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Chapter 5

Optics, Modern Physics and Electronics

TU BBS past exam questions

Past questions and answers

37 questions set from this chapter, 2 of them more than once. Most repeated first.

  • Asked 2 times
  • 2082 · PHY. 201 (New Course) · 8 marks
  • 2081 · PHY. 201 · 8 marks

How can diffraction patterns be obtained through a single and double slit? Discuss difference between single and double slit diffractions.

Answer

Single slit. Monochromatic light of wavelength λ\lambda falls on a narrow slit of width aa, and a screen is placed at distance DD. Every point of the slit acts as a secondary source (Huygens' principle), and the wavelets from different parts of the same slit interfere. For an angle θ\theta, the waves from the two edges differ in path by asin⁡θa\sin\theta.

  • Minima (dark): asin⁡θ=nλ,  n=±1,±2,…a\sin\theta = n\lambda,\; n=\pm1,\pm2,\dots
  • Secondary maxima (approximately): asin⁡θ=(2n+1)λ2,  n=±1,±2,…a\sin\theta = (2n+1)\dfrac{\lambda}{2},\; n=\pm1,\pm2,\dots
  • The central maximum at θ=0\theta=0 is the brightest and widest, with width 2λD/a2\lambda D/a. The secondary maxima are much weaker and are half as wide.

Double slit. Light falls on two parallel narrow slits, each of width aa and separated by dd (centre to centre). Each slit diffracts the light, and the two diffracted beams then overlap and interfere. The pattern is a set of interference fringes under the single-slit diffraction envelope.

  • Bright fringes: dsin⁡θ=nλ,  n=0,±1,±2,…d\sin\theta = n\lambda,\; n=0,\pm1,\pm2,\dots
  • Dark fringes: dsin⁡θ=(2n+1)λ2d\sin\theta = (2n+1)\dfrac{\lambda}{2}
  • Fringe width: β=λDd\beta = \dfrac{\lambda D}{d}, the same for all fringes.
  • If an interference maximum falls at a diffraction minimum, that order is missing. This happens when d/a=n/md/a = n/m for integers nn and mm.

Difference between single-slit and double-slit patterns

BasisSingle slitDouble slit
CauseDiffraction only (interference of wavelets from one slit)Diffraction at each slit together with interference between the two slits
IntensityCentral maximum is very bright and the secondary maxima fall off rapidlyMany fringes of nearly equal intensity, modulated by the diffraction envelope
Central bandCentral maximum is twice as wide as the othersAll bright fringes have the same width λD/d\lambda D/d
Width of patternDepends on slit width aa (narrower slit gives a wider pattern)Fringe spacing depends on slit separation dd
Minima conditionasin⁡θ=nλa\sin\theta = n\lambdadsin⁡θ=(2n+1)λ/2d\sin\theta = (2n+1)\lambda/2
Maxima conditionApproximately asin⁡θ=(2n+1)λ/2a\sin\theta=(2n+1)\lambda/2dsin⁡θ=nλd\sin\theta = n\lambda
Missing ordersNoneSome orders may be missing when d/a=n/md/a = n/m

Answer checked by Claude Sonnet · Oct 21, 2026

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  • Asked 2 times
  • 2082 · PHY. 201 (New Course) · 5 marks
  • 2081 · PHY. 201 · 5 marks

Convert 111001 and 110101 into their decimal number & add them.

Answer

Binary 111001 to decimal

1110012=1×32+1×16+1×8+0×4+0×2+1×1=57111001_2 = 1\times32 + 1\times16 + 1\times8 + 0\times4 + 0\times2 + 1\times1 = 57

Binary 110101 to decimal

1101012=1×32+1×16+0×8+1×4+0×2+1×1=53110101_2 = 1\times32 + 1\times16 + 0\times8 + 1\times4 + 0\times2 + 1\times1 = 53

Sum

57+53=11057 + 53 = 110

Check by adding in binary: 1110012+1101012=11011102=64+32+8+4+2=110111001_2 + 110101_2 = 1101110_2 = 64+32+8+4+2 = 110.

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 10 marks

Interference pattern can be obtained by either the division of amplitude or the division of wave front of the source. Describe it. Also explain spatial and temporal coherence.
OR
Describe the working of a plane transmission grating with necessary theory. Also discuss how the number of diffraction maxima can be known from it. Define and write down expression for its resolving power.

Answer

Interference by division of wavefront and division of amplitude

Interference needs two coherent sources. Since independent sources are incoherent, coherent beams are obtained from a single source in two ways.

1. Division of wavefront: The wavefront from a narrow source is divided into two parts by slits, mirrors or prisms, and the parts are superposed. Both parts come from the same wavefront, so they stay coherent. The source must be small (a point or narrow slit).

  • Examples: Young's double slit, Fresnel's biprism, Lloyd's mirror.
  • Fringes are usually equally spaced, e.g. β=λDd\beta = \dfrac{\lambda D}{d} in Young's experiment.

2. Division of amplitude: A beam is divided into a reflected and a transmitted part by partial reflection at a surface; the amplitude (intensity) is shared and the parts are later recombined. An extended source can be used.

  • Examples: thin films, wedge fringes, Newton's rings, Michelson interferometer.
  • Path difference in a thin film (reflected light): 2μtcos⁡r=(2n+1)λ22\mu t\cos r = (2n+1)\dfrac{\lambda}{2} for maxima.

Coherence

Temporal coherence is the correlation of phase of the wave at the same point at different times. It depends on the spectral purity (bandwidth Δν\Delta\nu) of the source. A wave train lasts for a coherence time τc≈1/Δν\tau_c \approx 1/\Delta\nu, giving the coherence length Lc=c τc=λ2ΔλL_c = c\,\tau_c = \frac{\lambda^2}{\Delta\lambda} Fringes are visible only if the path difference is less than LcL_c.

Spatial coherence is the correlation of phase at different points of the wavefront at the same instant. It depends on the size of the source. For a source of angular size θ\theta, the transverse coherence length is lc≈λθl_c \approx \frac{\lambda}{\theta} Fringes are sharp only when the two slits lie within this width.

A laser has both high temporal and high spatial coherence; a sodium lamp has good spatial coherence only when a narrow slit is used.


OR

Plane transmission grating

A plane transmission grating is a large number NN of equal, parallel, equidistant slits ruled on a glass plate, each of width aa and separated by opaque width bb. (a+b)(a+b) is the grating element (grating constant), a+b=1/(lines per metre)a+b = 1/(\text{lines per metre}).

Theory: Monochromatic parallel light falls normally on the grating. Light diffracted at angle θ\theta from corresponding points of adjacent slits has path difference (a+b)sin⁡θ(a+b)\sin\theta. The diffracted waves from all slits are in phase (principal maxima) when (a+b)sin⁡θ=nλ,n=0,1,2,…(a+b)\sin\theta = n\lambda, \quad n = 0, 1, 2, \dots This is the grating equation; nn is the order. The intensity distribution is I=I0(sin⁡αα)2(sin⁡Nβsin⁡β)2,α=πasin⁡θλ, β=π(a+b)sin⁡θλI = I_0\left(\frac{\sin\alpha}{\alpha}\right)^2\left(\frac{\sin N\beta}{\sin\beta}\right)^2,\quad \alpha=\frac{\pi a\sin\theta}{\lambda},\ \beta=\frac{\pi(a+b)\sin\theta}{\lambda}

  • Principal maxima at β=nπ\beta = n\pi, i.e. the grating equation.
  • Minima at Nβ=mπN\beta = m\pi (m≠0,N,2N,…m\ne 0, N, 2N,\dots), i.e. (a+b)sin⁡θ=mNλ(a+b)\sin\theta = \dfrac{m}{N}\lambda.
  • Between two principal maxima there are (N−1)(N-1) minima and (N−2)(N-2) weak secondary maxima.
  • With white light, the central maximum is white and higher orders are spectra (violet nearest the centre).

Maximum number of orders: Since sin⁡θ≤1\sin\theta \le 1, nmax≤a+bλn_{max} \le \frac{a+b}{\lambda} nmaxn_{max} is the largest integer not exceeding (a+b)/λ(a+b)/\lambda. Maxima occur on both sides of the centre, so the total number of maxima is 2nmax+12n_{max}+1. (Example: 6000 lines/cm and λ=5890\lambda = 5890 Å: a+b=1.667×10−6a+b = 1.667\times10^{-6} m, (a+b)/λ=2.83(a+b)/\lambda = 2.83, so nmax=2n_{max}=2 and 5 maxima are seen.)

Resolving power: The resolving power of a grating is its ability to separate two close spectral lines of wavelengths λ\lambda and λ+dλ\lambda + d\lambda: R=λdλR = \frac{\lambda}{d\lambda} By Rayleigh's criterion, the nnth maximum of λ+dλ\lambda+d\lambda falls on the first minimum next to the nnth maximum of λ\lambda: n(λ+dλ)=(n+1N)λ  ⇒  n dλ=λNn(\lambda + d\lambda) = \left(n + \frac1N\right)\lambda \;\Rightarrow\; n\,d\lambda = \frac{\lambda}{N} R=λdλ=nN\boxed{R = \frac{\lambda}{d\lambda} = nN} Resolving power is proportional to the order nn and the total number of rulings NN illuminated.

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 10 marks

Describe Frank-Hertz experiment and discuss the advantages and limitations of Bohr's model. How Schrodinger modified Bohr's model? Explain.
OR
Compare and contrast the fine structures of hydrogen and helium.

Answer

Frank-Hertz Experiment, Bohr's Model and Schrödinger's Modification

1. Frank-Hertz Experiment

The Frank-Hertz experiment (1914) gave direct experimental proof of the quantisation of atomic energy levels, confirming Bohr's postulates.

Apparatus: A glass tube containing mercury vapour at low pressure, a heated filament (cathode) F, a grid G (accelerating electrode) and a plate P (collector). A small retarding potential VrV_r (about 0.5 V) is applied between G and P.

Working:

  • Electrons emitted thermionically from F are accelerated by the potential VV between F and G.
  • Electrons passing through the grid reach P only if they still have enough energy to overcome VrV_r. The plate current IpI_p is measured as a function of VV.

Observation: The current rises, then falls sharply at V=4.9V = 4.9 V, rises again, falls at 9.89.8 V, and so on: peaks repeat at intervals of 4.9 V.

Explanation: At V=4.9V = 4.9 V an electron has kinetic energy

E=eV=1.6×10−19×4.9=7.84×10−19 J≈4.9 eVE = eV = 1.6\times10^{-19}\times 4.9 = 7.84\times10^{-19}\ \text{J} \approx 4.9\ \text{eV}

This equals the energy needed to raise a mercury atom from the ground state to its first excited state. The electron loses almost all its energy in an inelastic collision and cannot overcome the retarding potential, so the current drops. The excited atom returns to the ground state emitting a photon of wavelength

λ=hcE=124004.9≈2530 A˚\lambda = \frac{hc}{E} = \frac{12400}{4.9} \approx 2530\ \text{Å}

which agrees with the mercury ultraviolet line at 2537 Å (energy 4.886 eV). The same process repeats at 2×4.9=9.82\times4.9 = 9.8 V, etc.

Conclusion: Atoms absorb energy only in discrete quanta, confirming stationary energy levels.


2. Advantages of Bohr's Model

  1. Explains the hydrogen spectrum: gives 1λ=R(1n12−1n22)\dfrac{1}{\lambda} = R\left(\dfrac{1}{n_1^2}-\dfrac{1}{n_2^2}\right) and predicts the Lyman, Balmer, Paschen, Brackett and Pfund series.
  2. Explains the stability of the atom: electrons in stationary orbits do not radiate.
  3. Introduces quantisation: mvr=nℏmvr = n\hbar and En=−13.6/n2E_n = -13.6/n^2 eV.
  4. Explains ionisation and excitation potentials of hydrogen and hydrogen-like ions (He⁺, Li²⁺).
  5. Gives the correct Rydberg constant and Bohr radius a0=0.529a_0 = 0.529 Å.
  6. Explains the Frank-Hertz results and Moseley's X-ray law qualitatively.

3. Limitations of Bohr's Model

  1. Works only for one-electron atoms; fails for helium and heavier atoms.
  2. Cannot explain fine structure (needs spin and relativistic corrections).
  3. Cannot explain the Zeeman effect or the Stark effect.
  4. Cannot explain molecular spectra or chemical bonding.
  5. Violates the uncertainty principle by assigning a definite orbit (exact rr and pp).
  6. Mixes classical and quantum ideas; gives no reason why only certain orbits are allowed.
  7. Cannot explain relative intensities of lines or selection rules.
  8. Does not include electron spin or the Pauli exclusion principle.

4. How Schrödinger Modified Bohr's Model

Schrödinger (1926) replaced Bohr's definite orbits with probability distributions (wave mechanics). The electron is described by a wave function ψ(x,y,z,t)\psi(x,y,z,t) satisfying

−ℏ22m∇2ψ+Vψ=iℏ∂ψ∂t-\frac{\hbar^2}{2m}\nabla^2\psi + V\psi = i\hbar\frac{\partial\psi}{\partial t}

For a stationary state, ψ=ψ0e−iEt/ℏ\psi = \psi_0 e^{-iEt/\hbar}, giving the time-independent equation

∇2ψ+2mℏ2(E−V)ψ=0\nabla^2\psi + \frac{2m}{\hbar^2}(E-V)\psi = 0

Bohr's modelSchrödinger's model
Definite circular orbitsProbability clouds / orbitals
mvr=nℏmvr = n\hbar imposed as a postulateQuantisation arises naturally from boundary conditions on ψ\psi
One quantum number nnThree quantum numbers n,l,mln, l, m_l (four with spin)
Gives only energyGives energy, angular momentum and its orientation
Fails for multi-electron atomsApplicable to all atoms and molecules

Results:

  1. Energy of hydrogen: En=−13.6n2E_n = -\dfrac{13.6}{n^2} eV, the same as Bohr's, so the hydrogen spectrum is reproduced.
  2. Angular momentum: L=l(l+1) ℏL = \sqrt{l(l+1)}\,\hbar, l=0,1,…,(n−1)l = 0,1,\dots,(n-1), different from Bohr's nℏn\hbar.
  3. Magnetic quantum number: ml=−l,…,+lm_l = -l,\dots,+l explains the Zeeman effect and space quantisation.
  4. Electron spin: ms=±12m_s = \pm\tfrac12 (Uhlenbeck and Goudsmit) explains fine structure and the Stern-Gerlach experiment.
  5. Probability density: ∣ψ∣2dV|\psi|^2 dV is the probability of finding the electron in dVdV; the radial probability of the ground state peaks at r=a0r = a_0, recovering Bohr's radius as the most probable distance.
  6. Selection rules Δl=±1\Delta l = \pm1, Δml=0,±1\Delta m_l = 0,\pm1 follow from the mathematics.
  7. The Pauli exclusion principle and electron configurations of multi-electron atoms follow naturally.

Conclusion: Bohr's model is a limiting case of Schrödinger's theory for large nn (correspondence principle).


OR

Fine Structure of Hydrogen and Helium: Comparison

Fine structure is the splitting of a spectral line into closely spaced components due to spin-orbit coupling and the relativistic correction to the electron mass.

Hydrogen

  • System: one electron, one proton. In simple Bohr theory the energy depends only on nn.
  • Corrections: relativistic mass correction + spin-orbit interaction + Darwin term.
  • Result: levels of the same nn but different jj split:

En,j=−13.6n2[1+α2n2(nj+12−34)] eVE_{n,j} = -\frac{13.6}{n^2}\left[1 + \frac{\alpha^2}{n^2}\left(\frac{n}{j+\tfrac12} - \frac{3}{4}\right)\right]\text{ eV}

where α=e24πε0ℏc≈1137\alpha = \dfrac{e^2}{4\pi\varepsilon_0\hbar c} \approx \dfrac{1}{137} is the fine structure constant.

