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Section A: Long Answer Questions

Attempt all questions.

5 questions
1long10 marks

Derive the differential equation of a damped harmonic oscillator and obtain its general solution for the under-damped case. Define the relaxation time and quality factor.

A damped oscillator of mass m=0.20 kgm = 0.20\ \text{kg} has a spring constant k=80 N/mk = 80\ \text{N/m} and a damping constant b=0.40 kg/sb = 0.40\ \text{kg/s}. Calculate (i) the angular frequency of the damped oscillation, (ii) the time in which the amplitude falls to 1/e1/e of its initial value, and (iii) the quality factor of the oscillator.

Differential equation

A particle of mass mm acted on by a linear restoring force kx-kx and a velocity-proportional damping force bdxdt-b\dfrac{dx}{dt} obeys Newton's second law:

md2xdt2=kxbdxdtm\frac{d^2x}{dt^2} = -kx - b\frac{dx}{dt} d2xdt2+bmdxdt+kmx=0\frac{d^2x}{dt^2} + \frac{b}{m}\frac{dx}{dt} + \frac{k}{m}x = 0

Writing 2β=b/m2\beta = b/m (damping coefficient) 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

General solution

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}

For the under-damped case β<ω0\beta < \omega_0, let ω=ω02β2\omega = \sqrt{\omega_0^2 - \beta^2}:

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

The motion is oscillatory with an exponentially decaying amplitude A0eβtA_0 e^{-\beta t}.

Relaxation time τ=1/β\tau = 1/\beta: the time for the amplitude to fall to 1/e1/e of its value.

Quality factor Q=ω02β=ω0mbQ = \dfrac{\omega_0}{2\beta} = \dfrac{\omega_0 m}{b}: a measure of how lightly damped the oscillator is.

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 = \frac{b}{2m} = \frac{0.40}{2(0.20)} = 1.0\ \text{s}^{-1}

(i) Damped angular frequency:

ω=ω02β2=4001=399=19.975 rad/s19.97 rad/s\omega = \sqrt{\omega_0^2 - \beta^2} = \sqrt{400 - 1} = \sqrt{399} = 19.975\ \text{rad/s} \approx \mathbf{19.97\ rad/s}

(ii) Amplitude falls to 1/e1/e when eβt=e1e^{-\beta t}=e^{-1}, i.e. t=τ=1/βt = \tau = 1/\beta:

τ=11.0=1.0 s\tau = \frac{1}{1.0} = \mathbf{1.0\ s}

(iii) Quality factor:

Q=ω02β=202(1.0)=10Q = \frac{\omega_0}{2\beta} = \frac{20}{2(1.0)} = \mathbf{10}
oscillationsdamped-oscillationlcr-circuit
2long8 marks

Explain the formation of Newton's rings by reflected light and show that the radius of the nn-th dark ring is proportional to n\sqrt{n}. Why is the centre dark?

In a Newton's rings experiment the diameter of the 10th dark ring is 4.00 mm4.00\ \text{mm} and that of the 20th dark ring is 5.66 mm5.66\ \text{mm}. Light of wavelength 589 nm589\ \text{nm} is used. Determine the radius of curvature of the plano-convex lens.

Formation

A plano-convex lens of large radius of curvature RR rests on a flat glass plate, enclosing a thin air film whose thickness tt increases radially. Monochromatic light reflected from the top and bottom of the air film interferes. Because reflection at the lower (denser) surface introduces an extra phase of π\pi, the condition for dark rings is

2t=nλ(n=0,1,2,)2t = n\lambda \quad (n = 0,1,2,\dots)

For a sphere of radius RR, the film thickness at radius rr satisfies r2=2Rtr^2 = 2Rt (since tRt \ll R), so 2t=r2/R2t = r^2/R. Hence for the nn-th dark ring:

rn2R=nλ    rn=nRλn\frac{r_n^2}{R} = n\lambda \;\Rightarrow\; r_n = \sqrt{nR\lambda} \propto \sqrt{n}

Centre dark: at the point of contact t=0t=0, the only path difference is the λ/2\lambda/2 from reflection, giving destructive interference — so the centre is dark.

