Browse papers
A

Section A: Long Answer Questions

Attempt all / any as specified.

4 questions
1long14 marks

(a) Set up the differential equation of a damped harmonic oscillator and obtain its solution for the under-damped (weakly damped) case. Hence explain the terms under-damping, critical damping and over-damping with appropriate displacement–time sketches. (9)

(b) A body of mass 0.2 kg executes damped oscillations with a force constant of 80 N/m and a damping constant of 0.16 kg/s. Calculate the angular frequency of the damped oscillation and the time in which the amplitude falls to half of its initial value. (5)

(a) Damped harmonic oscillator (9 marks)

A particle of mass mm experiences a restoring force kx-kx and a velocity-dependent damping force bdxdt-b\dfrac{dx}{dt}. By Newton's second law:

md2xdt2=kxbdxdtm\frac{d^2x}{dt^2} = -kx - b\frac{dx}{dt} d2xdt2+2βdxdt+ω02x=0,2β=bm,    ω02=km\frac{d^2x}{dt^2} + 2\beta\frac{dx}{dt} + \omega_0^2 x = 0, \qquad 2\beta=\frac{b}{m},\;\; \omega_0^2=\frac{k}{m}

Trying x=eαtx = e^{\alpha t} gives the auxiliary equation α2+2βα+ω02=0\alpha^2 + 2\beta\alpha + \omega_0^2 = 0, so

α=β±β2ω02\alpha = -\beta \pm \sqrt{\beta^2 - \omega_0^2}

Under-damped case (β<ω0\beta < \omega_0): the root is complex, α=β±iωd\alpha=-\beta\pm i\omega_d with ωd=ω02β2\omega_d=\sqrt{\omega_0^2-\beta^2}. The solution is an exponentially decaying oscillation:

x(t)=A0eβtcos(ωdt+ϕ)\boxed{x(t) = A_0\,e^{-\beta t}\cos(\omega_d t + \phi)}

The amplitude A0eβtA_0 e^{-\beta t} decays slowly while the system oscillates at the reduced frequency ωd\omega_d.

Three cases

  • Under-damping (β<ω0\beta<\omega_0): oscillatory motion with amplitude falling exponentially; the displacement crosses zero many times. Sketch: a cosine curve bounded by a decaying ±A0eβt\pm A_0e^{-\beta t} envelope.
  • Critical damping (β=ω0\beta=\omega_0): equal roots; x=(A+Bt)eβtx=(A+Bt)e^{-\beta t}. The system returns to equilibrium in the shortest time without oscillating. Sketch: a single smooth curve rising/falling to zero with no overshoot.
  • Over-damping (β>ω0\beta>\omega_0): two real negative roots; motion is a slow non-oscillatory return to equilibrium, slower than critical. Sketch: a sluggish exponential decay to zero, lying above the critical curve.

(b) Numerical (5 marks)

Given m=0.2kgm=0.2\,\text{kg}, k=80N/mk=80\,\text{N/m}, b=0.16kg/sb=0.16\,\text{kg/s}.

ω02=km=800.2=400s2,β=b2m=0.160.4=0.4s1\omega_0^2=\frac{k}{m}=\frac{80}{0.2}=400\,\text{s}^{-2}, \qquad \beta=\frac{b}{2m}=\frac{0.16}{0.4}=0.4\,\text{s}^{-1}

Damped angular frequency:

ωd=ω02β2=4000.16=399.8420.0rad/s\omega_d=\sqrt{\omega_0^2-\beta^2}=\sqrt{400-0.16}=\sqrt{399.84}\approx 20.0\,\text{rad/s}

Time for amplitude to halve: amplitude eβt\propto e^{-\beta t}, so eβt=12e^{-\beta t}=\tfrac12:

t1/2=ln2β=0.6930.41.73st_{1/2}=\frac{\ln 2}{\beta}=\frac{0.693}{0.4}\approx 1.73\,\text{s}
oscillationsdamped-oscillationforced-oscillation
2long14 marks

(a) State Maxwell's equations of electromagnetism in differential form and explain the physical significance of each. Show how Maxwell modified Ampere's law by introducing the concept of displacement current. (8)