  • States with the same nn and jj but different ll stay degenerate (e.g. 2s1/22s_{1/2} and 2p1/22p_{1/2}); only the Lamb shift lifts this slightly.
  • Scale: splitting ∼α2En\sim \alpha^2 E_n, of the order of 10−410^{-4} eV.

Helium

  • System: two electrons, one nucleus. Spin-orbit coupling and electron-electron (exchange) interaction both contribute.
  • Two systems: parahelium (spins antiparallel, S=0S=0, singlet) and orthohelium (spins parallel, S=1S=1, triplet). Transitions between them (intercombination lines) are very weak.
  • Result: separate singlet and triplet series; triplet levels show three-component fine structure.
  • Scale: exchange splittings are much larger, of the order of 10−210^{-2} to 10−110^{-1} eV, while the true spin-orbit fine structure is small.

Comparison

FeatureHydrogenHelium
Electrons12
Cause of fine structureSpin-orbit + relativistic correctionSpin-orbit + electron-electron exchange
Spin statesDoublet (S=12S=\tfrac12)Singlet (S=0S=0) and triplet (S=1S=1)
Spectral seriesLyman, Balmer, ... each with fine componentsSeparate singlet and triplet series
Selection rulesΔl=±1\Delta l=\pm1, Δj=0,±1\Delta j=0,\pm1Also ΔS=0\Delta S=0
Degeneracy2s1/22s_{1/2}, 2p1/22p_{1/2} degenerateLevels of different ll well separated
Magnitude of splitting∼10−4\sim10^{-4} eVup to 10−210^{-2}-10−110^{-1} eV
TheoryExactly solvable (Dirac equation)Needs approximation (perturbation, Hartree-Fock)

Conclusion: Both show fine structure due to spin-orbit coupling, but in hydrogen it is a small correction to a one-electron problem, while in helium electron-electron interaction dominates and produces two distinct term systems.

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 10 marks

Explain current gain in common emitter, common base and common collector configuration. Establish the relation between α\alpha and β\beta for dc where α\alpha and β\beta have their usual meaning.
OR
Discuss working of inverting and non-inverting mode of Operational Amplifier. Explain the terms differential and common mode gain.

Answer

Current Gain in CE, CB and CC Configurations

Common Emitter (CE) Configuration

In CE configuration, the emitter is common to input and output, input is applied between base and emitter, and output is taken between collector and emitter. The current gain is the ratio of collector current to base current at constant collector-emitter voltage:

β=ICIB∣VCE\beta = \frac{I_C}{I_B}\Big|_{V_{CE}}

Since ICI_C is much larger than IBI_B (typically β≈20\beta \approx 20–500500), CE gives high current gain and also high voltage and power gain. It is the most widely used configuration.

Common Base (CB) Configuration

Here the base is common, input is applied between emitter and base, and output is taken between collector and base. The current gain is the ratio of collector current to emitter current at constant collector-base voltage:

α=ICIE∣VCB\alpha = \frac{I_C}{I_E}\Big|_{V_{CB}}

Since ICI_C is slightly less than IEI_E (some current is lost as base current), α\alpha is less than unity (typically 0.950.95–0.990.99). Hence CB gives no current gain but high voltage gain.

Common Collector (CC) Configuration

Here the collector is common, input is applied between base and collector, and output is taken between emitter and collector. The current gain is the ratio of emitter current to base current at constant collector-emitter voltage:

γ=IEIB∣VCE\gamma = \frac{I_E}{I_B}\Big|_{V_{CE}}

Since IE≈ICI_E \approx I_C and IBI_B is small, γ\gamma is very high (slightly greater than β\beta), so CC gives high current gain but voltage gain less than unity. It is used as a buffer (emitter follower).

Relation between α\alpha and β\beta

By Kirchhoff's current law in the transistor,

IE=IC+IB...(1)I_E = I_C + I_B \quad \text{...(1)}

Step 1. Divide (1) by ICI_C:

IEIC=1+IBIC\frac{I_E}{I_C} = 1 + \frac{I_B}{I_C}

1α=1+1β=β+1β\frac{1}{\alpha} = 1 + \frac{1}{\beta} = \frac{\beta + 1}{\beta}

Step 2. Inverting,

α=ββ+1\boxed{\alpha = \frac{\beta}{\beta + 1}}

Step 3. From (1), divide by IBI_B:

IEIB=ICIB+1  ⇒  γ=β+1\frac{I_E}{I_B} = \frac{I_C}{I_B} + 1 \;\Rightarrow\; \gamma = \beta + 1

Also, from α=ββ+1\alpha = \dfrac{\beta}{\beta+1},

α(β+1)=β  ⇒  αβ+α=β  ⇒  β(1−α)=α\alpha(\beta + 1) = \beta \;\Rightarrow\; \alpha\beta + \alpha = \beta \;\Rightarrow\; \beta(1-\alpha) = \alpha

β=α1−α\boxed{\beta = \frac{\alpha}{1-\alpha}}

Since α<1\alpha < 1, the denominator (1−α)(1-\alpha) is small, so β\beta is large. For example, if α=0.98\alpha = 0.98, then β=0.98/0.02=49\beta = 0.98/0.02 = 49.


OR

Inverting and Non-inverting Modes of an Operational Amplifier

An operational amplifier (op-amp) is a high-gain, direct-coupled differential amplifier. Its output is given by

Vo=AOL(V2−V1)V_o = A_{OL}(V_2 - V_1)

where V1V_1 is the voltage at the inverting (−-) input, V2V_2 at the non-inverting (++) input, and AOLA_{OL} is the open-loop gain. By connecting external resistors, two useful modes are obtained.

(a) Inverting Mode

The input signal is applied to the inverting input through R1R_1, while the non-inverting input is grounded. A feedback resistor RfR_f connects the output back to the inverting input. The inverting input is a virtual ground (V1≈V2=0V_1 \approx V_2 = 0).

Current through R1R_1: I1=VinR1I_1 = \dfrac{V_{in}}{R_1}

Since no current enters the ideal op-amp input, the same current flows through RfR_f:

If=I1  ⇒  0−VoRf=VinR1I_f = I_1 \;\Rightarrow\; \frac{0 - V_o}{R_f} = \frac{V_{in}}{R_1}

Vo=−RfR1 Vin\boxed{V_o = -\frac{R_f}{R_1}\,V_{in}}

The output is 180° out of phase with the input, and the voltage gain Av=−Rf/R1A_v = -R_f/R_1 depends only on external resistors.

(b) Non-inverting Mode

The input signal is applied to the non-inverting input, and R1R_1 is connected from the inverting input to ground with RfR_f from output to inverting input. Since V1=V2=VinV_1 = V_2 = V_{in} and the same current flows through R1R_1 and RfR_f:

Vo−VinRf=VinR1\frac{V_o - V_{in}}{R_f} = \frac{V_{in}}{R_1}

Vo=Vin(1+RfR1)V_o = V_{in}\left(1 + \frac{R_f}{R_1}\right)

Vo=(1+RfR1)Vin\boxed{V_o = \left(1 + \frac{R_f}{R_1}\right)V_{in}}

The output is in phase with the input, and the gain is always greater than unity. If Rf=0R_f = 0 and R1=∞R_1 = \infty, the gain becomes 1, giving the voltage follower.

Differential Mode Gain

When equal and opposite signals are applied to the two inputs (V1=−V2=Vd/2V_1 = -V_2 = V_d/2), the output is

Vo=Ad Vd,Ad=VoVdV_o = A_d\,V_d, \qquad A_d = \frac{V_o}{V_d}

AdA_d is the differential gain — the amplification of the difference signal. For an ideal op-amp, Ad→∞A_d \to \infty; practically it is very large (∼105\sim 10^5).

Common Mode Gain

When the same signal is applied to both inputs (V1=V2=VcV_1 = V_2 = V_c), the output should ideally be zero. In practice a small output appears:

Vo=Ac VcV_o = A_c\,V_c

AcA_c is the common mode gain, which is very small. The quality of an op-amp is measured by the Common Mode Rejection Ratio:

CMRR=AdAc\text{CMRR} = \frac{A_d}{A_c}

For an ideal op-amp, Ac=0A_c = 0 and CMRR =∞= \infty; practically CMRR is very high (about 10510^5), meaning the op-amp amplifies difference signals but rejects signals common to both inputs.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 8 marks

Explain with outline sketches and examples, the concepts of double refraction, ordinary and extraordinary rays. Also describe the working principle of a Nicol prism.

Answer

Double Refraction

When a ray of light enters certain crystals (calcite, quartz, tourmaline, etc.), it splits into two refracted rays that travel with different speeds and are plane-polarised in mutually perpendicular planes. This phenomenon is called double refraction or birefringence.

Outline sketch:

                 Incident ray
                      |
                      |  (unpolarised)
        ──────────────┼──────────────  ← crystal surface
             O ray  ↙      ↘  E ray
          (obeys      (does not obey
           Snell's)    Snell's law)

The two rays are:

PropertyOrdinary ray (O-ray)Extraordinary ray (E-ray)
Refractive indexSame in all directionsVaries with direction
Snell's lawObeyedNot obeyed
Speed in crystalSame in all directionsDepends on direction
PolarisationPlane-polarisedPlane-polarised
Vibration planePerpendicular to principal sectionParallel to principal section

The principal section is any plane containing the optic axis and the direction of the incident ray. The O-ray vibrates perpendicular to this section, while the E-ray vibrates in it. The two rays are therefore polarised in mutually perpendicular planes.

Example: A calcite crystal (Iceland spar) has refractive indices μo=1.658\mu_o = 1.658 and μe=1.486\mu_e = 1.486. A ray incident normally on its surface still splits into two — the O-ray goes straight through, while the E-ray is deviated sideways. This is why a dot viewed through calcite appears as two dots.


Nicol Prism

A Nicol prism is a polarising device made from a calcite crystal, used to produce and analyse plane-polarised light.

Construction:

        A ─────────────── B
         \               /
          \   Canada    /     ← E-ray absorbed
           \  balsam   /        at cemented face
            \         /
             \       /
        A' ─────────────── B'
              ↑
          O-ray transmitted
          (plane-polarised)
  • A calcite crystal is cut with its length about 3 times its breadth, with end faces inclined at 68°68° and side faces at 71°71°.
  • The crystal is cut diagonally along a plane perpendicular to the principal section and the two halves are cemented together with Canada balsam (refractive index μ=1.55\mu = 1.55).

Working:

  1. For the O-ray, μo=1.658>μbalsam=1.55\mu_o = 1.658 > \mu_{\text{balsam}} = 1.55, so it passes from a denser to a rarer medium at the balsam layer. Since the angle of incidence exceeds the critical angle, the O-ray suffers total internal reflection and is absorbed by the blackened side of the prism.
  2. For the E-ray, μe=1.486<μbalsam=1.55\mu_e = 1.486 < \mu_{\text{balsam}} = 1.55, so it passes from a rarer to a denser medium and is transmitted straight through without deviation.
  3. The emergent light is therefore plane-polarised, with vibrations in the principal section.

Uses: Producing plane-polarised light, analysing polarised light, in polarimeters and saccharimeters.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 8 marks

Describe with necessary theory Stern-Gerlach experiment. What conclusion can be drawn from the result of the experiment?

Answer

Stern–Gerlach Experiment

Theory

The Stern–Gerlach experiment (1922), performed by Otto Stern and Walther Gerlach, was designed to test the spatial quantization of angular momentum predicted by the old quantum theory (Sommerfeld–Bohr model).

Principle: A beam of neutral atoms with a permanent magnetic moment μ⃗\vec{\mu} is passed through a non-uniform magnetic field. The field exerts a net force on the magnetic dipole:

F⃗=∇(μ⃗⋅B⃗)\vec{F} = \nabla(\vec{\mu}\cdot\vec{B})

If the field is non-uniform along the zz-axis only, the force is

Fz=μz∂Bz∂zF_z = \mu_z \frac{\partial B_z}{\partial z}

Classical prediction: The magnetic moment μ⃗\vec{\mu} can take any orientation in space, so μz=μcos⁡θ\mu_z = \mu\cos\theta varies continuously from −μ-\mu to +μ+\mu. The beam should therefore spread into a continuous smear on the screen.

Quantum prediction: The component μz\mu_z is quantized. For orbital angular momentum quantum number ll, the magnetic quantum number takes 2l+12l+1 discrete values:

μz=−ml μB,ml=−l, −l+1, …, +l\mu_z = -m_l\,\mu_B,\quad m_l = -l,\ -l+1,\ \dots,\ +l

So the beam should split into an odd number (2l+1)(2l+1) of discrete beams.

Experimental Setup

  1. Source (oven): Silver (Ag) is heated in an oven to about 1000 °C. Silver atoms evaporate and escape through a small hole, forming a narrow beam. Silver is chosen because it has a single unpaired outer electron and behaves as a neutral atom (so it is unaffected by electric fields).

  2. Collimating slits: Two narrow slits produce a well-defined, pencil-thin beam.

  3. Non-uniform magnetic field: The beam passes between specially shaped pole pieces — one flat, one knife-edged — so that the field is strong near the knife edge and weak near the flat pole. This gives a large, constant gradient ∂Bz/∂z\partial B_z/\partial z along the vertical direction.

  4. Detector (glass plate): The atoms strike a glass plate and are detected by the silver deposit they leave (developed photographically).

Observation

  • Classically, a continuous vertical smear was expected.
  • Actually observed: The beam split into two distinct, sharp traces on the plate — one deflected upward, one downward — with nothing in between.

Conclusion

  1. Space quantization is real: The magnetic moment (and hence angular momentum) of an atom can take only certain discrete orientations in space — it is quantized, not continuous. This confirms the quantum picture and rules out the classical one.

  2. Two beams, not three: For silver, the outer electron is in an ss-state, so the orbital angular momentum is zero (l=0l = 0), which would give 2l+1=12l+1 = 1 beam. The observed two beams therefore cannot come from orbital angular momentum.

  3. Existence of electron spin: The splitting into exactly two beams shows the electron possesses an intrinsic angular momentum — spin — with s=12s = \tfrac{1}{2}, giving 2s+1=22s+1 = 2 orientations (ms=+12,−12m_s = +\tfrac{1}{2}, -\tfrac{1}{2}). This was the first direct evidence of electron spin (later explained by Uhlenbeck and Goudsmit, 1925).

  4. Magnetic moment of the electron: The measured deflection gives μz=±μB\mu_z = \pm \mu_B (one Bohr magneton), confirming the spin magnetic moment of the electron.

  5. Foundation for quantum mechanics: The experiment provides direct experimental proof of the quantization of angular momentum and the projection of a quantum state, and it is the basis of modern spin and Stern–Gerlach spin-filter experiments in quantum measurement theory.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 8 marks

What is an oscillator? What is its need? Draw circuit diagram of Colpitt's oscillator and explain its working. Which component provide the positive feedback in the circuit?

Answer

Oscillator: An oscillator is an electronic circuit that generates a continuous, periodic (usually sinusoidal) output of a desired frequency without any external input signal. It converts DC energy from the supply into AC energy. It works on the principle of positive feedback: a part of the output is fed back to the input in phase with it.

Need of an oscillator:

  1. To generate carrier waves in radio and TV transmitters and communication systems.
  2. To produce clock pulses and timing signals in digital circuits, computers and microprocessors.
  3. To generate RF signals in radar, induction heating and dielectric heating.
  4. To produce audio-frequency signals in signal generators, function generators and test equipment.
  5. To supply the local oscillator signal in superheterodyne receivers.
  6. For electronic watches, calculators, medical equipment and ultrasonic generators.

Circuit diagram of Colpitts oscillator

               +Vcc
                 |
               [RFC]
                 |
        +--------+--------+  
        |        | C      |
       [C1]   +--+--+     |
        |     |  Q  |    [L]
        +-----+ E   |     |
        |     |   B +--+  |
       [C2]   +-----+  |  |
        |               |  |
        +---------------+--+

Tank circuit: inductor LL in parallel with the series combination of C1C_1 and C2C_2. The junction of C1C_1 and C2C_2 is connected to the emitter (ground for AC); the collector goes to the top end of the tank and the base to the bottom end. Biasing resistors and coupling/bypass capacitors are omitted for clarity.


Working

  1. Tank circuit: When the supply is switched on, noise or the transient surge of collector current makes the LC circuit oscillate at its natural frequency.
  2. Amplifier action: The voltage across C2C_2 is applied between base and emitter. The transistor amplifies it and gives a larger output (phase-inverted, 180∘180^\circ) at the collector, across C1C_1.
  3. Positive feedback: The grounded junction of C1C_1 and C2C_2 makes the voltages across them 180∘180^\circ out of phase. This provides another 180∘180^\circ shift, so the total loop phase shift is 360∘360^\circ (0°) and the feedback is positive (regenerative).
  4. Sustained oscillations: Losses in the tank are made up from the DC supply through the transistor. When the loop gain satisfies Aβ=1A\beta = 1, oscillations are continuous and of constant amplitude. The feedback fraction is β=C1/C2\beta = C_1/C_2, so the condition is hfe≥C2/C1h_{fe} \ge C_2/C_1.
  5. Frequency of oscillation: f=12πL Ceq,Ceq=C1C2C1+C2f = \frac{1}{2\pi\sqrt{L\,C_{eq}}}, \qquad C_{eq} = \frac{C_1 C_2}{C_1 + C_2}

Component providing positive feedback

The capacitive voltage divider formed by C1C_1 and C2C_2 provides the positive feedback. The voltage across C2C_2 is fed back to the base-emitter input, and with the 180∘180^\circ shift of the transistor plus the 180∘180^\circ shift of the divider, the net phase shift is zero.

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 6 marks

Answer any TWO of the following. [2×3=6] a) Elucidate the theory of laser. b) Explain Raman scattering. c) Describe Meson theory of nuclear forces. d) Write a short note on "Zener diode".

Answer

a) Theory of Laser

LASER stands for Light Amplification by Stimulated Emission of Radiation. It is based on the interaction of radiation with matter, which involves three fundamental processes:

  1. Stimulated Absorption: An atom in the ground state E1E_1 absorbs a photon of energy hν=E2−E1h\nu = E_2 - E_1 and jumps to the excited state E2E_2.

  2. Spontaneous Emission: An atom in the excited state E2E_2 spontaneously returns to the ground state E1E_1, emitting a photon of energy hνh\nu in a random direction with random phase.

  3. Stimulated Emission: A photon of energy hνh\nu incident on an atom already in the excited state E2E_2 stimulates it to return to E1E_1, emitting a second photon that is identical in frequency, phase, direction and polarization to the stimulating photon. Thus one photon produces two coherent photons.

Condition for laser action — Population Inversion: Under normal thermal equilibrium, N1>N2N_1 > N_2 (Boltzmann distribution), so stimulated absorption dominates and light is absorbed. For amplification, the population of the excited state must exceed that of the ground state, i.e. N2>N1N_2 > N_1. This condition is called population inversion, achieved by pumping (optical, electrical or chemical excitation) using a three-level or four-level system.

Optical Resonator: The active medium is placed between two mirrors — one fully reflecting and one partially reflecting. Photons emitted along the axis are reflected back and forth, stimulating further emissions and building up an intense, highly monochromatic and coherent beam, which emerges through the partial mirror as the laser beam.

Properties of laser light: (i) high monochromaticity, (ii) high coherence, (iii) high directionality, (iv) very high intensity/brightness.


b) Raman Scattering

When a beam of monochromatic light (usually from a laser) is passed through a transparent medium such as gas, liquid or solid, most of the light is scattered with the same frequency as the incident light (Rayleigh scattering). However, a small fraction of the scattered light is found to have frequencies different from that of the incident light. This phenomenon was discovered by C. V. Raman in 1928 and is called Raman scattering (Raman effect); he received the Nobel Prize in 1930.

Explanation: Let the incident photon of frequency ν0\nu_0 interact with a molecule of the medium. The molecule may be in its ground state or in a vibrational/rotational excited state.

  • If the molecule gains energy ΔE\Delta E from the photon, the scattered photon has lower energy: hν′=hν0−ΔE⇒ν′=ν0−ΔEhh\nu' = h\nu_0 - \Delta E \quad \Rightarrow \quad \nu' = \nu_0 - \frac{\Delta E}{h} These lower-frequency lines form the Stokes lines.

  • If the molecule was already excited and gives energy ΔE\Delta E to the photon, the scattered photon has higher energy: ν′=ν0+ΔEh\nu' = \nu_0 + \frac{\Delta E}{h} These higher-frequency lines form the anti-Stokes lines.

The frequency shift Δν=∣ν′−ν0∣\Delta\nu = |\nu' - \nu_0| is called the Raman shift and is independent of the frequency of the incident light; it depends only on the nature of the scattering molecule. Anti-Stokes lines are weaker than Stokes lines because fewer molecules are initially in the excited state.

Significance: Raman spectroscopy is used to study molecular structure, vibrational and rotational energy levels, and is applied in chemistry, biology and materials science.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 10 marks

Answer all questions. [4×2.5=10] a) Explain Huygen's wave theory of light. b) State and explain Moseley's law. c) Clarify Thevenin's theorem. d) Describe UJT as a relaxation oscillator.

Answer

a) Huygen's wave theory of light

Huygen's wave theory (proposed by Christian Huygens in 1678) explains the propagation of light as a wave phenomenon.

Postulates:

  1. Luminous source as centre of disturbance: Every point on a luminous body acts as a source of secondary disturbances. The medium surrounding it is filled with ether, and vibrations travel through it.

  2. Wavefront: The locus of all particles of the medium which are in the same phase of vibration is called a wavefront. Light travels perpendicular to the wavefront.

  3. Secondary wavelets: Every point on a given wavefront acts as a fresh source of new disturbances called secondary wavelets, which spread out in all directions with the same speed as the original wave.

  4. New wavefront (Huygens' principle): The forward-going envelope (common tangent surface) of all the secondary wavelets at any later instant gives the new position of the wavefront. The backward envelope is ineffective.

Explanation of reflection and refraction:

  • Reflection: When a wavefront strikes a reflecting surface, secondary wavelets from different points travel back into the same medium. The envelope of these wavelets gives the reflected wavefront. Since the speed is unchanged, the angle of incidence equals the angle of reflection.

  • Refraction: When light passes from a rarer to a denser medium, the speed of secondary wavelets decreases. The envelope of these wavelets gives the refracted wavefront, which bends towards the normal. Snell's law sin⁡isin⁡r=v1v2=μ\dfrac{\sin i}{\sin r} = \dfrac{v_1}{v_2} = \mu follows directly.

Merits: Explains reflection, refraction, interference, diffraction and polarisation. Demerits: Could not explain rectilinear propagation convincingly, the photoelectric effect, or the existence of ether.


b) Moseley's law

Statement: The frequency of the characteristic X-ray spectral line emitted by an element is directly proportional to the square of the atomic number of the element.

ν∝(Z−b)2orν=a(Z−b)\nu \propto (Z-b)^2 \quad \text{or} \quad \sqrt{\nu} = a(Z-b)

where ZZ is the atomic number, bb is the screening constant (about 1 for the KαK_\alpha line) and aa is a constant.

Explanation: Moseley (1913) bombarded various elements with high-speed electrons and measured the frequency of the emitted characteristic X-rays. He found that the frequency depends only on the atomic number of the target element and not on the nature of the bombarding particle. Plotting ν\sqrt{\nu} against ZZ gives a straight line.

Physical reason: The characteristic X-ray is emitted when an electron jumps from an outer shell to a vacancy in an inner shell. The energy difference between these shells depends on the nuclear charge, i.e. on ZZ. Hence the frequency of the emitted X-ray is governed by ZZ.

Importance:

  1. It established atomic number as the fundamental property of an element (more basic than atomic weight).
  2. It was used to predict new elements and to fix their positions in the periodic table.
  3. It confirmed Bohr's theory of the atom and the shell structure of electrons.

c) Thevenin's theorem

Statement: Any linear active network with two terminals can be replaced by a single equivalent voltage source VthV_{th} in series with a single equivalent resistance RthR_{th}, where:

  • VthV_{th} (Thevenin voltage) is the open-circuit voltage across the two terminals, and
  • RthR_{th} (Thevenin resistance) is the resistance measured across the two terminals with all independent sources removed (voltage sources short-circuited, current sources open-circuited) and all internal resistances retained.

Steps to apply the theorem:

  1. Remove the load resistance RLR_L from the terminals A and B.
  2. Find the open-circuit voltage VthV_{th} across A and B.
  3. Replace all voltage sources by short circuits and all current sources by open circuits; find the resistance RthR_{th} looking into A and B.
  4. Reconnect RLR_L in series with VthV_{th} and RthR_{th}.
  5. Load current: IL=VthRth+RLI_L = \dfrac{V_{th}}{R_{th} + R_L}.

Explanation: The theorem works because the terminal behaviour of any linear network is completely described by its open-circuit voltage and its internal resistance. It greatly simplifies the analysis of complex networks, especially when only the current through one particular branch (the load) is required. It is the dual of Norton's theorem.


d) UJT as a relaxation oscillator

Construction: A Uni-Junction Transistor (UJT) consists of a lightly doped n-type silicon bar with two ohmic contacts B1B_1 (base 1) and B2B_2 (base 2) at the two ends, and a heavily doped p-type emitter E alloyed near B2B_2. The p-n junction between E and the bar gives it the name "uni-junction". The resistance between B1B_1 and B2B_2 with E open is RBBR_{BB} (typically 5–10 kΩ).

Circuit: A capacitor CC is connected from emitter to ground, a resistor RR from supply VBBV_{BB} to emitter, and R1R_1, R2R_2 are base resistors. The UJT is connected across VBBV_{BB}.

Working:

  1. When VBBV_{BB} is switched on, the capacitor CC charges through RR with time constant τ=RC\tau = RC. The emitter voltage VEV_E rises exponentially.
  2. As long as VE<VPV_E < V_P (peak voltage, VP=ηVBB+VDV_P = \eta V_{BB} + V_D where η\eta is the intrinsic stand-off ratio), the emitter junction is reverse biased and the UJT is OFF. The capacitor keeps charging.
  3. When VEV_E reaches VPV_P, the emitter junction becomes forward biased. The emitter region injects holes into the n-bar, which lowers the resistance between B1B_1 and EE. This is negative resistance region: as IEI_E increases, VEV_E falls.
  4. The capacitor now discharges rapidly through EE–B1B_1 and R1R_1, producing a sharp pulse of current through R1R_1.
  5. When VEV_E falls to the valley voltage VVV_V, the junction again becomes reverse biased, the UJT turns OFF, and the capacitor starts charging again.

Result: A sawtooth (relaxation) oscillation is obtained across the capacitor and sharp pulses across R1R_1.

Frequency of oscillation:

f=1T≈1RCln⁡(11−η)f = \frac{1}{T} \approx \frac{1}{RC \ln\left(\dfrac{1}{1-\eta}\right)}

Uses: Triggering SCRs and triacs, timing circuits, pulse generators and sawtooth wave generators.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 5 marks

Newton's rings are observed in reflected light of wavelength 5900 A˚5900\ \text{Å}. The diameter of 10th10^{\text{th}} dark ring is 50 mm50\ \text{mm}. Find the radius of curvature of the lens and the thickness of air film.

Answer

Given:

  • Wavelength, (\lambda = 5900\ \text{Å} = 5900 \times 10^{-10}\ \text{m} = 5.9 \times 10^{-7}\ \text{m})
  • Order of dark ring, (n = 10)
  • Diameter of 10th dark ring, (D_{10} = 50\ \text{mm} = 0.05\ \text{m})

Formula: For Newton’s rings in reflected light, the diameter of the (n^{\text{th}}) dark ring is

[ D_n^2 = 4n\lambda R ]

So,

[ R = \frac{D_n^2}{4n\lambda} ]

The thickness of the air film at the (n^{\text{th}}) dark ring is

[ t = \frac{n\lambda}{2} ]

Calculation of radius of curvature (R):

[ R = \frac{(0.05)^2}{4 \times 10 \times 5.9 \times 10^{-7}} ]

[ R = \frac{0.0025}{2.36 \times 10^{-5}} ]

[ R = 105.93\ \text{m} ]

Calculation of thickness (t):

[ t = \frac{10 \times 5.9 \times 10^{-7}}{2} ]

[ t = 2.95 \times 10^{-6}\ \text{m} ]

[ t = 2.95\ \mu\text{m} ]

Result:

  • Radius of curvature of the lens surface, (R \approx 105.93\ \text{m})
  • Thickness of the air film at the 10th dark ring, (t = 2.95 \times 10^{-6}\ \text{m} = 2.95\ \mu\text{m})

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 5 marks

Number of lines per centimeter on a plane transmission grating is 6000. If a light of wavelength 600 nm600\ \text{nm} is incident normally on the grating find the difference in angles of deviation between 2nd2^{\text{nd}} and 3rd3^{\text{rd}} order spectra.

Answer

Given:

  • Number of lines per cm, (N = 6000\ \text{lines/cm})
  • Wavelength, (\lambda = 600\ \text{nm} = 6\times 10^{-7}\ \text{m})

Grating element:

[ d=\frac{1}{N}=\frac{1}{6000}\ \text{cm} ]

[ d=\frac{10^{-2}}{6000}\ \text{m} =1.667\times 10^{-6}\ \text{m} ]

Grating equation for normal incidence:

[ d\sin\theta_n=n\lambda ]

[ \sin\theta_n=\frac{n\lambda}{d} ]

For (n=2),

[ \sin\theta_2=\frac{2\times 600\times 10^{-9}}{1.667\times 10^{-6}} ]

[ \sin\theta_2=0.72 ]

[ \theta_2=\sin^{-1}(0.72)=46.05^\circ ]

For (n=3),

[ \sin\theta_3=\frac{3\times 600\times 10^{-9}}{1.667\times 10^{-6}} ]

[ \sin\theta_3=1.08 ]

But (\sin\theta_3=1.08>1), which is impossible. Therefore the third-order spectrum does not exist for this grating and wavelength.

The maximum possible order is

[ n_{\max}<\frac{d}{\lambda} =\frac{1.667\times 10^{-6}}{6\times 10^{-7}} =2.78 ]

So only orders (n=0,1,2) are possible.

Answer: The third-order spectrum is absent, so the difference in angles of deviation between the second and third order spectra cannot be defined.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 5 marks

The wavelength of the LαL_{\alpha} line of x-ray in the case of platinum (Z=78)(Z=78) is 1.321 A˚1.321\ \text{Å}. An unknown substance emits LαL_{\alpha} of wavelength 4.174 A˚4.174\ \text{Å}. Calculate the atomic number of the unknown sub-stance. Given that screening constant b=7.4b = 7.4 for LαL_{\alpha} lines.

