Physics

UPSC Physics 2026 — Paper II

All 8 questions from UPSC Civil Services Mains Physics 2026 Paper II (400 marks total). Every stem reproduced in full, with directive-word analysis, marks, word limits, and answer-approach pointers.

8Questions
400Total marks
2026Year
Paper IIPaper

Topics covered

Quantum mechanics, NMR, hydrogen atom (1)

A

Q1
50M Compulsory state

(a) (i) The de Broglie wavelength of a particle in thermal equilibrium at a temperature of 27°C is λ. At what temperature will it be λ/2 ? (ii) The wave function of a spin 1/2 particle is given by (−i, 2). What is the probability of finding the particle in the spin-up state ? (10 marks) (b) The OH-radical has a moment of inertia of 1·48 × 10⁻⁴⁶ kg.m². For J = 6, calculate its angular velocity and angular momentum. Find the energy absorbed in the J = 6 → J = 7 transition. (10 marks) (c) In a Stern-Gerlach experiment, the magnetic field varies with distance in the z-direction according to dB_z/dz = 1·5 T/mm. The speed of silver atoms coming from the oven is 725 m/s. Silver atoms travel a distance of 3 cm through the magnet. Calculate the separation of the two beams of atoms when they leave the magnet. [Given : The mass of a silver atom = 1·8 × 10⁻²⁵ kg and its magnetic moment is 1 Bohr magneton.] (10 marks) (d) If the position and momentum operators in 1-D are represented by x̂ and p̂ respectively, calculate the commutator [x̂², cos (p̂)]. (10 marks) (e) Find the eigenvalues and eigenfunctions of a system described by Hamiltonian H = ae^(bσ_x), where a, b are constants and σ_x is the x-component of Pauli matrix σ⃗. (10 marks)

हिंदी में पढ़ें

(a) (i) तापक्रम 27°C पर तापीय संतुलन में एक कण की दे ब्रॉग्ली तरंगदैर्ध्य λ है। यह किस तापमान पर λ/2 हो जाएगा ? (ii) एक प्रचक्रण 1/2 कण का तरंग फलन (−i, 2) द्वारा दिया गया है। कण के स्पिन-अप अवस्था में होने की प्रायिकता क्या है ? (10 अंक) (b) OH-मूलक (रैडिकल) का जड़त्व आघूर्ण 1·48 × 10⁻⁴⁶ kg.m² है। J = 6 स्तर के लिए, उसके कोणीय वेग एवं कोणीय संवेग की गणना कीजिए। J = 6 → J = 7 संक्रमण में अवशोषित ऊर्जा ज्ञात कीजिए। (10 अंक) (c) एक स्टर्न-गर्लैक प्रयोग में, चुम्बकीय क्षेत्र z-दिशा में दूरी के साथ dB_z/dz = 1·5 T/mm के अनुसार विचरित होता है। अवन से आने वाले सिल्वर परमाणुओं की गति 725 m/s है। सिल्वर के परमाणु 3 cm की दूरी चुम्बक से होकर तय करते हैं। जब परमाणुओं के दो पुंज चुम्बक को छोड़ते हैं, तब उनके पृथक्करण की गणना कीजिए। [दिया गया है : सिल्वर परमाणु का द्रव्यमान = 1·8 × 10⁻²⁵ kg और उसका चुम्बकीय आघूर्ण 1 बोर मैग्नेटॉन है।] (10 अंक) (d) यदि एक-विमीय (1-D) स्थिति एवं संवेग संकारकों को क्रमशः x̂ एवं p̂ से निरूपित किया जाता है, तो कम्यूटेटर [x̂², cos (p̂)] की गणना कीजिए। (10 अंक) (e) हैमिल्टोनियन H = ae^(bσ_x) द्वारा वर्णित एक निकाय के आइगेनमान एवं आइगेनफलन ज्ञात कीजिए, जहाँ a, b स्थिरांक हैं एवं σ_x पाउली मैट्रिक्स σ⃗ का x-घटक है। (10 अंक)

Answer approach & key points

(a) Two independent 5-mark numericals: (i) use the thermal de Broglie wavelength λ = h/√(3mkT) to find the temperature at which λ halves, starting from 27 °C; (ii) normalise the unnormalised spinor (−i, 2) and compute the probability of a spin-up measurement. (b) A three-part rigid-rotor numerical on the OH radical with I = 1.48 × 10⁻⁴⁶ kg m²: compute (a) the angular momentum for J = 6, (b) the corresponding angular velocity, and (c) the energy absorbed in the J = 6 → J = 7 rotational transition. (c) Compute the beam separation in a Stern–Gerlach apparatus: silver atoms (m = 1.8 × 10⁻²⁵ kg, μ = 1 Bohr magneton) at v = 725 m s⁻¹ traverse 3 cm of a field gradient dB_z/dz = 1.5 T mm⁻¹. The answer required is the separation of the TWO beams at the exit of the magnet (not the deflection of one beam). (d) Evaluate the operator commutator [x̂², cos p̂] in one dimension. The candidate must use the canonical relation [x̂, p̂] = iħ, the identity [x̂, f(p̂)] = iħ ∂f/∂p̂, and the product rule for commutators, and present the ordered (non-commuting) result. (e) Find BOTH the eigenvalues and the eigenfunctions (eigenspinors) of H = a e^(b σ_x). The key idea is that any function of σ_x is diagonal in the eigenbasis of σ_x, so the eigenvectors are those of σ_x and the eigenvalues are a e^(±b).