Numerical part

For dark rings the diameter satisfies Dn2=4nRλD_n^2 = 4nR\lambda. Using two rings eliminates uncertainty in the contact point:

Dn+p2Dn2=4pRλ    R=D202D1024(10)λD_{n+p}^2 - D_n^2 = 4pR\lambda \;\Rightarrow\; R = \frac{D_{20}^2 - D_{10}^2}{4(10)\lambda}

Data: D10=4.00 mmD_{10} = 4.00\ \text{mm}, D20=5.66 mmD_{20} = 5.66\ \text{mm}, λ=589×109 m\lambda = 589\times10^{-9}\ \text{m}.

D202=(5.66×103)2=3.2036×105 m2D_{20}^2 = (5.66\times10^{-3})^2 = 3.2036\times10^{-5}\ \text{m}^2 D102=(4.00×103)2=1.6000×105 m2D_{10}^2 = (4.00\times10^{-3})^2 = 1.6000\times10^{-5}\ \text{m}^2 D202D102=1.6036×105 m2D_{20}^2 - D_{10}^2 = 1.6036\times10^{-5}\ \text{m}^2 R=1.6036×10540×589×109=1.6036×1052.356×105=0.6806 mR = \frac{1.6036\times10^{-5}}{40 \times 589\times10^{-9}} = \frac{1.6036\times10^{-5}}{2.356\times10^{-5}} = 0.6806\ \text{m}

R0.68 mR \approx 0.68\ \text{m}.

physical-opticsinterferencenewtons-rings
3long8 marks

State Maxwell's equations in integral form and explain the physical meaning of each. Introduce the concept of displacement current and show that for a charging parallel-plate capacitor the displacement current equals the conduction current.

Maxwell's equations (integral form)

  1. Gauss's law (electricity): SEdA=Qencε0\displaystyle \oint_S \vec{E}\cdot d\vec{A} = \frac{Q_{enc}}{\varepsilon_0} — electric flux through a closed surface equals the enclosed charge over ε0\varepsilon_0; charges are sources of E\vec{E}.

  2. Gauss's law (magnetism): SBdA=0\displaystyle \oint_S \vec{B}\cdot d\vec{A} = 0 — net magnetic flux through any closed surface is zero; no magnetic monopoles.

  3. Faraday's law: CEdl=dΦBdt\displaystyle \oint_C \vec{E}\cdot d\vec{l} = -\frac{d\Phi_B}{dt} — a changing magnetic flux induces an electric field (emf).

  4. Ampère–Maxwell law: CBdl=μ0(Ic+ε0dΦEdt)\displaystyle \oint_C \vec{B}\cdot d\vec{l} = \mu_0\left(I_c + \varepsilon_0\frac{d\Phi_E}{dt}\right) — both conduction current and a changing electric flux (displacement current) produce a magnetic field.

Displacement current

Maxwell noted that Ampère's law Bdl=μ0Ic\oint \vec{B}\cdot d\vec{l} = \mu_0 I_c fails for a charging capacitor: choosing a surface that passes between the plates encloses no conduction current, yet B0\vec B \ne 0. He added the displacement current

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

Equality for a parallel-plate capacitor

Let plate area AA, charge QQ. The field between plates is E=σ/ε0=Q/(ε0A)E = \sigma/\varepsilon_0 = Q/(\varepsilon_0 A), so the electric flux is

ΦE=EA=Qε0\Phi_E = EA = \frac{Q}{\varepsilon_0}

Then the displacement current is

Id=ε0dΦEdt=ε01ε0dQdt=dQdt=IcI_d = \varepsilon_0 \frac{d\Phi_E}{dt} = \varepsilon_0 \cdot \frac{1}{\varepsilon_0}\frac{dQ}{dt} = \frac{dQ}{dt} = I_c

Thus the displacement current between the plates exactly equals the conduction current Ic=dQ/dtI_c = dQ/dt in the wire, restoring continuity of current and making Ampère's law consistent.

electromagnetismmaxwell-equationsdisplacement-current
4long8 marks

Set up the time-independent Schrödinger equation for a particle confined in a one-dimensional infinite potential well of width LL. Derive the expressions for the normalized wavefunctions and the energy eigenvalues.

