Physics

UPSC Physics 2025

All 16 questions from the 2025 Civil Services Mains Physics paper across 2 papers — 800 marks in total. Each question comes with a detailed evaluation rubric, directive word analysis, and model answer points.

16Questions
800Total marks
2Papers
2025Exam year

Paper I

8 questions · 400 marks
Q1
50M Compulsory derive Classical mechanics, gravitation, relativity, optics

(a) Consider a large stationary cylinder of inner radius R. A smaller solid cylinder of radius r rolls without slipping inside the larger cylinder. Determine the equation of motion of the smaller cylinder. 10 (b) Derive the expression for the gravitational self-energy of a uniform solid sphere of mass M and radius R. 10 (c) A particle of rest mass 1 kg and velocity of magnitude 0·9c collides with a particle of mass 2 kg at rest. After collision the two particles coalesce and form a single particle of mass M and velocity V. Determine M and V. 10 (d) In a double slit Fraunhofer diffraction experiment, the slit width is 0·12 mm and the spacing between the two slits is 0·48 mm. The distance of the screen from the slits is 1·5 m. If the wavelength of the light used is 600 nm, determine (i) the missing orders of the interference maxima, and (ii) the distance between the central maxima and the first minima. 10 (e) A light beam of wavelength 600 nm produced by a 20 mW laser source is incident on a plane mirror. Determine : (i) number of photons per second striking the surface of the mirror. (ii) force exerted by the light beam on the mirror. 10

Answer approach & key points

Begin with clear statement of physical principles for each sub-part. For (a), set up Lagrangian with constraint; for (b), integrate gravitational potential energy; for (c), apply relativistic energy-momentum conservation; for (d), combine single-slit diffraction envelope with double-slit interference; for (e), use photon energy and radiation pressure concepts. Allocate approximately 20% time each to (a), (b), (c), (d), and (e) combined, with (e)(i) and (e)(ii) sharing that final 20%. Present derivations step-wise with final boxed answers for numerical parts.

  • (a) Rolling constraint: arc length relation (R-r)θ = rφ; correct Lagrangian with kinetic energy of CM plus rotational energy; equation of motion as simple harmonic oscillator with period depending on √(R-r)/g
  • (b) Gravitational self-energy: assemble sphere shell by shell; integration of -GM(r)dm/r from 0 to R; final result U = -3GM²/5R with correct handling of negative sign
  • (c) Relativistic collision: calculate γ = 1/√(1-0.9²) ≈ 2.294; conserve total energy and momentum; solve for M and V with M > 3kg due to kinetic energy conversion to mass
  • (d) Missing orders: condition d/a = 4 implies interference maxima at n=4,8,12... coincide with diffraction minima; first minima distance using y = λD/d for interference pattern
  • (e)(i) Photon flux: N = Pλ/(hc) ≈ 6.03 × 10¹⁶ photons/second; (e)(ii) Force: F = 2P/c = 2×20mW/c ≈ 1.33 × 10⁻¹⁰ N for perfect reflection
Q2
50M solve Rigid body dynamics, damped harmonic oscillator, special relativity

(a) A body moves about a point 'O' under no force, the principal moments of inertia at 'O' being 3A, 5A and 6A. The components of the initial angular velocity about the principal axes are ω₁ = n, ω₂ = 0 and ω₃ = n. Find the components ω₁, ω₂ and ω₃ for large values of time t. 20 (b) A harmonic oscillator is represented by the equation m d²x/dt² + γ dx/dt + kx = 0; where m = 0·25 kg, γ = 0·07 kg s⁻¹ and k = 85 Nm⁻¹. Determine (i) the period of oscillation, and (ii) the number of oscillations in which its amplitude will become half of its original value. 15 (c) Show that the electromagnetic wave equation is invariant under Lorentz transformations. 15

Answer approach & key points

This is a multi-part problem requiring analytical solutions: spend approximately 40% of effort on part (a) given its 20 marks, using Euler's equations for force-free rigid body motion; allocate 30% each to parts (b) and (c). For (b), solve the damped harmonic oscillator differential equation and extract numerical values; for (c), apply Lorentz transformation to electromagnetic wave equation and demonstrate invariance. Present derivations step-by-step with clear final boxed answers.

  • Part (a): Apply Euler's equations for force-free rotation, identify that motion occurs in 1-3 plane with I₁=3A, I₃=6A, use conservation of energy and angular momentum to find asymptotic behavior where ω₂→0 and ω₁, ω₃ approach constant values
  • Part (b): Identify underdamped regime (γ² < 4mk), calculate damped angular frequency ω' = √(k/m - γ²/4m²), find period T = 2π/ω', and determine logarithmic decrement to find number of oscillations for amplitude halving
  • Part (c): State Lorentz transformation equations, transform ∂²/∂x² - (1/c²)∂²/∂t² using chain rule, show wave operator remains invariant (∂²/∂x'² - (1/c²)∂²/∂t'² = ∂²/∂x² - (1/c²)∂²/∂t²)
  • Correct identification of intermediate axis instability in part (a) — rotation about axis with intermediate moment of inertia (I₂=5A) is unstable, causing ω₂ to decay
  • Numerical calculation in (b): ω' ≈ 18.44 rad/s, T ≈ 0.34 s, and n ≈ 31 oscillations for amplitude to halve using ln(2)/ln(A₁/A₂) relationship
  • Explicit demonstration that phase velocity c remains invariant under Lorentz transformation in part (c), connecting to Einstein's second postulate
Q3
50M derive Laser physics and rotational dynamics