  • λ = h/√(3mk_BT) ⇒ λ ∝ 1/√T
  • T₂ = 4 × 300 K = 1200 K (927 °C)
  • Norm ⟨χ|χ⟩ = 5 ⇒ P(↑) = 1/5 = 0.2
  • |L| = √(J(J + 1)) ħ = √42 ħ = 6.83 × 10⁻³⁴ J s
  • ω = L/I = 4.62 × 10¹² rad s⁻¹
  • ΔE = (ħ²/2I)[7·8 − 6·7] = 7ħ²/I = 5.26 × 10⁻²² J (3.28 × 10⁻³ eV)
  • F = μ_B dB_z/dz with 1.5 T/mm = 1500 T/m ⇒ 1.39 × 10⁻²⁰ N
  • a = 7.73 × 10⁴ m s⁻², t = L/v = 4.14 × 10⁻⁵ s, z = ½at² = 6.6 × 10⁻⁵ m
  • Separation 2z = 1.32 × 10⁻⁴ m
  • [x̂, f(p̂)] = iħ f′(p̂) ⇒ [x̂, cos p̂] = −iħ sin p̂
  • Product rule [x̂², C] = x̂[x̂, C] + [x̂, C]x̂
  • [x̂², cos p̂] = −iħ(x̂ sin p̂ + sin p̂ x̂) = −2iħ x̂ sin p̂ − ħ² cos p̂
  • σ_x² = I ⇒ e^{bσ_x} = I cosh b + σ_x sinh b
  • Eigenvalues E± = a e^{±b}
  • Eigenvectors (1/√2)(1, ±1)ᵀ, the eigenvectors of σ_x
Q2
50M calculate

(a) A particle is in the ground state of a 1-D simple harmonic oscillator potential, V(x) = 1/2 mω²x². Calculate the position uncertainty of the particle. (15 marks) (b) (i) A particle is in a normalized state ψ which is a superposition of the energy eigenstates ψ₁ and ψ₂ of energies 10 eV and 30 eV respectively. The average energy of the particle in the state ψ is 24 eV. Find the state ψ in terms of ψ₁ and ψ₂. (10 marks) (ii) Obtain the allowed energy eigenvalues of a half 1-D simple harmonic oscillator defined by the Hamiltonian H = p²/2m + V(x), where V(x) = 1/2 mω²x² for x ≥ 0 = ∞ for x < 0 Express its eigenstates in terms of the eigenstates of a complete 1-D oscillator. (10 marks) (c) (i) Why does the electron paramagnetic resonance (EPR) spectroscopy utilize the microwave region of the electromagnetic spectrum, while nuclear magnetic resonance (NMR) uses radio waves ? (7 marks) (ii) Why can the experimental observation of the Lamb shift not be explained by the Dirac theory ? (8 marks)

हिंदी में पढ़ें

(a) एक कण एक-विमीय (1-D) सरल आवर्त दोलक के विभव, V(x) = 1/2 mω²x² की आद्य (निम्नतम) अवस्था में है। कण की स्थिति अनिश्चितता की गणना कीजिए। (15 अंक) (b) (i) एक कण प्रसामान्यीकृत अवस्था ψ में है जो क्रमशः 10 eV एवं 30 eV की ऊर्जा आइगेनअवस्थाओं ψ₁ एवं ψ₂ का अध्यारोपण है। ψ अवस्था में कण की औसत ऊर्जा का मान 24 eV है। ψ अवस्था को ψ₁ एवं ψ₂ के पदों में ज्ञात कीजिए। (10 अंक) (ii) अर्ध एक-विमीय (1-D) सरल आवर्त दोलक की अनुमत आइगेनऊर्जाओं को प्राप्त कीजिए जो हैमिल्टोनियन H = p²/2m + V(x), जहाँ V(x) = 1/2 mω²x² x ≥ 0 के लिए = ∞ x < 0 के लिए से परिभाषित है। इसकी आइगेनअवस्थाओं को पूर्ण एक-विमीय (1-D) दोलक की आइगेनअवस्थाओं के पदों में व्यक्त कीजिए। (10 अंक) (c) (i) इलेक्ट्रॉन अनुचुंबकीय अनुनाद (EPR) स्पेक्ट्रमिकी में विद्युत-चुंबकीय स्पेक्ट्रम के सूक्ष्म तरंग क्षेत्र का उपयोग क्यों होता है, जबकि नाभिक चुंबकीय अनुनाद (NMR) में रेडियो तरंगों का उपयोग होता है ? (7 अंक) (ii) लैम्ब शिफ्ट के प्रयोगात्मक प्रेक्षण को डिरैक सिद्धांत द्वारा क्यों व्याख्यायित नहीं किया जा सकता है ? (8 अंक)

Answer approach & key points

(a) For the ground state of the 1-D harmonic oscillator V = ½mω²x², calculate the position uncertainty Δx = √(⟨x²⟩ − ⟨x⟩²). This requires writing the normalised ground-state Gaussian (or using ladder operators), evaluating ⟨x⟩ and ⟨x²⟩ explicitly, and giving the closed-form result. (b(i)) A normalised state ψ is a superposition of two energy eigenstates (10 eV and 30 eV) with mean energy 24 eV. Determine the expansion coefficients and write ψ explicitly in terms of ψ₁ and ψ₂. (b(ii)) Obtain the allowed energy eigenvalues of the half-oscillator (V = ½mω²x² for x ≥ 0, V = ∞ for x < 0) AND express its eigenstates in terms of the eigenstates of the full 1-D oscillator. Both parts must be answered; the key argument is the boundary condition ψ(0) = 0. (c(i)) Explain, with the resonance condition and the relevant magnitudes, WHY EPR resonances fall in the microwave region while NMR resonances fall in the radiofrequency region at laboratory magnetic fields. The answer hinges on the ratio of the electron magnetic moment to the nuclear magnetic moment. (c(ii)) Explain why the observed Lamb shift lies outside the Dirac theory: state what Dirac theory predicts for 2S₁/₂ and 2P₁/₂, what is actually measured, and identify the missing physics (quantisation of the radiation field, i.e. QED).

  • Normalised ψ₀ = (mω/πħ)^{1/4} e^{−mωx²/2ħ}
  • ⟨x⟩ = 0 by parity; ⟨x²⟩ = ħ/(2mω) from the Gaussian integral (or ladder operators)
  • Δx = √(ħ/2mω)
  • ⟨E⟩ = |c₁|²E₁ + |c₂|²E₂ with |c₁|² + |c₂|² = 1
  • |c₁|² = 0.3, |c₂|² = 0.7
  • ψ = √0.3 ψ₁ + √0.7 ψ₂ (up to a relative phase)
  • ψ(0) = 0 from the infinite wall
  • Only odd-n full-oscillator states allowed ⇒ E_k = (2k + 3/2)ħω, k = 0, 1, 2, …
  • φ_k = √2 ψ_{2k+1} for x ≥ 0, 0 for x < 0
  • Resonance hν = gμB for both
  • μ_B/μ_N = m_p/m_e ≈ 1836 (nuclear moment far smaller)
  • At lab fields: electron ≈ 28 GHz T⁻¹ (microwave, e.g. 9.5 GHz at 0.34 T); proton 42.58 MHz T⁻¹ (radio frequency)
  • Dirac: energy depends on n and j only ⇒ 2S₁/₂ and 2P₁/₂ degenerate
  • Lamb–Retherford (1947): 2S₁/₂ above 2P₁/₂ by ≈ 1057 MHz
  • Missing physics is field quantisation (QED): self-energy from vacuum fluctuations raising s states, plus vacuum polarisation
Q3
50M calculate Quantum mechanics, NMR, hydrogen atom

(a) (i) Calculate the number of permitted electrons in a sub-shell and a shell in an atom. (ii) Explain how Pauli's exclusion principle helps in determining the electronic configuration in a many-electron system. (8+12 marks) (b) (i) Why is the relaxation process so important in nuclear magnetic resonance (NMR)? (ii) Why are 12C and 16C nuclei not suitable for the study of NMR? (10+5 marks) (c) (i) The wave function of a hydrogen atom is written as ψn, l, m (r, θ, φ). Explain the quantum numbers n, l, m and mention their ranges. Show that ψn, l, m (r, θ, φ) is n² degenerate. (ii) The electron in the hydrogen atom is found in the state ψ (r, θ, φ) = A R(r) sin θ cos θ e⁻ⁱφ. Find the z-component of angular momentum of the electron. (10+5 marks)

हिंदी में पढ़ें

(a) (i) एक परमाणु के एक उपकोश एवं कोश में अनुमत इलेक्ट्रॉनों की संख्या की गणना कीजिए। (ii) समझाइए कि पाउली का अपवर्जन सिद्धांत किस प्रकार एक बहु-इलेक्ट्रॉन निकाय में इलेक्ट्रॉनिक विन्यास को निर्धारित करने में सहायता करता है। (8+12 अंक) (b) (i) नाभिकीय चुम्बकीय अनुनाद (NMR) में विश्रांति प्रक्रिया इतनी महत्वपूर्ण क्यों है? (ii) 12C एवं 16C नाभिक एनएमआर (NMR) के अध्ययन के लिए उपयुक्त क्यों नहीं हैं? (10+5 अंक) (c) (i) एक हाइड्रोजन परमाणु के तरंग फलन को ψn, l, m (r, θ, φ) के रूप में लिखा जाता है। क्वांटम संख्याओं n, l, m की व्याख्या कीजिए एवं उनके परासों का उल्लेख कीजिए। दर्शाइए कि ψn, l, m (r, θ, φ), n² समप्रभ (डिजनरेट) है। (ii) हाइड्रोजन परमाणु में इलेक्ट्रॉन ψ (r, θ, φ) = A R(r) sin θ cos θ e⁻ⁱφ अवस्था में पाया जाता है। इलेक्ट्रॉन के कोणीय संवेग का z-घटक ज्ञात कीजिए। (10+5 अंक)

Answer approach & key points

Framework: Principle > Setup and diagram > Derivation > Result and limiting case. (a(i)) calculate: given > formula > substitution > result with units > interpretation | (a(ii)) explain: definition/context > points in order > small example > short close | (b(i)) explain: definition/context > points in order > small example > short close | (b(ii)) explain: definition/context > points in order > small example > short close | (c(i)) explain: definition/context > points in order > small example > short close | (c(ii)) calculate: given > formula > substitution > result with units > interpretation Full marks: Rigorous derivations, correct quantum number logic, clear NMR physics, and accurate calculation of Lz.

  • 2l + 1 values of m_l, two spins each ⇒ 2(2l + 1) per sub-shell
  • Σ_{l=0}^{n−1} 2(2l + 1) = 2n² per shell
  • Basis: Pauli exclusion principle
  • Statement with all four quantum numbers (or antisymmetry of the wavefunction)
  • Limits: 2 per orbital, 2(2l + 1) per sub-shell, 2n² per shell ⇒ electrons fill successive levels (Aufbau)
  • Hund's rule for partly filled sub-shells, with an example configuration
  • Relaxation restores the Boltzmann population difference after excitation
  • T₁ (spin–lattice) prevents saturation and sets the repetition rate
  • T₂ (spin–spin) governs FID decay and line width Δν ≈ 1/πT₂
  • NMR needs nuclear spin I ≠ 0 (magnetic moment)
  • ¹²C and ¹⁶C are even–even nuclei with I = 0, so no Zeeman splitting
  • n = 1, 2, …; l = 0 … n − 1; m = −l … +l, with physical meaning of each
  • Energy depends only on n for hydrogen
  • Σ_{l=0}^{n−1}(2l + 1) = n² ⇒ n²-fold degeneracy
  • L̂_z = −iħ ∂/∂φ applied to e^{−iφ}
  • L_z = −ħ (m = −1)
Q4
50M explain