For an electron confined in such a well of width L=0.20 nmL = 0.20\ \text{nm}, compute the energy of the ground state in electron-volts. (Take h=6.626×1034 J\cdotpsh = 6.626\times10^{-34}\ \text{J·s}, me=9.11×1031 kgm_e = 9.11\times10^{-31}\ \text{kg}.)

Set-up

Inside the well (0<x<L0 < x < L) the potential V=0V=0; outside it is infinite, forcing ψ=0\psi=0 there. The time-independent Schrödinger equation inside is

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

ψ(0)=0B=0\psi(0)=0 \Rightarrow B=0. ψ(L)=0sinkL=0kL=nπ\psi(L)=0 \Rightarrow \sin kL = 0 \Rightarrow kL = n\pi, n=1,2,3,n=1,2,3,\dots

So kn=nπ/Lk_n = n\pi/L.

Energy eigenvalues

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}

Normalized wavefunctions

Normalization 0LA2sin2(knx)dx=1\int_0^L A^2\sin^2(k_n x)\,dx = 1 gives A2(L/2)=1A^2 (L/2) = 1, so A=2/LA=\sqrt{2/L}:

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

Numerical part (ground state, n=1n=1)

L=0.20×109 m=2.0×1010 mL = 0.20\times10^{-9}\ \text{m} = 2.0\times10^{-10}\ \text{m}.

E1=h28mL2=(6.626×1034)28(9.11×1031)(2.0×1010)2E_1 = \frac{h^2}{8mL^2} = \frac{(6.626\times10^{-34})^2}{8(9.11\times10^{-31})(2.0\times10^{-10})^2}

Numerator: (6.626×1034)2=4.390×1067 J2s2(6.626\times10^{-34})^2 = 4.390\times10^{-67}\ \text{J}^2\text{s}^2.

Denominator: 8×9.11×1031×4.0×1020=2.915×10498 \times 9.11\times10^{-31} \times 4.0\times10^{-20} = 2.915\times10^{-49}.

E1=4.390×10672.915×1049=1.506×1018 JE_1 = \frac{4.390\times10^{-67}}{2.915\times10^{-49}} = 1.506\times10^{-18}\ \text{J}

Convert: E1=1.506×10181.602×1019=9.40 eVE_1 = \dfrac{1.506\times10^{-18}}{1.602\times10^{-19}} = \mathbf{9.40\ eV}.

quantum-mechanicsschrodinger-equationparticle-in-a-box
5long6 marks

Explain the principle of laser action with reference to stimulated emission, metastable states and population inversion. Distinguish between spontaneous and stimulated emission.

A step-index optical fibre has a core of refractive index 1.501.50 and cladding of refractive index 1.461.46. Calculate its numerical aperture and the acceptance angle (in air).

Laser action

An atom in an excited state can drop to a lower state by spontaneous emission (random, incoherent) or, when struck by a photon of matching energy, by stimulated emission, which produces a second photon identical in phase, direction, frequency and polarization. Light amplification requires more atoms in the upper than the lower level — a population inversion — which is impossible in a two-level system at equilibrium. A metastable state (long lifetime) lets atoms accumulate in the upper level so that stimulated emission dominates. An optical resonator (mirrors) feeds photons back, building a coherent, monochromatic, highly directional beam.

Spontaneous vs stimulated emission

PropertySpontaneousStimulated
Triggernone (random)incident photon
Phase/directionrandomidentical to incident photon
Coherenceincoherentcoherent
Role in lasernoise/seedamplification

Numerical part

Numerical aperture:

NA=n12n22=1.5021.462=2.252.1316=0.1184=0.3441\text{NA} = \sqrt{n_1^2 - n_2^2} = \sqrt{1.50^2 - 1.46^2} = \sqrt{2.25 - 2.1316} = \sqrt{0.1184} = 0.3441

NA 0.344\approx 0.344.