Answer

For the (L_{\alpha}) line, Moseley’s law gives

[ \sqrt{\nu}=a(Z-b) ]

Since (\nu=\dfrac{c}{\lambda}),

[ \sqrt{\frac{c}{\lambda}}=a(Z-b) ]

For two substances emitting the same (L_{\alpha}) line,

[ \frac{Z_2-b}{Z_1-b}=\sqrt{\frac{\lambda_1}{\lambda_2}} ]

Given:

[ Z_1=78,\quad b=7.4,\quad \lambda_1=1.321\ \text{Å},\quad \lambda_2=4.174\ \text{Å} ]

[ Z_2-b=(Z_1-b)\sqrt{\frac{\lambda_1}{\lambda_2}} ]

[ Z_2-7.4=(78-7.4)\sqrt{\frac{1.321}{4.174}} ]

[ Z_2-7.4=70.6\sqrt{0.3165} ]

[ Z_2-7.4=70.6\times 0.5626 ]

[ Z_2-7.4=39.72 ]

[ Z_2=39.72+7.4=47.12 ]

Hence,

[ \boxed{Z_2 \approx 47} ]

The unknown substance has atomic number 47, so it is silver (Ag).

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 5 marks

A reactor is producing nuclear energy at a rate of 30,000 kW30,000\ \text{kW}. How many atoms of U235U^{235} would be used up in 1000 hours of operations? Avogadro number, NA=6×1026N_A = 6 \times 10^{26} atoms per kg.

Answer

Given:

  • Power, (P = 30{,}000\ \text{kW} = 3\times 10^7\ \text{W})
  • Time, (t = 1000\ \text{h} = 1000 \times 3600 = 3.6\times 10^6\ \text{s})
  • Energy released per fission of (U^{235}) (standard value) (= 200\ \text{MeV})

Energy per fission in joule: [ E_f = 200\ \text{MeV} = 200 \times 1.6\times 10^{-13}\ \text{J} ] [ E_f = 3.2\times 10^{-11}\ \text{J} ]

Total energy produced: [ E = P t = 3\times 10^7 \times 3.6\times 10^6 ] [ E = 1.08\times 10^{14}\ \text{J} ]

Number of (U^{235}) atoms used up: [ N = \frac{E}{E_f} = \frac{1.08\times 10^{14}}{3.2\times 10^{-11}} ] [ N = 3.375\times 10^{24} ]

[ \boxed{N \approx 3.4\times 10^{24}\ \text{atoms of } U^{235}} ]

So, about (3.4\times 10^{24}) atoms of (U^{235}) would be used up in 1000 hours of operation.
(The given Avogadro number is not needed for the atom count itself.)

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 5 marks

When the inputs to a differential amplifier are Vi1=0.1sin⁡ωtV_{i1} = 0.1 \sin \omega t and Vi2=−0.1sin⁡(ωt)V_{i2} = -0.1 \sin(\omega t), it is found that the outputs are Vo1=−5sin⁡(ωt)V_{o1} = -5 \sin(\omega t) and Vo2=5sin⁡(ωt)V_{o2} = 5 \sin(\omega t). When both outputs are 2 sin ωt\omega t the outputs are Vo1=0.05sin⁡(ωt)V_{o1} = 0.05 \sin(\omega t) and Vo2=−0.05sin⁡(ωt)V_{o2} = -0.05 \sin(\omega t). Find the value of CMRR in dB.

Answer

Given:

Case 1: Vi1=0.1sin⁡ωt,Vi2=−0.1sin⁡ωtV_{i1}=0.1\sin\omega t,\qquad V_{i2}=-0.1\sin\omega t Vo1=−5sin⁡ωt,Vo2=5sin⁡ωtV_{o1}=-5\sin\omega t,\qquad V_{o2}=5\sin\omega t

Differential input: Vd=Vi1−Vi2=0.1sin⁡ωt−(−0.1sin⁡ωt)=0.2sin⁡ωtV_d=V_{i1}-V_{i2}=0.1\sin\omega t-(-0.1\sin\omega t)=0.2\sin\omega t

Differential output: Vod=Vo1−Vo2=−5sin⁡ωt−5sin⁡ωt=−10sin⁡ωtV_{od}=V_{o1}-V_{o2}=-5\sin\omega t-5\sin\omega t=-10\sin\omega t

So differential gain: Ad=∣VodVd∣=100.2=50A_d=\left|\frac{V_{od}}{V_d}\right|=\frac{10}{0.2}=50

Case 2: both inputs are equal, so Vi1=Vi2=2sin⁡ωtV_{i1}=V_{i2}=2\sin\omega t Vo1=0.05sin⁡ωt,Vo2=−0.05sin⁡ωtV_{o1}=0.05\sin\omega t,\qquad V_{o2}=-0.05\sin\omega t

Common-mode input: Vc=2sin⁡ωtV_c=2\sin\omega t

Differential output: Vod=Vo1−Vo2=0.05sin⁡ωt−(−0.05sin⁡ωt)=0.1sin⁡ωtV_{od}=V_{o1}-V_{o2}=0.05\sin\omega t-(-0.05\sin\omega t)=0.1\sin\omega t

So common-mode gain: Ac=∣VodVc∣=0.12=0.05A_c=\left|\frac{V_{od}}{V_c}\right|=\frac{0.1}{2}=0.05

Now, CMRR=AdAc=500.05=1000\text{CMRR}=\frac{A_d}{A_c}=\frac{50}{0.05}=1000

In decibels: CMRR(dB)=20log⁡10(1000)\text{CMRR(dB)}=20\log_{10}(1000) =20×3=60 dB=20\times 3=60\ \text{dB}

CMRR=60 dB\boxed{\text{CMRR}=60\ \text{dB}}

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2083 · Optics, Modern Physics and Electronics; PHY. 201 · 5 marks

The two capacitors in a Colpitt's Oscillator have values 0.2 μH0.2\ \mu\text{H} and 0.02 μH0.02\ \mu\text{H}. The frequency of the oscillator is 10 kHz10\ \text{kHz}. Find the inductor used in the circuit.

Answer

For a Colpitt’s oscillator, the two capacitors are in series, so their equivalent capacitance is

Ceq=C1C2C1+C2C_{eq}=\frac{C_1C_2}{C_1+C_2}

Taking the capacitor values as
C1=0.2 μF,C2=0.02 μFC_1=0.2\ \mu\text{F},\qquad C_2=0.02\ \mu\text{F}

Ceq=0.2×0.020.2+0.02 μFC_{eq}=\frac{0.2\times 0.02}{0.2+0.02}\ \mu\text{F} Ceq=0.0040.22 μF=0.01818 μFC_{eq}=\frac{0.004}{0.22}\ \mu\text{F}=0.01818\ \mu\text{F} Ceq=1.818×10−8 FC_{eq}=1.818\times 10^{-8}\ \text{F}

The frequency of a Colpitt’s oscillator is

f=12πLCeqf=\frac{1}{2\pi\sqrt{LC_{eq}}}

So,

L=14π2f2CeqL=\frac{1}{4\pi^2 f^2 C_{eq}}

Given,

f=10 kHz=104 Hzf=10\ \text{kHz}=10^4\ \text{Hz}

Substituting,

L=14π2(104)2(1.818×10−8)L=\frac{1}{4\pi^2(10^4)^2(1.818\times 10^{-8})}

L=13.9478×109×1.818×10−8L=\frac{1}{3.9478\times 10^9\times 1.818\times 10^{-8}}

L=171.78L=\frac{1}{71.78}

L=0.01393 HL=0.01393\ \text{H}

L=13.93 mH\boxed{L=13.93\ \text{mH}}

So, the inductor used in the Colpitt’s oscillator is approximately 13.93 mH.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2082 · PHY. 201 (New Course) · 8 marks

Discuss Vector atom model. Explain how Space quantization has been verified the experiments.

Answer

Vector Atom Model and Experimental Verification of Space Quantization

1. Vector Atom Model

The vector atom model was developed (by Sommerfeld, Debye, and others) to remove the shortcomings of Bohr's atomic model. In this model, the various properties of an electron in an atom are represented by vectors having definite magnitude and direction.

The two fundamental vectors are:

  1. Orbital angular momentum vector (L⃗\vec{L}) — due to the orbital motion of the electron around the nucleus. Its magnitude is ∣L⃗∣=l(l+1) h2π\left|\vec{L}\right| = \sqrt{l(l+1)}\,\frac{h}{2\pi} where l=0,1,2,…,(n−1)l = 0,1,2,\dots,(n-1) is the orbital quantum number.

  2. Spin angular momentum vector (S⃗\vec{S}) — due to the spin (intrinsic rotation) of the electron about its own axis. Its magnitude is ∣S⃗∣=s(s+1) h2π,s=12\left|\vec{S}\right| = \sqrt{s(s+1)}\,\frac{h}{2\pi},\qquad s = \tfrac{1}{2}

The total angular momentum is the vector sum J⃗=L⃗+S⃗,∣J⃗∣=j(j+1) h2π\vec{J} = \vec{L} + \vec{S},\qquad \left|\vec{J}\right| = \sqrt{j(j+1)}\,\frac{h}{2\pi}

Associated with these vectors are the magnetic moment vectors μ⃗l\vec{\mu}_l and μ⃗s\vec{\mu}_s, which are oppositely directed to L⃗\vec{L} and S⃗\vec{S} respectively.

Basic postulates of the vector atom model

  • Quantization of direction (space quantization): The angular momentum vectors can take only certain discrete orientations in space, so that their components along a fixed reference direction (say the ZZ-axis) are integral or half-integral multiples of h/2πh/2\pi.
  • Quantization of magnitude: The magnitude of each vector is fixed by its quantum number, as given above.
  • Spinning electron: The electron possesses an intrinsic spin and hence a spin magnetic moment.
  • Coupling of vectors: L⃗\vec{L} and S⃗\vec{S} couple to give the resultant J⃗\vec{J} (spin–orbit coupling).

Space quantization

If a magnetic field is applied along the ZZ-direction, the orbital angular momentum vector L⃗\vec{L} can orient itself only in those directions for which the component along ZZ is Lz=ml h2π,ml=−l, −l+1,…,0,…,+lL_z = m_l\,\frac{h}{2\pi},\qquad m_l = -l,\,-l+1,\dots,0,\dots,+l Thus there are (2l+1)(2l+1) possible orientations. This restriction of the orientation of an angular momentum vector to discrete directions is called space quantization.

Similarly, for the spin vector, Sz=ms h2π,ms=±12S_z = m_s\,\frac{h}{2\pi},\qquad m_s = \pm\tfrac{1}{2}


2. Experimental Verification — Stern–Gerlach Experiment

Space quantization was directly verified by Stern and Gerlach (1922) using a beam of silver atoms.

Experimental arrangement

  • Silver is heated in an electric furnace and the vapour is allowed to escape through a fine hole, producing a narrow beam of silver atoms.
  • The beam is collimated by slits and passed through a highly non-uniform magnetic field produced by specially shaped pole pieces (one sharp knife-edge, the other flat).
  • The atoms are finally collected on a glass plate (detector), where the deposit is examined.

Working

A silver atom has one unpaired electron in the outermost shell, so its magnetic moment is due to that electron. In a non-uniform field the atom experiences a force Fz=μz∂B∂zF_z = \mu_z\frac{\partial B}{\partial z}

  • Classical prediction: If the orbital angular momentum could have any orientation, μz\mu_z would vary continuously and the beam should produce a continuous smear on the plate.
  • Quantum prediction: Since LzL_z (and hence μz\mu_z) is space-quantized, the beam should split into a discrete number of beams.

Result

The beam was found to split into two distinct traces (a symmetrical splitting), not a continuous band. This confirms space quantization directly.

Interpretation

For silver, the orbital angular momentum is zero (l=0l=0), so the splitting cannot be explained by orbital quantization. It is explained only by the spin of the electron with s=1/2s = 1/2, giving ms=±1/2m_s = \pm 1/2, i.e. exactly two orientations. Hence the experiment verifies:

  1. Space quantization of angular momentum, and
  2. The existence of electron spin (spin quantum number s=1/2s = 1/2).

Other supporting evidence

  • Zeeman effect: Splitting of spectral lines in a magnetic field into discrete components is explained only by space quantization of L⃗\vec{L} and S⃗\vec{S}.
  • Anomalous Zeeman effect confirms the spin magnetic moment and the coupling J⃗=L⃗+S⃗\vec{J} = \vec{L} + \vec{S}.

Conclusion

The vector atom model represents orbital and spin angular momenta as vectors with quantized magnitude and direction. Space quantization — the restriction of these vectors to (2l+1)(2l+1) or (2s+1)(2s+1) discrete orientations — is experimentally verified by the Stern–Gerlach experiment (two-fold splitting of a silver atomic beam) and by the Zeeman effect.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2082 · PHY. 201 (New Course) · 8 marks

Discuss the working characteristics features and applications of Zener diode.

Answer

Zener Diode

A Zener diode is a heavily doped silicon p-n junction diode designed to operate safely in the reverse breakdown region. Because of heavy doping, the depletion layer is very thin, so breakdown occurs at a low, sharply defined reverse voltage called the Zener voltage (VZV_Z).

Working

  1. Forward bias: It behaves like an ordinary diode, conducting at about 0.7 V.
  2. Reverse bias (below VZV_Z): Only a small reverse saturation current flows.
  3. At VZV_Z: Breakdown occurs and a large reverse current flows. In a Zener diode this breakdown is non-destructive (if power rating is not exceeded), so the diode can be operated continuously in this region.
  4. Voltage regulation: In the breakdown region the voltage across the diode stays almost constant at VZV_Z even when the current changes greatly. The series resistor RSR_S absorbs the excess voltage:

VS=Vin−VZ,IZ=IL+ISV_S = V_{in} - V_Z, \qquad I_Z = I_L + I_S

If VinV_{in} rises, IZI_Z rises and the extra voltage drops across RSR_S, keeping VZV_Z (and hence the load voltage) constant. If VinV_{in} falls, IZI_Z falls and the voltage is again maintained. Thus the Zener acts as a voltage reference/regulator.

Characteristic Features

  • Sharp breakdown voltage: VZV_Z is fixed and precise (from about 2.4 V to 200 V).
  • Constant voltage in breakdown: Voltage remains nearly constant over a wide range of reverse current.
  • Two breakdown mechanisms:
    • Zener breakdown — dominant below about 6 V; due to direct rupture of covalent bonds by a strong electric field (negative temperature coefficient).
    • Avalanche breakdown — dominant above about 6 V; due to collision multiplication of carriers (positive temperature coefficient).
  • Dynamic resistance rZ=ΔVZ/ΔIZr_Z = \Delta V_Z / \Delta I_Z is very small in the breakdown region.
  • Power rating PZ=VZIZP_Z = V_Z I_Z must not be exceeded, otherwise the diode is destroyed.
  • Heavily doped, so the depletion region is narrow and breakdown is sharp.
  • Available in standard voltages (e.g. 5.1 V, 6.2 V, 9.1 V, 12 V) and power ratings (0.5 W, 1 W, 5 W).

Applications

  1. Voltage regulator — maintains a constant DC output against changes in input voltage or load current.
  2. Voltage reference — provides a stable reference voltage in power supplies, voltmeters and comparator circuits.
  3. Wave clipping / limiting — clamps or limits signal amplitude in wave-shaping circuits.
  4. Overvoltage protection — protects sensitive circuits and meters from excessive voltage surges.
  5. Meter protection — shunts excess current away from a galvanometer or meter movement.
  6. Voltage shifter — shifts the DC level of a signal by a fixed amount.
  7. Square-wave generation — used with an amplifier to produce square waves from sine waves.

Conclusion: The Zener diode is the simplest and most widely used solid-state device for voltage regulation and reference, because its reverse breakdown voltage is sharp, stable and repeatable.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2082 · PHY. 201 (New Course) · 6 marks

Answer any TWO of the following. [2×3=6]
a) What is holography? Explain.
b) Why Ramsdens eye piece is more preferable than Huygene's eyepiece?
c) What are the importance and conclusions of Moseley's law?
d) Explain the phase inversion in CE-amplifier.