(a) Consider a laser system consisting of an active medium placed between a pair of mirrors forming a resonator. Obtain an expression for the threshold population inversion required for the oscillations of laser. (20 marks) (b) For a He – Ne laser system, what will be the magnitude of $\Delta\omega_D$ which represents FWHM of the line shape function g($\omega$), if resonant frequency $\omega_0 = 3 \times 10^{15}$ s$^{-1}$ and temperature T = 300 K ? (10 marks) (c) A cube of mass M and side 'a' is rotating with angular velocity $\omega$ around one of its edges, which is, say, along the x-axis. Obtain the expressions for its angular momentum and kinetic energy. (Given that the $I_{XX} = \frac{2}{3} Ma^2$, $I_{YX} = -\frac{1}{4} Ma^2$ and $I_{ZX} = -\frac{1}{4} Ma^2$) (20 marks)

Answer approach & key points

Derive the threshold population inversion for laser oscillations in part (a) by balancing gain and cavity losses, showing how mirror reflectivity and spontaneous emission enter the condition. For part (b), calculate the Doppler-broadened linewidth using the Maxwell-Boltzmann distribution at 300 K. In part (c), construct the inertia tensor for the cube and use it to find angular momentum components and rotational kinetic energy, noting that ω is along x-axis but L has non-zero y,z components due to non-diagonal elements. Allocate roughly 40% time to (a), 20% to (b), and 40% to (c) based on marks distribution.

  • Part (a): Rate equation analysis showing gain coefficient γ(ν) = (N₂-N₁)B₂₁hνg(ν)/c and threshold condition γₜₕ = α + (1/2L)ln(1/R₁R₂)
  • Part (a): Final threshold population inversion expression (N₂-N₁)ₜₕ = 8πν²τₛₚ/c³g(ν₀) × loss terms, or equivalent with cavity lifetime τc
  • Part (b): Doppler broadening formula ΔνD = (2ν₀/c)√(2kTln2/m) or ΔωD = (2ω₀/c)√(2kTln2/m) for He-Ne with m = 20 amu (Neon)
  • Part (b): Numerical substitution yielding ΔωD ≈ 2π × 1.5 GHz or ~9.4 × 10⁹ rad/s (order of magnitude check essential)
  • Part (c): Recognition that ω⃗ = (ω, 0, 0) and use of Lᵢ = Σⱼ Iᵢⱼωⱼ giving Lx = (2/3)Ma²ω, Ly = -(1/4)Ma²ω, Lz = -(1/4)Ma²ω
  • Part (c): Kinetic energy calculation K = ½ω⃗·L⃗ = ½Iₓₓω² = (1/3)Ma²ω², or equivalently ½ΣᵢⱼIᵢⱼωᵢωⱼ
  • Part (c): Physical explanation that angular momentum is NOT parallel to angular velocity due to non-diagonal inertia tensor (principal axes ≠ coordinate axes)
Q4
50M derive Optics and elasticity

(a) Consider a thick lens of thickness t made of a material of relative refractive index n. Let $R_1$ and $R_2$ be the radii of curvature of its two surfaces. Obtain the system matrix of the lens. (15 marks) (b) Consider multiple reflections from a plane parallel film of thickness h and refractive index $n_2$ and derive an expression for the total reflectivity from the surface of the film. (20 marks) (c) A solid shaft of mass M, length $l$ and radius r is to be replaced by a lighter hollow shaft of the same length $l$ and having the same ratings of $\tau/\theta$, where $\tau$ is the couple and $\theta$ is the angle of twist. Estimate the percentage reduction in mass of the hollow shaft if the outer radius of the shaft is twice the inner radius. Assume the material of the new shaft is same as that of the replaced shaft. (15 marks)

Answer approach & key points

Begin with a brief introduction distinguishing matrix optics from Gaussian optics. For part (a), derive the system matrix by multiplying refraction and translation matrices in correct order. For part (b), use the method of summing infinite geometric series of reflected amplitudes with proper phase considerations. For part (c), equate torsional rigidity C = τ/θ for both shafts and solve for mass ratio. Allocate approximately 30% time to (a), 40% to (b) as it carries highest marks, and 30% to (c). Conclude with brief remarks on practical applications in optical instruments and mechanical engineering.

  • Part (a): Correct identification of individual matrices — refraction at first surface (R1), translation through thickness t, and refraction at second surface (R2) with proper sign convention
  • Part (a): Proper matrix multiplication order R2 × T × R1 yielding final system matrix with elements A, B, C, D satisfying AD-BC=1 for unimodular property
  • Part (b): Application of Fresnel coefficients at each interface with correct amplitude reflection/transmission coefficients r12, t12, r23, t23
  • Part (b): Inclusion of phase factor δ = (4πn2h cosθ2)/λ and summation of infinite series leading to Airy formula for reflectivity
  • Part (c): Expression for torsional rigidity C = πGr⁴/(2l) for solid shaft and C = πG(r₂⁴-r₁⁴)/(2l) for hollow shaft
  • Part (c): Setting equal rigidity ratings, substituting r₂ = 2r₁, solving for r₁ in terms of r, then calculating mass ratio and percentage reduction
  • Clear statement of assumptions: paraxial approximation for (a) and (b), same material (same G, ρ) for (c), thin film interference conditions
Q5
50M Compulsory solve Electromagnetism and thermodynamics