(a) (i) What are hot bands in vibrational spectroscopy ? Why are they called so ? (8 marks) (ii) The fundamental and 2nd harmonic transitions of ¹⁴N¹⁶O are recorded at 1876·06 cm⁻¹ and 3724·2 cm⁻¹, respectively. Calculate the equilibrium vibrational frequency, the anharmonicity constant and the zero-point energy of the molecule. [Given : Mass of ¹⁴N = 23·25 × 10⁻²⁷ kg, Mass of ¹⁶O = 26·56 × 10⁻²⁷ kg] (7 marks) (b) A particle of mass m is in the ground state of a 1-D box of infinite potential of length a. If the length of the box is changed to 2a symmetrically without disturbing the wave function of the particle, find the probability that the particle will be in the ground state of the new box. (20 marks) (c) (i) Explain why the rotational transition for J = 0 → J = 1 is usually not of maximum intensity. (8 marks) (ii) Determine the positions of the first four rotational Raman lines in the spectrum of hydrogen (H₂), given that its bond length is 0·742 Å. What effect will the nuclear spin have on the spectrum ? [Given : Mass of ¹H = 1·673 × 10⁻²⁷ kg] (7 marks)

हिंदी में पढ़ें

(a) (i) कंपनिक स्पेक्ट्रमिकी में तप्त बैंड्स (हॉट बैंड्स) क्या हैं ? इन्हें ऐसा क्यों कहा जाता है ? (8 अंक) (ii) ¹⁴N¹⁶O के मूल एवं द्वितीय हार्मोनिक संक्रमणों को क्रमश: 1876·06 cm⁻¹ एवं 3724·2 cm⁻¹ पर अभिलेखित (रिकॉर्डिंग) किया जाता है । अणु की साम्यावस्था कंपन आवृत्ति, अप्रसंवादिता स्थिरांक एवं शून्य-बिंदु ऊर्जा की गणना कीजिए । [दिया गया है : ¹⁴N का द्रव्यमान = 23·25 × 10⁻²⁷ kg, ¹⁶O का द्रव्यमान = 26·56 × 10⁻²⁷ kg] (7 अंक) (b) एक m द्रव्यमान का कण, अनंत विभव के 1-D बॉक्स, जिसकी लम्बाई a है, की आद्य (निम्नतम) अवस्था में है । यदि बॉक्स की लम्बाई, कण के तरंग फलन में विचलन के बिना, सममितीय रूप से 2a कर दी जाती है, तो नए बॉक्स की आद्य अवस्था में कण के होने की प्रायिकता ज्ञात कीजिए । (20 अंक) (c) (i) समझाइए कि क्यों J = 0 → J = 1 के लिए घूर्णी संक्रमण प्राय: अधिकतम तीव्रता का नहीं होता है । (8 अंक) (ii) हाइड्रोजन (H₂) के स्पेक्ट्रम में प्रथम चार घूर्णी रमन रेखाओं की स्थितियों को ज्ञात कीजिए, यदि उसके आबंध की लम्बाई 0·742 Å है । नाभिकीय प्रचक्रण का स्पेक्ट्रम पर क्या प्रभाव पड़ेगा ? [दिया गया है : ¹H का द्रव्यमान = 1·673 × 10⁻²⁷ kg] (7 अंक)

Answer approach & key points

(a(i)) Define hot bands in vibrational (IR/Raman) spectroscopy and explain the origin of the name — both halves must be answered, the second requiring the Boltzmann population argument. (a(ii)) From the fundamental (1876.06 cm⁻¹) and the '2nd harmonic' (first overtone, 3724.2 cm⁻¹) of ¹⁴N¹⁶O, calculate THREE quantities: the equilibrium vibrational frequency ω̃_e, the anharmonicity constant, and the zero-point energy of the molecule. (b) A particle sits in the ground state of an infinite well of width a; the well is suddenly widened SYMMETRICALLY to width 2a with the wave function unchanged. Compute the probability of finding the particle in the ground state of the new well — i.e. apply the sudden approximation and evaluate the overlap integral. (c(i)) Explain why the J = 0 → J = 1 line is usually NOT the most intense line in a rotational (microwave) spectrum: the intensity follows the thermal population of the lower level, which is the product of the degeneracy (2J+1) and the Boltzmann factor, and peaks at an intermediate J. (c(ii)) Two demands: (a) compute the positions (Raman shifts) of the first four rotational Raman lines of H₂ given r = 0.742 Å and m(¹H) = 1.673 × 10⁻²⁷ kg; (b) state the effect of nuclear spin (ortho/para hydrogen) on the spectrum.

