List-I shows various functional dependencies of energy $ E $ on the atomic number $ Z $. Energies associated with certain phenomena are given in List-II. Choose the option that describes the correct match between the entries in List-I to those in List-II. 
P \( \rightarrow \) 3, Q \( \rightarrow \) 2, R \( \rightarrow \) 1, S \( \rightarrow \) 5
(P) \( E \propto Z^2 \)
This is the energy dependence for hydrogen-like atoms (Bohr model). The energy of electronic transitions in such atoms varies as: \[ E_n = - \frac{Z^2}{n^2} \cdot \text{constant} \] \[ \Rightarrow \text{P} \rightarrow 5 \quad \text{(Energy of electronic transitions in hydrogen-like atoms)} \] (Q) \( E \propto (Z - 1)^2 \)
This is the empirical formula for characteristic x-rays (Moseley’s law), accounting for screening by inner electrons: \[ E = a (Z - 1)^2 \Rightarrow \text{Q} \rightarrow 1 \] (R) \( E \propto Z(Z - 1) \)
This is the electrostatic (Coulomb) part of nuclear binding energy between protons, modeled as: \[ E_{\text{Coulomb}} \propto \frac{Z(Z - 1)}{A^{1/3}} \Rightarrow \text{R} \rightarrow 2 \] (S) \( E \) practically independent of \( Z \)
The average nuclear binding energy per nucleon for stable nuclei (mass number 30 to 170) is nearly constant, i.e., independent of \( Z \): \[ \Rightarrow \text{S} \rightarrow 4 \]