(a) Consider a point charge of 5 nC placed at a distance of 1 m from a perfect conducting plane (z = 0) of infinite extent. Find the electric field at a point (2, 2, 0) m and show that it is normal to the plane. (10 marks) (b) A rectangular coil consists of 50 closely wrapped turns and has dimensions of 0·5 m × 0·4 m. It carries a current of 1·5 A. If a uniform magnetic field B = 0·1 T is applied such that the direction of the magnetic field makes an angle of 60° with respect to the plane of the coil, what is the torque exerted on the coil by the magnetic field? (10 marks) (c) State and explain Kirchhoff's current law and Kirchhoff's voltage law. Derive these laws from the principles of charge conservation and energy conservation. (10 marks) (d) A parallel plate capacitor having circular plates of radius 10 cm is being charged. If the electric field at any instant within the capacitor changes at the rate 5·0 V m⁻¹ s⁻¹, calculate the magnetic intensity |H⃗| inside the capacitor. (10 marks) (e) A reversible heat engine operates with three reservoirs at 300 K, 400 K and 1200 K. It absorbs 1200 kJ energy as heat from the reservoir at 1200 K and delivers 400 kJ work. Determine the heat interactions with the other two reservoirs. (10 marks)

Answer approach & key points

Solve each sub-part systematically with equal time allocation (~20% each) since all carry equal marks. Begin with method of images for (a), torque formula for (b), clear statement-derivation pairs for (c), displacement current for (d), and entropy balance for (e). Present derivations before substituting numerical values, and conclude each part with physical verification of results.

  • Part (a): Apply method of images with image charge -5 nC at (0,0,-1); calculate field at (2,2,0) from both charges and prove tangential component vanishes on z=0 plane
  • Part (b): Use torque formula τ = NIAB sinθ with θ = 30° (angle between normal and B), not 60°; calculate magnitude correctly as 0.75 Nm
  • Part (c): State KCL (ΣI = 0 at junction) and KVL (ΣV = 0 in loop); derive KCL from ∮J·dA = -dQ/dt and KVL from ∮E·dl = -dΦB/dt = 0 for electrostatics
  • Part (d): Apply Maxwell-Ampère law with displacement current; use ∮H·dl = ε₀(dΦE/dt) to find H = (r/2)(dD/dt) = (rε₀/2)(dE/dt) at radius r
  • Part (e): Apply entropy conservation for reversible engine: Q₁/T₁ + Q₂/T₂ + Q₃/T₃ = 0 with Q₃ = +1200 kJ, W = 400 kJ; solve simultaneous equations for Q₁ and Q₂
Q6
50M derive Electromagnetism, AC circuits and statistical mechanics

(a) Consider a long straight wire of length L carrying a current I. Determine the magnetic vector potential $\vec{A}$ at a point P located at distance x from the wire. (20 marks) (b) As shown in the figure, a series circuit connected across a 200 V, 60 Hz line consists of a capacitor of capacitive reactance of 30 Ω, a non-inductive resistor of 44 Ω and a coil of inductive reactance 90 Ω and resistance 36 Ω. Determine: (i) Power factor of the circuit (ii) Power absorbed by the circuit (iii) Power dissipated in the coil (c) Consider a mixture of N_A molecules of a monatomic gas A and N_B molecules of a monatomic gas B. For this mixture, obtain the Helmholtz free energy and pressure. (The particle partition function for a monatomic gas is q = (2π mkT/h²)^(3/2) V).

Answer approach & key points

Derive the magnetic vector potential for the finite wire in part (a) using proper integration limits and Coulomb gauge, then solve the AC circuit problem in part (b) by calculating impedance, phase angle, and power quantities stepwise, and finally derive the Helmholtz free energy for the gas mixture in part (c) using Maxwell-Boltzmann statistics. Allocate approximately 40% effort to part (a) given its 20-mark weight in the original scheme, 35% to part (b) for its three numerical sub-parts, and 25% to part (c) for the statistical mechanics derivation.

  • Part (a): Setup of integral for vector potential using A = (μ₀I/4π)∫(dl'/|r-r'|) with proper coordinate system and limits from -L/2 to +L/2
  • Part (a): Final expression A = (μ₀I/4π)ln[(L/2+√(x²+L²/4))/(-L/2+√(x²+L²/4))]ẑ or equivalent, with discussion of infinite wire limit
  • Part (b)(i): Calculation of total impedance Z = √[(R₁+R₂)²+(X_L-X_C)²] = √[80²+60²] = 100Ω, leading to power factor cosφ = 80/100 = 0.8 lagging
  • Part (b)(ii)-(iii): Power absorbed P = VIcosφ = 200×2×0.8 = 320W (or I²R_total = 4×80 = 320W), and power in coil = I²R_coil = 4×36 = 144W
  • Part (c): Derivation of Helmholtz free energy F = -kT[N_A ln(q_A/N_A) + N_B ln(q_B/N_B) + N_A + N_B] using Stirling's approximation
  • Part (c): Pressure derivation P = -(∂F/∂V)_T = (N_A+N_B)kT/V = nRT/V, showing ideal gas mixture law with Dalton's law implicit
Q7
50M derive Gibbs phase rule, Van der Waals equation, conducting sphere in electric field