Answer

Answer any TWO of the following.


a) What is holography? Explain.

Holography is the technique of recording and reproducing the complete three-dimensional image of an object by means of the interference pattern of light waves. The recorded photograph is called a hologram.

Explanation:

  1. A beam of coherent light from a laser is split into two parts: the object beam and the reference beam.
  2. The object beam is made to fall on the object, and the light scattered from the object falls on a photographic plate.
  3. The reference beam is made to fall directly on the same photographic plate.
  4. The two beams interfere and produce a complex interference pattern on the plate. This plate, after development, is the hologram.
  5. When the hologram is illuminated by the reference beam (or a similar coherent beam), the light diffracts from the recorded pattern and reconstructs the original wavefront, giving a three-dimensional image of the object.

Key features:

  • The image is truly three-dimensional — it shows parallax and depth.
  • No lens is needed for recording or reconstruction.
  • Any small part of the hologram can reproduce the whole image.

b) Why Ramsden's eyepiece is more preferable than Huygens's eyepiece?

  1. Cross-wire arrangement: In Ramsden's eyepiece the field lens is placed below the cross-wires (between the objective and the cross-wires), so the cross-wires can be adjusted at the focus of the eye lens and are clearly visible. In Huygens's eyepiece the cross-wires cannot be used, as they would be blurred.
  2. Real image formation: Ramsden's eyepiece forms a real image outside the eyepiece, so a micrometer or scale can be mounted at the image plane for measurement. This is not possible in Huygens's eyepiece.
  3. Wider field of view and less spherical aberration: The two lenses in Ramsden's eyepiece are placed farther apart, giving a larger field of view and reduced spherical aberration compared with Huygens's eyepiece.

For these reasons Ramsden's eyepiece is preferred in optical instruments where measurement and cross-wires are required.


c) What are the importance and conclusions of Moseley's law?

Moseley's law: The frequency of the characteristic X-ray emitted when an electron jumps from the L-shell to the K-shell is given by

ν=a(Z−b)2\nu = a(Z-b)^2

where ZZ is the atomic number, and aa, bb are constants for a given series.

Conclusions:

  1. The frequency of characteristic X-rays depends on the atomic number of the target element, not on its atomic weight.
  2. The quantity ν\sqrt{\nu} varies linearly with ZZ, so a plot of ν\sqrt{\nu} against ZZ is a straight line.
  3. The atomic number is the fundamental property that decides the position of an element in the periodic table.

Importance:

  1. It established atomic number as the basic criterion for arranging elements in the periodic table, correcting the earlier order based on atomic weight.
  2. It helped in the discovery of new elements and in fixing the position of doubtful elements (e.g. correcting the positions of Co–Ni, Te–I).
  3. It gave direct experimental evidence for the Bohr model of the atom and for the shell structure of electrons.
  4. It is used in X-ray spectroscopy for the identification of elements and in chemical analysis.

d) Explain the phase inversion in CE-amplifier.

In a common-emitter (CE) amplifier, the input signal is applied between base and emitter, and the output is taken between collector and emitter. The output voltage is 180° out of phase with the input voltage — this is called phase inversion.

Explanation:

  1. During the positive half-cycle of the input signal, the base voltage increases, so the base current increases. This increases the collector current ICI_C.
  2. The collector voltage is VCE=VCC−ICRCV_{CE} = V_{CC} - I_C R_C. As ICI_C increases, the drop ICRCI_C R_C increases, so VCEV_{CE} (the output) decreases. Thus a positive input gives a negative output.
  3. During the negative half-cycle of the input, the base current decreases, ICI_C decreases, the drop ICRCI_C R_C decreases, and hence VCEV_{CE} increases. Thus a negative input gives a positive output.

Since the output changes in the opposite direction to the input, the output is shifted by 180° in phase with respect to the input. Hence a CE amplifier introduces a phase reversal of 180° between input and output.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2082 · PHY. 201 (New Course) · 10 marks

Answer all questions. [4×2.5=10]
a) Elucidate the application of Ruby laser.
b) Briefly Explain the pair production phenomena.
c) Write down the steps to a typical electric circuit through Thevenin's Theorem.
d) Why can not electrons be present inside the nucleus?

Answer

(a) Applications of the ruby laser

The ruby laser (Cr³⁺ ions in an Al₂O₃ crystal) is a pulsed three-level solid-state laser that emits red light of wavelength 694.3 nm. Its main applications are:

  1. Holography: its coherence and high pulse energy make it suitable for recording holograms of large objects.
  2. Pulsed laser deposition: it ablates a target to deposit thin films of oxides and superconductors.
  3. Range finding and LIDAR: short, high-energy pulses allow accurate measurement of long distances.
  4. Dentistry and dermatology: drilling teeth, removing tattoos and treating pigmented skin lesions.
  5. Industry and defence: target designation, drilling holes in diamonds and hard metals, and welding.
  6. Research: nonlinear optics, plasma generation and studies of stimulated emission.

(b) Pair production

Pair production is the conversion of a high-energy photon (γ\gamma-ray) into an electron-positron pair in the strong Coulomb field of a nucleus. It is a direct consequence of E=mc2E = mc^2.

  • The photon energy must be at least the rest energy of the two particles: Emin⁡=2m0c2=2×0.511 MeV=1.022 MeVE_{\min} = 2m_0c^2 = 2 \times 0.511\ \text{MeV} = 1.022\ \text{MeV}
  • The nucleus takes up some recoil momentum, so energy and momentum are both conserved. A photon cannot produce a pair in empty space.
  • The excess photon energy appears as kinetic energy of the pair: hν=2m0c2+Ke+Kph\nu = 2m_0c^2 + K_e + K_p
  • The positron soon meets an electron and annihilates, giving two photons of 0.511 MeV each.

(c) Steps to solve a circuit by Thevenin's theorem

  1. Remove the load resistance RLR_L and leave the two terminals open.
  2. Calculate the open-circuit voltage VthV_{th} across these terminals (by mesh, nodal analysis or superposition).
  3. Replace all independent voltage sources by short circuits and all independent current sources by open circuits.
  4. Find the equivalent resistance RthR_{th} looking into the open terminals.
  5. Draw the Thevenin equivalent, which is VthV_{th} in series with RthR_{th}, and reconnect RLR_L across it.
  6. Calculate the load current and voltage: IL=VthRth+RL,VL=ILRLI_L = \frac{V_{th}}{R_{th} + R_L}, \qquad V_L = I_L R_L

(d) Why electrons cannot be present inside the nucleus

  1. Uncertainty principle. For an electron confined in a nucleus of size Δx≈10−14\Delta x \approx 10^{-14} m, Δp≈h2πΔx≈6.63×10−342π×10−14≈1.06×10−20 kg m/s\Delta p \approx \frac{h}{2\pi \Delta x} \approx \frac{6.63\times10^{-34}}{2\pi \times 10^{-14}} \approx 1.06\times10^{-20}\ \text{kg m/s} The corresponding kinetic energy (relativistically E≈pcE \approx pc) is about E≈pc≈1.06×10−20×3×108≈3.2×10−12 J≈20 MeVE \approx pc \approx 1.06\times10^{-20}\times 3\times10^{8} \approx 3.2\times10^{-12}\ \text{J} \approx 20\ \text{MeV} This is much more than the binding energy per nucleon (about 8 MeV), so an electron could not be held in the nucleus.
  2. Beta decay. β\beta-particles are emitted with a continuous energy spectrum. They are created at the moment of decay (n→p+e−+νˉen \rightarrow p + e^- + \bar{\nu}_e) and do not pre-exist in the nucleus.
  3. Nuclear spin. Counting protons and electrons as constituents gives wrong spin values. For example, nitrogen-14 would have 21 particles (odd), which would give half-integer spin, but the observed spin is 1.
  4. Magnetic moment. Measured nuclear magnetic moments are of the order of the nuclear magneton. If electrons were present, they would be of the order of the much larger Bohr magneton.

Hence electrons are not constituents of the nucleus; they appear only in β\beta-decay.

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2082 · PHY. 201 (New Course) · 5 marks

In Fraunhofer diffraction due to narrow slit a screen is placed 2 m away from the lens to obtain the pattern. If the slit width is 0.3 mm and the first minima lies 6 mm on either side of the central maxima. Find the wavelength of light.

Answer

Given:

  • Distance of screen from lens, (D = 2\ \text{m})
  • Slit width, (a = 0.3\ \text{mm} = 0.3 \times 10^{-3}\ \text{m})
  • Distance of first minimum from central maximum, (y = 6\ \text{mm} = 6 \times 10^{-3}\ \text{m})
  • Order of minimum, (n = 1)

Formula: For Fraunhofer diffraction at a single slit, the condition for minima is [ a\sin\theta = n\lambda ] For small angle, [ \sin\theta \approx \tan\theta = \frac{y}{D} ] So, [ \lambda = \frac{a y}{nD} ]

Substitution: [ \lambda = \frac{(0.3 \times 10^{-3})(6 \times 10^{-3})}{1 \times 2} ] [ \lambda = \frac{1.8 \times 10^{-6}}{2} ] [ \lambda = 0.9 \times 10^{-6}\ \text{m} ] [ \lambda = 9 \times 10^{-7}\ \text{m} ]

Result: [ \boxed{\lambda = 900\ \text{nm} = 9000\ \text{Å}} ]

Thus, the wavelength of light used is 900 nm (or 9000 Å).

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2082 · PHY. 201 (New Course) · 5 marks

The refractive indices of a piece of optical glass for the blue & green lines of the mercury spectrum, λ\lambda=4358 Å and λ\lambda= 5461 Å are 1.6525 and 1.6245 respectively. Using the two constant Cauchy equation, calculate values for the constants A and B.

Answer

The two-constant Cauchy equation is

n=A+Bλ2n=A+\frac{B}{\lambda^2}

Given:

  • For blue line: λ1=4358 A˚\lambda_1=4358\ \text{Å}, n1=1.6525n_1=1.6525
  • For green line: λ2=5461 A˚\lambda_2=5461\ \text{Å}, n2=1.6245n_2=1.6245

So,

1.6525=A+B(4358)21.6525=A+\frac{B}{(4358)^2}

1.6245=A+B(5461)21.6245=A+\frac{B}{(5461)^2}

Subtracting,

1.6525−1.6245=B(143582−154612)1.6525-1.6245=B\left(\frac{1}{4358^2}-\frac{1}{5461^2}\right)

0.0280=B(118,992,164−129,822,521)0.0280=B\left(\frac{1}{18{,}992{,}164}-\frac{1}{29{,}822{,}521}\right)

0.0280=B(5.2653×10−8−3.3532×10−8)0.0280=B(5.2653\times10^{-8}-3.3532\times10^{-8})

0.0280=B(1.9121×10−8)0.0280=B(1.9121\times10^{-8})

B=0.02801.9121×10−8B=\frac{0.0280}{1.9121\times10^{-8}}

B=1.464×106 A˚2B=1.464\times10^6\ \text{Å}^2

Now,

A=1.6525−B(4358)2A=1.6525-\frac{B}{(4358)^2}

A=1.6525−1.464×10618,992,164A=1.6525-\frac{1.464\times10^6}{18{,}992{,}164}

A=1.6525−0.0771A=1.6525-0.0771

A=1.5754A=1.5754

Hence,

A=1.5754\boxed{A=1.5754}

B=1.464×106 A˚2\boxed{B=1.464\times10^6\ \text{Å}^2}

If λ\lambda is taken in nm, then

B=1.464×104 nm2B=1.464\times10^4\ \text{nm}^2

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  • 2082 · PHY. 201 (New Course) · 5 marks

Deutrons in a cyclotron describe a circle of radius 0.32 m just before emerging from the dees. The frequency of the applied emf is 10 MHz. Find the flux density of the magnetic field and the velocity of the deutrons emerging out of the cyclotron. (Mass of the deutron = 3.32×10−273.32 \times 10^{-27} kg)

Answer

Given:

  • Radius just before emergence, (r = 0.32\ \text{m})
  • Frequency of applied emf, (f = 10\ \text{MHz} = 10^7\ \text{Hz})
  • Mass of deuteron, (m = 3.32 \times 10^{-27}\ \text{kg})
  • Charge of deuteron, (q = +e = 1.6 \times 10^{-19}\ \text{C})

In a cyclotron, the frequency of the applied emf is equal to the cyclotron frequency:

[ f = \frac{qB}{2\pi m} ]

So the magnetic flux density is

[ B = \frac{2\pi m f}{q} ]

Substituting the values:

[ B = \frac{2\pi (3.32 \times 10^{-27})(10^7)}{1.6 \times 10^{-19}} ]

[ B = \frac{2\pi \times 3.32 \times 10^{-20}}{1.6 \times 10^{-19}} ]

[ B = 2\pi \times 0.2075 ]

[ \boxed{B \approx 1.30\ \text{T}} ]

The velocity of the deuteron just before emerging is

[ v = \omega r = 2\pi f r ]

[ v = 2\pi (10^7)(0.32) ]

[ v = 2\pi \times 3.2 \times 10^6 ]

[ \boxed{v \approx 2.01 \times 10^7\ \text{m/s}} ]

Answer: [ \boxed{B \approx 1.30\ \text{T},\qquad v \approx 2.01 \times 10^7\ \text{m/s}} ]

Since (v \approx 0.067c), the non-relativistic cyclotron formula is valid here.

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  • 2082 · PHY. 201 (New Course) · 5 marks

A reactor is producing nuclear energy at a rate of 30 MW. How many kilograms of U235U^{235} would be used up in 1000 hr of operation. Assume U235U^{235} release an energy of 200 MeV per fission and Avogadro's number NA=6.02×1023N_A = 6.02 \times 10^{23} atoms per gram.

Answer

Given:

  • Power, (P = 30\ \text{MW} = 30 \times 10^6\ \text{J/s})
  • Time, (t = 1000\ \text{hr} = 1000 \times 3600 = 3.6 \times 10^6\ \text{s})
  • Energy per fission, (E = 200\ \text{MeV})
  • Avogadro’s number, (N_A = 6.02 \times 10^{23}\ \text{atoms/g})

Total energy produced: [ E_{\text{total}} = P t ] [ E_{\text{total}} = 30 \times 10^6 \times 3.6 \times 10^6 ] [ E_{\text{total}} = 1.08 \times 10^{14}\ \text{J} ]

Energy released per fission in joule: [ 1\ \text{eV} = 1.602 \times 10^{-19}\ \text{J} ] [ 200\ \text{MeV} = 200 \times 10^6 \times 1.602 \times 10^{-19} ] [ E = 3.204 \times 10^{-11}\ \text{J} ]

Number of fissions required: [ N = \frac{E_{\text{total}}}{E} ] [ N = \frac{1.08 \times 10^{14}}{3.204 \times 10^{-11}} ] [ N = 3.37 \times 10^{24} ]

Mass of (U^{235}) used: [ m = \frac{N}{N_A} ] [ m = \frac{3.37 \times 10^{24}}{6.02 \times 10^{23}} ] [ m = 5.60\ \text{g} ]

[ m = 5.60 \times 10^{-3}\ \text{kg} ]

Answer: [ \boxed{m \approx 5.6 \times 10^{-3}\ \text{kg}} ]

So, about 0.0056 kg of (U^{235}) would be used up.

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  • 2082 · PHY. 201 (New Course) · 5 marks

In the circuit, the transistor has β=50\beta = 50
[Circuit diagram: +30V supply; 10kΩ resistor from +30V to base node; 3kΩ resistor from +30V to collector node; transistor with base at base node, collector at collector node, emitter to ground; 5kΩ resistor from base node to ground; 1mV rms AC source connected to base node; 6kΩ resistor from collector node to output; output taken across 6kΩ resistor]
Find the output voltage and input impedance.