Acceptance angle (in air, n0=1n_0=1): sinθa=NA\sin\theta_a = \text{NA}, so

θa=sin1(0.3441)=20.1\theta_a = \sin^{-1}(0.3441) = \mathbf{20.1^{\circ}}
lasersfiber-opticspopulation-inversion
B

Section B: Short Answer Questions

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6 questions
6short8 marks

State Sabine's formula for reverberation time and explain each term. A hall of volume 2500 m32500\ \text{m}^3 has a total sound-absorbing surface giving an effective absorption of 400 m2400\ \text{m}^2 (in sabins, open-window units). Calculate its reverberation time. If 90 m290\ \text{m}^2 sabin of extra absorption is added (acoustic tiles), find the new reverberation time.

Sabine's formula

T=0.161VA=0.161VaiSiT = \frac{0.161\,V}{A} = \frac{0.161\,V}{\sum a_i S_i}

where TT = reverberation time (s) — the time for sound intensity to fall to 10610^{-6} of its initial value (a 60 dB drop); VV = volume of the hall (m³); A=aiSiA = \sum a_i S_i = total absorption (m² sabin), with aia_i the absorption coefficient and SiS_i the area of each surface; the constant 0.161 s/m0.161\ \text{s/m} follows from the speed of sound.

Calculation

V=2500 m3V = 2500\ \text{m}^3, A=400 m2A = 400\ \text{m}^2 sabin.

T=0.161×2500400=402.5400=1.006 sT = \frac{0.161 \times 2500}{400} = \frac{402.5}{400} = 1.006\ \text{s}

T1.01 sT \approx 1.01\ \text{s}.

With extra absorption

New total absorption A=400+90=490 m2A' = 400 + 90 = 490\ \text{m}^2 sabin.

T=0.161×2500490=402.5490=0.8214 sT' = \frac{0.161 \times 2500}{490} = \frac{402.5}{490} = 0.8214\ \text{s}

T0.82 sT' \approx 0.82\ \text{s} — the added absorption shortens the reverberation time, improving clarity.

acousticsreverberationsabine-formula
7short6 marks

What is a plane diffraction grating? Write the grating equation. A grating has 5000 lines per cm5000\ \text{lines per cm}. Find the angle of the first-order maximum for light of wavelength 600 nm600\ \text{nm} incident normally.

Diffraction grating

A plane diffraction grating is an optical element with a large number of equally spaced parallel slits (or lines) of period dd. When light passes through, the diffracted beams interfere, producing sharp principal maxima where

dsinθ=nλ(n=0,1,2,)d\sin\theta = n\lambda \quad (n = 0, 1, 2, \dots)

Here dd is the grating element (slit separation), θ\theta the diffraction angle and nn the order.

Calculation

Grating constant:

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=600×109 m\lambda = 600\times10^{-9}\ \text{m}:

sinθ=nλd=1×600×1092.0×106=0.300\sin\theta = \frac{n\lambda}{d} = \frac{1 \times 600\times10^{-9}}{2.0\times10^{-6}} = 0.300 θ=sin1(0.300)=17.46\theta = \sin^{-1}(0.300) = \mathbf{17.46^{\circ}}
physical-opticsdiffractiondiffraction-grating
8short6 marks

Using Gauss's law, derive the expression for the electric field at a distance rr from an infinitely long straight wire carrying a uniform linear charge density λ\lambda. A long wire carries λ=4.0×108 C/m\lambda = 4.0\times10^{-8}\ \text{C/m}. Find the electric field at a point 0.20 m0.20\ \text{m} from the wire.