(b) Starting from Maxwell's equations in free space, derive the wave equation for the electric field and hence obtain an expression for the speed of electromagnetic waves in vacuum. (6)

(a) Maxwell's equations and displacement current (8 marks)

In differential form, in a medium of permittivity ε\varepsilon and permeability μ\mu:

EquationFormPhysical significance
Gauss's law (electric)E=ρε0\nabla\cdot\mathbf{E}=\dfrac{\rho}{\varepsilon_0}Electric charges are the sources of the electric field.
Gauss's law (magnetic)B=0\nabla\cdot\mathbf{B}=0No magnetic monopoles; magnetic field lines are closed.
Faraday's law×E=Bt\nabla\times\mathbf{E}=-\dfrac{\partial \mathbf{B}}{\partial t}A changing magnetic field induces an electric field.
Ampère–Maxwell law×B=μ0J+μ0ε0Et\nabla\times\mathbf{B}=\mu_0\mathbf{J}+\mu_0\varepsilon_0\dfrac{\partial \mathbf{E}}{\partial t}Conduction current and changing electric field both produce a magnetic field.

Displacement current. The original Ampère's law ×B=μ0J\nabla\times\mathbf{B}=\mu_0\mathbf{J} gives (×B)=μ0J=0\nabla\cdot(\nabla\times\mathbf{B})=\mu_0\nabla\cdot\mathbf{J}=0, but the continuity equation requires J=ρ/t\nabla\cdot\mathbf{J}=-\partial\rho/\partial t, which is non-zero when charge accumulates (e.g. between capacitor plates while charging). Maxwell removed the inconsistency by adding a term. Using ρ=ε0E\rho=\varepsilon_0\nabla\cdot\mathbf{E},

J+t(ε0E)=0     ⁣(J+ε0Et)=0\nabla\cdot\mathbf{J} + \frac{\partial}{\partial t}(\varepsilon_0\nabla\cdot\mathbf{E})=0 \;\Rightarrow\; \nabla\cdot\!\left(\mathbf{J}+\varepsilon_0\frac{\partial\mathbf{E}}{\partial t}\right)=0

The extra term Jd=ε0Et\mathbf{J}_d=\varepsilon_0\dfrac{\partial\mathbf{E}}{\partial t} is the displacement current density, giving the corrected law ×B=μ0(J+Jd)\nabla\times\mathbf{B}=\mu_0(\mathbf{J}+\mathbf{J}_d).

(b) Wave equation and speed of EM waves (6 marks)

In free space ρ=0, J=0\rho=0,\ \mathbf{J}=0. Take the curl of Faraday's law:

×(×E)=t(×B)=μ0ε02Et2\nabla\times(\nabla\times\mathbf{E})=-\frac{\partial}{\partial t}(\nabla\times\mathbf{B})=-\mu_0\varepsilon_0\frac{\partial^2\mathbf{E}}{\partial t^2}

Using the identity ×(×E)=(E)2E\nabla\times(\nabla\times\mathbf{E})=\nabla(\nabla\cdot\mathbf{E})-\nabla^2\mathbf{E} with E=0\nabla\cdot\mathbf{E}=0:

2E=μ0ε02Et2\boxed{\nabla^2\mathbf{E}=\mu_0\varepsilon_0\frac{\partial^2\mathbf{E}}{\partial t^2}}

Comparing with the standard wave equation 2E=1c22Et2\nabla^2\mathbf{E}=\dfrac{1}{c^2}\dfrac{\partial^2\mathbf{E}}{\partial t^2} gives the speed of EM waves in vacuum:

c=1μ0ε0=1(4π×107)(8.85×1012)3×108m/sc=\frac{1}{\sqrt{\mu_0\varepsilon_0}}=\frac{1}{\sqrt{(4\pi\times10^{-7})(8.85\times10^{-12})}}\approx 3\times10^{8}\,\text{m/s}

which matches the measured speed of light, establishing that light is an electromagnetic wave.