Answer

Step 1: DC bias (Thevenin equivalent of the base network)

Vth=30×510+5=10 V,Rth=10∥5=3.33 kΩV_{th} = 30\times\frac{5}{10+5} = 10\ \text{V}, \qquad R_{th} = 10\parallel 5 = 3.33\ \text{k}\Omega

Taking VBE≈0.7V_{BE}\approx 0.7 V and β=50\beta = 50:

IB=Vth−VBERth=10−0.73.33 kΩ≈2.8 mAI_B = \frac{V_{th}-V_{BE}}{R_{th}} = \frac{10-0.7}{3.33\ \text{k}\Omega} \approx 2.8\ \text{mA}

If the transistor were in the active region, IC=βIB≈140I_C = \beta I_B \approx 140 mA. But the largest collector current the 3 kΩ resistor can allow is

IC(sat)≈30−0.23 kΩ≈9.9 mA≪140 mAI_{C(sat)} \approx \frac{30-0.2}{3\ \text{k}\Omega} \approx 9.9\ \text{mA} \ll 140\ \text{mA}

So the transistor is driven deep into saturation, with VCE≈0.2V_{CE}\approx 0.2 V. There is no active-region amplification with this bias.

Step 2: Output voltage

In saturation the collector voltage cannot follow the base signal. The 1 mV rms input produces essentially no change at the collector, so the small-signal gain is almost zero:

vout≈0 V (a negligible fraction of a microvolt)v_{out} \approx 0\ \text{V (a negligible fraction of a microvolt)}

For comparison, if the transistor were correctly biased in the active region at about IC≈10I_C \approx 10 mA, the ideal figures would be

re=25 mV10 mA=2.5 Ω,rπ=βre=125 Ω,Av=−β(RC∥RL)rπ=−50×2 kΩ125 Ω=−800r_e = \frac{25\ \text{mV}}{10\ \text{mA}} = 2.5\ \Omega,\quad r_\pi = \beta r_e = 125\ \Omega,\quad A_v = -\frac{\beta (R_C\parallel R_L)}{r_\pi} = -\frac{50\times 2\ \text{k}\Omega}{125\ \Omega} = -800

which would give ∣vout∣≈0.8|v_{out}| \approx 0.8 V rms. The saturated circuit cannot achieve this.

Step 3: Input impedance

The signal source sees the base divider in parallel with the base input resistance of the transistor:

Zin=R1∥R2∥rπ=3.33 kΩ∥rπZ_{in} = R_1\parallel R_2\parallel r_\pi = 3.33\ \text{k}\Omega \parallel r_\pi

With rπ≈125 Ωr_\pi \approx 125\ \Omega (as above),

Zin≈3.33 kΩ∥125 Ω≈120 ΩZ_{in} \approx 3.33\ \text{k}\Omega \parallel 125\ \Omega \approx 120\ \Omega

The main result is that the output is negligible because of saturation, and ZinZ_{in} is about 0.12 kΩ.

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2081 · PHY. 201 · 10 marks

Explain construction, working and applications of Michelson interferometer. How would you use it to measure the wavelength of monochromatic light.
OR
Describe how, with the help of a Nicol prism and quarter wave plate, plane polarised light, circularly polarised light and elliptically polarised light are produced and detected.

Answer

Michelson Interferometer

Construction

The Michelson interferometer consists of the following parts:

  1. Extended source S — a broad monochromatic source (e.g., sodium lamp) placed at the focus of a convex lens LL, so that light falls on the plate as a parallel beam.
  2. Glass plate G1G_1 (beam splitter) — inclined at 45∘45^\circ to the incident beam. Its back surface is silvered (half-silvered). It divides the incident light into two parts: one reflected towards mirror M1M_1 and one transmitted towards mirror M2M_2.
  3. Compensating plate G2G_2 — identical to G1G_1 in material and thickness, placed parallel to G1G_1 in the path of the transmitted beam. It equalises the optical paths so that both beams pass through the same thickness of glass.
  4. Two plane mirrors M1M_1 and M2M_2 — highly polished and silvered on the front surface. M1M_1 is fixed; M2M_2 is mounted on a fine screw (micrometer) so it can be moved parallel to itself. The mirrors are made exactly perpendicular to each other by adjusting screws.
  5. Telescope T — to receive the interfering beams and observe the fringes.

Working

Light from the source is split at G1G_1 into two beams:

  • Beam 1 — reflected at G1G_1, travels to M1M_1, is reflected back, and after transmission through G1G_1 enters the telescope.
  • Beam 2 — transmitted through G1G_1, passes through G2G_2, travels to M2M_2, is reflected back, and after reflection at G1G_1 enters the telescope.

The two beams are coherent (they come from the same source) and travel different optical paths. When they superpose in the telescope, interference fringes are formed. The path difference is

Δ=2(d1−d2)=2d\Delta = 2(d_1 - d_2) = 2d

where d1d_1 and d2d_2 are the distances of M1M_1 and M2M_2 from G1G_1, and d=d1−d2d = d_1 - d_2 is the difference in the distances of the two mirrors from the plate.

Types of fringes:

  • If the mirrors are not exactly perpendicular, the fringes are straight and localised near the mirrors.
  • If the mirrors are exactly perpendicular (i.e. M1M_1 and the image of M2M_2 are parallel), the fringes are circular and localised at infinity. These are obtained by using an extended source and a telescope focused for infinity.

Condition for bright and dark fringes:

Bright: 2dcos⁡θ=nλDark: 2dcos⁡θ=(2n+1)λ2\text{Bright: } 2d\cos\theta = n\lambda \qquad \text{Dark: } 2d\cos\theta = (2n+1)\frac{\lambda}{2}

where θ\theta is the angle of the ray with the normal and n=0,1,2,…n = 0, 1, 2, \dots

Applications

  1. Measurement of wavelength of monochromatic light.
  2. Measurement of refractive index of a thin transparent plate or film.
  3. Measurement of thickness of a thin sheet or film.
  4. Determination of the difference in wavelengths of two nearby spectral lines (e.g. the sodium doublet).
  5. Measurement of the standard metre in terms of wavelength of light.
  6. Study of the fine structure of spectral lines and the Doppler broadening of spectral lines.
  7. Measurement of the coherence length of a source.

Measurement of Wavelength of Monochromatic Light

Principle: When the movable mirror M2M_2 is displaced through a distance xx, the path difference changes by 2x2x. If NN fringes cross the field of view, then

2x=Nλ⇒λ=2xN2x = N\lambda \quad\Rightarrow\quad \lambda = \frac{2x}{N}

Procedure:

  1. Adjust the mirrors so that circular fringes are obtained in the telescope, with the cross-wire at the centre of the field of view.
  2. Set the micrometer screw at some initial reading and note the position of the cross-wire on a particular fringe.
  3. Slowly rotate the micrometer screw so that the mirror M2M_2 moves and fringes cross the cross-wire one by one. Count the number of fringes, say NN (usually 50 or 100), that cross the cross-wire.
  4. Note the final micrometer reading. The difference between the final and initial readings gives the displacement xx of the mirror M2M_2.
  5. Repeat the observation several times and take the mean value of xx for the same number of fringes NN.
  6. Calculate the wavelength using

λ=2xN\lambda = \frac{2x}{N}

Precautions:

  • The screw must be rotated in one direction only to avoid backlash error.
  • Fringes must be counted carefully and the cross-wire kept at the centre of the field.
  • The source must be strictly monochromatic for sharp, well-defined fringes.

OR

Production and Detection of Polarised Light using Nicol Prism and Quarter Wave Plate

1. Plane Polarised Light

Production: A beam of unpolarised light is passed through a Nicol prism. Inside the prism, the ordinary ray is totally internally reflected at the Canada-balsam layer and is absorbed by the blackened side, while the extraordinary ray is transmitted. The emergent beam is plane polarised, with its electric vector vibrating in a single plane.

Detection: The emergent beam is passed through a second Nicol prism (analyser). As the analyser is rotated about the direction of propagation:

  • When the analyser is parallel to the polariser, maximum intensity is transmitted.
  • When the analyser is perpendicular to the polariser, the field becomes completely dark.

This variation of intensity from maximum to zero on rotating the analyser confirms that the light is plane polarised.

2. Circularly Polarised Light

Production: A beam of plane polarised light (obtained from a Nicol prism) is allowed to fall normally on a quarter wave plate, with its plane of vibration making an angle of 45∘45^\circ with the optic axis of the plate. The incident vibration is resolved into two equal components:

  • one along the optic axis (extraordinary ray),
  • one perpendicular to it (ordinary ray).

Since the plate introduces a path difference of λ/4\lambda/4 (phase difference π/2\pi/2) between the two components, and the amplitudes are equal, the resultant vibration at any point rotates uniformly with constant magnitude. The emergent light is circularly polarised.

Detection: The emergent beam is passed through a rotating Nicol analyser.

  • The intensity remains constant for all positions of the analyser (no variation from maximum to zero).
  • When the beam is first passed through another quarter wave plate (with its optic axis parallel to the first) and then through a rotating Nicol, the light becomes plane polarised and the intensity varies from maximum to zero.

This confirms circular polarisation. (The direction of rotation — right or left handed — can be found by using a quarter wave plate and noting the sense of rotation of the analyser.)

3. Elliptically Polarised Light

Production: A beam of plane polarised light is passed normally through a quarter wave plate, but now the plane of vibration makes an angle other than 45∘45^\circ (and other than 0∘0^\circ or 90∘90^\circ) with the optic axis. The two resolved components have unequal amplitudes, and the plate introduces a phase difference of π/2\pi/2. The resultant vibration traces an ellipse, so the emergent light is elliptically polarised.

Detection: The emergent beam is examined with a rotating Nicol analyser.

  • The intensity varies from a maximum to a minimum, but the minimum is not zero (unlike in plane polarised light).
  • The variation of intensity with the angle of the analyser follows the equation of an ellipse.

This confirms elliptical polarisation. If the beam is passed through a quarter wave plate whose optic axis is parallel to that of the first, the elliptical vibration is converted back into plane polarised light, and the intensity then falls to zero at one position of the analyser.

Summary Table

Type of lightProductionDetection with rotating Nicol
Plane polarisedNicol prismIntensity varies from max to zero
Circularly polarisedPlane polarised light + quarter wave plate at 45∘45^\circ to optic axisIntensity constant; becomes plane polarised after another quarter wave plate
Elliptically polarisedPlane polarised light + quarter wave plate at angle ≠45∘\neq 45^\circIntensity varies from max to non-zero minimum

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2081 · PHY. 201 · 10 marks

What do you mean by Zeeman effect and Stark effect? Discuss anomalous Zeeman effect.
OR
Explain Stern-Gerlach experiment, set up and its working. Discuss the results of this experiment concerning vector atom model. How did Sommerfeld modify Bohr's model?

Answer

Zeeman Effect and Stark Effect

Zeeman Effect

When an atom is placed in an external magnetic field, its spectral lines split into several closely spaced components. This splitting of spectral lines in a magnetic field is called the Zeeman effect.

The energy shift of an atomic level in a magnetic field BB is

ΔE=mj g μB B\Delta E = m_j \, g \, \mu_B \, B

where mjm_j is the magnetic quantum number, gg the Landé gg-factor, and μB=eℏ2m\mu_B = \dfrac{e\hbar}{2m} the Bohr magneton. The frequency of the emitted line therefore shifts by

Δν=ΔEh=mjgμBBh\Delta \nu = \frac{\Delta E}{h} = \frac{m_j g \mu_B B}{h}

Normal Zeeman effect: A line splits into three components (a central undisplaced line and two symmetrically placed lines). It is observed for atoms with zero net spin (singlet states, S=0S = 0), where the splitting depends only on mlm_l.

Anomalous Zeeman effect: A line splits into more than three components (often four, six, or more), with unequal spacing. It is observed in atoms having non-zero resultant spin, i.e. when S≠0S \neq 0.

Stark Effect

When an atom is placed in an external electric field, its spectral lines split into several components. This is the Stark effect, discovered by Johannes Stark in 1913. The energy shift is

ΔE=−e E z\Delta E = -e \, E \, z

where EE is the electric field strength. The Stark effect is the electric analogue of the Zeeman effect. For hydrogen it is linear in the field (first-order Stark effect); for most other atoms it is quadratic in the field (second-order Stark effect).

Anomalous Zeeman Effect

When an atom has both orbital and spin angular momenta, the total magnetic moment is

μ⃗=μ⃗L+μ⃗S=−e2m(L⃗+2S⃗)\vec{\mu} = \vec{\mu}_L + \vec{\mu}_S = -\frac{e}{2m}\left(\vec{L} + 2\vec{S}\right)

Since μ⃗\vec{\mu} is not antiparallel to the total angular momentum J⃗=L⃗+S⃗\vec{J} = \vec{L} + \vec{S}, the effective magnetic moment along J⃗\vec{J} is obtained by projection:

μJ=−e2m(L⃗⋅J^+2S⃗⋅J^)\mu_J = -\frac{e}{2m}\left(\vec{L}\cdot\hat{J} + 2\vec{S}\cdot\hat{J}\right)

Using the vector model results L⃗⋅J⃗=ℏ22[J(J+1)+L(L+1)−S(S+1)]\vec{L}\cdot\vec{J} = \frac{\hbar^2}{2}\left[J(J+1) + L(L+1) - S(S+1)\right] and similarly for S⃗⋅J⃗\vec{S}\cdot\vec{J}, one obtains the Landé gg-factor

g=1+J(J+1)+S(S+1)−L(L+1)2J(J+1)g = 1 + \frac{J(J+1) + S(S+1) - L(L+1)}{2J(J+1)}

The energy of the level in the field is therefore

E=E0+mj g μB B,mj=−J,…,+JE = E_0 + m_j \, g \, \mu_B \, B, \qquad m_j = -J, \ldots, +J

Because gg differs from level to level, the number of components and their spacing are governed by the selection rule Δmj=0,±1\Delta m_j = 0, \pm 1. This gives the characteristic anomalous pattern — more than three lines, unequally spaced — which the classical theory could not explain. The anomalous Zeeman effect is thus direct evidence for the spin of the electron and for space quantization of J⃗\vec{J}.


OR

Stern–Gerlach Experiment

Principle

A beam of neutral atoms possessing a magnetic moment μ⃗\vec{\mu} passing through a non-uniform magnetic field experiences a force

Fz=μz∂Bz∂zF_z = \mu_z \frac{\partial B_z}{\partial z}

If space quantization is real, μz\mu_z takes only discrete values, so the beam should split into a discrete number of beams.

Set-up

  1. Source: Silver (Ag) is heated in an electric oven; atoms escape through a small hole and form a beam.
  2. Collimation: The beam is passed through narrow slits to make it a fine pencil.
  3. Magnetic field: The beam passes between specially shaped pole pieces — one flat, one knife-edged — producing a strong, strongly non-uniform field along the zz-axis.
  4. Detector: Atoms are collected on a glass plate, where they form a deposit visible as a thin line.

Working

The whole apparatus is enclosed in a high vacuum to avoid collisions. The beam travels along the xx-axis; the inhomogeneous field is along zz. Atoms with different values of μz\mu_z experience different vertical forces and are deflected by different amounts, producing separate traces on the plate.

Results

  • A beam of silver atoms splits into two distinct traces, symmetric about the undeflected position.
  • This shows the beam is split into two beams, i.e. space quantization is real.
  • Silver has one unpaired electron in the 5s5s state, so l=0l = 0 and ml=0m_l = 0. Classically and from the old quantum theory, the beam should not split at all. The observed splitting into two therefore cannot come from orbital motion.