Derivation

By symmetry the field E\vec E is radial and uniform on a coaxial Gaussian cylinder of radius rr and length \ell. Flux through the curved surface only (ends contribute zero):

EdA=E(2πr)\oint \vec E\cdot d\vec A = E\,(2\pi r\,\ell)

Enclosed charge Qenc=λQ_{enc} = \lambda\ell. Gauss's law EdA=Qenc/ε0\oint\vec E\cdot d\vec A = Q_{enc}/\varepsilon_0 gives

E(2πr)=λε0    E=λ2πε0rE\,(2\pi r\ell) = \frac{\lambda\ell}{\varepsilon_0} \;\Rightarrow\; \boxed{E = \frac{\lambda}{2\pi\varepsilon_0 r}}

Calculation

λ=4.0×108 C/m\lambda = 4.0\times10^{-8}\ \text{C/m}, r=0.20 mr = 0.20\ \text{m}, 12πε0=2k=1.798×1010 N\cdotpm2/C2\dfrac{1}{2\pi\varepsilon_0} = 2k = 1.798\times10^{10}\ \text{N·m}^2/\text{C}^2 (using k=8.99×109k = 8.99\times10^9).

E=2kλr=2(8.99×109)(4.0×108)0.20=719.20.20=3596 N/CE = \frac{2k\lambda}{r} = \frac{2(8.99\times10^9)(4.0\times10^{-8})}{0.20} = \frac{719.2}{0.20} = 3596\ \text{N/C}

E3.6×103 N/CE \approx 3.6\times10^{3}\ \text{N/C}, directed radially outward.

electrostaticsgauss-lawelectric-field
9short6 marks

Define the Poynting vector and state what it represents. A plane electromagnetic wave in vacuum has a peak electric field amplitude E0=50 V/mE_0 = 50\ \text{V/m}. Calculate (i) the peak magnetic field amplitude and (ii) the average intensity (time-averaged Poynting vector magnitude) of the wave.

Poynting vector

S=1μ0E×B\vec S = \frac{1}{\mu_0}\,\vec E\times\vec B

It gives the instantaneous rate of energy flow per unit area (W/m²) carried by the electromagnetic field, directed along the propagation of the wave. Its time average is the wave intensity.

Calculation

(i) In vacuum E0=cB0E_0 = cB_0, so

B0=E0c=503.0×108=1.667×107 T1.67×107 TB_0 = \frac{E_0}{c} = \frac{50}{3.0\times10^8} = 1.667\times10^{-7}\ \text{T} \approx \mathbf{1.67\times10^{-7}\ T}

(ii) Average intensity:

I=S=12cε0E02I = \langle S\rangle = \frac{1}{2}\,c\,\varepsilon_0 E_0^2 I=12(3.0×108)(8.85×1012)(50)2I = \frac{1}{2}(3.0\times10^8)(8.85\times10^{-12})(50)^2 =12(3.0×108)(8.85×1012)(2500)= \frac{1}{2}(3.0\times10^8)(8.85\times10^{-12})(2500)

Step: 3.0×108×8.85×1012=2.655×1033.0\times10^8 \times 8.85\times10^{-12} = 2.655\times10^{-3}. Then ×2500=6.6375\times 2500 = 6.6375. Half: 3.3193.319.

I3.32 W/m2I \approx 3.32\ \text{W/m}^2.

em-wavespoynting-vectorelectromagnetic-radiation
10short7 marks

Explain the Hall effect and write the expression for the Hall coefficient. A semiconductor strip of thickness 1.0 mm1.0\ \text{mm} carries a current of 3.0 A3.0\ \text{A} in a magnetic field of 0.50 T0.50\ \text{T} perpendicular to the strip, producing a Hall voltage of 6.0 mV6.0\ \text{mV}. Calculate (i) the Hall coefficient and (ii) the charge-carrier concentration nn.

Hall effect

When a current-carrying conductor is placed in a magnetic field perpendicular to the current, the moving charge carriers experience a Lorentz force qv×Bq\vec v\times\vec B that pushes them to one side. Charge accumulates until the transverse electric field balances the magnetic force, producing a measurable Hall voltage VHV_H across the width. Its sign reveals the carrier type (n- or p-).

The Hall coefficient is

RH=1nq=VHtIBR_H = \frac{1}{nq} = \frac{V_H\,t}{I\,B}

where tt is the thickness along B\vec B, II the current and BB the field.

