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Class XII · Chapter 13

Nuclei — Exam Practice

Practice questions in CBSE, NEET, and JEE Main style covering binding energy, radioactive decay, and nuclear fission/fusion.

📝 10 questions 🎯 CBSE · NEET · JEE Main
A note on these questions: these are original practice questions, written to match the exact style, format, and difficulty of CBSE Board, NEET, and JEE Main papers — not verbatim reproductions of specific past papers.

1CBSE Board Exam Style

CBSE · 1 Mark
Q1. Why is nuclear density approximately the same for all nuclei, regardless of mass number?
Answer Nuclear radius follows R = R₀A1/3, so volume ∝ A. Since mass also scales with A (each nucleon contributes roughly the same mass), density = mass/volume stays roughly constant across every nucleus, light or heavy.
CBSE · 3 Marks
Q2. Describe the variation of binding energy per nucleon with mass number, and explain how this curve accounts for the release of energy in both nuclear fission and fusion.
Answer Binding energy per nucleon rises sharply for light nuclei, peaks around A ≈ 56 (iron/nickel), then declines slowly for heavier nuclei.

Fission splits a heavy nucleus (on the declining side) into two lighter nuclei closer to the peak — each fragment is more tightly bound per nucleon than the original, releasing the difference as energy.

Fusion combines light nuclei (on the rising side) into a heavier one, also moving toward the peak and releasing energy for the same underlying reason — either direction of movement toward the peak releases energy.
CBSE · 5 Marks
Q3. (a) State the law of radioactive decay, and derive the relation between half-life and the decay constant. (b) A radioactive sample has a half-life of 20 days. Find the time taken for its activity to fall to 1/8 of its initial value.
Answer (a) N = N₀e−λt. At t = T½, N = N₀/2:
N₀/2 = N₀e−λT½ → ln(2) = λT½T½ = 0.693/λ.

(b) 1/8 = (1/2)ⁿ → n = 3 half-lives.
Time = 3 × 20 = 60 days.

2NEET Style (Single-Correct MCQ)

NEET Style
Q4. Mass defect of a nucleus represents:
The nucleus's total mass
✓ The difference between the sum of individual nucleon masses and the actual nucleus mass
The mass of emitted radiation
The atomic mass unit itself
Solution Δm = [Zmp + (A−Z)mn] − Mnucleus — this "missing" mass has been converted to binding energy holding the nucleus together.
NEET Style
Q5. In beta-minus (β⁻) decay, the mass number A of the nucleus:
Increases by 1
✓ Remains unchanged
Decreases by 1
Decreases by 4
Solution β⁻ decay converts a neutron to a proton within the nucleus — total nucleon count (A) stays the same, while atomic number Z increases by 1.
NEET Style
Q6. The nuclear force between nucleons is best described as:
Long-range and charge-dependent
✓ Short-range and charge-independent
Identical in strength to gravity
Repulsive at all distances
Solution Effective only over a few femtometres, and acts the same way between proton-proton, proton-neutron, and neutron-neutron pairs alike.
NEET Style
Q7. In nuclear fission, most of the released energy appears as:
Gamma radiation only
✓ Kinetic energy of the fission fragments
Neutrino energy
Sound energy
Solution The two (or more) fragments fly apart carrying the bulk of the ~200 MeV released per fission event as kinetic energy, with smaller contributions from gamma rays and neutrons.

3JEE Main Style

JEE Main Style · Numerical
Q8. A nucleus has a mass defect of 0.025 u. Find its binding energy.
Solution Eb = Δm × 931.5 MeV = 0.025 × 931.5 ≈ 23.3 MeV.
JEE Main Style · MCQ
Q9. Alpha decay changes the mass number A of the parent nucleus by:
No change
✓ Decreases by 4
Increases by 4
Decreases by 2
Solution An emitted alpha particle is a helium nucleus (2 protons + 2 neutrons), so A decreases by exactly 4, and Z decreases by 2.
JEE Main Style · Numerical
Q10. A radioactive sample has a decay constant of 0.0231 per day. Find its half-life.
Solution T½ = 0.693/λ = 0.693/0.0231 ≈ 30 days.
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