Nuclear Binding Energy and Nuclear Radiation

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Flashcards for reviewing key concepts from the lecture on Nuclear Binding Energy and Nuclear Radiation.

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10 Terms

1
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What is the mass defect in nuclear physics?

The difference between the measured mass of a nucleus and the sum total of the masses of its constituents.

2
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How is binding energy defined in nuclear physics?

The energy required to break a nucleus into its constituent protons and neutrons.

3
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What does mass-energy equivalence imply about the relationship between mass and energy?

Mass can be converted into energy and energy can be converted into mass.

4
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What is the unified atomic mass unit (u)?

Roughly equal to the mass of one proton or neutron, defined as the mass of exactly one-twelfth of an atom of carbon-12.

5
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How is the binding energy per nucleon related to the stability of a nucleus?

A higher binding energy per nucleon indicates higher stability since it requires more energy to pull the nucleus apart.

6
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What type of reaction is the formation of a nucleus from isolated protons and neutrons considered?

An exothermic reaction, since it releases energy.

7
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What are the conditions necessary for nuclear fusion to occur?

Both nuclei must have high kinetic energy and be in a very high-density environment, such as the core of a star.

8
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Which element has the highest binding energy per nucleon?

Iron (A = 56) is the most stable element with the highest binding energy per nucleon.

9
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What occurs when deuterium and tritium nuclei fuse?

They combine to form a helium nucleus and release energy.

10
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How is the mass-energy equivalence equation represented?

E = mc², where E is energy, m is mass, and c is the speed of light.