  • Transition from a thermally populated excited level (v = 1 → 2), not from v = 0
  • Named 'hot' because intensity ∝ Boltzmann population of v = 1, rising with temperature
  • Anharmonicity puts it ≈ 2ω̃_e x_e below the fundamental
  • ω̃_e − 2ω̃_e x_e = 1876.06 and 2ω̃_e − 6ω̃_e x_e = 3724.2 (0 → 2 overtone)
  • ω̃_e x_e = 13.96 cm⁻¹, x_e = 7.33 × 10⁻³
  • ω̃_e = 1903.98 cm⁻¹
  • ZPE = ½ω̃_e − ¼ω̃_e x_e = 948.5 cm⁻¹
  • Sudden approximation: P = |⟨φ₁|ψ⟩|²
  • ψ = √(2/a) cos(πx/a) on |x| ≤ a/2; φ₁ = √(1/a) cos(πx/2a) on |x| ≤ a
  • Overlap integral over |x| ≤ a/2 only: c = 8/(3π) = 0.849
  • P = 64/(9π²) ≈ 0.72
  • Line intensity follows the population of the lower level J
  • N_J ∝ (2J + 1) e^{−hcBJ(J + 1)/k_BT}: degeneracy rises, Boltzmann factor falls
  • Maximum at J_max = √(k_BT/2hcB) − ½, not at J = 0
  • μ = m_H/2, I = 4.61 × 10⁻⁴⁸ kg m², B = 60.8 cm⁻¹
  • ΔJ = ±2, Δν̃ = B(4J + 6): 364.7, 607.8, 850.9, 1094.1 cm⁻¹
  • Nuclear spin: ortho (odd J, weight 3) and para (even J, weight 1) ⇒ 1 : 3 intensity alternation, starting weak

B

Q5
50M Compulsory justify

(a) Are the nucleons inside the nucleus governed by the laws of quantum physics ? Justify your answer. (10 marks) (b) Binding energy and rest mass energy of a two-nucleon bound state are denoted by B and Mc², respectively, where c is the speed of light. Calculate the minimum energy of a photon required to dissociate this bound state in terms of B and Mc². (10 marks) (c) A nucleus of rest mass M is initially in an excited state whose energy is ΔE above its ground state. The nucleus emits a γ-ray of energy hν and makes a transition to its ground state. Calculate the fractional change in energy for the nucleus. (10 marks) (d) (i) What is the effective mass of an electron ? (ii) For what physical reasons can the effective mass of an electron be infinite and negative ? (iii) Near the top of the valence band, the energy of a crystal is given by E = – 10⁻³⁹ k² Jm². An electron with wave vector 10¹⁰ k̂ₓ m⁻¹ is removed from an orbital in a completely filled valence band. Determine its effective mass and momentum. (10 marks) (e) Explain briefly the two-fluid model proposed by the London brothers and obtain the expressions for the penetration depth and the number of superelectrons in a superconducting specimen. (10 marks)

हिंदी में पढ़ें

(a) क्या नाभिक के अन्दर न्यूक्लिऑन्स क्वांटम भौतिकी के नियमानुसार नियंत्रित होते हैं ? अपने उत्तर की पुष्टि कीजिए । (10 अंक) (b) दो-न्यूक्लिऑन परिबद्ध अवस्था की बंधन ऊर्जा एवं विराम द्रव्यमान ऊर्जा को क्रमश: B एवं Mc² द्वारा निरूपित किया गया है, जहाँ c प्रकाश की चाल है । इस परिबद्ध अवस्था को वियोजित करने के लिए आवश्यक एक फोटॉन की न्यूनतम ऊर्जा की B और Mc² के पदों में गणना कीजिए । (10 अंक) (c) विराम द्रव्यमान M का एक नाभिक प्रारम्भ में उसकी आद्य (निम्नतम) अवस्था से ΔE ऊर्जा ऊपर की एक उत्तेजित अवस्था में है । नाभिक hν ऊर्जा की γ-किरण उत्सर्जित करता है और आद्य अवस्था में संक्रमण करता है । नाभिक की ऊर्जा में आंशिक परिवर्तन की गणना कीजिए । (10 अंक) (d) (i) इलेक्ट्रॉन का प्रभावी द्रव्यमान क्या है ? (ii) किन भौतिक कारणों से इलेक्ट्रॉन का प्रभावी द्रव्यमान अनंत एवं ऋणात्मक हो सकता है ? (iii) संयोजकता बैंड के उच्चतम स्तर के समीप एक क्रिस्टल की ऊर्जा E = – 10⁻³⁹ k² Jm² दी गई है । एक इलेक्ट्रॉन, जिसका तरंग सदिश 10¹⁰ k̂ₓ m⁻¹ है, को पूर्णतया भरे संयोजकता बैंड में एक कक्षक (ऑर्बिटल) से निकाला गया है । उसके प्रभावी द्रव्यमान एवं संवेग का मान निर्धारित कीजिए । (10 अंक) (e) लंदन बन्धुओं द्वारा प्रस्तावित दो-तरल मॉडल की संक्षेप में व्याख्या कीजिए एवं अतिचालक पदार्थ में वेधन गहराई और सुपर-इलेक्ट्रॉनों की संख्या के लिए व्यंजक प्राप्त कीजिए । (10 अंक)

Answer approach & key points

(a) Answer yes/no and JUSTIFY: are nucleons inside the nucleus governed by quantum mechanics? The justification must be evidential — uncertainty-principle estimates, discrete levels and shell structure, Pauli statistics, and tunnelling phenomena. (b) Find the threshold (minimum) photon energy to photodisintegrate a two-nucleon bound state of binding energy B and rest-mass energy Mc². The answer must exceed B because the photon carries momentum and the system must recoil; express the result in terms of B and Mc² only. (c) A nucleus of rest mass M de-excites from a level ΔE above the ground state by emitting a γ-ray of energy hν. Calculate the fractional change in the nucleus's energy — i.e. obtain the recoil energy and the fractional shift ΔE − hν relative to the transition energy. (d) Three parts, printed 2 + 3 + 5: (i) define the effective mass of an electron in a crystal; (ii) give the physical reasons why m* can be infinite and why it can be negative; (iii) for E = −10⁻³⁹ k² J m² near the top of the valence band, compute the effective mass and the momentum of an electron with k = 10¹⁰ x̂ m⁻¹ that is removed from a filled band. (e) Explain the London brothers' two-fluid model of superconductivity AND obtain expressions for (a) the London penetration depth and (b) the number density of superelectrons. Both derived expressions must appear.

