Level 4 — ApplicationModern Physics

Modern Physics

60 minutes60 marksprintable — key stays hidden on paper

Level 4 — Application (novel/unseen problems, no hints) Time limit: 60 minutes Total marks: 60

Constants (use as needed): h=6.626×1034J⋅sh = 6.626\times10^{-34}\,\text{J·s}, =1.055×1034J⋅s\hbar = 1.055\times10^{-34}\,\text{J·s}, c=3.00×108m/sc = 3.00\times10^{8}\,\text{m/s}, me=9.11×1031kgm_e = 9.11\times10^{-31}\,\text{kg}, e=1.602×1019Ce = 1.602\times10^{-19}\,\text{C}, 1u=931.5MeV/c21\,\text{u} = 931.5\,\text{MeV}/c^2.


Question 1 — Photoelectrics meets Compton (12 marks)

A clean sodium surface (work function ϕ=2.28eV\phi = 2.28\,\text{eV}) is illuminated by ultraviolet light of wavelength 180nm180\,\text{nm}.

(a) Compute the maximum kinetic energy (in eV) of the emitted photoelectrons. (3)

(b) These same 180nm180\,\text{nm} photons are instead Compton-scattered off free electrons through an angle of 9090^\circ. Find the wavelength of the scattered photon and comment on whether the fractional wavelength shift is larger or smaller than it would be for X-rays. (5)

(c) A photon and an electron each have the same de Broglie / actual wavelength of 180nm180\,\text{nm}. Which carries more momentum? Justify with a calculation. (4)


Question 2 — Particle in a box, redesigned (12 marks)

An electron is confined to a one-dimensional infinite square well of width LL.

(a) The energy gap between the ground state and the first excited state is measured to be 3.0eV3.0\,\text{eV}. Determine the well width LL (in nm). (5)

(b) For this width, find the probability of locating the electron in the region 0xL/40 \le x \le L/4 when it is in the first excited state (n=2n=2). (5)

(c) State qualitatively how the answer to (b) changes if the electron is instead in the ground state, and give one physical reason. (2)


Question 3 — Nuclear energetics and decay (14 marks)

Consider the alpha decay 92238U 90234Th+α^{238}_{92}\text{U} \rightarrow\ ^{234}_{90}\text{Th} + \alpha.

Atomic masses: m(238U)=238.05079um(^{238}\text{U}) = 238.05079\,\text{u}, m(234Th)=234.04360um(^{234}\text{Th}) = 234.04360\,\text{u}, m(4He)=4.00260um(^{4}\text{He}) = 4.00260\,\text{u}.

(a) Calculate the Q-value of the decay in MeV. (4)

(b) Assuming the parent nucleus is initially at rest, use conservation of momentum and energy to find the kinetic energy carried by the alpha particle (non-relativistic). (5)

(c) 238U^{238}\text{U} has a half-life of 4.5×1094.5\times10^{9} years. A rock contains 2.0×10222.0\times10^{22} uranium-238 atoms. Compute its activity in becquerels. (5)


Question 4 — Relativistic collision (12 marks)

An electron is accelerated until its total energy equals 3.0MeV3.0\,\text{MeV}. (Rest energy of electron =0.511MeV= 0.511\,\text{MeV}.)

(a) Find the electron's speed as a fraction of cc. (4)

(b) Find its relativistic momentum in MeV/cc using E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2. (3)

(c) This electron travels a 10m10\,\text{m} tube in the lab frame. How long is the tube in the electron's own rest frame? (5)


Question 5 — Uncertainty & spectra short applications (10 marks)

(a) An electron is confined to a region of size 0.10nm0.10\,\text{nm} (atomic scale). Estimate the minimum uncertainty in its momentum, and hence a minimum kinetic energy (in eV). Comment on the order of magnitude relative to atomic binding energies. (5)

(b) A hydrogen atom emits a photon in the Balmer series corresponding to the transition n=4n=2n=4 \to n=2. Calculate the wavelength of the emitted photon and state which colour region it falls in. (5)


Answer keyMark scheme & solutions

Question 1

(a) Photon energy E=hc/λ=1240eV⋅nm180nm=6.89eVE = hc/\lambda = \dfrac{1240\,\text{eV·nm}}{180\,\text{nm}} = 6.89\,\text{eV}. (1) Kmax=Eϕ=6.892.28=4.61eVK_{max} = E - \phi = 6.89 - 2.28 = 4.61\,\text{eV}. (2) Why: Einstein's photoelectric equation — each photon gives all its energy to one electron; the work function is the minimum escape energy.

