
Very high density
- So nuclei are close enough to fuse
- So collision rate is high to maintain fusion