Chapter 26 - Nuclear Physics Flashcards

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1
Q

what is Einstein’s mass-energy equation

A

E = mc^2

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2
Q

what are the main two ideas behind his mass-energy equation and give an example of each

A

1) Mass is a form of energy
- mass can be destroyed, releasing huge amounts of energy
- e.g. annihilation of an electron-positron pair into gamma photons

2) Energy has mass
- a change in energy of a system can lead to a change in mass of a system
- e.g. a tennis ball stationary weighs less than a moving one with K.E.

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3
Q

what can we say about the mass of the decay products of an alpha decay compared to the parent nuclei and what has happened to the lost mass

A

mass of the daughter nucleus and emitted particle < mass of the parent nucleus

  • this is because energy is released when the particle is emitted
  • this released energy has a mass equal to the difference in mass between the parent nucleus and the daughter nucleus/emitted particle
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4
Q

what occurs in annihilation

A
  • when a particle and an antiparticle meet they completely destroy each other and all of their mass is converted to energy
  • this energy is in the form of two very high energy photons
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5
Q

what are some minimum energies/energy changes for an electron-positron annihilation

A

change in mass = 2(Me)
change in energy = 2(Me)(c^2)
energy of a single photon = (Me)(c^2)

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6
Q

what occurs in pair production

A
  • a high energy photon can disappear and form a particle and its respective antiparticle
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7
Q

why does a full nucleus weigh a different amount to the same number of protons/neutrons but separated

A
  • when you separate nucleons, work must be done to overcome the strong nuclear force
  • therefore the individual nucleons have a greater energy than the nucleus as a whole
  • therefore they have a greater mass according to E = mc^2
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8
Q

define mass defect

A

“the mass defect of a nucleus is the difference in mass between the compete nucleus and the sum of the masses of the separate nucleons”

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9
Q

define binding energy

A

“the binding energy of a nucleus is defined as the MINIMUM energy required to completely separate a nucleus into its constituent nucleons”

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10
Q

how can we calculate binding energy from mass defect

A

binding energy = mass defect x c^2

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11
Q

is binding energy the same for all nuclei

A

no

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12
Q

how can we tell the stability of a nucleus

A
  • calculate its binding energy per nucleon
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13
Q

how to calculate binding energy per nucleon

A

binding energy per nucleon = total binding energy / number of nucleons

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14
Q

what are the 4 main points we should remember about binding energy per nucleon and nucleon number

A
  • for nuclei where A < 56, B.E. per nucleon increases with A
  • for nuclei where A > 56, B.E. per nucleon decreases with A
  • 56,26 Fe is the most stable nucleus
  • 4,2 He, 12,6 C, and 16,8 O are have abnormally high B.E. per nucleon
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15
Q

how can we explain energy changes of spontaneous radioactive decay (alpha) in terms of binding energy

A
  • binding energy of a parent nucleus < binding energy of daughter nucleus + alpha particle
  • therefore energy is released as the kinetic energy of the alpha particle
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16
Q

how can we explain energy release of nuclear fusion in terms of binding energy

A
  • two small (low mass/low A number) nuclei bond to form a bigger (higher mass/higher A number) nucleus
  • given B.E. per nucleon increases with A for small nuclei, the total binding energy of the resultant nucleus is greater than the total binding energy of the individual nuclei
  • therefore energy is released
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17
Q

how can we explain energy release of nuclear fission in terms of binding energy

A
  • a big (high mass/high A number) nucleus splits into 2 smaller (lower mass/lower A number) nuclei
  • given B.E. per nucleon increases when A decreases for a large nucleus, the total binding energy of the resultant nuclei is greater than the total binding energy of the parent nucleus
  • so energy is released
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18
Q

how do we know where fission will occur in terms of nucleon number

A
  • where A is large, fission will occur because binding energy per nucleon will increase when A decreases (nucleus splits)
  • this means the products will be more energetically stable
19
Q

how do we know where fusion will occur in terms of nucleon number

A
  • where A is small, fusion will occur because binding energy per nucleon will increase when A increases (nuclei fuse)
  • this means the product will be more energetically stable
20
Q

what does fission involve and what is induced fission

A
  • fission involves the splitting of a large nucleus into smaller daughter nuclei
  • some isotopes split by themselves but many are induced by absorbing a neutron
21
Q

what is the isotope generally used in fission reactors and what is used to induce its fission, which isotopes split spontaneously

A

Uranium - 235
U - 235

  • we use ‘slow’ or thermal neutrons to induce fission as they will be absorbed by the nucleus making it unstable and causing it to undergo spontaneous fission
    U-238 and U-235 rarely split spontaneously but U-236 does hence making U-235 absorb a neutron
22
Q

what is the equation for nuclear fission, briefly explain what happens and how we can check it is correct

A

1,0 n + 235,92 U —> 236,92 U
—> 141,56 Ba + 92,36 Kr + 3(1,0 n)

