Chapter 13: Nuclei

Energy released in nuclear reactions is due to:

Nuclear reactions obey:

Binding energy per nucleon is maximum for:

Most stable nucleus is around:

Nuclear force range is about:

Nuclear forces are independent of:

Fission increases stability because:

Fusion increases stability because:

Heavier nuclei are less stable because:

Nuclear density is constant because:

Fusion is more energy efficient because:

Fusion releases energy because:

Fission produces:

Q-value formula:

Q-value represents:

Fusion occurs at:

Example of fission fuel:

Energy in stars is due to:

Nuclear fusion is:

Nuclear fission is:

Higher mass defect implies:

Unit of binding energy:

Energy equivalent of mass defect is:

Stable nuclei have:

For light nuclei, BE/A:

For heavy nuclei, BE/A:

Binding energy per nucleon curve peaks at:

Most stable nuclei have mass number near:

Binding energy per nucleon indicates:

1 amu =

Binding energy depends on:

Binding energy formula:

Binding energy is:

Mass defect formula is:

Mass defect is:

Value of R₀ ≈

Unit of nuclear radius constant R₀ is:

Nuclear force shows:

Nuclear force is:

Nuclear force is strongest among:

Nuclear forces are:

Nuclear density is:

Nuclear radius formula is:

Nuclear radius depends on:

Isotones have:

Isobars have:

Isotopes have:

Mass number is:

Atomic number represents:

The nucleus consists of: