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Section A: Long Answer Questions

Attempt all questions.

5 questions
1long8 marks

Set up the differential equation of a damped harmonic oscillator and obtain its solution for the under-damped case. Explain how the amplitude decays with time.

A mass of 0.20 kg0.20\ \text{kg} is attached to a spring of force constant k=80 N/mk = 80\ \text{N/m} and oscillates in a medium that exerts a resistive force F=bvF = -b v with b=0.40 kg/sb = 0.40\ \text{kg/s}. Determine (i) the angular frequency of the damped oscillation and (ii) the time in which the amplitude falls to 1/e1/e of its initial value.

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

md2xdt2=kxbdxdtm\frac{d^2x}{dt^2} = -kx - b\frac{dx}{dt}

Dividing by mm and writing 2β=b/m2\beta = b/m (damping constant) and ω02=k/m\omega_0^2 = k/m (natural frequency):

d2xdt2+2βdxdt+ω02x=0\frac{d^2x}{dt^2} + 2\beta\frac{dx}{dt} + \omega_0^2 x = 0

Solution (under-damped, β<ω0\beta < \omega_0). Trying x=eλtx = e^{\lambda t} gives the auxiliary equation λ2+2βλ+ω02=0\lambda^2 + 2\beta\lambda + \omega_0^2 = 0, so λ=β±β2ω02\lambda = -\beta \pm \sqrt{\beta^2 - \omega_0^2}. For β<ω0\beta < \omega_0 the root is complex, λ=β±iωd\lambda = -\beta \pm i\omega_d with ωd=ω02β2\omega_d = \sqrt{\omega_0^2 - \beta^2}. The real solution is

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

Amplitude decay. The envelope A(t)=A0eβtA(t) = A_0 e^{-\beta t} decays exponentially; the oscillation frequency ωd\omega_d is slightly less than ω0\omega_0.

 x
 |   .-.        envelope A0 e^{-bt}
 |  /   \   _
 | /     \ / \  _
 |/       V   \/ \___ ...
 +----------------------- t

Numerical part. Given m=0.20 kgm = 0.20\ \text{kg}, k=80 N/mk = 80\ \text{N/m}, b=0.40 kg/sb = 0.40\ \text{kg/s}.

ω0=k/m=80/0.20=400=20 rad/s\omega_0 = \sqrt{k/m} = \sqrt{80/0.20} = \sqrt{400} = 20\ \text{rad/s}

β=b2m=0.402(0.20)=1.0 s1\beta = \dfrac{b}{2m} = \dfrac{0.40}{2(0.20)} = 1.0\ \text{s}^{-1}

(i) ωd=ω02β2=4001=399=19.975 rad/s\omega_d = \sqrt{\omega_0^2 - \beta^2} = \sqrt{400 - 1} = \sqrt{399} = 19.975\ \text{rad/s}.

ωd19.97 rad/s\omega_d \approx 19.97\ \text{rad/s}.

(ii) Amplitude A(t)=A0eβtA(t) = A_0 e^{-\beta t} falls to A0/eA_0/e when βt=1\beta t = 1, i.e. t=1/β=1/1.0=1.0 st = 1/\beta = 1/1.0 = 1.0\ \text{s}.

Time constant τ=1.0 s\tau = 1.0\ \text{s}.

oscillationsdamped-shmresonance
2long8 marks

Describe the formation of Newton's rings by reflected light and derive an expression for the diameter of the nn-th dark ring. How can this arrangement be used to find the wavelength of monochromatic light?

In a Newton's rings experiment the diameter of the 1010-th dark ring is 4.00 mm4.00\ \text{mm} and that of the 2020-th dark ring is 5.66 mm5.66\ \text{mm}. If the radius of curvature of the plano-convex lens is 1.00 m1.00\ \text{m}, calculate the wavelength of the light used.

Formation. A plano-convex lens of large radius of curvature RR rests on a flat glass plate, enclosing a thin air film whose thickness increases radially from the contact point. Monochromatic light incident from above is partly reflected at the top and bottom of the air film; the two reflected beams interfere. Because of the central symmetry, loci of equal thickness are circles, giving concentric bright and dark rings (Newton's rings). An extra phase change of π\pi occurs at the air-to-glass reflection at the lower surface.

Diameter of the nn-th dark ring. For a film of thickness tt, the path difference is 2t+λ/22t + \lambda/2. Dark ring (destructive) requires 2t=nλ2t = n\lambda. From the geometry of the lens, if rr is the ring radius, r2=(2Rt)t2Rtr^2 = (2R - t)t \approx 2Rt for tRt \ll R, so t=r2/2Rt = r^2/2R. Hence

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

With diameter Dn=2rnD_n = 2r_n:

Dn2=4nRλD_n^2 = 4nR\lambda

Finding λ\lambda. Measuring two rings nn and mm eliminates uncertainty at the contact point:

Dm2Dn2=4(mn)Rλ    λ=Dm2Dn24(mn)RD_m^2 - D_n^2 = 4(m-n)R\lambda \implies \lambda = \frac{D_m^2 - D_n^2}{4(m-n)R}

Numerical part. D10=4.00 mm=4.00×103 mD_{10} = 4.00\ \text{mm} = 4.00\times10^{-3}\ \text{m}, so D102=16.00×106 m2D_{10}^2 = 16.00\times10^{-6}\ \text{m}^2.

D20=5.66 mm=5.66×103 mD_{20} = 5.66\ \text{mm} = 5.66\times10^{-3}\ \text{m}, so D202=32.0356×106 m2D_{20}^2 = 32.0356\times10^{-6}\ \text{m}^2.

D202D102=(32.035616.00)×106=16.0356×106 m2D_{20}^2 - D_{10}^2 = (32.0356 - 16.00)\times10^{-6} = 16.0356\times10^{-6}\ \text{m}^2.

mn=2010=10m - n = 20 - 10 = 10, R=1.00 mR = 1.00\ \text{m}.

λ=16.0356×1064×10×1.00=16.0356×10640=4.009×107 m\lambda = \frac{16.0356\times10^{-6}}{4\times10\times1.00} = \frac{16.0356\times10^{-6}}{40} = 4.009\times10^{-7}\ \text{m}

λ401 nm\lambda \approx 401\ \text{nm} (violet-blue light).

physical-opticsnewtons-ringsinterference
3long8 marks

State Gauss's law in electrostatics and use it to find the electric field due to an infinitely long uniformly charged straight wire. Hence derive the capacitance per unit length of a coaxial cylindrical capacitor.

A coaxial cable has an inner conductor of radius 1.0 mm1.0\ \text{mm} and an outer conductor of inner radius 4.0 mm4.0\ \text{mm}, with air between them. Calculate the capacitance per metre of the cable. (Take ε0=8.85×1012 F/m\varepsilon_0 = 8.85\times10^{-12}\ \text{F/m}.)

Gauss's law. The net electric flux through any closed surface equals the charge enclosed divided by ε0\varepsilon_0:

EdA=Qencε0\oint \vec{E}\cdot d\vec{A} = \frac{Q_{enc}}{\varepsilon_0}

Field of a line charge. Consider an infinite wire with linear charge density λ\lambda. By symmetry E\vec E is radial. Take a coaxial Gaussian cylinder of radius rr and length LL. Flux through the curved surface is E(2πrL)E(2\pi r L) (ends contribute nothing). Enclosed charge =λL= \lambda L:

E(2πrL)=λLε0    E=λ2πε0rE\,(2\pi r L) = \frac{\lambda L}{\varepsilon_0} \implies E = \frac{\lambda}{2\pi\varepsilon_0 r}

Coaxial capacitor. Inner cylinder radius aa carries +λ+\lambda per unit length, outer cylinder radius bb carries λ-\lambda. The potential difference is

V=abEdr=λ2πε0abdrr=λ2πε0lnbaV = \int_a^b E\,dr = \frac{\lambda}{2\pi\varepsilon_0}\int_a^b \frac{dr}{r} = \frac{\lambda}{2\pi\varepsilon_0}\ln\frac{b}{a}

Capacitance per unit length C/L=λ/VC/L = \lambda/V:

CL=2πε0ln(b/a)\boxed{\frac{C}{L} = \frac{2\pi\varepsilon_0}{\ln(b/a)}}

Numerical part. a=1.0 mma = 1.0\ \text{mm}, b=4.0 mmb = 4.0\ \text{mm}, so b/a=4.0b/a = 4.0 and ln4.0=1.3863\ln 4.0 = 1.3863.

CL=2π(8.85×1012)1.3863=5.561×10111.3863=4.011×1011 F/m\frac{C}{L} = \frac{2\pi(8.85\times10^{-12})}{1.3863} = \frac{5.561\times10^{-11}}{1.3863} = 4.011\times10^{-11}\ \text{F/m}

C/L40.1 pF/mC/L \approx 40.1\ \text{pF/m}.

electrostaticsgauss-lawcapacitance
4long8 marks

Write down Maxwell's equations in integral form for free space and explain the physical meaning of each. Introduce the concept of displacement current and show that it makes Ampere's law consistent for a charging capacitor.

A parallel-plate capacitor with circular plates of radius 5.0 cm5.0\ \text{cm} is being charged so that the potential difference increases at 2.0×106 V/s2.0\times10^{6}\ \text{V/s}. The plate separation is 2.0 mm2.0\ \text{mm}. Find the displacement current between the plates.

Maxwell's equations (integral form, free space).

  1. Gauss's law (electric): EdA=Qε0\displaystyle\oint \vec E\cdot d\vec A = \frac{Q}{\varepsilon_0} — electric flux originates from charge.
  2. Gauss's law (magnetic): BdA=0\displaystyle\oint \vec B\cdot d\vec A = 0 — no magnetic monopoles; field lines are closed.
  3. Faraday's law: Edl=dΦBdt\displaystyle\oint \vec E\cdot d\vec l = -\frac{d\Phi_B}{dt} — a changing magnetic flux induces an electric field.
  4. Ampere-Maxwell law: Bdl=μ0I+μ0ε0dΦEdt\displaystyle\oint \vec B\cdot d\vec l = \mu_0 I + \mu_0\varepsilon_0\frac{d\Phi_E}{dt} — currents and changing electric flux produce magnetic fields.

Displacement current. Consider Ampere's loop around the wire feeding a charging capacitor. A flat surface pierced by the wire gives conduction current II, but a bulging surface passing between the plates carries no conduction current — a contradiction. Maxwell resolved this by adding the displacement current

Id=ε0dΦEdtI_d = \varepsilon_0\frac{d\Phi_E}{dt}

Between the plates E=σ/ε0=Q/(ε0A)E = \sigma/\varepsilon_0 = Q/(\varepsilon_0 A), so ΦE=EA=Q/ε0\Phi_E = EA = Q/\varepsilon_0 and Id=ε0dΦE/dt=dQ/dt=II_d = \varepsilon_0\,d\Phi_E/dt = dQ/dt = I. Thus IdI_d exactly equals the conduction current, making Ampere's law surface-independent.

Numerical part. A=πr2=π(0.050)2=π(2.5×103)=7.854×103 m2A = \pi r^2 = \pi(0.050)^2 = \pi(2.5\times10^{-3}) = 7.854\times10^{-3}\ \text{m}^2.

Field: E=V/dE = V/d, so dEdt=1ddVdt=2.0×1062.0×103=1.0×109 V/(m\cdotps)\dfrac{dE}{dt} = \dfrac{1}{d}\dfrac{dV}{dt} = \dfrac{2.0\times10^{6}}{2.0\times10^{-3}} = 1.0\times10^{9}\ \text{V/(m·s)}.

Id=ε0AdEdt=(8.85×1012)(7.854×103)(1.0×109)I_d = \varepsilon_0 A\frac{dE}{dt} = (8.85\times10^{-12})(7.854\times10^{-3})(1.0\times10^{9}) Id=8.85×1012×7.854×103×109=6.95×105 AI_d = 8.85\times10^{-12}\times7.854\times10^{-3}\times10^{9} = 6.95\times10^{-5}\ \text{A}

Id69.5 μAI_d \approx 69.5\ \mu\text{A}.

electromagnetismmaxwells-equationsdisplacement-current
5long8 marks

Set up the time-independent Schrodinger equation for a particle confined in a one-dimensional infinite potential well of width LL. Obtain the normalized wave functions and the quantized energy levels.

An electron is confined in such a well of width 0.10 nm0.10\ \text{nm}. Calculate the energy (in eV) of the ground state and the first excited state. (Take h=6.63×1034 J\cdotpsh = 6.63\times10^{-34}\ \text{J·s}, me=9.11×1031 kgm_e = 9.11\times10^{-31}\ \text{kg}, 1 eV=1.60×1019 J1\ \text{eV} = 1.60\times10^{-19}\ \text{J}.)

Schrodinger equation. Inside the well (0<x<L0 < x < L) the potential V=0V = 0:

22md2ψdx2=Eψ    d2ψdx2+k2ψ=0,k2=2mE2-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2} = E\psi \implies \frac{d^2\psi}{dx^2} + k^2\psi = 0,\quad k^2 = \frac{2mE}{\hbar^2}

General solution ψ(x)=Asinkx+Bcoskx\psi(x) = A\sin kx + B\cos kx.

Boundary conditions. Walls are infinite, so ψ(0)=ψ(L)=0\psi(0) = \psi(L) = 0. At x=0x = 0: B=0B = 0. At x=Lx = L: AsinkL=0kL=nπA\sin kL = 0 \Rightarrow kL = n\pi, n=1,2,3,n = 1,2,3,\dots Hence kn=nπ/Lk_n = n\pi/L.

Energy levels. From k2=2mE/2k^2 = 2mE/\hbar^2:

En=2kn22m=n2π222mL2=n2h28mL2E_n = \frac{\hbar^2 k_n^2}{2m} = \frac{n^2\pi^2\hbar^2}{2mL^2} = \frac{n^2 h^2}{8mL^2}

Normalization. 0LA2sin2(nπx/L)dx=A2L/2=1A=2/L\int_0^L |A|^2\sin^2(n\pi x/L)\,dx = |A|^2 L/2 = 1 \Rightarrow A = \sqrt{2/L}. Thus

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

Numerical part. L=0.10 nm=1.0×1010 mL = 0.10\ \text{nm} = 1.0\times10^{-10}\ \text{m}.

Ground state (n=1n=1):

E1=h28mL2=(6.63×1034)28(9.11×1031)(1.0×1010)2E_1 = \frac{h^2}{8mL^2} = \frac{(6.63\times10^{-34})^2}{8(9.11\times10^{-31})(1.0\times10^{-10})^2}

Numerator: (6.63×1034)2=4.396×1067 J2s2(6.63\times10^{-34})^2 = 4.396\times10^{-67}\ \text{J}^2\text{s}^2.

Denominator: 8×9.11×1031×1.0×1020=7.288×10508\times9.11\times10^{-31}\times1.0\times10^{-20} = 7.288\times10^{-50}.

E1=4.396×10677.288×1050=6.032×1018 JE_1 = \frac{4.396\times10^{-67}}{7.288\times10^{-50}} = 6.032\times10^{-18}\ \text{J}

In eV: E1=6.032×10181.60×1019=37.7 eVE_1 = \dfrac{6.032\times10^{-18}}{1.60\times10^{-19}} = 37.7\ \text{eV}.

First excited state (n=2n=2): E2=4E1=4×37.7=150.8 eVE_2 = 4E_1 = 4\times37.7 = 150.8\ \text{eV}.

E137.7 eVE_1 \approx 37.7\ \text{eV},   E2150.8 eV\;E_2 \approx 150.8\ \text{eV}.

quantum-mechanicsschrodinger-equationparticle-in-box
B

Section B: Short Answer Questions

Attempt all questions.

6 questions
6short7 marks

Define reverberation time and state Sabine's formula. A hall of volume 1500 m31500\ \text{m}^3 has a total sound-absorbing surface giving an equivalent absorption of 120 m2120\ \text{m}^2 (sabine). Calculate the reverberation time. What additional absorption is required to reduce the reverberation time to 1.5 s1.5\ \text{s}?

Reverberation time is the time taken for the sound intensity in an enclosure to fall to 10610^{-6} of its steady value, i.e. for the sound level to drop by 60 dB60\ \text{dB} after the source stops.

Sabine's formula:

T=0.161VAT = \frac{0.161\,V}{A}

where VV is the room volume in m3\text{m}^3 and A=αiSiA = \sum \alpha_i S_i is the total absorption in sabine (m2\text{m}^2).

Initial reverberation time. V=1500 m3V = 1500\ \text{m}^3, A=120 m2A = 120\ \text{m}^2:

T=0.161×1500120=241.5120=2.01 sT = \frac{0.161\times1500}{120} = \frac{241.5}{120} = 2.01\ \text{s}

T2.01 sT \approx 2.01\ \text{s}.

Absorption needed for T=1.5 sT' = 1.5\ \text{s}. Rearranging:

A=0.161VT=241.51.5=161 m2A' = \frac{0.161\,V}{T'} = \frac{241.5}{1.5} = 161\ \text{m}^2

Additional absorption =AA=161120=41 m2= A' - A = 161 - 120 = 41\ \text{m}^2 (sabine).

Extra absorption required 41 m2\approx 41\ \text{m}^2.

acousticsreverberationsabine-formula
7short7 marks

Explain the action of a plane diffraction grating and write its grating equation. A grating has 50005000 lines per centimetre. Light of wavelength 589 nm589\ \text{nm} falls normally on it. Find the angle of diffraction for the first-order spectrum and the highest order that can be observed.

Action of a grating. A plane transmission grating is a large number of equally spaced parallel slits. When a plane wave is incident normally, each slit diffracts light; the diffracted wavelets from successive slits interfere. Constructive interference (principal maxima) occurs when the path difference between adjacent slits equals an integral number of wavelengths.

Grating equation:

dsinθ=nλd\sin\theta = n\lambda

where dd is the grating spacing, θ\theta the diffraction angle and nn the order.

Grating spacing. 50005000 lines/cm means

d=1 cm5000=1×102 m5000=2.0×106 md = \frac{1\ \text{cm}}{5000} = \frac{1\times10^{-2}\ \text{m}}{5000} = 2.0\times10^{-6}\ \text{m}

First order (n=1n = 1). λ=589 nm=5.89×107 m\lambda = 589\ \text{nm} = 5.89\times10^{-7}\ \text{m}.

sinθ1=nλd=5.89×1072.0×106=0.2945\sin\theta_1 = \frac{n\lambda}{d} = \frac{5.89\times10^{-7}}{2.0\times10^{-6}} = 0.2945 θ1=sin1(0.2945)=17.1\theta_1 = \sin^{-1}(0.2945) = 17.1^\circ

θ117.1\theta_1 \approx 17.1^\circ.

Highest order. Maximum when sinθ=1\sin\theta = 1:

nmax=dλ=2.0×1065.89×107=3.40n_{max} = \frac{d}{\lambda} = \frac{2.0\times10^{-6}}{5.89\times10^{-7}} = 3.40

Since nn must be an integer, the highest observable order is nmax=3n_{max} = 3.

physical-opticsdiffraction-gratingresolution
8short7 marks

What is meant by the acceptance angle and numerical aperture of a step-index optical fibre? Derive the expression for numerical aperture in terms of the refractive indices of the core and cladding. A fibre has a core of refractive index 1.501.50 and cladding of refractive index 1.461.46. Calculate its numerical aperture and acceptance angle (fibre in air).

Acceptance angle. The maximum half-angle of the cone of light, measured from the fibre axis, within which incident rays will undergo total internal reflection at the core-cladding boundary and so be guided along the fibre. Rays entering at larger angles escape into the cladding.

Numerical aperture (NA) is the sine of the acceptance angle; it measures the light-gathering capacity of the fibre.

Derivation. Let core index n1n_1, cladding index n2n_2, surrounding medium n0n_0. A ray entering at angle θa\theta_a refracts into the core at angle θr\theta_r and strikes the core-cladding interface at angle (90θr)(90^\circ - \theta_r). For total internal reflection this must equal the critical angle θc\theta_c where sinθc=n2/n1\sin\theta_c = n_2/n_1.

At the entry face (Snell): n0sinθa=n1sinθr=n1cosθc=n11(n2/n1)2n_0\sin\theta_a = n_1\sin\theta_r = n_1\cos\theta_c = n_1\sqrt{1 - (n_2/n_1)^2}.

n0sinθa=n12n22n_0\sin\theta_a = \sqrt{n_1^2 - n_2^2}

For air n0=1n_0 = 1:

NA=sinθa=n12n22\text{NA} = \sin\theta_a = \sqrt{n_1^2 - n_2^2}

Numerical part. n1=1.50n_1 = 1.50, n2=1.46n_2 = 1.46.

n12=2.2500n_1^2 = 2.2500, n22=2.1316n_2^2 = 2.1316, difference =0.1184= 0.1184.

NA=0.1184=0.3441\text{NA} = \sqrt{0.1184} = 0.3441

NA 0.344\approx 0.344.

Acceptance angle: θa=sin1(0.344)=20.1\theta_a = \sin^{-1}(0.344) = 20.1^\circ.

θa20.1\theta_a \approx 20.1^\circ (full acceptance cone 40.2\approx 40.2^\circ).

fiber-opticsnumerical-aperturetotal-internal-reflection
9short6 marks

Describe the Hall effect and derive an expression for the Hall coefficient. A current of 5.0 A5.0\ \text{A} flows along the length of an n-type semiconductor slab of thickness 1.0 mm1.0\ \text{mm} placed in a magnetic field of 0.40 T0.40\ \text{T} perpendicular to the slab. The measured Hall voltage is 1.25×103 V1.25\times10^{-3}\ \text{V}. Find the carrier concentration. (Take e=1.60×1019 Ce = 1.60\times10^{-19}\ \text{C}.)

Hall effect. When a current-carrying conductor is placed in a transverse magnetic field, the moving charge carriers experience a Lorentz force F=qv×B\vec F = q\vec v\times\vec B that deflects them to one face. Charge accumulates there, setting up a transverse electric field (Hall field) until the electric force balances the magnetic force. The resulting transverse voltage is the Hall voltage VHV_H.

Derivation. At equilibrium eEH=evdBeE_H = e v_d B, so EH=vdBE_H = v_d B. The drift velocity relates to current by I=nevdA=nevd(wt)I = n e v_d A = n e v_d (w t) where ww is width, tt thickness, so vd=I/(newt)v_d = I/(n e w t). The Hall voltage across width ww is VH=EHw=vdBw=IBnetV_H = E_H w = v_d B w = \dfrac{I B}{n e t}.

The Hall coefficient RH=1neR_H = \dfrac{1}{ne} (for electrons, sign negative), giving

VH=RHIBt,RH=VHtIBV_H = \frac{R_H I B}{t},\qquad R_H = \frac{V_H\,t}{I B}

Numerical part. I=5.0 AI = 5.0\ \text{A}, B=0.40 TB = 0.40\ \text{T}, t=1.0×103 mt = 1.0\times10^{-3}\ \text{m}, VH=1.25×103 VV_H = 1.25\times10^{-3}\ \text{V}.

From VH=IBnetV_H = \dfrac{IB}{net}:

n=IBetVH=(5.0)(0.40)(1.60×1019)(1.0×103)(1.25×103)n = \frac{IB}{e\,t\,V_H} = \frac{(5.0)(0.40)}{(1.60\times10^{-19})(1.0\times10^{-3})(1.25\times10^{-3})}

Numerator: 5.0×0.40=2.05.0\times0.40 = 2.0.

Denominator: 1.60×1019×1.0×103×1.25×103=2.0×10251.60\times10^{-19}\times1.0\times10^{-3}\times1.25\times10^{-3} = 2.0\times10^{-25}.

n=2.02.0×1025=1.0×1025 m3n = \frac{2.0}{2.0\times10^{-25}} = 1.0\times10^{25}\ \text{m}^{-3}

Carrier concentration n1.0×1025 m3n \approx 1.0\times10^{25}\ \text{m}^{-3}.

semiconductorshall-effectcharge-carriers
10short6 marks

Distinguish between spontaneous and stimulated emission. Explain the conditions of population inversion and metastable states necessary for laser action, and state two properties of laser light. Why is a three-level laser less efficient than a four-level laser?