(b) Compton shift: Δλ=hmec(1cosθ)\Delta\lambda = \dfrac{h}{m_e c}(1-\cos\theta). At 9090^\circ, Δλ=λC=2.43×103nm\Delta\lambda = \lambda_C = 2.43\times10^{-3}\,\text{nm}. (2) Scattered wavelength =180+0.00243=180.00243nm= 180 + 0.00243 = 180.00243\,\text{nm}. (1) Fractional shift Δλ/λ1.35×105\Delta\lambda/\lambda \approx 1.35\times10^{-5} — negligibly small. For X-rays (λ0.01\lambda\sim0.010.1nm0.1\,\text{nm}) the same absolute shift is a much larger fraction, which is why Compton scattering is observable with X-rays, not visible/UV light. (2) Why: Δλ\Delta\lambda is independent of incident wavelength; only the fraction depends on λ\lambda.

(c) Photon: p=h/λp = h/\lambda. Electron with de Broglie wavelength λ\lambda: p=h/λp = h/\lambdaidentical. (2) Numerically p=6.626×1034180×109=3.68×1027kg⋅m/sp = \dfrac{6.626\times10^{-34}}{180\times10^{-9}} = 3.68\times10^{-27}\,\text{kg·m/s} for both. Neither carries more; de Broglie relation makes momenta equal for equal wavelength. (2) Why: Both obey p=h/λp=h/\lambda; the trick is recognising the "same wavelength" removes any difference.


Question 2

(a) En=n2h28meL2E_n = \dfrac{n^2 h^2}{8m_e L^2}. Gap: E2E1=(41)h28meL2=3h28meL2=3.0eVE_2 - E_1 = \dfrac{(4-1)h^2}{8m_e L^2} = \dfrac{3h^2}{8m_e L^2} = 3.0\,\text{eV}. (2) L2=3h28me(3.0e)=h28meeL^2 = \dfrac{3h^2}{8m_e (3.0\,e)} = \dfrac{h^2}{8m_e\,e}. (1) =(6.626×1034)28(9.11×1031)(1.602×1019)=3.76×1019m2= \dfrac{(6.626\times10^{-34})^2}{8(9.11\times10^{-31})(1.602\times10^{-19})} = 3.76\times10^{-19}\,\text{m}^2. (1) L=6.13×1010m0.61nmL = 6.13\times10^{-10}\,\text{m} \approx 0.61\,\text{nm}. (1)

(b) ψ2=2/Lsin(2πx/L)\psi_2 = \sqrt{2/L}\sin(2\pi x/L); P=0L/42Lsin2 ⁣2πxLdxP = \int_0^{L/4}\frac{2}{L}\sin^2\!\frac{2\pi x}{L}\,dx. (2) =2L[x2L8πsin4πxL]0L/4= \frac{2}{L}\left[\frac{x}{2} - \frac{L}{8\pi}\sin\frac{4\pi x}{L}\right]_0^{L/4}. (1) At x=L/4x=L/4: sin(π)=0\sin(\pi)=0, so P=2LL8=14=0.25P = \frac{2}{L}\cdot\frac{L}{8} = \frac14 = 0.25. (2)

(c) For the ground state (n=1n=1) the probability in [0,L/4][0,L/4] is less than 0.25 (about 0.0910.091), because the ground-state ψ2|\psi|^2 peaks at the centre L/2L/2 and is small near the walls, so less probability sits in the outer quarter. (2)


Question 3

(a) Δm=238.05079(234.04360+4.00260)=0.00459u\Delta m = 238.05079 - (234.04360 + 4.00260) = 0.00459\,\text{u}. (2) Q=0.00459×931.5=4.27MeVQ = 0.00459 \times 931.5 = 4.27\,\text{MeV}. (2) Why: Q is the mass defect converted to energy; positive Q ⇒ spontaneous decay.

(b) Momentum conservation: pα=pThp_\alpha = p_{Th}. Energy: Q=Kα+KThQ = K_\alpha + K_{Th}, with K=p2/2mK = p^2/2m. KαKTh=mThmα\dfrac{K_\alpha}{K_{Th}} = \dfrac{m_{Th}}{m_\alpha}, so Kα=QmThmTh+mαK_\alpha = Q\cdot\dfrac{m_{Th}}{m_{Th}+m_\alpha}. (3) Kα=4.27×234238=4.20MeVK_\alpha = 4.27\times\dfrac{234}{238} = 4.20\,\text{MeV}. (2) Why: The lighter alpha takes most of the kinetic energy since KE splits inversely to mass at equal momentum.