  • U-235 absorbs a slow neutron
  • this makes it U-236
  • this isotope is very unstable and breaks down into 3 fast neutrons and two daughter nuclei, Ba and Kr (or La and Br)
23
Q

why is energy released in nuclear fission and how can we calculate this

A
  • the mass of U-235 is higher than the mass of the daughter nuclei
  • because the total binding energy of the daughter nuclei is higher than the total binding energy in U-235
  • this missing mass/mass defect is released as energy in the form of kinetic energy
  • we can use E=mc^2 to calculate it
24
Q

what is the importance of chain reactions in nuclear fission and how can these be controlled

A
  • the fission of U-235 produces 3 fast moving neutrons
  • if these neutrons could be slowed then the reaction could be made into a chain reaction
  • but the number of neutrons and therefore rate of reaction would grow exponentially if not controlled
  • so control rods and moderators are used to help control this and prevent an uncontrolled reaction
  • it is made so that on average, 1 of the 3 fast moving neutrons survives as a slow neutron
25
Q

what are the same general components that all fission reactors have

A

all have:

  • fuel rods
  • control rods
  • coolant
  • moderator
26
Q

explain what fuel rods are

A

generally enriched uranium rods evenly spaced in the reactor core, contain mostly U-238 but about 2-3% U-235

27
Q

explain what the moderator is and what it does

A
  • the moderator must slow down fast moving electrons but NOT ABSORB them
  • fast neutrons are not slowed sufficiently by their collisions with Uranium because their collisions are generally elastic
  • they are slowed when they collide with water/heavy water or carbon because the collisions are inelastic
  • so these make good moderators
28
Q

explain what control rods are and how they can be used to control the reaction

A
  • they absorb excess neutrons, they are usually made of boron or cadmium
  • they can be lifted or dropped to control the rate of reaction
  • if lifted, the reaction rate increases as more neutrons are available
  • if dropped, the reaction rate decreases as fewer neutrons are available
29
Q

explain what the coolant is and what the two types are

A

primary coolant - carries heat from the reactor core, usually gas or liquid, becomes radioactive

secondary coolant - water, heated to produce steam to turn the turbines, does not become radioactive

30
Q

describe some advantages of nuclear power

A
  • Uranium is non-renewable but there is plenty of it so can almost be classed as such
  • no greenhouse gases are produced, only water vapour
  • millions of times more energy is released from nuclear power than an equal mass of fossil fuels would produce
31
Q

describe the issues associated with nuclear waste

A
  • U-238 can absorb medium energy neutrons to form Pu -239, this is highly toxic, radioactive and has a very long half life, it also forms radioactive daughter nuclei
  • spent fuel rods are high level waste, they are generally stored underground but there are limited facilities for this
  • low level waste is also produced but this is generally stored on site
32
Q

define what nuclear fusion is and give an example of where it occurs

A

“nuclear fusion is a process in which small nuclei bond together/fuse to form larger nuclei”

it occurs in the sun

33
Q

how does fusion occur/what conditions

A
  • for nuclei to fuse together they must get very close, about 10^-15m
  • at this distance the strong nuclear force acts and attracts them
  • high temperatures are required for fusion to occur, this is because the nuclei need a very high kinetic energy in order to do work against and overcome the strong electrostatic repulsion between them
  • high pressures/densities can also help
34
Q

what is the most basic example of nuclear fusion and what is a link we can draw to radiation

A

two protons fuse together to form deuterium
(1,1)p + (1,1)p —-> (2,1)H + (0,1)e + v

it effectively forms (2,2)He then decays via Beta +

35
Q

what fusion can occur to a deuterium nucleus and a proton

A

(2,1)H + (1,1)p —-> (3,2)He

a deuterium nucleus fuses with a proton to form a helium nucleus

36
Q

what fusion can occur between helium nuclei and how does this link to the most simple fusion reaction

A

(3,2)He + (3,2)He —-> (4,2)He + 2(1,1)p

these two protons formed can again fuse to form deuterium and keep a chain going

37
Q

why is energy released in nuclear fusion

A
  • when small nuclei fuse, the binding energy per nucleon increases, this causes the overall binding energy to increase so energy is released because the products have a greater binding energy than the reactants
38
Q

why can we not produce efficient fusion on earth yet

A
  • it requires very high temperatures and pressures for long durations
39
Q

what form is energy released in during nuclear fission or fusion

A

kinetic (and therefore thermal)

40
Q

what temperature does fusion (of hydrogen) generally occur at and why can fusion sometimes occur at lower temperatures

A

generally around 10^9K
sometimes occurs lower at 10^7K because MEAN Ek is directly prop to temperature but at a lower temp some molecules will still have a high enough Ek to fuse as they have higher than average Ek

41
Q

Describe the process of nuclear fission

A
  • a neutron is absorbed by a massive (uranium) nucleus

- the nucleus splits and undergoes fission to form two smaller daughter nuclei AND one or more neutrons

42
Q

Compare the energy release of nuclear fusion of hydrogen with alpha particle decay

A
  • energy is released in both
  • more energy is released in fusion of hydrogen because the mass defect is greater/ there is a greater difference in binding energy
43
Q

explain the importance of gravity in making fusion reactions possible inside the sun

A
  • gravity pulls together plasma/protons etc.
  • so increases density
  • so frequency of collisions between nuclei is greater
  • GPE to thermal transfer of energy gives the high temperatures required