Sublevo
ISC 2027
All chaptersPhysics · Unit 8

Atoms and Nuclei

6 articles25 formulas32 ways the board asks it
PHYExam Practice

Multiple Choice & Assertion-Reason

This is a whole-chapter revision set: the one-mark MCQs and Assertion-Reason items sweep across both halves of the chapter — Bohr's atom (orbit radius rn∝n2/Zr_n \propto n^2/Z, energy En∝−Z2/n2E_n \propto -Z^2/n^2, spectral series) and the nucleus (size R∝A1/3R \propto A^{1/3}, binding-energy-per-nucleon curve, the mass-energy unit 1 u=931.5 MeV1\,\text{u} = 931.5\,\text{MeV}, and the decay law N=N0e−λtN = N_0 e^{-\lambda t}).

They reward knowing the structure of each relation — what is proportional to what — far more than heavy arithmetic. Examiners favour these because a single line such as 'nuclear density is independent of AA' or 'mean life τ=T1/2/0.693\tau = T_{1/2}/0.693' lets them test cause-and-effect reasoning, which is exactly what Assertion-Reason questions probe.

Bohr orbit radius and energy (hydrogen-like)
rn=n2Z a0,En=−13.6 Z2n2 eVr_n = \dfrac{n^2}{Z}\,a_0, \qquad E_n = -13.6\,\dfrac{Z^2}{n^2}\ \text{eV}
nn is the principal quantum number, ZZ the atomic number, a0=0.53 A˚a_0 = 0.53\,\text{Å} the Bohr radius. Radius grows as n2n^2 (so r∝n2r \propto n^2 for hydrogen, Z=1Z=1); energy is negative (bound), rising toward 00 as n→∞n \to \infty. For n=2n=2 in hydrogen, E2=−13.6/4=−3.4 eVE_2 = -13.6/4 = -3.4\,\text{eV}.
Number of spectral lines on de-excitation
lines=n(n−1)2\text{lines} = \dfrac{n(n-1)}{2}
nn is the highest level the atoms are excited to (de-exciting to the ground state). For n=4n=4 this gives 4×32=6\dfrac{4\times 3}{2} = 6 distinct lines. The total counts every allowed downward transition, spread across the Lyman, Balmer and Paschen series.
Nuclear radius and density
R=R0A1/3,ρ=3mN4πR03R = R_0 A^{1/3}, \qquad \rho = \dfrac{3 m_N}{4\pi R_0^{3}}
R0≈1.2 fmR_0 \approx 1.2\,\text{fm}, AA the mass number, mNm_N the mass of one nucleon. Since mass ∝A\propto A and volume ∝R3∝A\propto R^3 \propto A, the density ρ\rho is independent of AA — the same for all nuclei (∼2.3×1017 kg m−3\sim 2.3\times 10^{17}\,\text{kg m}^{-3}).
Mass-energy equivalence and the atomic mass unit
E=Δm c2,1 u=931.5 MeV/c2E = \Delta m\,c^2, \qquad 1\,\text{u} = 931.5\,\text{MeV}/c^2
Δm\Delta m is the mass defect. The conversion 1 u→931.5 MeV1\,\text{u} \to 931.5\,\text{MeV} (MeV, not eV or keV) is the single most-used number in the nuclear half of the chapter; binding-energy-per-nucleon peaks near 8.8 MeV8.8\,\text{MeV} for iron (A≈56A \approx 56).
Radioactive decay: remaining fraction, half-life and mean life
NN0=(12)t/T1/2,T1/2=ln⁡2λ=0.693 τ\dfrac{N}{N_0} = \left(\dfrac{1}{2}\right)^{t/T_{1/2}}, \qquad T_{1/2} = \dfrac{\ln 2}{\lambda} = 0.693\,\tau
T1/2T_{1/2} is the half-life, τ=1/λ\tau = 1/\lambda the mean (average) life, λ\lambda the decay constant. After nn half-lives the surviving fraction is (1/2)n(1/2)^n (so 1/81/8 after 33). Mean life is longer than half-life: τ=T1/2/0.693\tau = T_{1/2}/0.693.
  • Radius scales as n2n^2 and energy as −1/n2-1/n^2 for hydrogen; restore the ZZ-dependence for hydrogen-like ions as r∝n2/Zr \propto n^2/Z and E∝−Z2/n2E \propto -Z^2/n^2. Speed in an orbit goes as v∝Z/nv \propto Z/n, so it decreases for higher orbits.
  • Spectral series are fixed by the lower level: Lyman ends on n=1n=1 (UV), Balmer on n=2n=2 (the only series wholly in the visible), Paschen on n=3n=3 (IR), Brackett on n=4n=4 (IR). 'Visible' on an MCQ almost always means Balmer.
  • The line count n(n−1)/2n(n-1)/2 is the number of distinct wavelengths emitted when a gas of atoms (not a single atom) de-excites from level nn; a single atom makes only one downward jump at a time.
  • R∝A1/3R \propto A^{1/3} is the master nuclear-size relation: it makes nuclear volume proportional to AA, which is why nuclear density is constant and why packing nucleons does not dilute the nucleus.