Spontaneous vs stimulated emission.

FeatureSpontaneous emissionStimulated emission
TriggerRandom, no external photonTriggered by an incident photon
Phase/directionRandomSame phase, frequency, direction as incident photon
CoherenceIncoherentCoherent
ResultOrdinary lightAmplified, coherent light (basis of lasing)

In stimulated emission an excited atom is struck by a photon of energy hν=E2E1h\nu = E_2 - E_1 and drops to the lower level, emitting a second identical photon, giving light amplification.

Population inversion. Normally, by the Boltzmann distribution, lower levels are more populated than upper ones, so absorption dominates. Lasing requires the opposite: more atoms in the upper level E2E_2 than in E1E_1 (N2>N1N_2 > N_1). This non-equilibrium state is called population inversion and is achieved by pumping (optical or electrical).

Metastable state. A metastable level has a long lifetime (103 s\sim10^{-3}\ \text{s} vs 108 s\sim10^{-8}\ \text{s} for ordinary excited states). Atoms accumulate there long enough to build up the inversion before stimulated emission de-excites them.

Two properties of laser light: (1) high monochromaticity (very narrow spectral width); (2) high coherence and directionality (the beam is nearly parallel and in phase). (Also high intensity/brightness.)

Three-level vs four-level. In a three-level laser the lower lasing level is the ground state, which is heavily populated; more than half the atoms must be pumped above ground state to achieve inversion, requiring a high pumping threshold. In a four-level laser the lower lasing level lies above the ground state and is normally almost empty (it depopulates rapidly to the ground state), so inversion is achieved with much less pumping. Hence the four-level system is more efficient and can operate continuously.

lasersstimulated-emissionpopulation-inversion
11short7 marks

Define superconductivity and the critical temperature. Explain the Meissner effect and distinguish between Type I and Type II superconductors. The critical magnetic field of a superconductor at 0 K0\ \text{K} is 0.0640 T0.0640\ \text{T} and its critical temperature is 7.2 K7.2\ \text{K}. Using Hc(T)=Hc(0)[1(T/Tc)2]H_c(T) = H_c(0)\left[1 - (T/T_c)^2\right], find the critical field at 4.2 K4.2\ \text{K}.

Superconductivity is the phenomenon in which certain materials, cooled below a characteristic temperature, exhibit exactly zero electrical resistance and expel magnetic flux from their interior.

Critical temperature (TcT_c) is the temperature below which a material becomes superconducting; above TcT_c it behaves as a normal conductor.

Meissner effect. When a superconductor is cooled below TcT_c in a magnetic field, it expels the magnetic flux from its interior, becoming a perfect diamagnet (B=0B = 0 inside). This is a distinct property beyond mere zero resistance — it shows superconductivity is a true thermodynamic state, not just perfect conductivity.

Type I vs Type II.

Type IType II
Single critical field HcH_cTwo critical fields Hc1,Hc2H_{c1}, H_{c2}
Complete Meissner effect up to HcH_c, then abrupt lossComplete expulsion below Hc1H_{c1}; mixed (vortex) state between Hc1H_{c1} and Hc2H_{c2}
Soft, pure metals (Pb, Hg, Al)Alloys and compounds (Nb-Ti, Nb3_3Sn)
Low critical fieldsHigh critical fields, useful for magnets

Numerical part. Hc(0)=0.0640 TH_c(0) = 0.0640\ \text{T}, Tc=7.2 KT_c = 7.2\ \text{K}, T=4.2 KT = 4.2\ \text{K}.

TTc=4.27.2=0.5833,(TTc)2=0.3403\frac{T}{T_c} = \frac{4.2}{7.2} = 0.5833,\qquad \left(\frac{T}{T_c}\right)^2 = 0.3403 Hc(T)=0.0640[10.3403]=0.0640×0.6597=0.04222 TH_c(T) = 0.0640\,[1 - 0.3403] = 0.0640\times0.6597 = 0.04222\ \text{T}

Hc(4.2 K)0.0422 TH_c(4.2\ \text{K}) \approx 0.0422\ \text{T} (about 42.2 mT42.2\ \text{mT}).

superconductivitymeissner-effectcritical-field

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