  • Yes; Δx Δp ≥ ħ/2 with Δx of a few fm (R = 1.2 A^(1/3) fm) gives Δp of order 100 MeV/c and kinetic energy of several MeV
  • Discrete levels and magic numbers 2, 8, 20, 28, 50, 82, 126 (shell model)
  • Nucleons are spin-½ fermions obeying the Pauli exclusion principle (Fermi gas)
  • α-decay by tunnelling (Gamow theory) and the Geiger-Nuttall law
  • Photodisintegration γ + d → n + p; photon momentum p = Eγ/c
  • At threshold the products are at rest in the centre-of-mass frame; invariant s = (Mc²)² + 2Mc²Eγ = (Mc² + B)²
  • Eγ(min) = B + B²/(2Mc²) = B(1 + B/2Mc²)
  • Recoil momentum p = hν/c and recoil energy E_R = (hν)²/(2Mc²)
  • Energy balance ΔE = hν + E_R
  • Fractional change E_R/ΔE ≈ ΔE/(2Mc²)
  • Consequence: the emitted line is shifted, which prevents resonant absorption by free nuclei (Mössbauer effect)
  • m* = ħ²/(d²E/dk²), with group velocity v_g = (1/ħ)dE/dk
  • Infinite at the inflection point of E(k), where d²E/dk² = 0; negative near the band top where the curvature is negative (the lattice takes more momentum than the applied force gives)
  • m* = -5.56 × 10⁻³⁰ kg (about -6.1 mₑ)
  • Crystal momentum p = ħk = 1.05 × 10⁻²⁴ kg m s⁻¹
  • Two-fluid model: n = nₛ + nₙ, nₛ/n = 1 - (T/T_c)⁴ (Gorter-Casimir), nₛ → 0 at T_c
  • London equations: dJₛ/dt = (nₛe²/m)E and ∇ × Jₛ = -(nₛe²/m)B
  • ∇²B = B/λ_L² with B(x) = B₀e^(-x/λ_L); Meissner effect
  • λ_L = √(m/(μ₀nₛe²)) and nₛ = m/(μ₀e²λ_L²)
Q6
50M explain

(a) By considering the three-dimensional harmonic oscillator potential, explain the energy levels of nucleons inside the nucleus. Also, derive the zero-point energy of nucleons. Why did this assumption fail to explain the existence of nuclei with higher magic number ? (20 marks) (b) What do you understand by the packing fraction ‘f’ and the binding energy ‘Eb’ of a nucleus ? Draw the graphs for packing fraction f versus mass number (A) and binding energy fraction f_b (= E_b / A) versus mass number (A). Further, explain how the graphs of the variation of f and f_b with A have complementary approaches. (10 marks) (c) (i) What are the different methods used to increase the probability of exposure for the atomic planes with right orientation to X-rays in the X-rays diffraction studies ? (ii) Explain the principle and working of the Laue's diffraction method. Comment on the origin of Laue spots and the utility of Laue's diffraction pattern. (20 marks)

हिंदी में पढ़ें

(a) त्रिविमीय आवर्ती दोलक विभव को मानकर नाभिक के अन्दर न्यूक्लिऑनों के ऊर्जा स्तरों की व्याख्या कीजिए । साथ ही न्यूक्लिऑनों की शून्य-बिंदु ऊर्जा की व्युत्पत्ति कीजिए । उच्च मैजिक संख्या के नाभिकों के अस्तित्व की व्याख्या करने में यह अभिगृहीत क्यों विफल रहा ? (20 अंक) (b) एक नाभिक के संकुलन गुणांक ‘f’ और बंधन ऊर्जा ‘E_b’ से आप क्या समझते हैं ? संकुलन गुणांक f बनाम द्रव्यमान संख्या (A) एवं बंधन ऊर्जा भिन्न f_b (= E_b / A) बनाम द्रव्यमान संख्या (A) के आलेखों को रेखांकित कीजिए । आगे व्याख्या कीजिए कि f और f_b के A के साथ विचरण के आलेख एक दूसरे के पूरक दृष्टिकोण के हैं । (10 अंक) (c) (i) X-किरण विवर्तन अध्ययनों में X-किरणों से समुचित दिक्विन्यास के साथ परमाण्वीय समतलों के लिए उद्भासन की संभाव्यता (प्रायिकता) को बढ़ाने की विभिन्न विधियाँ क्या हैं ? (ii) लाउए की विवर्तन विधि के सिद्धान्त एवं कार्यप्रणाली की व्याख्या कीजिए । लाउए धब्बों (स्पॉट्स) की उत्पत्ति एवं लाउए के विवर्तन पैटर्न की उपयोगिता पर टिप्पणी कीजिए । (20 अंक)

Answer approach & key points

(a) Three demands: explain the nucleon energy levels generated by a three-dimensional harmonic-oscillator nuclear potential; DERIVE the zero-point energy of the nucleons; and explain why this assumption alone fails to reproduce the higher magic numbers. (b) Define packing fraction f and binding energy E_b; DRAW two graphs — f versus A and f_b = E_b/A versus A; and explain how the two variations are complementary (a minimum in f corresponds to a maximum in E_b/A). (c) Two parts (5 + 15): (i) list the experimental methods used to ensure that some atomic planes satisfy the Bragg condition in X-ray diffraction; (ii) explain the principle and working of the Laue method, and comment on the origin of the Laue spots and the utility of the Laue pattern.