electromagnetismmaxwell-equationsem-waves
3long12 marks

(a) Derive the time-independent Schrödinger wave equation for a particle of mass m moving in a region of potential energy V. (6)

(b) Apply the Schrödinger equation to a particle confined in a one-dimensional infinite potential well (rigid box) of width L. Obtain the normalized wave functions and show that the energy of the particle is quantized. Sketch the first three energy eigenstates. (6)

(a) Time-independent Schrödinger equation (6 marks)

A particle of mass mm is described by a wave Ψ(x,t)=ψ(x)eiEt/\Psi(x,t)=\psi(x)e^{-iEt/\hbar}. Starting from the classical plane wave Ψ=Aei(kxωt)\Psi=Ae^{i(kx-\omega t)} and using the de Broglie relations p=kp=\hbar k and E=ωE=\hbar\omega:

2Ψx2=k2Ψ=p22Ψ,iΨt=EΨ\frac{\partial^2\Psi}{\partial x^2}=-k^2\Psi=-\frac{p^2}{\hbar^2}\Psi, \qquad i\hbar\frac{\partial\Psi}{\partial t}=E\Psi

Total energy E=p22m+VE=\dfrac{p^2}{2m}+V, hence p2=2m(EV)p^2=2m(E-V). Substituting:

22md2ψdx2+Vψ=Eψ    d2ψdx2+2m2(EV)ψ=0-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2}+V\psi=E\psi \;\Rightarrow\; \boxed{\frac{d^2\psi}{dx^2}+\frac{2m}{\hbar^2}(E-V)\psi=0}

This is the time-independent Schrödinger equation (3-D form: 2ψ+2m2(EV)ψ=0\nabla^2\psi+\tfrac{2m}{\hbar^2}(E-V)\psi=0).

(b) Particle in a 1-D infinite well of width LL (6 marks)

Inside the box V=0V=0 (0<x<L0<x<L); outside V=V=\infty so ψ=0\psi=0. The equation becomes

d2ψdx2+k2ψ=0,k2=2mE2\frac{d^2\psi}{dx^2}+k^2\psi=0,\qquad k^2=\frac{2mE}{\hbar^2}

General solution ψ=Asinkx+Bcoskx\psi=A\sin kx + B\cos kx. Boundary condition ψ(0)=0B=0\psi(0)=0\Rightarrow B=0. Condition ψ(L)=0sinkL=0kL=nπ, n=1,2,3,\psi(L)=0\Rightarrow \sin kL=0\Rightarrow kL=n\pi,\ n=1,2,3,\dots

Quantized energy:

En=2k22m=n2π222mL2=n2h28mL2E_n=\frac{\hbar^2 k^2}{2m}=\boxed{\frac{n^2\pi^2\hbar^2}{2mL^2}=\frac{n^2 h^2}{8mL^2}}

Energy is discrete (quantized) and the lowest state (n=1n=1) has non-zero zero-point energy.

Normalization: 0LA2sin2 ⁣nπxLdx=1A=2L\displaystyle\int_0^L A^2\sin^2\!\frac{n\pi x}{L}\,dx=1\Rightarrow A=\sqrt{\tfrac{2}{L}}, so

ψn(x)=2Lsin ⁣nπxL\psi_n(x)=\sqrt{\frac{2}{L}}\,\sin\!\frac{n\pi x}{L}

Sketch of first three eigenstates: ψ1\psi_1 is a single half-sine (one antinode, no node inside); ψ2\psi_2 is a full sine (one node at x=L/2x=L/2); ψ3\psi_3 has two interior nodes. All vanish at x=0x=0 and x=Lx=L.

quantum-mechanicsschrodinger-equationparticle-in-a-box
4long12 marks

(a) Explain the principle of light propagation through an optical fibre based on total internal reflection. Define acceptance angle and numerical aperture, and derive an expression for the numerical aperture in terms of the refractive indices of the core and cladding. (8)

(b) An optical fibre has a core refractive index of 1.50 and a cladding refractive index of 1.46. Calculate its numerical aperture and the acceptance angle when the fibre is placed in air. (4)

(a) Light propagation, acceptance angle and numerical aperture (8 marks)

An optical fibre has a high-index core (n1n_1) surrounded by a lower-index cladding (n2<n1n_2<n_1). A ray entering the core strikes the core–cladding boundary; if the angle of incidence there exceeds the critical angle θc\theta_c (where sinθc=n2/n1\sin\theta_c=n_2/n_1), the ray undergoes total internal reflection and is guided down the fibre with negligible loss, repeatedly reflecting along its length.