(a) A ternary system consists of three components (A, B and C) in equilibrium with two phases. Determine the number of degrees of freedom using the Gibb's phase rule and discuss the effect of pressure and temperature variations on the phase equilibrium. (b) Discuss briefly the considerations which led Van der Waals to modify the gas equation. What are the critical constants of a gas ? Calculate the values of these constants in terms of the constants of the Van der Waals equation. (15 marks) (c) Consider a conducting sphere of radius 'a' in a uniform electric field $\vec{E}$. Find the induced surface charge density on the sphere and determine the electric field $\vec{E}$ at a point P characterized by radius vector $\vec{r}$. (20 marks)

Answer approach & key points

This multi-part question requires deriving key results across thermodynamics and electrostatics. Allocate approximately 15% time to part (a) on Gibbs phase rule, 35% to part (b) on Van der Waals equation and critical constants, and 50% to part (c) on the conducting sphere problem which carries the highest marks. Structure with clear headings for each sub-part, present derivations step-by-step with justified assumptions, and conclude with physical interpretations of each result.

  • Part (a): Correct application of Gibbs phase rule F = C - P + 2 for ternary system (C=3, P=2) yielding F=3 degrees of freedom; discussion of how fixing temperature and pressure reduces variance
  • Part (b): Physical reasoning for Van der Waals modifications (finite molecular volume via 'b', intermolecular attractions via 'a'); derivation of critical constants T_c = 8a/27Rb, V_c = 3b, P_c = a/27b² from inflection point conditions (∂P/∂V)_T=0 and (∂²P/∂V²)_T=0
  • Part (c): Setup using superposition of uniform field and induced dipole potential; boundary condition V=constant on sphere surface; derivation of induced surface charge density σ = 3ε₀E₀cosθ; expression for total field at arbitrary point P using Legendre expansion or method of images
  • Clear statement of assumptions: ideal solution behavior for (a), single-phase fluid for (b), perfectly conducting isolated sphere for (c)
  • Dimensional consistency checks and limiting case verification (e.g., field reduces to applied field far from sphere)
  • Physical interpretation: screening effect of conductor, dipole moment of induced distribution p = 4πε₀a³E₀
Q8
50M derive Electromagnetic waves, chemical potential equilibrium, Planck's radiation law

(a) (i) In free space, an electric field ($\vec{E}$) is given by the following expression : $$\vec{E} = 10 \cos (\omega t - 100 x)\hat{j} \text{ V/m}$$ Find the angular frequency $\omega$ and the displacement current. (10 marks) (ii) An electromagnetic wave has its magnetic field $|\vec{B}| = 55 \times 10^{-8}$ T. Determine the magnitude of the Poynting vector. (5 marks) (b) Explain why, at equilibrium, the chemical potential of a component must be the same in all coexisting phases. Derive the equilibrium condition for a binary liquid-vapour system in terms of chemical potential. (15 marks) (c) Derive the Planck's radiation law for blackbody radiation using the Bose-Einstein distribution function. Explain how results from quantum statistics differ from classical results derived from the Rayleigh-Jeans law. (20 marks)

Answer approach & key points

Begin with a concise introduction stating the electromagnetic wave parameters in (a), then systematically solve for angular frequency using c = ω/k, displacement current via Maxwell's equations, and Poynting vector magnitude. For (b), explain chemical potential equality using entropy maximization/Gibbs free energy minimization, then derive the binary liquid-vapor equilibrium condition μₗ = μᵥ for each component. For (c), derive Planck's law by applying Bose-Einstein statistics to photon gas, obtaining energy density u(ν,T), then explicitly contrast with Rayleigh-Jeans divergence at high frequencies (ultraviolet catastrophe). Allocate approximately 25% time to (a), 35% to (b), and 40% to (c) based on mark distribution.

  • For (a)(i): Calculate ω = ck = 3×10⁸ × 100 = 3×10¹⁰ rad/s, and displacement current density J_d = ε₀(∂E/∂t) = 10ε₀ω sin(ωt-100x) A/m² with correct magnitude
  • For (a)(ii): Apply Poynting vector magnitude S = B²c/μ₀ = (55×10⁻⁸)² × 3×10⁸/(4π×10⁻⁷) ≈ 72.4 W/m² with proper unit conversion
  • For (b): Explain that at equilibrium, dS = 0 requires equal chemical potentials to prevent particle flow; derive μᵢˡ = μᵢᵛ for binary system using Gibbs-Duhem or equality of fugacities
  • For (c): Derive Planck's law starting from Bose-Einstein distribution ⟨n⟩ = 1/(e^(hν/kT)-1), obtaining u(ν,T) = (8πhν³/c³)/(e^(hν/kT)-1) and energy density integration
  • For (c) contrast: Explicitly show Rayleigh-Jeans u(ν,T) = 8πν²kT/c³ diverges as ν→∞ (ultraviolet catastrophe) while Planck's law converges, introducing quantum h

Paper II

8 questions · 400 marks
Q1
50M Compulsory explain Quantum mechanics and atomic physics