  • E_N = (N + 3/2)ħω with N = 2(n - 1) + l; zero-point energy (3/2)ħω, i.e. ħω/2 for each of three degrees of freedom
  • Level degeneracy (N + 1)(N + 2) including spin; oscillator magic numbers 2, 8, 20, 40, 70, 112
  • Agreement only for 2, 8, 20; observed magic numbers 28, 50, 82, 126 not reproduced
  • Spin-orbit term -a l·s (Mayer and Jensen, 1949) lowers j = l + 1/2 and pulls down the intruder levels 1f7/2, 1g9/2, 1h11/2, 1i13/2
  • f = (M - A)/A × 10⁴ (M in atomic mass units); E_b = [Zm_H + (A - Z)m_n - M]c², with 1 u = 931.5 MeV
  • f falls from large positive values for light nuclei to a minimum near A ≈ 50-60 and rises to small positive values for the heaviest nuclei
  • E_b/A rises steeply for light nuclei (⁴He 7.07 MeV), peaks near ⁵⁶Fe (about 8.8 MeV) and falls slowly to about 7.6 MeV for ²³⁸U
  • f is essentially minus E_b/A: the minimum of f coincides with the maximum of E_b/A
  • Bragg's law 2d sinθ = nλ; three methods - Laue (white radiation, fixed crystal), rotating-crystal (monochromatic, rotated crystal), Debye-Scherrer powder
  • Laue principle: continuous X-ray spectrum (λ_min = 12.4/V(kV) Å) supplies the wavelength satisfying Bragg's law for each plane of a fixed single crystal; transmission and back-reflection arrangements
  • Origin of spots: Ewald sphere construction with reciprocal lattice points between limiting spheres; spots lie on ellipses (transmission) or hyperbolas (back reflection) for planes of a zone
  • Utility: crystal orientation and Laue symmetry (11 Laue groups from Friedel's law), detection of imperfections through asterism; limitation that wavelength of each spot is unknown
Q7
50M discuss

(a) (i) What is diamagnetism ? Why do diamagnetic materials have negative magnetic susceptibility ? (ii) Discuss the limitations of the quantum theory of diamagnetism. (iii) Draw a diagram of magnetic susceptibility as a function of temperature. Pay attention to the relative scales in your diagram so that the relative strengths of the magnetic phenomena are presented. (20 marks) (b) The input signal as shown in Figure (I) is applied to the comparator circuit given in Figure (II). Make a sketch of the output signal showing its proper relationship to the input signal. Assume that the maximum output levels of the op-amp are ± 12 V. (10 marks) (c) What is the criticality of a self-sustained nuclear reactor ? Write the basic processes affecting the nuclear chain reactions of a finite-size nuclear reactor. Also, write the critical size of reactors of different shapes in terms of geometrical buckling constant. (20 marks)

हिंदी में पढ़ें

(a) (i) प्रतिचुम्बकत्व क्या है ? प्रतिचुम्बकीय पदार्थों की चुम्बकीय सुग्राहिता ऋणात्मक क्यों होती है ? (ii) प्रतिचुम्बकत्व के क्वांटम सिद्धान्त की सीमाओं की विवेचना कीजिए । (iii) चुम्बकीय सुग्राहिता को तापमान फलन के रूप में आरेखित कीजिए । आरेख को दर्शिते समय सापेक्षिक पैमानों (स्केल्स) का ध्यान रखें जिससे कि चुम्बकीय परिघटनाओं की सापेक्षिक शक्तियाँ प्रस्तुत हो सकें । (20 अंक) (b) आकृति (I) में दर्शाए गए निवेशी संकेत को तुलनक (कम्पेरेटर) परिपथ में अनुप्रयुक्त किया गया है जो कि आकृति (II) में दिया गया है। निर्गत संकेत का निवेशी संकेत के साथ समुचित संबंध दर्शाते हुए एक रेखाचित्र संरचित कीजिए। मान लीजिए कि op-amp के अधिकतम निर्गत स्तर ± 12 V हैं। (10 अंक) (c) एक स्वपोषित नाभिकीय रिएक्टर की क्रांतिकता क्या है ? एक परिमित-आमाप के नाभिकीय रिएक्टर की नाभिकीय श्रृंखला अभिक्रियाओं को प्रभावित करने वाली मूल प्रक्रियाओं को लिखिए। विभिन्न आकारों के रिएक्टरों के क्रांतिक आमाप को ज्यामितीय आकुंचन (बकलिंग) स्थिरांक के पदों में भी लिखिए। (20 अंक)

Answer approach & key points

(a) Three parts (5 + 5 + 10): (i) define diamagnetism and explain the negative susceptibility; (ii) discuss the limitations of the quantum theory of diamagnetism; (iii) draw a susceptibility-versus-temperature diagram covering the magnetic phenomena, with attention to the RELATIVE SCALES so that their relative strengths are visible. (b) Read the given op-amp comparator circuit, compute the reference (threshold) voltage set by the resistive divider, and SKETCH the output waveform in correct time-alignment with the given ±5 V sinusoidal input, given that the op-amp saturates at ±12 V. (c) Three demands: define the criticality of a self-sustaining reactor (k_eff = 1); list the basic processes that affect the chain reaction in a FINITE reactor (the six-factor formula, including leakage); and write the critical size of reactors of different shapes in terms of the geometrical buckling.