Acceptance angle (θa\theta_a): the maximum half-angle of the entrance cone for which an incident ray is still totally internally reflected inside the core. Rays within this cone are guided; rays outside it escape into the cladding.

Numerical aperture (NA): the light-gathering ability of the fibre, NA=n0sinθaNA=n_0\sin\theta_a (with n0n_0 the index of the medium outside).

Derivation. Let a ray enter from a medium of index n0n_0 at angle θa\theta_a, refracting to angle θr\theta_r inside the core: n0sinθa=n1sinθrn_0\sin\theta_a=n_1\sin\theta_r. To be guided it must hit the wall at exactly the critical angle, so the angle with the wall normal is 90θr90^\circ-\theta_r and

sin(90θr)=cosθr=n2n1    sinθr=1n22n12\sin(90^\circ-\theta_r)=\cos\theta_r=\frac{n_2}{n_1}\;\Rightarrow\;\sin\theta_r=\sqrt{1-\frac{n_2^2}{n_1^2}}

Therefore

n0sinθa=n1sinθr=n11n22n12=n12n22n_0\sin\theta_a=n_1\sin\theta_r=n_1\sqrt{1-\frac{n_2^2}{n_1^2}}=\sqrt{n_1^2-n_2^2} NA=n0sinθa=n12n22(in air, n0=1)\boxed{NA=n_0\sin\theta_a=\sqrt{n_1^2-n_2^2}}\quad(\text{in air, }n_0=1)

(b) Numerical (4 marks)

Given n1=1.50, n2=1.46n_1=1.50,\ n_2=1.46, fibre in air (n0=1n_0=1).

NA=1.5021.462=2.252.1316=0.11840.344NA=\sqrt{1.50^2-1.46^2}=\sqrt{2.25-2.1316}=\sqrt{0.1184}\approx 0.344 θa=sin1(0.344)20.1\theta_a=\sin^{-1}(0.344)\approx 20.1^\circ

Numerical aperture 0.344\approx 0.344; acceptance angle 20.1\approx 20.1^\circ.

fibre-opticslaserstotal-internal-reflection
B

Section B: Short Answer Questions

Attempt all / any as specified.

9 questions
5short7 marks

Explain the formation of Newton's rings in reflected light. Derive an expression for the diameter of the n-th dark ring and show how the wavelength of monochromatic light can be determined using this arrangement.

Newton's rings in reflected light

When a plano-convex lens of large radius RR rests on a flat glass plate, a thin air film of gradually increasing thickness forms between them. Monochromatic light incident from above is partly reflected at the top and bottom of the air film; these two beams interfere. Because of the circular symmetry of the film, loci of constant thickness are circles, so a pattern of alternately bright and dark concentric rings with a dark central spot is seen in reflected light.

For near-normal incidence the path difference between the two reflected rays is 2μt2\mu t, plus an extra λ/2\lambda/2 from the phase change on reflection at the glass surface (rarer-to-denser). For an air film μ=1\mu=1:

  • Dark ring: 2t=nλ2t=n\lambda
  • Bright ring: 2t=(2n1)λ22t=(2n-1)\tfrac{\lambda}{2}

Diameter of the nn-th dark ring

From the geometry of the lens, the film thickness at radius rr is t=r22Rt=\dfrac{r^2}{2R}. For the nn-th dark ring 2t=nλ2t=n\lambda:

2rn22R=nλ    rn2=nRλ2\cdot\frac{r_n^2}{2R}=n\lambda \;\Rightarrow\; r_n^2=nR\lambda

With diameter Dn=2rnD_n=2r_n:

Dn2=4nRλ\boxed{D_n^2=4nR\lambda}

The diameter is proportional to n\sqrt{n}, so rings get closer together outward.

