Fission and Fusion Flashcards

1
Q

what is the mass of a proton and neutron

A

1.67x10-27 kg

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2
Q

what is the mass of an electron

A

9.11x10-31 kg

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3
Q

what did we discover about the masses of a nucleus compared to the sum of masses of the nucleons that formed it

A

the measured mass of the nucleus is always less than the total mass of the nucleons that form it

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4
Q

what is this difference called

A

mass deficit / defect

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5
Q

how would you calculate the mass deficit of a carbon-12 atom with a mass of 12u

A
  • subtract the mass of all its electrons from 12u
  • giving you the mass of the nucleus
  • work out the total mass of protons and neutrons
  • add them together to the the theoretical mass of the nucleus
  • subtract the theoretical mass from the real nucleus mass
  • multiply it by the mass value of 1u (given you were going the calculations in terms of u)
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6
Q

where does this loss of mass go

A

its converted into the binding energy of the nucleus

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7
Q

what is binding energy

A
  • the energy used to hold a nucleus together

- converted from the mass deficit

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8
Q

what is the equation that shows this relationship between mass deficit and energy

A

E = mc^2

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9
Q

if you have calculated the mass deficit in terms of kg, you would simply multiple it by c^2 to get E. however,if you have mass deficit in terms of u, how would you work out E

A
  • 1u = 931.5 MeV

- so you multiply what you have in terms of u by 931/5 MeV

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10
Q

how do you calculate binding energy per nucleon

A
  • work out the binding energy of the nucleus in MeV
  • and the number of nucleons within it
  • divide one by the other
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11
Q

in the graph for binding energy per nucleon against mass number, what does the graph look like

A
  • very steep line the beginning, almost vertical
  • then it becomes jagged as it reaches a peak
  • then the line slowly tapers off with a vert shallow gradient
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12
Q

what element is at the very peak of the line

A

iron

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13
Q

how can you relate this to the life cycle of a star

A
  • this is why the core of a star can only fuse up to iron
  • it has the largest binding energy
  • so fusion cannot happen anymore when its reached
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14
Q

what do elements to the left side of iron tend to do

A

fuse (nuclear fusion)

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15
Q

what do elements to the right side of iron tend to do

A

split up (nuclear fission)

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16
Q

when you fuse two light nuclei together, why is energy released

A
  • the heavier nucleus will have less mass than the sum of the daughter nuclei
  • as some of the mass has been converted into energy
  • however not all of it converted into binding energy
  • so the remaining energy will be released from the nucleus
17
Q

what is the first stage of proton-proton fusion

A

two protons fuse

18
Q

what is the second stage

A
  • one proton changes into a neutron
  • by emitting a b+ particle and a neutrino
  • leaving a deuterium nucleus
19
Q

what is the third stage

A
  • another proton fuses with the nucleus

- making a helium-3 nucleus

20
Q

what is the fourth stage

A

two helium-3 nuclei fuse

21
Q

what is the last stage

A
  • two protons break off

- leaving a helium-4 nucleus

22
Q

why have we not been able to use nuclear fusion as a source of energy on earth

A
  • because it is extremely difficult
  • and the amount of energy required to do it is extremely high
  • in most cases youd lose more energy than you gained
23
Q

what is the main problem that makes nuclear fusion so hard

A
  • forcing the oppositely charged protons to fuse

- the kinetic energy they need to overcome their electrostatic repulsion requires temps in the millions of degrees

24
Q

what is the other problem you run into

A
  • you need enough collisions to be happening in order to a good amount of energy to be produced
  • but youd require very high densities of protons
  • which is also very hard to do and maintain
25
Q

what is nuclear fission

A
  • the splitting up a larger nuclei into smaller nuclides

- releasing energy in the process

26
Q

how are man-made fission reactions triggered

A
  • when a nucleus absorbs a slow moving neutron

- making it unstable and causing it to break down