Conclusion concerning the Vector Atom Model

The two beams arise from the spin of the electron. The spin quantum number is s=12s = \tfrac{1}{2}, so ms=±12m_s = \pm \tfrac{1}{2}, giving exactly two orientations of the spin magnetic moment in the field. The experiment thus:

  1. Proves the existence of electron spin and spin magnetic moment μs=s(s+1) μB\mu_s = \sqrt{s(s+1)}\,\mu_B.
  2. Confirms space quantization of angular momentum in a magnetic field.
  3. Shows that the magnetic moment of the electron is due to spin, not orbital motion, in the ss-state.
  4. Supports the vector atom model, in which L⃗\vec{L}, S⃗\vec{S} and J⃗\vec{J} are treated as quantized vectors coupled to give a resultant J⃗\vec{J}.

Sommerfeld's Modification of Bohr's Model

Bohr's model assumed circular orbits only and could not explain the fine structure of spectral lines or the splitting in magnetic fields. Sommerfeld (1916) extended it as follows:

  1. Elliptical orbits: Besides circular orbits, electrons may move in ellipses with the nucleus at one focus. The shape is fixed by the azimuthal (orbital) quantum number kk (now ll), where k=1,2,…,nk = 1, 2, \ldots, n; k=nk = n gives a circle.
  2. Quantization of the major axis: The semi-major axis aa depends only on nn: a=n2h2ε0πme2a = \frac{n^2 h^2 \varepsilon_0}{\pi m e^2} so all orbits with the same nn have the same major axis but different eccentricities.
  3. Relativistic correction: The electron in an elliptical orbit moves faster near the nucleus (perihelion), so its mass increases relativistically. This makes orbits of the same nn but different kk have slightly different energies, producing the fine structure of spectral lines.
  4. New quantum number: The magnetic quantum number mm was introduced to describe the orientation of the orbit in space, leading to the space quantization later confirmed by the Stern–Gerlach experiment.
  5. Sommerfeld's relation: The energy in the relativistic treatment becomes

En,k=−me48ε02h2⋅1n2[1+α2n(1k−34n)]E_{n,k} = -\frac{m e^4}{8\varepsilon_0^2 h^2}\cdot\frac{1}{n^2}\left[1 + \frac{\alpha^2}{n}\left(\frac{1}{k} - \frac{3}{4n}\right)\right]

where α=e24πε0ℏc≈1137\alpha = \dfrac{e^2}{4\pi\varepsilon_0 \hbar c} \approx \dfrac{1}{137} is the fine structure constant. This explained the observed doublets in hydrogen and the alkali spectra, which Bohr's model could not.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2081 · PHY. 201 · 10 marks

Draw the circuit diagram of a class A FET amplifier and explain its operation.
OR
Discuss Thevenin's and Norton's Theorem with their applications. Write down the Steps to a typical electric circuit through Norton's Theorem.

Answer

Class A FET Amplifier

Circuit diagram (self-bias common-source amplifier)

                +V_DD
                  |
                [R_D]
                  |
                  +---------||---------o  V_out
                  |        C_C2
                 (D)
                  |
 V_in o--||--+---(G) FET
        C_C1 |    (S)
             |     |
           [R_G]   +-------+
             |     |       |
            GND  [R_S]   [C_S]
                   |       |
                   +-------+
                      |
                     GND

The input signal is applied to the gate through the coupling capacitor CC1C_{C1}. RGR_G connects the gate to ground. The source is grounded through RSR_S with the bypass capacitor CSC_S in parallel. The drain is connected to VDDV_{DD} through RDR_D, and the output is taken from the drain through the coupling capacitor CC2C_{C2}.

Operation

DC bias. The gate is at 0 V DC through RGR_G, and the drain current produces VS=IDRSV_S = I_D R_S, so VGS=−IDRSV_{GS} = -I_D R_S (self-bias). The Q-point is set near the middle of the load line: VDS=VDD−ID(RD+RS)V_{DS} = V_{DD} - I_D(R_D+R_S)

AC operation. The signal changes VGSV_{GS}, which changes the drain current, id=gmvgsi_d = g_m v_{gs}. The varying current through RDR_D gives the output voltage vout=−gmRD vgs,Av=−gmRDv_{out} = -g_m R_D\, v_{gs}, \qquad A_v = -g_m R_D The negative sign shows a 180∘180^\circ phase shift.

Class A. The Q-point is chosen so that the FET conducts for the full 360∘360^\circ of the input cycle. This gives low distortion, but the efficiency is low (at most about 25% for resistive load).

Capacitors. CC1C_{C1} and CC2C_{C2} block DC, so bias is not disturbed by the source or load. CSC_S bypasses RSR_S for AC so that the gain is not reduced.


OR

Thevenin's and Norton's Theorems

Thevenin's theorem. Any linear bilateral network can be replaced, as seen from two terminals, by a voltage source VthV_{th} in series with a resistance RthR_{th}. VthV_{th} is the open-circuit voltage and RthR_{th} is the resistance seen with all independent sources killed (voltage sources shorted, current sources opened).

Norton's theorem. The same network can be replaced by a current source INI_N in parallel with RNR_N. INI_N is the short-circuit current and RN=RthR_N = R_{th}.

Vth=INRN,RN=RthV_{th} = I_N R_N, \qquad R_N = R_{th}

Applications

  1. Reduces a complex network to a simple two-element equivalent.
  2. Gives the maximum power transfer condition (RL=RthR_L = R_{th}).
  3. Easy recalculation when only the load changes.
  4. Used in transistor biasing and in finding input/output impedance of amplifiers.
  5. Used in source-load matching in power and communication circuits.

Steps to solve a circuit by Norton's theorem

  1. Remove the load RLR_L from terminals aa-bb.
  2. Short aa-bb and find the short-circuit current INI_N.
  3. Kill all independent sources and find RNR_N looking into aa-bb.
  4. Draw the Norton equivalent, INI_N in parallel with RNR_N.
  5. Reconnect RLR_L across aa-bb.
  6. Find the load current by current division: IL=INRNRN+RL,VL=ILRLI_L = I_N\frac{R_N}{R_N+R_L}, \qquad V_L = I_L R_L

Example. V=12V = 12 V, R1=4 ΩR_1 = 4\ \Omega in series, R2=6 ΩR_2 = 6\ \Omega across the terminals, RL=3 ΩR_L = 3\ \Omega.

  • IN=12/4=3I_N = 12/4 = 3 A (short across the terminals)
  • RN=4∥6=2.4 ΩR_N = 4\parallel 6 = 2.4\ \Omega
  • IL=3×2.42.4+3=1.33I_L = 3\times\dfrac{2.4}{2.4+3} = 1.33 A
  • VL=1.33×3=4V_L = 1.33\times 3 = 4 V

Answer checked by Claude Sonnet · Oct 21, 2026

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  • 2081 · PHY. 201 · 8 marks

Explain the laws of successive radioactive disintegration. Use this law to explain any one natural radioactive series.

Answer

Laws of Successive Radioactive Disintegration

When a radioactive nuclide decays, it produces a daughter nuclide which may itself be radioactive. The daughter then decays to a granddaughter, and so on, forming a radioactive series (decay chain). The number of undecayed atoms of each member at any instant is governed by two laws.

1. Law of successive disintegration (parent–daughter growth)

Let a parent P decay with disintegration constant λ1\lambda_1 into a daughter D, which decays with constant λ2\lambda_2:

P→λ1D→λ2(stable or further daughter)\text{P} \xrightarrow{\lambda_1} \text{D} \xrightarrow{\lambda_2} \text{(stable or further daughter)}

Let N1N_1 and N2N_2 be the number of atoms of P and D at time tt, with N1=N0N_1 = N_0 at t=0t=0 and N2=0N_2 = 0 at t=0t=0.

For the parent: dN1dt=−λ1N1⇒N1=N0e−λ1t\frac{dN_1}{dt} = -\lambda_1 N_1 \quad\Rightarrow\quad N_1 = N_0 e^{-\lambda_1 t}

For the daughter, the rate of change is the rate of its production from the parent minus its own rate of decay: dN2dt=λ1N1−λ2N2=λ1N0e−λ1t−λ2N2\frac{dN_2}{dt} = \lambda_1 N_1 - \lambda_2 N_2 = \lambda_1 N_0 e^{-\lambda_1 t} - \lambda_2 N_2

Solving this first-order linear differential equation with N2=0N_2 = 0 at t=0t = 0 gives the law of successive disintegration:

N2=λ1N0λ2−λ1(e−λ1t−e−λ2t)\boxed{N_2 = \frac{\lambda_1 N_0}{\lambda_2 - \lambda_1}\left(e^{-\lambda_1 t} - e^{-\lambda_2 t}\right)}

2. Law of radioactive equilibrium

The activity of the daughter is A2=λ2N2A_2 = \lambda_2 N_2:

A2=λ1λ2N0λ2−λ1(e−λ1t−e−λ2t)A_2 = \frac{\lambda_1 \lambda_2 N_0}{\lambda_2 - \lambda_1}\left(e^{-\lambda_1 t} - e^{-\lambda_2 t}\right)

Two important special cases follow:

(a) Secular (permanent) equilibrium — when the parent is very long-lived compared with the daughter, i.e. λ1≪λ2\lambda_1 \ll \lambda_2 (parent half-life ≫\gg daughter half-life). After a sufficiently long time tt (t≫1/λ2t \gg 1/\lambda_2), the term e−λ2te^{-\lambda_2 t} becomes negligible, so

N2≈λ1λ2−λ1N0e−λ1t≈λ1λ2N1N_2 \approx \frac{\lambda_1}{\lambda_2 - \lambda_1} N_0 e^{-\lambda_1 t} \approx \frac{\lambda_1}{\lambda_2} N_1

∴λ1N1=λ2N2i.e.A1=A2\therefore \quad \lambda_1 N_1 = \lambda_2 N_2 \quad\text{i.e.}\quad A_1 = A_2

The daughter then decays at the same rate as it is produced, and the ratio N1:N2=λ2:λ1N_1 : N_2 = \lambda_2 : \lambda_1 stays constant.

(b) Transient equilibrium — when the parent half-life is somewhat longer than the daughter's (λ1<λ2\lambda_1 < \lambda_2 but not ≪\ll). After long time, e−λ2t→0e^{-\lambda_2 t} \to 0 and

N2=λ1λ2−λ1N1,A2=λ2λ2−λ1A1N_2 = \frac{\lambda_1}{\lambda_2 - \lambda_1} N_1, \qquad A_2 = \frac{\lambda_2}{\lambda_2 - \lambda_1} A_1

so the daughter activity exceeds the parent activity by the constant factor λ2/(λ2−λ1)\lambda_2/(\lambda_2 - \lambda_1).


Application to a natural radioactive series (Uranium series)

The uranium (4n + 2) series starts from 92238U^{238}_{92}\text{U} and ends in stable lead 82206Pb^{206}_{82}\text{Pb}. Each step is a successive disintegration, and the whole chain is described by the above law applied step by step.

92238U→α, T1/2=4.5×109 y90234Th→β91234Pa→β92234U→α90230Th→α88226Ra→α86222Rn→α⋯→82206Pb^{238}_{92}\text{U} \xrightarrow{\alpha,\ T_{1/2}=4.5\times10^9\text{ y}} {}^{234}_{90}\text{Th} \xrightarrow{\beta} {}^{234}_{91}\text{Pa} \xrightarrow{\beta} {}^{234}_{92}\text{U} \xrightarrow{\alpha} {}^{230}_{90}\text{Th} \xrightarrow{\alpha} {}^{226}_{88}\text{Ra} \xrightarrow{\alpha} {}^{222}_{86}\text{Rn} \xrightarrow{\alpha} \cdots \xrightarrow{} {}^{206}_{82}\text{Pb}

Explanation using the law:

  1. Parent 238^{238}U is extremely long-lived (T1/2=4.5×109T_{1/2} = 4.5 \times 10^9 years), so its decay constant λ1\lambda_1 is very small. Its number at any time is N1=N0e−λ1tN_1 = N_0 e^{-\lambda_1 t}.

  2. Daughter 234^{234}Th has a much shorter half-life (2424 days), so λ2≫λ1\lambda_2 \gg \lambda_1. This satisfies the condition for secular equilibrium. After a short build-up time, the rate at which 234^{234}Th is produced from 238^{238}U equals the rate at which it decays: λ1N1=λ2N2⇒AU=ATh\lambda_1 N_1 = \lambda_2 N_2 \quad\Rightarrow\quad A_{\text{U}} = A_{\text{Th}}

  3. The same argument applies to every short-lived member down the chain (234^{234}Pa, 234^{234}U, 230^{230}Th, 226^{226}Ra, 222^{222}Rn, etc.). Since all of them have half-lives far shorter than 238^{238}U, each reaches secular equilibrium with its parent, and ultimately

λUNU=λThNTh=λRaNRa=⋯=A (constant)\lambda_{\text{U}} N_{\text{U}} = \lambda_{\text{Th}} N_{\text{Th}} = \lambda_{\text{Ra}} N_{\text{Ra}} = \cdots = A \ (\text{constant})

That is, the activity of every member of the series is equal once equilibrium is established. This is why a uranium ore sample shows the same activity for U, Th, Ra and Rn, and why the amount of radium present in uranium ore is fixed at about 11 part in 3×1063 \times 10^6 of uranium.

  1. The end product 206^{206}Pb is stable (λ=0\lambda = 0), so it simply accumulates. Its amount grows with time and provides the basis of lead–uranium dating of rocks and minerals.

Thus the laws of successive disintegration explain both the growth of each daughter in the uranium series and the secular equilibrium that fixes the relative abundances of all members of the series.

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  • 2081 · PHY. 201 · 8 marks

Draw a circuit following a stable multivibrator and explain its operation. What is the frequency of the circuit?

Answer

The question refers to the astable multivibrator, a circuit with no stable state that switches continuously between two quasi-stable states and acts as a square-wave generator.

Circuit

        +V_CC
   -------+-----------+-----------+-----------+
          |           |           |           |
        [R_C1]      [R_B2]      [R_B1]      [R_C2]
          |           |           |           |
          +---C_1-----+           +-----C_2---+
          |           |           |           |
          |           +--->B2   B1<---+       |
          |                 |   |             |
          +--------------- C1   C2 -----------+
                         (Q1)   (Q2)
                          E1     E2
                          |       |
                         GND     GND

In words, the circuit has two identical NPN transistors Q1Q_1, Q2Q_2. The collector of Q1Q_1 is joined to the base of Q2Q_2 through capacitor C1C_1, and the collector of Q2Q_2 is joined to the base of Q1Q_1 through capacitor C2C_2 (cross-coupling). Collector resistors RC1R_{C1}, RC2R_{C2} and base resistors RB1R_{B1}, RB2R_{B2} connect to +VCC+V_{CC}, and the emitters are grounded. Output is taken from either collector.

Operation

  1. When the supply is switched on, no two transistors are exactly alike, so one conducts a little more, say Q1Q_1. Regenerative feedback through the coupling capacitors quickly drives Q1Q_1 into saturation and Q2Q_2 into cut-off.
  2. With Q1Q_1 ON, its collector falls to about 0 V. This pushes the base of Q2Q_2 negative through C1C_1, holding Q2Q_2 OFF.
  3. Capacitor C1C_1 now charges from VCCV_{CC} through RB2R_{B2}, and the base voltage of Q2Q_2 rises towards +VCC+V_{CC}. When it reaches about 0.7 V, Q2Q_2 begins to conduct.
  4. As Q2Q_2 turns ON, its collector voltage falls. This drop passes through C2C_2 to the base of Q1Q_1 and turns Q1Q_1 OFF. The roles are exchanged: Q2Q_2 saturated, Q1Q_1 cut off.
  5. Now C2C_2 charges through RB1R_{B1} until Q1Q_1 turns ON again, and the cycle repeats.