Determination of wavelength

Measure the diameters of the nn-th and mm-th dark rings. Then

Dn2=4nRλ,Dm2=4mRλ    Dm2Dn2=4(mn)RλD_n^2=4nR\lambda,\quad D_m^2=4mR\lambda \;\Rightarrow\; D_m^2-D_n^2=4(m-n)R\lambda λ=Dm2Dn24(mn)R\boxed{\lambda=\frac{D_m^2-D_n^2}{4(m-n)R}}

This subtraction eliminates errors from imperfect contact at the centre. Knowing RR (from a spherometer) and the measured diameters, λ\lambda is found.

interferencenewtons-rings
6short7 marks

What is a plane diffraction grating? Obtain the grating equation for the position of principal maxima. A grating having 5000 lines per cm is illuminated normally by light of wavelength 589 nm; find the angle of diffraction for the second-order maximum.

Plane diffraction grating

A plane diffraction grating is an optical component consisting of a large number of equally spaced, identical, parallel slits (rulings) on a flat transparent surface. If the slit width is aa and the opaque space between slits is bb, the grating element is d=a+bd=a+b, equal to the reciprocal of the number of lines per unit length.

Grating equation (principal maxima)

When light of wavelength λ\lambda falls normally on the grating, the secondary wavelets from corresponding points of adjacent slits travel an extra path dsinθd\sin\theta in a direction making angle θ\theta with the normal. Constructive interference (a principal maximum) occurs when this path difference is a whole number of wavelengths:

dsinθ=nλ,n=0,1,2,\boxed{d\sin\theta = n\lambda}, \qquad n=0,1,2,\dots

where nn is the order of the spectrum.

Numerical

Grating has N=5000N=5000 lines/cm, so

d=15000cm=2×104cm=2×106md=\frac{1}{5000}\,\text{cm}=2\times10^{-4}\,\text{cm}=2\times10^{-6}\,\text{m}

For n=2n=2, λ=589nm=589×109m\lambda=589\,\text{nm}=589\times10^{-9}\,\text{m}:

sinθ=nλd=2×589×1092×106=0.589\sin\theta=\frac{n\lambda}{d}=\frac{2\times589\times10^{-9}}{2\times10^{-6}}=0.589 θ=sin1(0.589)36.1\theta=\sin^{-1}(0.589)\approx 36.1^\circ

Angle of diffraction for the second-order maximum 36.1\approx 36.1^\circ.

diffractiondiffraction-grating
7short7 marks

(a) State and explain Brewster's law and use it to define the polarizing angle. (4)

(b) Distinguish between a quarter-wave plate and a half-wave plate, stating one practical use of each. (3)

(a) Brewster's law and polarizing angle (4 marks)

Brewster's law: When unpolarized light is incident on a transparent dielectric, there is a particular angle of incidence, the polarizing (Brewster) angle θp\theta_p, at which the reflected light is completely plane-polarized (vibrations perpendicular to the plane of incidence). At this angle the refractive index equals the tangent of the polarizing angle:

μ=tanθp\boxed{\mu=\tan\theta_p}

At θp\theta_p the reflected and refracted rays are mutually perpendicular (θp+θr=90\theta_p+\theta_r=90^\circ). Proof: by Snell's law μ=sinθpsinθr=sinθpsin(90θp)=sinθpcosθp=tanθp\mu=\dfrac{\sin\theta_p}{\sin\theta_r}=\dfrac{\sin\theta_p}{\sin(90^\circ-\theta_p)}=\dfrac{\sin\theta_p}{\cos\theta_p}=\tan\theta_p. The polarizing angle is thus the angle of incidence for which the reflected beam is fully polarized.