(c) λ=ln2T1/2\lambda = \dfrac{\ln 2}{T_{1/2}}. T1/2=4.5×109×3.156×107s=1.42×1017sT_{1/2} = 4.5\times10^9\times3.156\times10^7\,\text{s} = 1.42\times10^{17}\,\text{s}. (1) λ=0.693/1.42×1017=4.88×1018s1\lambda = 0.693/1.42\times10^{17} = 4.88\times10^{-18}\,\text{s}^{-1}. (2) Activity A=λN=4.88×1018×2.0×1022=9.76×104BqA = \lambda N = 4.88\times10^{-18}\times2.0\times10^{22} = 9.76\times10^{4}\,\text{Bq}. (2)


Question 4

(a) γ=E/mc2=3.0/0.511=5.87\gamma = E/mc^2 = 3.0/0.511 = 5.87. (1) v/c=11/γ2=11/34.5=0.971=0.985v/c = \sqrt{1 - 1/\gamma^2} = \sqrt{1 - 1/34.5} = \sqrt{0.971} = 0.985. (3)

(b) (pc)2=E2(mc2)2=3.020.5112=9.00.261=8.739(pc)^2 = E^2 - (mc^2)^2 = 3.0^2 - 0.511^2 = 9.0 - 0.261 = 8.739. (2) pc=2.956MeVp=2.96MeV/cpc = 2.956\,\text{MeV} \Rightarrow p = 2.96\,\text{MeV}/c. (1)

(c) Tube length in lab L0=10mL_0 = 10\,\text{m} (proper length of tube — tube is at rest in lab). In electron frame it is contracted: L=L0/γ=10/5.87=1.70mL = L_0/\gamma = 10/5.87 = 1.70\,\text{m}. (4) Why: The tube is at rest in the lab, so 1010 m is its proper length; the moving electron sees it Lorentz-contracted. (1)


Question 5

(a) Δp2Δx=1.055×10342×1010=5.27×1025kg⋅m/s\Delta p \ge \dfrac{\hbar}{2\Delta x} = \dfrac{1.055\times10^{-34}}{2\times10^{-10}} = 5.27\times10^{-25}\,\text{kg·m/s}. (2) K(Δp)22me=(5.27×1025)22×9.11×1031=1.53×1019J=0.95eVK \approx \dfrac{(\Delta p)^2}{2m_e} = \dfrac{(5.27\times10^{-25})^2}{2\times9.11\times10^{-31}} = 1.53\times10^{-19}\,\text{J} = 0.95\,\text{eV}. (2) This is of order 1 eV — comparable to atomic binding/ionisation energies (a few eV), confirming the uncertainty principle sets the quantum energy scale of atoms. (1)

(b) 1λ=R(122142)\dfrac{1}{\lambda} = R\left(\dfrac{1}{2^2} - \dfrac{1}{4^2}\right), R=1.097×107m1R = 1.097\times10^7\,\text{m}^{-1}. =1.097×107(0.250.0625)=1.097×107×0.1875=2.057×106m1= 1.097\times10^7(0.25 - 0.0625) = 1.097\times10^7\times0.1875 = 2.057\times10^6\,\text{m}^{-1}. (3) λ=4.86×107m=486nm\lambda = 4.86\times10^{-7}\,\text{m} = 486\,\text{nm}blue-green (Hβ_\beta) line. (2)


[
  {"claim":"Q1a photoelectron KE = 4.61 eV","code":"E=1240/180; K=E-2.28; result=abs(K-4.61)<0.05"},
  {"claim":"Q2b probability in [0,L/4] for n=2 equals 1/4","code":"from sympy import symbols,sin,pi,integrate,Rational; x,L=symbols('x L',positive=True); P=integrate(2/L*sin(2*pi*x/L)**2,(x,0,L/4)); result=simplify(P-Rational(1,4))==0"},
  {"claim":"Q3a Q-value = 4.27 MeV","code":"dm=238.05079-(234.04360+4.00260); Q=dm*931.5; result=abs(Q-4.27)<0.05"},
  {"claim":"Q3b alpha KE = 4.20 MeV","code":"Q=4.27; Ka=Q*234/238; result=abs(Ka-4.20)<0.05"},
  {"claim":"Q4a v/c = 0.985","code":"g=3.0/0.511; v=(1-1/g**2)**0.5; result=abs(v-0.985)<0.005"},
  {"claim":"Q5b Balmer 4->2 wavelength = 486 nm","code":"R=1.097e7; inv=R*(1/4-1/16); lam=1/inv*1e9; result=abs(lam-486)<3"}
]