The collector voltage of each transistor is therefore a rectangular wave, with the two outputs in opposite phase.

Frequency

The time for which one transistor stays OFF is 0.693 RBC0.693\,R_B C, so

T=0.693 (RB1C1+RB2C2)T = 0.693\,(R_{B1}C_1 + R_{B2}C_2)

For a symmetrical circuit (RB1=RB2=RR_{B1}=R_{B2}=R, C1=C2=CC_1=C_2=C):

T=1.386 RC,f=1T=11.386 RC≈0.72RCT = 1.386\,RC, \qquad f = \frac{1}{T} = \frac{1}{1.386\,RC} \approx \frac{0.72}{RC}

The duty cycle is 50%.

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  • 2081 · PHY. 201 · 6 marks

Answer any TWO of the following: [2×3=6] a) Explain in brief the dispersive and resolving power of grating. b) Explain in brief about astigmatism. c) What is common mode rejection ratio (CMRR) in operational amplifier? d) Distinguish Rutherford and Compton scattering.

Answer

a) Dispersive and resolving power of a grating

Dispersive power of a grating is its ability to separate light of different wavelengths into distinct directions. It is measured by the angular dispersion, defined as the rate of change of the diffraction angle with wavelength:

dθdλ=ndcos⁡θ\frac{d\theta}{d\lambda} = \frac{n}{d\cos\theta}

where nn is the order of the spectrum, dd is the grating element (grating constant), and θ\theta is the diffraction angle. A larger value of dθdλ\dfrac{d\theta}{d\lambda} means the grating spreads the wavelengths more widely, so it has greater dispersive power. Dispersion increases with order nn and decreases as the grating element dd increases.

Resolving power of a grating is its ability to distinguish two spectral lines of nearly equal wavelengths as separate. It is defined as

R=λdλ=nNR = \frac{\lambda}{d\lambda} = nN

where dλd\lambda is the smallest wavelength difference that can just be resolved, nn is the order, and NN is the total number of lines on the illuminated part of the grating. Thus resolving power increases with the order of the spectrum and with the total number of ruled lines. A grating with more lines and used in a higher order can resolve finer wavelength differences.


b) Astigmatism

Astigmatism is a defect of vision (or of a lens) in which the eye cannot focus both horizontal and vertical lines sharply at the same time. It arises when the refracting surfaces of the eye, especially the cornea or the lens, are not perfectly spherical but have different curvatures in different meridians. As a result, the eye has different focal lengths for different planes, so a point object is imaged not as a point but as two short perpendicular lines (focal lines) at different distances.

Effect: A person with astigmatism sees objects distorted — lines in one direction appear sharp while lines perpendicular to them appear blurred. For example, a cross may appear with one arm clear and the other blurred.

Correction: It is corrected by using a cylindrical lens, which has different curvature in one direction only. The cylindrical lens is placed with its axis in the appropriate direction so that it compensates for the unequal curvature of the eye and brings the rays from all meridians to a common focus on the retina.


c) Common Mode Rejection Ratio (CMRR)

An operational amplifier has two input terminals. A common-mode signal is the voltage applied equally to both inputs, while a differential signal is the difference between the two inputs. An ideal op-amp should amplify only the differential signal and give zero output for a common-mode signal. In practice, a small common-mode output appears.

The Common Mode Rejection Ratio is defined as the ratio of the differential voltage gain to the common-mode voltage gain:

CMRR=AdAc\text{CMRR} = \frac{A_d}{A_c}

where AdA_d is the differential gain and AcA_c is the common-mode gain. It is usually expressed in decibels:

CMRR (dB)=20log⁡10(AdAc)\text{CMRR (dB)} = 20\log_{10}\left(\frac{A_d}{A_c}\right)

A high CMRR means the amplifier strongly amplifies the desired difference signal while rejecting unwanted signals common to both inputs (such as noise and interference). An ideal op-amp has infinite CMRR; practical op-amps have values of the order of 10410^4 to 10610^6 (80–120 dB).


d) Rutherford and Compton scattering

Rutherford scatteringCompton scattering
Scattering of charged particles (e.g. alpha particles) by the nucleus of an atom.Scattering of X-ray photons by loosely bound or free electrons.
The incident particle is heavy and charged; it is deflected by the Coulomb force of the nucleus.The incident particle is a photon; it collides with an electron and transfers part of its energy.
The wavelength of the scattered particle is unchanged.The wavelength of the scattered photon increases (Compton shift), Δλ=hm0c(1−cos⁡θ)\Delta\lambda = \dfrac{h}{m_0c}(1-\cos\theta).
Explained by classical Coulomb interaction; the scattering angle depends on impact parameter.Explained by photon–electron collision using conservation of energy and momentum (quantum theory).
Scattered particles show a continuous distribution of angles; no change in energy of the particle.Scattered photons show a definite shift in wavelength depending on the scattering angle.
Confirms the existence of a small, massive, positively charged nucleus.Confirms the particle (photon) nature of electromagnetic radiation.

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  • 2081 · PHY. 201 · 10 marks

Answer all questions [4×2.5=10] a) What are the applications of holography? b) Briefly describe the objectives of Large Hadron Collider (LHC). c) What is gravitational red shift? d) Describe X-OR gate with truth table.

Answer

(a) Applications of holography

Holography is the technique of recording and reconstructing the complete wavefront (both amplitude and phase) of light using the interference of a reference beam and an object beam. Its main applications are:

  1. Holographic data storage — data is stored throughout the volume of a medium, giving very high storage density and fast parallel readout.
  2. Holographic interferometry (non-destructive testing) — small deformations, stresses and vibrations in materials, tyres and turbine blades are detected by comparing two holograms.
  3. Three-dimensional imaging and display — true 3-D images used in art, advertising, museums and security holograms on currency, credit cards and ID cards.
  4. Holographic optical elements (HOEs) — used as lenses, gratings and filters in scanners, optical computers and head-up displays.
  5. Medical and biological imaging — holographic microscopy and holographic endoscopy for imaging internal organs and cells.
  6. Particle size analysis and velocimetry — measurement of size, position and velocity of moving particles in fluids.
  7. Acoustic holography — imaging with sound waves for underwater detection and seismic studies.

(b) Objectives of the Large Hadron Collider (LHC)

The LHC is the world's largest and most powerful particle accelerator, built by CERN near Geneva in a 27 km underground ring. Its main objectives are:

  1. To discover the Higgs boson — the particle responsible for giving mass to other particles, thus confirming the Standard Model (achieved in 2012).
  2. To search for new physics beyond the Standard Model — such as supersymmetry, extra dimensions and new heavy particles.
  3. To study the conditions of the early universe — by colliding heavy lead ions to produce quark–gluon plasma, the state of matter just after the Big Bang.
  4. To explain the matter–antimatter asymmetry — why the universe contains more matter than antimatter.
  5. To investigate the nature of dark matter and dark energy and to look for the possible existence of microscopic black holes.
  6. To test theories of gravity and unification of the fundamental forces at very high energies.

(c) Gravitational red shift

Gravitational red shift is the increase in the wavelength (shift towards the red end of the spectrum) of electromagnetic radiation when it travels from a region of stronger gravitational field to a region of weaker gravitational field, i.e. away from a massive body.

According to Einstein's general theory of relativity, a photon climbing out of a gravitational potential well loses energy. Since its energy is (E = h\nu), a decrease in energy means a decrease in frequency (\nu) and hence an increase in wavelength (\lambda). The fractional shift is

[ \frac{\Delta \lambda}{\lambda} = \frac{GM}{Rc^{2}} ]

where (M) and (R) are the mass and radius of the body, (G) is the gravitational constant and (c) is the speed of light. The effect is very small for the Earth but measurable for the Sun and is large for white dwarfs and neutron stars. It is a direct experimental confirmation of general relativity.


(d) X-OR gate

The X-OR (Exclusive-OR) gate is a two-input logic gate whose output is HIGH (1) only when the two inputs are different, and LOW (0) when the inputs are the same. Its Boolean expression is

[ Y = A \oplus B = A\bar{B} + \bar{A}B ]

Truth table:

(A)(B)(Y = A \oplus B)
000
011
101
110

The X-OR gate is used as a parity checker/generator, in half adders and full adders, and in digital comparators.

Answer checked by Claude Haiku · Oct 21, 2026

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  • 2081 · PHY. 201 · 5 marks

A Ramsden's eyepiece is to have an effective focal length of 3 cm. Calculate the focal length of its lenses and their distance of separation.

Answer

For a Ramsden’s eyepiece, the two plano-convex lenses have equal focal length (f), and their separation is

[ d=\frac{2f}{3} ]

The equivalent focal length (F) of two thin lenses separated by distance (d) is

[ \frac{1}{F}=\frac{1}{f_1}+\frac{1}{f_2}-\frac{d}{f_1f_2} ]

Since (f_1=f_2=f),

[ \frac{1}{F}=\frac{2}{f}-\frac{d}{f^2} ]

Putting (d=\frac{2f}{3}),

[ \frac{1}{F}=\frac{2}{f}-\frac{2f/3}{f^2} =\frac{2}{f}-\frac{2}{3f} =\frac{4}{3f} ]

So,

[ F=\frac{3f}{4} ]

Given effective focal length,

[ F=3\text{ cm} ]

[ 3=\frac{3f}{4} ]

[ f=4\text{ cm} ]

Thus each lens has focal length

[ \boxed{f=4\text{ cm}} ]

Distance of separation:

[ d=\frac{2f}{3}=\frac{2\times 4}{3} ]

[ \boxed{d=\frac{8}{3}\text{ cm}=2.67\text{ cm}} ]

So, the focal length of each lens is 4 cm, and the distance between the two lenses is 2.67 cm.

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  • 2081 · PHY. 201 · 5 marks

How many orders will be observed by a grating having 4000 lines/cm if it is illuminated by a visible light of wave length in the range of 4000 Å to 7500 Å?

Answer

Given:
Number of lines per cm, (N = 4000)
Grating element,
[ d = \frac{1}{N} = \frac{1}{4000}\ \text{cm} = 2.5\times 10^{-4}\ \text{cm} ] [ d = 2.5\times 10^{-4}\times 10^8\ \text{Å} = 25000\ \text{Å} ]

Wavelength range:
[ \lambda_{\min} = 4000\ \text{Å},\qquad \lambda_{\max} = 7500\ \text{Å} ]

For a diffraction grating,
[ d\sin\theta = n\lambda ] The maximum order is obtained when (\sin\theta = 1):
[ n_{\max} = \frac{d}{\lambda} ]

For (\lambda = 4000\ \text{Å}):
[ n_{\max} = \frac{25000}{4000} = 6.25 ] So the maximum possible order is (6).

For (\lambda = 7500\ \text{Å}):
[ n_{\max} = \frac{25000}{7500} = 3.33 ] So only up to the (3)rd order is complete for the whole visible range.

Thus orders (n = 1,2,3) are complete, while (n = 4,5,6) appear only for shorter wavelengths. No order beyond (n = 6) is possible.

[ \boxed{\text{Number of orders observed on each side} = 6} ]

Including the central zero order, the total number of orders is
[ 2\times 6 + 1 = \boxed{13} ]

So the grating will show 6 orders on each side of the central maximum.

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  • 2081 · PHY. 201 · 5 marks

Calculate the time required for 10% of a sample of thorium to disintegrate. Assume the half life of thorium to be 1.4×10101.4 \times 10^{10} years.

Answer

Given:

  • Half-life, (T_{1/2}=1.4\times 10^{10}) years
  • Fraction disintegrated (=10%)
  • Fraction remaining, (\dfrac{N}{N_0}=90%=0.9)

Formula: [ t=\frac{T_{1/2}}{\ln 2}\ln\left(\frac{N_0}{N}\right) ]

Substitution: [ t=\frac{1.4\times 10^{10}}{0.693}\ln\left(\frac{1}{0.9}\right) ] [ t=\frac{1.4\times 10^{10}}{0.693}\times 0.10536 ] [ t=2.128\times 10^9 \text{ years} ]

[ \boxed{t \approx 2.13\times 10^9 \text{ years}} ]

So, about 2.13 billion years are required for 10% of the thorium sample to disintegrate.

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  • 2081 · PHY. 201 · 5 marks

X-rays of wavelength 1.0×10−11 m1.0 \times 10^{-11} \, \text{m} are incident on free stationary electrons. What is the wavelength of the X-ray that are scattered directly backwards? What is the energy gained by the scattered electron's in this case. Given : me=9.11×10−31 kgm_e = 9.11 \times 10^{-31} \, \text{kg} c=3×108 m/sc = 3 \times 10^8 \, \text{m/s} h=6.62×10−34 JSh = 6.62 \times 10^{-34} \, \text{JS}

Answer

Given: λ=1.0×10−11\lambda = 1.0\times10^{-11} m, scattering angle ϕ=180∘\phi = 180^\circ (directly backwards), h=6.62×10−34h = 6.62\times10^{-34} J s, me=9.11×10−31m_e = 9.11\times10^{-31} kg, c=3×108c = 3\times10^{8} m/s.

Compton wavelength of the electron

hmec=6.62×10−349.11×10−31×3×108=2.42×10−12 m\frac{h}{m_e c} = \frac{6.62\times10^{-34}}{9.11\times10^{-31}\times 3\times10^{8}} = 2.42\times10^{-12}\ \text{m}

Wavelength of scattered X-rays

Δλ=hmec(1−cos⁡ϕ)=2.42×10−12×2=4.84×10−12 m\Delta\lambda = \frac{h}{m_e c}(1-\cos\phi) = 2.42\times10^{-12}\times 2 = 4.84\times10^{-12}\ \text{m}

λ′=λ+Δλ=1.0×10−11+0.484×10−11≈1.48×10−11 m\lambda' = \lambda + \Delta\lambda = 1.0\times10^{-11} + 0.484\times10^{-11} \approx 1.48\times10^{-11}\ \text{m}

Energy gained by the electron (equal to the energy lost by the photon)

K=hc(1λ−1λ′)=6.62×10−34×3×108(11.0×10−11−11.484×10−11)K = hc\left(\frac{1}{\lambda}-\frac{1}{\lambda'}\right) = 6.62\times10^{-34}\times3\times10^{8}\left(\frac{1}{1.0\times10^{-11}}-\frac{1}{1.484\times10^{-11}}\right)

K=1.986×10−25×3.26×1010≈6.5×10−15 J≈40 keVK = 1.986\times10^{-25}\times 3.26\times10^{10} \approx 6.5\times10^{-15}\ \text{J} \approx 40\ \text{keV}

So the scattered X-ray has wavelength 1.48×10−111.48\times10^{-11} m, and the electron gains about 6.5×10−156.5\times10^{-15} J (about 40 keV).

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  • 2081 · PHY. 201 · 5 marks

A dc and ac voltmeter were used to measure the output voltage from a filter circuit. If the readings of the two voltmeters are 25 volt and 2.5 volt respectively, calculate the ripple factor of the filter circuit.

Answer

Given:

  • DC voltmeter reading, (V_{dc} = 25\ \text{V})
  • AC voltmeter reading, (V_{rms} = 2.5\ \text{V})

Formula: [ \text{Ripple factor},\ r = \frac{V_{rms}}{V_{dc}} ]

Calculation: [ r = \frac{2.5}{25} = 0.1 ]

In percentage, [ r = 0.1 \times 100% = 10% ]

Result: The ripple factor of the filter circuit is 0.1, i.e. 10%.

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