(b) Quarter-wave vs half-wave plate (3 marks)

Quarter-wave plateHalf-wave plate
Path difference introducedλ/4\lambda/4λ/2\lambda/2
Phase differenceπ/2\pi/2π\pi
EffectConverts linearly polarized light into circularly/elliptically polarized light (and vice versa)Rotates the plane of linearly polarized light by 2θ2\theta (keeps it linear)
Thicknesst=λ4(μoμe)t=\dfrac{\lambda}{4(\mu_o-\mu_e)}t=λ2(μoμe)t=\dfrac{\lambda}{2(\mu_o-\mu_e)}
Practical useProduction/analysis of circularly polarized light (e.g. in optical isolators, anti-glare devices)Rotating the polarization plane in polarimeters and laser optics
polarizationdouble-refractionbrewsters-law
8short6 marks

Explain the terms spontaneous emission, stimulated emission and population inversion. Why is population inversion essential for laser action, and how is it achieved in a three-level laser system?

Emission processes and population inversion

Spontaneous emission: An atom in an excited state E2E_2 decays on its own to a lower state E1E_1, emitting a photon of energy hν=E2E1h\nu=E_2-E_1. The photons are emitted in random directions, with random phase — the light is incoherent (ordinary light).

Stimulated emission: An incident photon of energy hν=E2E1h\nu=E_2-E_1 induces an excited atom to drop to E1E_1, emitting a second photon identical in frequency, phase, direction and polarization to the incident one. This produces coherent light amplification — the basis of laser action.

Population inversion: A non-equilibrium condition in which the number of atoms in the higher energy state exceeds that in the lower state (N2>N1N_2>N_1). In thermal equilibrium the Boltzmann distribution gives N2<N1N_2<N_1, so inversion must be created artificially.

Why population inversion is essential

Stimulated emission (gain) competes with absorption. The net rate of stimulated emission (N2N1)\propto (N_2-N_1), so a photon beam is amplified only if N2>N1N_2>N_1; otherwise absorption dominates and there is no light amplification. Hence population inversion is a necessary condition for laser action.

Three-level system

Atoms are pumped (optically) from the ground state E1E_1 to a high state E3E_3. From E3E_3 they decay rapidly and non-radiatively to a metastable state E2E_2 which has a long lifetime, so atoms accumulate there. When the population of E2E_2 exceeds that of the ground state E1E_1, inversion between E2E_2 and E1E_1 is achieved, and lasing occurs on the E2E1E_2\to E_1 transition (e.g. the ruby laser). A drawback is that the lower laser level is the heavily populated ground state, so very strong pumping is required.

laserspopulation-inversion
9short6 marks

Describe the formation of a depletion region in an unbiased p–n junction diode. Explain qualitatively, with the help of energy-band diagrams, how the junction behaves under forward bias and reverse bias.

Formation of the depletion region

When p-type and n-type semiconductors are joined, the large concentration gradient causes majority electrons to diffuse from n to p and holes from p to n. Near the junction electrons fill holes; the n-side is left with fixed positive donor ions and the p-side with fixed negative acceptor ions. This region, depleted of mobile charge carriers, is the depletion region. The exposed immobile ions set up an internal electric field (and a built-in potential barrier V0V_0, about 0.7 V for Si, 0.3 V for Ge) directed from n to p, which opposes further diffusion. At equilibrium the diffusion current is exactly balanced by the drift current and no net current flows.

In the band picture, the Fermi levels of the two sides align; the conduction and valence bands of the p-side bend upward relative to the n-side, the offset eV0eV_0 being the barrier height.

Forward bias

The p-side is connected to the positive terminal and the n-side to the negative terminal. The external field opposes the built-in field, reducing the barrier height to e(V0V)e(V_0-V) and narrowing the depletion region. The bands shift so the offset decreases. Majority carriers cross the junction easily, and a large current flows that rises steeply once VV exceeds the knee voltage.

Reverse bias

The p-side is made negative and the n-side positive. The external field aids the built-in field, increasing the barrier to e(V0+V)e(V_0+V) and widening the depletion region. The bands bend further apart. Majority-carrier flow is blocked; only a tiny reverse saturation current due to thermally generated minority carriers flows, nearly independent of voltage until breakdown.

semiconductor-physicspn-junction
10short6 marks

State the Hall effect and derive an expression for the Hall coefficient. Mention two important applications of the Hall effect in characterizing semiconductor materials.