(a) Explain how the uncertainty in position is different from the uncertainty or inaccuracy of the measuring instruments. 10 marks (b) Determine the ground state energy of an electron in an infinite potential well of width of 2 Å. 10 marks (c) Draw the normal Zeeman pattern for ¹F₃—¹D₂ transition. 10 marks (d) In case of pure rotational states, if the temperature will be doubled, then calculate the rotational quantum number corresponding to maximum population density. [Assume that temperature is high] 10 marks (e) The quantum numbers of two electrons in a two-valence electron atom are n₁ = 6, l₁ = 3, s₁ = ½; n₂ = 5, l₂ = 1, s₂ = ½. Assuming L-S coupling, find the possible values of L and J. 10 marks

Answer approach & key points

Begin with part (a) explaining the fundamental distinction between Heisenberg's intrinsic quantum uncertainty and classical instrumental error, using clear conceptual distinction. For part (b), derive the ground state energy formula for infinite potential well and substitute a = 1 Å (half-width), showing E₁ = h²/(8ma²). Part (c) requires drawing the normal Zeeman triplet pattern with proper spacing and polarization labels. Part (d) involves deriving that J_max ≈ √(kT/2B) - ½, showing J_max increases by √2 when T doubles. Part (e) applies L-S coupling rules: L ranges from |l₁-l₂| to l₁+l₂ (i.e., 2,3,4), S=0 or 1, then J from |L-S| to L+S for each case. Allocate approximately 20% time to each part given equal marks distribution.

  • Part (a): Distinguish Heisenberg uncertainty principle (intrinsic, ΔxΔp ≥ ℏ/2) from classical instrumental error (reducible with better apparatus); cite that uncertainty principle holds even with perfect instruments
  • Part (b): Ground state energy E₁ = h²/(8ma²) = π²ℏ²/(2mL²) where L = 2a = 2 Å; calculate numerical value ~9.4 eV or 150 aJ
  • Part (c): Normal Zeeman effect shows triplet pattern: π component (Δm=0, unshifted) and σ⁺, σ⁻ components (Δm=±1, shifted by ±eℏB/2m); draw energy level diagram with proper spacing and label polarizations
  • Part (d): Rotational population N_J ∝ (2J+1)exp[-BJ(J+1)/kT]; find J_max by differentiation, yielding J_max ≈ √(kT/2B) - ½; when T→2T, J_max increases by factor of √2
  • Part (e): L-S coupling: L = 2,3,4; S = 0 (singlet) or 1 (triplet); for S=0: J=L so J=2,3,4; for S=1: J ranges from |L-1| to L+1 giving appropriate values for each L
Q2
50M prove Quantum mechanics and statistical mechanics

(a) What is the density of states? For a relativistic particle of rest mass μ, prove that the density of states in the extreme relativistic limit (E ≫ μc²) is g(E) = V/π²ℏ³c³ E² where g(E) = density of states, V = volume of the system containing the particle, E = total energy, c = velocity of light and h = Planck's constant. 20 marks (b) Obtain the expressions for reflection coefficient (R) and transmission coefficient (T) for reflected waves and transmitted waves from an infinite thin barrier. 15 marks (c) For a potential with the boundary conditions V(x) = {0, x < -a; V, -a < x < a; 0, x > a}, solve the Schrödinger's equation in one dimension and find out the conditions for tunnelling. 15 marks

Answer approach & key points

This question demands rigorous mathematical derivation across all three parts. Begin with a brief conceptual introduction to density of states, then allocate approximately 40% of effort to part (a) given its 20 marks weightage, with 30% each to parts (b) and (c). For (a), start from relativistic energy-momentum relation and integrate over phase space; for (b), apply boundary conditions at a delta-function barrier; for (c), solve the Schrödinger equation in three regions and match wavefunctions at boundaries to derive tunnelling conditions. Conclude with physical significance of each result.

  • Part (a): Definition of density of states as number of quantum states per unit energy interval; derivation starting from relativistic dispersion relation E² = p²c² + μ²c⁴ and phase space volume element
  • Part (a): Transformation to spherical coordinates in momentum space, integration over angular variables yielding factor 4π, and proper handling of extreme relativistic limit E ≫ μc² where E ≈ pc
  • Part (b): Setup of Schrödinger equation with delta-function potential V(x) = V₀δ(x); wavefunction ansatz in regions x<0 and x>0 with incident, reflected, and transmitted components
  • Part (b): Application of continuity condition at x=0 and discontinuity condition for derivative from integration across delta barrier; derivation of R = |B/A|² and T = |C/A|² with R + T = 1
  • Part (c): General solution forms in three regions: plane waves e^(±ikx) for |x|>a with k = √(2mE)/ℏ, and decaying/growing exponentials e^(±κx) for |x|<a with κ = √[2m(V-E)]/ℏ
  • Part (c): Matching conditions at x = ±a for wavefunction and first derivative; derivation of transcendental equation for bound states and tunnelling condition when E < V involving real κ
  • Physical interpretation: Connection between density of states and blackbody radiation/fermion systems; tunnelling applications to nuclear alpha decay and scanning tunnelling microscopy
Q3
50M calculate Atomic and molecular spectroscopy

(a) Find out the difference in frequencies of Lyman-alpha line in hydrogen and deuterium atoms. 15 marks (b) The Stern-Gerlach experiment is a landmark experiment in quantum mechanics. Discuss about the most important findings of this experiment. 15 marks (c) (i) From the pure rotational absorption spectra of a diatomic molecule (HF), the wave number difference between the consecutive rotational lines is found to be Δν̄ = 4050 m⁻¹. Calculate the following: (1) Rotational constant (2) Moment of inertia (3) Distance between two atoms (bond length) [Given, M_H = 1 u, M_F = 19 u] 10 marks (ii) The force constant of HCl molecule is 4.8×10⁵ dyne/cm. Calculate the wave numbers of Stokes and anti-Stokes lines, when excited with a radiation of wavelength 4358 Å. [Given, μ_HCl = 1.61×10⁻²⁴ g] 10 marks

