List-I shows various functional dependencies of energy () on the atomic number (). 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.
| List-I | List-II |
|---|---|
| (P) | (1) energy of characteristic x-rays |
| (Q) | (2) electrostatic part of the nuclear binding energy for stable nuclei with mass numbers in the range 30 to 170 |
| (R) | (3) energy of continuous x-rays |
| (S) is practically independent of | (4) average nuclear binding energy per nucleon for stable nuclei with mass number in the range 30 to 170 |
| (5) energy of radiation due to electronic transitions from hydrogen-like atoms |
- A
P 4; Q 3; R 1; S 2
- B
P 5; Q 2; R 1; S 4
- C
P 5; Q 1; R 2; S 4
- D
P 3; Q 2; R 1; S 5
(P) Energy of a hydrogen-like atom: eV, so . This is the energy of radiation from electronic transitions in hydrogen-like atoms. Matches (5).
(Q) Moseley's law for characteristic X-rays gives , so . Matches (1).
(R) The Coulomb (electrostatic) contribution to nuclear binding energy scales as , proportional to . Matches (2).
(S) In the mass-number range 30 to 170, the binding energy per nucleon is approximately constant (around 8.5 MeV), so it is practically independent of . Matches (4).
P5, Q1, R2, S4. Option (C).