The binding energy per nucleon is proportional to the number of neighbours \( p \), and the constant \( k \). Since the binding energy is related to the range of nuclear force, which affects how the force is distributed among nucleons, the energy is directly proportional to the number of neighbouring nucleons. Therefore, the binding energy per nucleon is given by:
\[ \text{Binding energy per nucleon} \propto p k \]
Thus, the binding energy per nucleon is \( p k \).
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of