Answer approach & key points

Begin with the directive to calculate and discuss across four sub-parts: spend ~30% time on (a) isotope shift calculation using reduced mass correction; ~25% on (b) discussing Stern-Gerlach findings with experimental schematic; ~25% on (c)(i) rotational spectroscopy of HF; and ~20% on (c)(ii) Raman spectroscopy of HCl. Structure as: brief theory → step-by-step derivation → numerical substitution → final result with units → physical significance.

  • (a) Reduced mass calculation for H (μ_H) and D (μ_D), Rydberg formula with reduced mass correction, frequency difference Δν = ν_H − ν_D ≈ 4.53×10¹¹ Hz or equivalent
  • (b) Experimental setup with inhomogeneous magnetic field, silver atom beam splitting into two discrete components, direct evidence of space quantization and electron spin (intrinsic angular momentum ℏ/2)
  • (c)(i) Rotational constant B = Δν̄/2 = 2025 m⁻¹, moment of inertia I = h/(8π²cB), bond length r₀ = √(I/μ) ≈ 0.92 Å for HF
  • (c)(ii) Vibrational frequency ω = (1/2π)√(k/μ), Raman shift Δν̄ = ±(ν₀ ∓ ν_vib), Stokes and anti-Stokes lines at ν̄₀ − ν̄_vib and ν̄₀ + ν̄_vib respectively
  • Proper unit conversions throughout: CGS to SI for (c)(ii), unified atomic mass to kg, wavenumber to frequency where needed
  • Physical significance: isotope shift tests QED predictions, Stern-Gerlach validates quantum mechanics vs classical expectations, spectroscopic constants determine molecular structure
Q4
50M state Quantum mechanics and atomic physics

(a) State how for spin-half particles, the spin (σ) can be expressed by its three components σ_x, σ_y and σ_z. 20 marks (b) By applying the Schrödinger's equation to the ground state of hydrogen atom, determine the zero-point energy. 15 marks (c) Distinguish between fluorescence and phosphorescence. Explain the mechanisms responsible for these phenomena. Discuss the applications of fluorescence and phosphorescence in the fields such as biochemistry, material science, etc. 15 marks

Answer approach & key points

The directive 'state' in part (a) demands precise, formal presentation of spin-half algebra with Pauli matrices, while parts (b) and (c) require 'determine' and 'distinguish/explain/discuss' respectively. Allocate approximately 40% of effort to part (a) given its 20 marks: present σ = (σ_x, σ_y, σ_z) with explicit 2×2 Pauli matrices, their commutation relations, and eigenvalue properties. Spend ~30% on part (b): solve radial Schrödinger equation for n=1, l=0, derive E₁ = -13.6 eV and identify zero-point energy from kinetic term or uncertainty principle. Allocate remaining ~30% to part (c): construct clear comparison table, explain singlet vs. triplet states and intersystem crossing, cite Indian applications such as fluorescence microscopy at IISc Bengaluru or phosphorescent safety signage in Indian Railways. Conclude with integrated remarks on quantum phenomena spanning atomic to molecular scales.

  • Part (a): Pauli spin matrices σ_x = [[0,1],[1,0]], σ_y = [[0,-i],[i,0]], σ_z = [[1,0],[0,-1]]; spin operator S = (ℏ/2)σ; commutation relations [σ_i, σ_j] = 2iε_ijk σ_k; eigenvalues ±1 for each component
  • Part (a): Spin as vector operator σ = σ_x î + σ_y ĵ + σ_z k̂; total spin magnitude S² = s(s+1)ℏ² with s=1/2; connection to SU(2) representation
  • Part (b): Radial Schrödinger equation for hydrogen ground state: -ℏ²/2μ ∇²ψ - e²/4πε₀r ψ = Eψ; separation into radial and angular parts; ground state wavefunction ψ₁₀₀ = (1/√πa₀³) exp(-r/a₀)
  • Part (b): Zero-point energy derivation: E₁ = -μe⁴/8ε₀²ℏ² = -13.6 eV; kinetic energy expectation value ⟨T⟩ = +13.6 eV; potential energy ⟨V⟩ = -27.2 eV; zero-point energy identified as positive kinetic energy contribution or via ΔxΔp ≥ ℏ/2
  • Part (c): Distinction table: fluorescence (spin-allowed, S₁→S₀, 10⁻⁹-10⁻⁷ s) vs phosphorescence (spin-forbidden, T₁→S₀, 10⁻³-10³ s); Jablonski diagram with radiative and non-radiative transitions
  • Part (c): Mechanisms: fluorescence via prompt emission without change in spin multiplicity; phosphorescence requires intersystem crossing (ISC) with spin-orbit coupling, delayed emission through forbidden transition
  • Part (c): Applications: fluorescence—green fluorescent protein (GFP) tagging, flow cytometry, Indian biomedical research (CCMB Hyderabad); phosphorescence—organic light-emitting diodes (OLEDs), persistent luminescent materials for emergency exit signs, security inks in Indian currency
Q5
50M Compulsory derive Quantum states, particle physics, solid state physics, electronics