  • Larmor precession ω_L = eB/2mₑ, Lenz's law, and χ = -μ₀NZe²⟨r²⟩/6mₑ < 0 (Langevin-Larmor), of order -10⁻⁵ and temperature-independent
  • Limitations: independent closed-shell atoms only, need for ⟨r²⟩, Van Vleck paramagnetism, Landau diamagnetism of conduction electrons (χ_L = -⅓χ_Pauli), band-structure effects; Bohr-van Leeuwen theorem
  • Diagram: diamagnet flat and about -10⁻⁵; paramagnet C/T; ferromagnet Curie-Weiss above T_C and 10³-10⁵ below; antiferromagnet cusp at T_N; superconductor χ = -1
  • Relative scales stated or drawn (signed logarithmic axis), superconductor and ferromagnet far larger in magnitude than diamagnet and paramagnet
  • Open-loop comparator: R₁/R₂ junction to the inverting input, V_in to the non-inverting input; no feedback
  • V_ref = 15 × 1.0/(8.2 + 1.0) ≈ 1.63 V; output +12 V when V_in > V_ref and -12 V when V_in < V_ref
  • Switching at 5 sin θ = 1.63, θ ≈ 19° and 161°; output high for 142° per cycle (about 39%)
  • Output sketched as a square wave aligned with the input, switching at the V_ref crossings
  • Critical means k_eff = 1 (steady chain); reactivity ρ = (k_eff - 1)/k_eff
  • Four-factor formula k∞ = ηεpf, each factor defined; finite reactor k_eff = k∞P_FNLP_TNL (six-factor); delayed neutrons, β ≈ 0.0065
  • Criticality condition B_m² = B_g² with B_m² = (k∞ - 1)/M²
  • Sphere B_g² = (π/R)², R_c = π/B; cylinder (2.405/R)² + (π/H)²; box (π/a)² + (π/b)² + (π/c)²; extrapolated dimensions
Q8
50M discuss

(a) (i) Discuss the Debye model of lattice specific heat. What are the limitations of the Debye model ? (10 marks) (ii) At very low temperatures, the specific heat of rock salt varies with temperature according to the Debye T³ law. The Debye temperature for rock salt is 281 K. How much heat will be required to raise the temperature of 2 kilo-mol of rock salt from 10 K to 50 K ? (5 marks) (b) What is the photovoltaic effect ? What are the processes that are required to obtain a useful power output from photon interactions in a semiconductor ? List the factors that affect the efficiency of a solar cell. (15 marks) (c) What do you understand by the SU(3) symmetry for the classification of baryons and mesons ? Draw the octets for baryons and mesons along with their quarks and antiquarks. (20 marks)

हिंदी में पढ़ें

(a) (i) जालक विशिष्ट ऊष्मा के डेबाई मॉडल की चर्चा कीजिए। डेबाई मॉडल की सीमाएँ क्या हैं ? (10 अंक) (ii) बहुत निम्न तापक्रमों पर, रॉक सॉल्ट की विशिष्ट ऊष्मा तापमान के साथ डेबाई T³ नियम के अनुसार विचरित होती है। रॉक सॉल्ट का डेबाई तापमान 281 K है। 2 किलो-मोल रॉक सॉल्ट के तापमान को 10 K से 50 K तक बढ़ाने के लिए कितनी ऊष्मा की आवश्यकता होगी ? (5 अंक) (b) प्रकाश-वोल्टीय प्रभाव क्या है ? एक अर्धचालक में फोटॉन अन्योन्यक्रियाओं से उपयोगी शक्ति निर्गत प्राप्त करने के लिए आवश्यक प्रक्रियाएँ क्या हैं ? एक सोलर सेल की दक्षता को प्रभावित करने वाले कारकों को सूचीबद्ध कीजिए। (15 अंक) (c) बेरिऑन एवं मेसॉन के वर्गीकरण के लिए SU(3) सममिति से आप क्या समझते हैं ? बेरिऑन एवं मेसॉन के अष्टकों को उनके क्वार्कों एवं एंटीक्वार्कों के साथ संरिखित कीजिए । (20 अंक)

Answer approach & key points

(a(i)) Discuss the Debye model of lattice specific heat — its assumptions, the density of states and cut-off frequency, the resulting C_V expression and its two limits — and then state the limitations of the model. (a(ii)) Using the Debye T³ law with θ_D = 281 K for rock salt, compute the heat required to raise 2 kilomol of NaCl from 10 K to 50 K — i.e. integrate C_V(T) ∝ T³ between the two temperatures. (b) Three demands: define the photovoltaic effect; state the processes needed to extract useful electrical power from photon interactions in a semiconductor (generation, separation, collection); and LIST the factors affecting solar-cell efficiency. (c) Explain SU(3) flavour symmetry as the basis for classifying baryons and mesons, and DRAW both the baryon octet and the meson octet, labelling every member with its quark (or quark–antiquark) content.

  • Model: continuum, 3N modes, linear dispersion, cut-off ω_D, θ_D = ħω_D/k_B, g(ω) = 9Nω²/ω_D³, C_V integral form
  • Limits: 3R at high T and (12π⁴/5)R(T/θ_D)³ at low T
  • At least three limitations: isotropic single sound speed, no optical branches, harmonic (no thermal expansion), electrons ignored, θ_D varies with T
  • Q = n(3π⁴R/5θ_D³)(T₂⁴ − T₁⁴) ≈ 2.73×10⁵ J for n = 2 kmol
  • Definition: generation of voltage/current at a junction under illumination without bias
  • Three processes: absorption (hν ≥ E_g, pair creation), carrier separation by junction field, collection by contacts through the load
  • η = V_oc I_sc FF/P_in
  • At least five factors: band gap, reflection/shading, recombination, series/shunt resistance, temperature, illumination/spectrum
  • SU(3) flavour of u, d, s; generators, quantum numbers I₃ and Y = B + S, Q = I₃ + Y/2
  • Mesons 3 ⊗ 3̄ = 8 ⊕ 1; baryons 3⊗3⊗3 = 10 ⊕ 8 ⊕ 8 ⊕ 1
  • Baryon octet in the (I₃, Y) hexagon with correct quark content (p uud, n udd, Σ, Λ, Ξ)
  • Meson octet with π, K, K̄, η and quark-antiquark content (ud̄, us̄, and so on)

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