Nuclear Flashcards

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1
Q

What is the binding energy of free neutrons?

A

No binding energy for free neutrons or protons

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2
Q

Binding energy increases

A

During fission and fusion reactions

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3
Q

Explain the correletation between collisions of neutrons on a moderator and the nucleon number of the moderator atoms

A

During a collision between a neutron and a moderator atom, kinetic energy is lost.

If the nucleon number of the moderator atoms is high then not much Kinetic energy is lost, this means more collisions are needed.

More kinetic energy is lost when the nucleon number of the moderator atoms are close to that of the neutron.

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4
Q

Three benefits of using nuclear power

A

Some nuclear power stations can adjust their output quickly (boron control rods)

Nuclear power can be produces continuosly without the dependence of weather conditions

Little greenhouse gas emissions

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5
Q

State what happens to a neutron incident on the moderator

A

A neutron collides elastically with the moderator and loses some of its kinetic energy

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6
Q

Sources of Nuclear Waste

A

The most dangerous nuclear waste are the fission fragments

Spent fuel rods left over with radioactive isotopes

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7
Q

How the nuclear waste is treated?

A

The nuclear waste is intially placed in cooling ponds underwater.

The plutonium and uranium is separated to be recycled

High level waste is vitrified into pyrex glass and then places in concrete bunkers to be stored deep underground.

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8
Q

Problems and solutions with nuclear waste

A

The waste is intially very hot so it has to be cooled by being placed in water pools

In liquid form the high level of waste may leak hency the need to vitrify the nuclear waste

The waste will be radioactive for thousands of years due to a large half life, therefore it needs to be stored in geologically stable areas

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9
Q

Why are low nucleon atoms stable?

A

The strong nuclear force acts between all nucleons. This force is stronger than electrostatic repulsion

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10
Q

Why do bigger nuclei have more neutrons?

A

The neutrons help to spread the protons away from each other to reduce electromagnetic repulsion. When there are more protons, electromagnetic repulsion increases, therefore more neutrons are needed to reduce the repulsion.

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11
Q

Cloud chamber observations

A

Alpha particles produce straight lines and they are all the same length

Beta particles produce wispy tracks that are easily deflected as a result of collisions with air molecules. These tracks are less visible as they are less ionising

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12
Q

Activity Bq or s^-1

A

the number of nuclei of an isotope which disintegrate per second

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13
Q

Random nature of radioactive decay

A

Every nucleus of a radioactive isotope has an equal probability of undergoing radioactive decay

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14
Q

The decay constant

A

The decay constant is the probability of an individual nucleus decaying per second

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15
Q

Caron dating

A
  • carbon-14 isotope in living plants
  • it has a half life of 5500 years
  • this means there is negligible decay during a plants lifetime
  • when the plant dies it doesnt taken in any carbon-14
  • age can be calculated from activity
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16
Q

Radioactive tracers

A
  • need a half life which is long enough for an operation or scan but short enough to decay quickly after use
  • emit beta or gamma radiation so it can be detected outside the body without causing harm
17
Q

N-Z graph

A

N=Z is the line of stability

For light isotopes ( Z < 20 ) the stable nuclei follow the NZ line

As Z increases beyond 20 - stable nuclei have more neutrons than protons

18
Q

Alpha emitters

A

Are situated above the stable atoms and occur when Z > 60

the strong nuclear force is unable to overcome the electrostatic force of attraction between protons

19
Q

B- emitters

A

they are situated to the left of the stable nuclei where the isotopes are neutron rich

20
Q

B+ emitters

A

They occur to the right of the stability belt. This is where the isotopes are proton rich

21
Q

Metastable state

A

an excited state of the nuclei of an isotope that lasts long enough after alpha or beta emission for the isotope to be separated from the parent isotope

22
Q

Nuclear radius and debroglie wavelength of electron diffraction

A

Rsinθmin = 0.61λ

23
Q

R0

A

1.05 Fm

24
Q

Technetium-99 m

A

used to monitor blood flow

25
Q

Plotting R against A^1/3

A

Gradient is equal to r0 and it goes through the origin

26
Q

Plotting Ln R against LnA

A

Gives the gradient as 1/3 and the y intercept is Ln r0

27
Q

Nuclear density

A

Assuming the nucleus is spheical

Nuclear volume is proportional to the mass of the nucleus

Therefore nuclear density is constant

28
Q

Binding energy

A

The binding energy of the nucleus is the work that must be done to separate nucleus into its constituent neutrons and protons

29
Q

Binding energy explained

A

When a nucleus is formed, energy is released as the strong nuclear force does work pulling the nucleons together. This energy released is equal to the binding energy. This means the mass of the nucleus is less.

30
Q

Binding energy and mass defect

A

the binding energy is the same as the energy during mass defect calculation

31
Q

Nuclear Stability

A
  • The binding energy of each nuclide is different
32
Q

Binding energy per nucleon

A

A nuclide with a greater binding energy per nucleon is more stable

33
Q

Nuclear fusion

A

The product nucleus has more binding energy per nucleon