Atomic Structure (Classical)
Level 5 — Mastery (Cross-domain: Physics + Mathematics + Computation) Time limit: 75 minutes Total marks: 60
Instructions: Show all derivations. Use , eV, Å, J·s, m/s, kg, C, F/m. J.
Question 1 — Derivation & Proof [20 marks]
(a) Starting from the balance of Coulomb attraction and centripetal force, together with Bohr's angular-momentum quantization , derive from first principles the expressions Show every algebraic step. [10]
(b) Using your derived , plug in constants for and show numerically that the ground-state energy of hydrogen equals eV (to 3 significant figures). [4]
(c) Prove that the ratio of the total energy to the kinetic energy of the electron in any Bohr orbit is , and that the ratio of total energy to potential energy is (i.e. verify the virial theorem for the Coulomb potential). [6]
Question 2 — Spectra & Cross-domain Computation [22 marks]
(a) Derive the Rydberg formula from the Bohr energy expression, and give the theoretical value of in terms of fundamental constants. [5]
(b) For the hydrogen atom, compute the wavelength (in nm) of the series limit () of the Balmer series, and the wavelength of the line (). State the region of the electromagnetic spectrum for each. [6]
(c) Write pseudocode (or Python) for a function line_wavelength(n1, n2, Z) that returns the emission wavelength in nm using the Rydberg formula, and a loop that prints the first 4 lines of the Lyman series. Then hand-compute the shortest-wavelength line of the Lyman series to confirm your code's output for that case. [6]
(d) A ion () emits a photon that is found to have exactly the same wavelength as the line of hydrogen. Identify a possible transition in that produces this, and justify with the scaling . [5]
Question 3 — Conceptual Synthesis & Data Analysis [18 marks]
(a) Chlorine occurs as two isotopes, (mass 34.969 u) and (mass 36.966 u), with average atomic mass 35.453 u. Calculate the percentage abundance of each isotope. [5]
(b) Define isotopes, isobars, and isotones and give one example pair for each from among: , , , , . [5]
(c) The Bohr model successfully explained the hydrogen spectrum but failed elsewhere. State three specific limitations of the Bohr model and, for each, name the experimental observation it could not account for. Briefly connect one of these failures to why Rutherford's classical nuclear model was itself unstable. [8]
Answer keyMark scheme & solutions
Question 1
(a) Derivation [10]
Force balance (Coulomb = centripetal):
Quantization:
Substitute (2) into (1):
Energy: . Using (1), , so Insert :
(b) Numerical check [4]
Numerator [1] Denominator [1] J [1] eV ✓ [1]
(c) Virial theorem [6]
(positive) [1] [2] Therefore ... let me state carefully: , so ; and means . The commonly-quoted ratio ; here we prove: (Accept the virial relations .) The requested is proven. [1] Note: full-mark answer states and , consistent with the virial theorem .
Question 2
(a) Rydberg derivation [5]
Photon energy for transition : [1]
(b) Balmer computations [6]
Series limit (): m nm — UV/near-UV edge [2]
(): m nm — visible (red) [3] (1 mark each: setup, value, region) [1]
(c) Code + hand check [6]
RH = 1.097e7 # m^-1
def line_wavelength(n1, n2, Z=1):
inv_lambda = RH * Z**2 * (1/n1**2 - 1/n2**2)
return 1e9 / inv_lambda # nm
for n2 in range(2, 6): # Lyman: n1 = 1
print(n2, round(line_wavelength(1, n2), 2))[4] (correct formula, nm conversion, loop over Lyman lines)
Hand check, shortest Lyman line = series limit : nm. [2] (For line the code gives nm; series limit 91.2 nm confirms shortest.)
(d) He⁺ transition [5]
For , , so . [1] : . Need He⁺ transition with , i.e. . [2] Try : ✓ [2] So the transition in gives the same wavelength as (indeed all He⁺ even-level transitions map onto H because scaling doubles the quantum numbers).
Question 3
(a) Abundance [5]
Let = fraction of Cl. [1] [2] [1] [1]
(b) Definitions + examples [5]
- Isotopes: same , different (different neutrons). Example: & (also & ). [1+1]
- Isobars: same , different . Example: & . [1]
- Isotones: same number of neutrons . Example: () & (); also () & (). [1+1]
(c) Limitations [8]
Three limitations (2 marks each, ½ concept + ½ observation, up to 6):
- Fails for multi-electron atoms — cannot predict spectra of He, Li, etc. (no electron–electron repulsion). [2]
- No fine structure / spectral line splitting — closely spaced lines seen under high resolution unexplained; also cannot explain Zeeman/Stark effects (splitting in magnetic/electric fields). [2]
- Violates Heisenberg's uncertainty principle — assumes definite orbit (fixed and simultaneously); also gives no intensity of spectral lines and treats angular momentum incorrectly ( vs ). [2]
Connection to Rutherford instability [2]: Rutherford's classical model has an accelerating (orbiting) electron which, by Maxwell's electrodynamics, must continuously radiate energy, spiral inward, and collapse into the nucleus in s — the atom would not be stable and would emit a continuous spectrum. Bohr's quantized stationary states were introduced precisely to forbid this radiation (postulate: no energy loss in allowed orbits), but this was an ad hoc fix without theoretical justification — itself a conceptual limitation resolved only by quantum mechanics.
[
{"claim":"Bohr ground-state energy of H equals -13.6 eV to 3 sig figs",
"code":"me=9.109e-31; e=1.602e-19; eps0=8.854e-12; h=6.626e-34; E=-me*e**4/(8*eps0**2*h**2)/e; result = round(E,1)==-13.6"},
{"claim":"Balmer series limit wavelength ~= 364.6 nm",
"code":"RH=1.097e7; lam=1/(RH*(1/2**2))*1e9; result = abs(lam-364.6)<0.5"},
{"claim":"H-alpha (3->2) wavelength ~= 656.3 nm",
"code":"RH=1.097e7; lam=1/(RH*(1/4-1/9))*1e9; result = abs(lam-656.3)<0.5"},
{"claim":"Chlorine 35-Cl abundance ~ 75.76 percent",
"code":"x=(36.966-35.453)/(36.966-34.969); result = abs(x*100-75.76)<0.1"},
{"claim":"He+ 6->4 transition matches H-alpha scaling: 4*(1/16-1/36)=5/36",
"code":"lhs=Rational(4)*(Rational(1,16)-Rational(1,36)); result = lhs==Rational(5,36)"}
]