  • On the binding-energy-per-nucleon curve, the peak near A≈56A \approx 56 (iron) marks the most stable nuclei; light nuclei release energy by fusion and heavy nuclei by fission, both moving toward the peak.
  • Always quote the unit conversion as 1 u=931.5 MeV1\,\text{u} = 931.5\,\text{MeV} — the trap options replace MeV with eV, keV or GeV, which are wrong by factors of 10610^6, 10310^3 and 10310^3 respectively.
  • Surviving fraction after nn half-lives is (1/2)n(1/2)^n: 1/2,1/4,1/8,…1/2, 1/4, 1/8, \dots — never 1/n1/n or 1/n21/n^2. Decay is exponential, not linear.
  • Assertion-Reason method: judge the Assertion and the Reason as independently true or false first, then ask whether the Reason actually explains the Assertion. For 'nuclear density is constant' the Reason 'R∝A1/3R \propto A^{1/3} so volume ∝A\propto A' is true and is the correct explanation, giving the 'both true, Reason explains Assertion' option.
Where the marks go
  • Confusing the nn-scalings: writing r∝nr \propto n or E∝−1/nE \propto -1/n instead of r∝n2r \propto n^2 and E∝−1/n2E \propto -1/n^2. Energy of the n=2n=2 state is −3.4 eV-3.4\,\text{eV} (=−13.6/4=-13.6/4), not −6.8 eV-6.8\,\text{eV}.
  • Using 1/n1/n for the surviving fraction after nn half-lives: after 33 half-lives the answer is 1/81/8, not 1/31/3.
  • Inverting the mean-life relation, writing τ=0.693 T1/2\tau = 0.693\,T_{1/2}. It is the other way round: τ=T1/2/0.693≈1.44 T1/2\tau = T_{1/2}/0.693 \approx 1.44\,T_{1/2}, so mean life exceeds half-life.
  • Picking 931.5 keV931.5\,\text{keV} or eV\text{eV} for 1 u1\,\text{u}, or thinking nuclear density depends on AA — both follow from forgetting R∝A1/3R \propto A^{1/3} and the MeV scale of nuclear energies.
How the board asks it
  • Assertion–ReasonR∝A1/3R \propto A^{1/3} and nuclear density
    Assertion: The density of a nucleus is independent of its mass number AA. Reason: The nuclear radius is given by R=R0A1/3R = R_0 A^{1/3}, so nuclear volume is proportional to AA. Choose: (a) both true and Reason explains Assertion; (b) both true but Reason does not explain Assertion; (c) Assertion true, Reason false; (d) Assertion false, Reason true.
  • Assertion–Reasonmean life vs half-life
    Assertion: The mean life of a radioactive sample is greater than its half-life. Reason: Mean life and half-life are related by τ=T1/2/0.693≈1.44 T1/2\tau = T_{1/2}/0.693 \approx 1.44\,T_{1/2}. Choose: (a) both true and Reason explains Assertion; (b) both true but Reason does not explain Assertion; (c) Assertion true, Reason false; (d) Assertion false, Reason true.
  • Assertion–ReasonBohr nn-scalings for orbital speed
    Assertion: The orbital speed of the electron in a hydrogen atom decreases as it moves to higher orbits. Reason: For a hydrogen-like atom v∝Z/nv \propto Z/n, so speed falls as nn rises. Choose: (a) both true and Reason explains Assertion; (b) both true but Reason does not explain Assertion; (c) Assertion true, Reason false; (d) Assertion false, Reason true.
  • Multiple choicesurviving fraction (1/2)n(1/2)^n
    The fraction of a radioactive sample that remains undecayed after 33 half-lives is: (a) 1/31/3 (b) 1/61/6 (c) 1/81/8 (d) 1/91/9. Choose the correct option.
  • Multiple choice1 u=931.5 MeV1\,\text{u} = 931.5\,\text{MeV} and spectral series
    Which one of the following statements is correct? (a) 1 u=931.5 keV1\,\text{u} = 931.5\,\text{keV} (b) the Balmer series lies in the visible region (c) the Lyman series ends on n=2n = 2 (d) nuclear density increases with AA. Choose the correct option.
  • Multiple choicebinding-energy-per-nucleon curve
    On the binding-energy-per-nucleon curve, the most stable nuclei lie near the peak at: (a) A≈4A \approx 4 (b) A≈56A \approx 56 (c) A≈120A \approx 120 (d) A≈238A \approx 238. Choose the correct option.

Written for Sublevo. Question text quoted anywhere in these notes is the Council’s and carries its year and paper; the board’s own diagrams are not reproduced.