Calculation

VH=6.0×103 VV_H = 6.0\times10^{-3}\ \text{V}, t=1.0×103 mt = 1.0\times10^{-3}\ \text{m}, I=3.0 AI = 3.0\ \text{A}, B=0.50 TB = 0.50\ \text{T}.

(i)

RH=VHtIB=(6.0×103)(1.0×103)(3.0)(0.50)=6.0×1061.5=4.0×106 m3/CR_H = \frac{V_H\,t}{I\,B} = \frac{(6.0\times10^{-3})(1.0\times10^{-3})}{(3.0)(0.50)} = \frac{6.0\times10^{-6}}{1.5} = 4.0\times10^{-6}\ \text{m}^3/\text{C}

RH=4.0×106 m3/CR_H = 4.0\times10^{-6}\ \text{m}^3/\text{C}.

(ii) From RH=1/(nq)R_H = 1/(nq) with q=1.602×1019 Cq = 1.602\times10^{-19}\ \text{C}:

n=1RHq=1(4.0×106)(1.602×1019)=16.408×1025=1.56×1024 m3n = \frac{1}{R_H\,q} = \frac{1}{(4.0\times10^{-6})(1.602\times10^{-19})} = \frac{1}{6.408\times10^{-25}} = 1.56\times10^{24}\ \text{m}^{-3}

n1.56×1024 m3n \approx 1.56\times10^{24}\ \text{m}^{-3}.

semiconductorshall-effectcharge-carriers
11short7 marks

What is superconductivity? Explain the Meissner effect and distinguish between Type-I and Type-II superconductors. The critical magnetic field of a superconductor is 0.030 T0.030\ \text{T} at 0 K0\ \text{K} and its critical temperature is 7.0 K7.0\ \text{K}. Estimate (i) the critical field at 3.0 K3.0\ \text{K} and (ii) the temperature at which the critical field falls to half of its 0 K0\ \text{K} value.

Superconductivity and the Meissner effect

Superconductivity is the complete loss of electrical resistance in certain materials below a critical temperature TcT_c. The Meissner effect is the expulsion of magnetic flux from the interior of a superconductor as it is cooled below TcT_c: the material becomes a perfect diamagnet (B=0B = 0 inside), which is a stronger condition than mere zero resistance.

Type-I vs Type-II

Type-IType-II
Magnetic behavioursingle critical field HcH_c, abrupt transitiontwo critical fields Hc1,Hc2H_{c1}, H_{c2}
Intermediate statenonemixed (vortex) state between Hc1H_{c1} and Hc2H_{c2}
Examplespure metals (Hg, Pb)alloys, Nb-Ti, ceramics

Calculation

The critical field varies with temperature as

Hc(T)=Hc(0)[1(TTc)2]H_c(T) = H_c(0)\left[1 - \left(\frac{T}{T_c}\right)^2\right]

With Hc(0)=0.030 TH_c(0) = 0.030\ \text{T}, T=3.0 KT = 3.0\ \text{K}, Tc=7.0 KT_c = 7.0\ \text{K}:

(TTc)2=(3.07.0)2=(0.4286)2=0.1837\left(\frac{T}{T_c}\right)^2 = \left(\frac{3.0}{7.0}\right)^2 = (0.4286)^2 = 0.1837 Hc(3.0)=0.030(10.1837)=0.030×0.8163=0.02449 TH_c(3.0) = 0.030\,(1 - 0.1837) = 0.030 \times 0.8163 = 0.02449\ \text{T}

(i) Hc(3.0 K)0.0245 TH_c(3.0\ \text{K}) \approx 0.0245\ \text{T}.

(ii) Setting Hc(T)=12Hc(0)H_c(T) = \tfrac{1}{2}H_c(0):

1(TTc)2=0.5    TTc=0.5=0.70711 - \left(\frac{T}{T_c}\right)^2 = 0.5 \;\Rightarrow\; \frac{T}{T_c} = \sqrt{0.5} = 0.7071 T=0.7071×7.0=4.95 KT = 0.7071 \times 7.0 = 4.95\ \text{K}

T4.95 KT \approx 4.95\ \text{K}.

superconductivitymeissner-effectcritical-field

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