Hall effect

When a current-carrying conductor (or semiconductor) is placed in a magnetic field perpendicular to the current, a transverse potential difference (the Hall voltage VHV_H) develops across the specimen, perpendicular to both the current and the field. This is the Hall effect, and it arises from the magnetic Lorentz force on the moving charge carriers.

Derivation of the Hall coefficient

Let current II flow along xx in a slab of width ww and thickness tt, with magnetic field BB along zz. Carriers of charge qq drift with velocity vdv_d. The Lorentz force qvdBqv_dB pushes them sideways (along yy) until the resulting transverse electric field EHE_H balances it:

qEH=qvdB    EH=vdBqE_H=qv_dB \;\Rightarrow\; E_H=v_dB

The current density is J=nqvdJ=nqv_d, where nn is the carrier concentration, so vd=Jnqv_d=\dfrac{J}{nq} and

EH=JBnqE_H=\frac{JB}{nq}

The Hall coefficient is defined as RH=EHJBR_H=\dfrac{E_H}{JB}:

RH=1nq\boxed{R_H=\frac{1}{nq}}

In terms of measurable quantities, VH=EHwV_H=E_H w and J=IwtJ=\dfrac{I}{wt}, giving VH=IBnqtV_H=\dfrac{IB}{nqt} and RH=VHtIBR_H=\dfrac{V_H t}{IB}. The sign of RHR_H is negative for n-type (electrons) and positive for p-type (holes).

Applications

  1. Determination of carrier type and concentration — the sign of RHR_H gives the majority-carrier type and its magnitude gives n=1/(RHq)n=1/(R_H q).
  2. Measurement of carrier mobility — combining RHR_H with the conductivity σ\sigma gives the Hall mobility μH=RHσ\mu_H=R_H\sigma. (Also used in Hall-effect magnetic-field sensors/probes.)
semiconductor-physicshall-effect
11short7 marks

Explain the different types of polarization mechanisms in a dielectric material. Derive the Clausius–Mossotti relation connecting the dielectric constant of a material to its atomic polarizability.

Polarization mechanisms in dielectrics

When a dielectric is placed in an electric field, bound charges shift slightly, giving each unit volume a dipole moment (polarization PP). The main mechanisms are:

  1. Electronic polarization: displacement of the electron cloud relative to the nucleus of each atom. Present in all dielectrics, very fast (up to optical frequencies).
  2. Ionic (atomic) polarization: in ionic solids, positive and negative ions displace in opposite directions, changing inter-ionic distances.
  3. Orientational (dipolar) polarization: in polar molecules (with permanent dipoles, e.g. water), the field tends to align the dipoles against thermal randomization; strongly temperature-dependent.
  4. Space-charge (interfacial) polarization: accumulation of mobile charges at grain boundaries/interfaces; significant only at low frequencies.

Clausius–Mossotti relation

For a non-polar dielectric, the local field acting on an atom (Lorentz field) is

Eloc=E+P3ε0E_{loc}=E+\frac{P}{3\varepsilon_0}

The induced dipole moment per atom is p=αElocp=\alpha E_{loc}, and with NN atoms per unit volume the polarization is

P=NαEloc=Nα(E+P3ε0)P=N\alpha E_{loc}=N\alpha\left(E+\frac{P}{3\varepsilon_0}\right)

Solving for PP:

P=NαE1Nα3ε0P=\frac{N\alpha E}{1-\dfrac{N\alpha}{3\varepsilon_0}}

Using P=ε0(εr1)EP=\varepsilon_0(\varepsilon_r-1)E to eliminate P/EP/E and simplifying gives the Clausius–Mossotti relation:

εr1εr+2=Nα3ε0\boxed{\frac{\varepsilon_r-1}{\varepsilon_r+2}=\frac{N\alpha}{3\varepsilon_0}}

This links the macroscopic dielectric constant εr\varepsilon_r to the microscopic atomic polarizability α\alpha and the number density NN.

dielectricspolarization
12short6 marks

Distinguish between diamagnetic, paramagnetic and ferromagnetic materials on the basis of their magnetic susceptibility and behaviour in an external magnetic field, giving one example of each.