(a) Show that the energy of the triplet state (S = 1) is not equal to the energy of the singlet state (S = 0). 10 marks (b) ρ⁰ and K⁰ mesons both decay mostly to π⁺ and π⁻. Why the mean lifetime of ρ⁰ is 10⁻²³ s, whereas that of K⁰ is 0·89 × 10⁻¹⁰ s? 10 marks (c) Find the radius of the interstitial sphere which can just fit into the void at the body centre of the fcc structure coordinated by the facial atoms. 10 marks (d) In powder diffraction method pattern for lead with radiation of wavelength λ = 1·54 Å, the (220) Bragg reflection angle is θ = 32°. Find the radius of the atom. 10 marks (e) (i) What are the differences in electrical characteristics of FET (JFET) and MOSFET? 7 marks (ii) How does n-channel FET differ from p-channel FET? 3 marks

Answer approach & key points

Begin with a brief introduction acknowledging the diverse physics domains covered (quantum mechanics, particle physics, solid state, and electronics). For part (a), derive the energy splitting using exchange interaction and spin wavefunctions; for (b), explain using strong vs. weak decay selection rules; for (c), derive the octahedral void geometry in FCC; for (d), apply Bragg's law and unit cell calculation; for (e)(i)-(ii), tabulate comparative characteristics. Allocate approximately 20% time to (a), 15% to (b), 20% to (c), 20% to (d), and 25% to (e) combined, reflecting mark distribution and derivation complexity.

  • (a) Derivation of triplet-singlet energy splitting using symmetric/antisymmetric spin wavefunctions and exchange integral J, showing E_triplet = E_0 - J and E_singlet = E_0 + J for two-electron system
  • (b) Explanation of ρ⁰ decay via strong interaction (OZI-allowed, resonant, Γ ~ 150 MeV) versus K⁰ decay via weak interaction (ΔS = 1, strangeness changing, CP violation context with K_S and K_L)
  • (c) Geometric derivation: octahedral void radius r = 0.414R where R is atomic radius, using FCC geometry with face-center to body-center distance relationship
  • (d) Application of Bragg's law nλ = 2d sinθ, calculation of d_220 = a/√8, determination of lattice parameter a, and atomic radius r = a√2/4 for FCC lead
  • (e)(i) Distinction between JFET (depletion-mode only, pn-junction gate, higher input impedance ~10⁹ Ω) and MOSFET (enhancement/depletion modes, insulated gate, higher input impedance ~10¹² Ω, threshold voltage concept)
  • (e)(ii) Carrier type (electrons vs holes), mobility differences, threshold voltage polarity, and drain current direction in n-channel versus p-channel FETs
Q6
50M calculate Nuclear physics, shell model, leptonic conservation

(a) The total binding energies of ¹⁵₈O, ¹⁶₈O and ¹⁷₈O are 111·96 MeV, 127·62 MeV and 131·76 MeV respectively. Determine the energy gap between 1p₁/₂ and 1d₅/₂ neutron shells for the nuclide whose mass number is close to 16. 15 marks (b) State the basic assumption of single-particle shell model. How do the centrifugal and spin-orbit terms remove the degeneracy of three-dimensional spherical harmonic oscillator? 10+10=20 marks (c) Explain the various leptonic family members. What is leptonic number conservation? Based on this conservation law, tell whether the following reactions are possible or not: (i) π⁻ → μ⁻ + ν̄ₜ (ii) n → p⁺ + e⁻ + ν̄ₑ 15 marks

Answer approach & key points

Begin with a clear statement of the shell model assumptions for part (b), then proceed to calculate the energy gap in part (a) using binding energy differences—this carries the highest marks (15) and requires careful identification of neutron shell transitions. Allocate approximately 35% effort to (a), 40% to (b) given its theoretical depth (20 marks), and 25% to (c). Structure as: (b) theoretical foundation → (a) numerical application → (c) particle physics application with conservation law verification.

  • Part (a): Correct identification that ¹⁶O has closed shells (Z=N=8), and that ¹⁵O has a 1d₅/₂ neutron hole while ¹⁷O has a 1d₅/₂ neutron particle; calculation of energy gap using BE(¹⁶O) - BE(¹⁵O) and BE(¹⁷O) - BE(¹⁶O) with proper averaging
  • Part (b): Statement of independent particle motion in a mean potential; explanation of how l(l+1)ħ²/2mr² centrifugal term lowers energy for higher l at same n, and spin-orbit coupling ξ(r)L·S splits j = l ± 1/2 states with inverted ordering for natural parity
  • Part (b): Clear derivation or explanation of the spin-orbit term origin from Dirac equation or phenomenological potential, showing how it creates the shell structure magic numbers 2, 8, 20, 28, 50, 82, 126
  • Part (c): Enumeration of three lepton families (e, μ, τ) with their neutrinos and antiparticles; definition of lepton number Lₑ, Lᵤ, Lₜ with L = +1 for leptons, -1 for antileptons, 0 for hadrons
  • Part (c)(i): Analysis showing π⁻ → μ⁻ + ν̄ₜ violates tau lepton number conservation (Lₜ: 0 → 0 + (-1)), hence forbidden; correct allowed decay is π⁻ → μ⁻ + ν̄ᵤ
  • Part (c)(ii): Verification that n → p⁺ + e⁻ + ν̄ₑ conserves baryon number, charge, and all lepton numbers (Lₑ: 0 → 0 + 1 + (-1) = 0), hence allowed as standard beta decay
Q7
50M calculate Nuclear physics and magnetic materials

(a) What is the minimum energy required to break a ₂He⁴ nucleus into free protons and neutrons? [ Given, m_H = 1·007825 amu, m_n = 1·008665 amu, m_e = 0·00055 amu and m_He = 4·002603 amu ] 15 (b) (i) Consider a uranium nucleus (₉₂U²³⁶) breaking up spontaneously into two equal parts. Estimate the reduction of electrostatic energy of the nucleus considering uniform charge distribution. [ Assume that nuclear radius is 1·2×10⁻¹³ A¹/³ cm ] 15 (ii) Is it possible for a photon to transfer all its energy to a free electron? Give reasons. 5 (c) Explain the cause of hysteresis phenomenon in ferromagnetic materials. What does the area of the hysteresis loop signify? 10+5=15

Answer approach & key points

This is a multi-part numerical-cum-descriptive question requiring precise calculations for (a) and (b)(i), conceptual reasoning for (b)(ii), and explanatory analysis for (c). Allocate approximately 35% time to part (a) for careful mass-energy conversion, 35% to part (b) including both calculation and reasoning, and 30% to part (c) with a clear hysteresis diagram. Begin with the binding energy calculation using atomic masses correctly, proceed through electrostatic energy estimation with proper radius scaling, address the photon-electron collision physics with reference to Compton scattering constraints, and conclude with domain theory explanation and energy dissipation interpretation.

  • Part (a): Correct identification that atomic mass of hydrogen includes electron, so use m_p = m_H - m_e or appropriate atomic mass accounting; calculation of mass defect Δm = [2m_H + 2m_n - m_He] or equivalent; conversion to energy using 1 amu = 931.5 MeV/c² yielding ~28.3 MeV
  • Part (b)(i): Application of electrostatic energy formula U = (3/5)(Z²e²)/(4πε₀R) for uniform sphere; correct radius scaling R ∝ A^(1/3) with R_He = R₀(4)^(1/3) and R_U = R₀(236)^(1/3); calculation of energy ratio and reduction factor considering two fragments each with Z/2 and A/2
  • Part (b)(ii): Recognition that photon-electron energy transfer requires momentum conservation; explanation that free electron cannot absorb photon completely due to simultaneous energy-momentum conservation violation; reference to Compton scattering or need for bound electron/third body
  • Part (c): Explanation of hysteresis via domain wall movement, irreversible domain rotation, and pinning by impurities/crystal defects; clear distinction between reversible and irreversible magnetization processes; area interpretation as energy dissipated per unit volume per cycle (hysteresis loss)
  • Part (c): Qualitative or quantitative sketch of B-H loop showing saturation, remanence, coercivity; labeling of key points and proper loop orientation
Q8
50M explain Magnetic materials, XRD and microprocessors

(a) Classify diamagnetic, paramagnetic and ferromagnetic materials in terms of their magnetic susceptibility (χ). Plot and explain the variation of 1/χ with temperature for the three materials. 20 (b) What is X-ray diffraction? How is an XRD pattern used to determine the crystal structure of the material? 15 (c) (i) What is a microprocessor? Describe the internal functioning of a microprocessor with block diagrams. (ii) How do thermistors and solar cells differ in structure and operation? 10+5=15

Answer approach & key points

Begin with a brief introduction acknowledging the interdisciplinary nature of the question spanning solid-state physics and electronics. For part (a), spend approximately 40% of your effort (20 marks) explaining magnetic susceptibility classifications with clear Curie-Weiss law derivations and properly labeled 1/χ vs T plots. Allocate 30% (15 marks) to part (b), describing Bragg's law and indexing XRD peaks for crystal structure determination. Distribute the remaining 30% (15 marks) between (c)(i) microprocessor architecture with block diagrams and (c)(ii) comparative analysis of thermistors versus solar cells, using Indian examples like ISRO's microprocessor developments or solar cell applications in rural electrification.

  • Part (a): Classification of diamagnetic (χ < 0, temperature-independent), paramagnetic (χ > 0, χ = C/T), and ferromagnetic (χ >> 0, follows Curie-Weiss law χ = C/(T-Tc)) with correct sign conventions and temperature dependence
  • Part (a): Accurate plots showing 1/χ vs T: horizontal line for diamagnetic, straight line through origin for paramagnetic, and linear with positive intercept (Tc) for ferromagnetic above Curie temperature
  • Part (b): Bragg's law (nλ = 2d sinθ) explanation, powder method/Bragg spectrometer, and systematic procedure for determining crystal structure through d-spacing calculation and comparison with standard tables
  • Part (c)(i): Definition of microprocessor as CPU on single chip, block diagram showing ALU, control unit, registers, address/data/control buses, and fetch-decode-execute cycle explanation
  • Part (c)(ii): Structural differences (thermistors: metal oxide semiconductors with negative temperature coefficient; solar cells: p-n junction with depletion region) and operational differences (resistance vs. photovoltaic effect)
  • Part (c)(ii): Indian context: mention indigenous microprocessors like Shakti processor (IIT-Madras) or ISRO's Vikram series, and solar applications in National Solar Mission

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