Classification of magnetic materials

PropertyDiamagneticParamagneticFerromagnetic
Susceptibility χ\chiSmall, negative (105\sim-10^{-5})Small, positive (103\sim10^{-3})Very large, positive (102\sim10^{2}10510^{5})
Relative permeability μr\mu_rSlightly <1<1Slightly >1>11\gg 1
Behaviour in a fieldWeakly repelled; moves from strong to weak fieldWeakly attracted; moves from weak to strong fieldStrongly attracted; can be permanently magnetized
Atomic originNo permanent dipoles; induced moments oppose fieldPermanent dipoles randomly oriented, partly align with fieldPermanent dipoles align in domains; strong exchange coupling
Temperature dependenceIndependent of TTχ1/T\chi\propto 1/T (Curie law)Ferromagnetic below Curie temperature; paramagnetic above it
ExampleBismuth, copper, waterAluminium, platinum, manganeseIron, cobalt, nickel

Summary: Diamagnetics oppose the applied field weakly, paramagnetics enhance it weakly, and ferromagnetics enhance it enormously and retain magnetization.

magnetismdia-para-ferromagnetism
13short6 marks

State Heisenberg's uncertainty principle. Using it, estimate the minimum energy (zero-point energy) of an electron confined within a nucleus of dimension 10⁻¹⁴ m and comment on whether electrons can exist inside the nucleus.

Heisenberg's uncertainty principle

It is impossible to determine simultaneously, with unlimited precision, both the position and the momentum of a particle. The product of the uncertainties is at least of the order of \hbar:

ΔxΔp2,=h2π=1.055×1034J\cdotps\Delta x\,\Delta p \ge \frac{\hbar}{2}, \qquad \hbar=\frac{h}{2\pi}=1.055\times10^{-34}\,\text{J·s}

Minimum energy of an electron confined in a nucleus

If the electron is confined within a nucleus, Δx1014m\Delta x \approx 10^{-14}\,\text{m}. Taking the minimum momentum pΔpΔxp\approx\Delta p\approx\dfrac{\hbar}{\Delta x}:

p1.055×10341014=1.055×1020kg\cdotpm/sp\approx\frac{1.055\times10^{-34}}{10^{-14}}=1.055\times10^{-20}\,\text{kg·m/s}

Since pc=(1.055×1020)(3×108)=3.16×1012Jpc=(1.055\times10^{-20})(3\times10^{8})=3.16\times10^{-12}\,\text{J} is far larger than the electron rest energy m0c2=8.2×1014Jm_0c^2=8.2\times10^{-14}\,\text{J}, the electron must be treated relativistically, EpcE\approx pc:

Epc=3.16×1012J=3.16×10121.6×1019eV1.98×107eV20MeVE\approx pc=3.16\times10^{-12}\,\text{J}=\frac{3.16\times10^{-12}}{1.6\times10^{-19}}\,\text{eV}\approx 1.98\times10^{7}\,\text{eV}\approx 20\,\text{MeV}

Comment

An electron bound inside the nucleus would need a minimum energy of about 20 MeV. However, electrons emitted in beta decay have energies of only a few MeV, and no nuclear binding mechanism can hold an electron with 20 MeV. Therefore electrons cannot exist inside the nucleus; the beta-decay electron is created at the instant of decay.

quantum-mechanicsuncertainty-principlewave-particle-duality

Frequently asked questions

Where can I find the BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) question paper 2079?
The full BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) 2079 (regular) question paper is available free on Kekkei. You can read every question online and attempt the paper under timed exam conditions.
Does the Applied Physics (PU, PHY 110) 2079 paper come with solutions?
Yes. Every question on this Applied Physics (PU, PHY 110) past paper includes a step-by-step solution, plus instant AI feedback when you attempt it on Kekkei.
How many marks is the BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) 2079 paper?
The BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) 2079 paper carries 100 full marks and is meant to be completed in 180 minutes, across 13 questions.
Is practising this Applied Physics (PU, PHY 110) past paper free?
Yes — reading and attempting this Applied Physics (PU, PHY 110) past paper on Kekkei is completely free.