Physics

UPSC Physics 2023 — Paper II

All 8 questions from UPSC Civil Services Mains Physics 2023 Paper II (400 marks total). Every stem reproduced in full, with directive-word analysis, marks, word limits, and answer-approach pointers.

8Questions
400Total marks
2023Year
Paper IIPaper

Topics covered

Quantum mechanics - potential wells and harmonic oscillator (1)Quantum mechanics - spin, potential barrier and particle in a box (1)Atomic structure and spectroscopy (1)Quantum mechanics and NMR (1)Particle physics, nuclear decay, reciprocal lattice, semiconductor Fermi level (1)Rutherford scattering, nuclear structure, nuclear forces and meson theory (1)Diamagnetism, Debye theory, Wien-Bridge oscillator (1)Nuclear reactor, superconductivity, operational amplifier (1)

A

Q1
50M Compulsory calculate Quantum mechanics - potential wells and harmonic oscillator

(a) Calculate the zero point energy for a particle in an infinite potential well for the following cases : (i) a 100 g ball confined on a 5 m long line. (ii) an oxygen atom confined to a 2×10⁻¹⁰ m lattice. (iii) an electron confined to a 10⁻¹⁰ m atom. Why zero point energy is not important for macroscopic objects ? Comment. 10 marks (b) Consider a particle of mass m and charge q moving under the influence of a one dimensional harmonic oscillator potential. Assume it is placed in a constant electric field E. The Hamiltonian of this particle is therefore given by H = p²/2m + ½mω²X² - qEX. Obtain the energy expression and the wave function of the nth excited state of the particle. 10 marks (c) A particle of mass m is in a spherically symmetric attractive potential of radius a. Find the minimum depth of the potential needed to have two bound states of zero angular momentum. 10 marks (d) A beam of hydrogen atoms emitted from an oven at 400 k is sent through a Stern-Gerlach experiment having magnet of length 1 m and a gradient field of 10 tesla/m. Calculate the transverse deflection of an atom at the point where the beam leaves the magnet. 10 marks (e) If an atom is placed in a magnetic field of strength 0·1 weber/m², then calculate the rate of precession and torque on an electron with l = 3 in the atom. Given that the magnetic moment of the electron makes an angle of 30° with the magnetic field. 10 marks

हिंदी में पढ़ें

(a) एक कण को अनंत विभव कूप में रखने पर निम्न स्थितियों के लिए शून्य बिंदु ऊर्जा की गणना करें : (i) एक 100 g की गेंद जो 5 m लंबी रेखा पर प्रतिबंधित है । (ii) एक ऑक्सीजन परमाणु जो 2×10⁻¹⁰ m जालक पर प्रतिबंधित है । (iii) एक इलेक्ट्रॉन जो 10⁻¹⁰ m परमाणु में प्रतिबंधित है । स्थूल वस्तुओं के लिए शून्य बिंदु ऊर्जा का महत्व क्यों नहीं है ? टिप्पणी करें । 10 अंक (b) द्रव्यमान m और आवेश q का एक कण एक एकविमीय आवर्ती दोलक विभव के प्रभाव के अधीन गतिशील है । मान लीजिये कि इसे एक स्थिर विद्युत क्षेत्र E में रखा गया है । इसलिये इस कण का हैमिल्टोनियन H = p²/2m + ½mω²X² - qEX द्वारा प्रदत है । कण की nth उत्तेजित अवस्था के लिये ऊर्जा व्यंजक और तरंग फलन प्राप्त कीजिये । 10 अंक (c) द्रव्यमान m का एक कण अर्धव्यास a के गोलीय सममित आकर्षक विभव में है । शून्य कोणीय संवेग की दो परिबद्ध अवस्थाओं के लिये आवश्यक विभव की न्यूनतम गहराई ज्ञात कीजिये । 10 अंक (d) तापमान 400 k पर एक अवन से उत्सर्जित हाइड्रोजन परमाणुओं का एक पुंज स्टर्न-गर्लैक प्रयोग में, जिसके चुंबक की लंबाई 1 m व चुंबकीय प्रवणता क्षेत्र 10 टेस्ला/मीटर है, भेजा जाता है । उस बिंदु पर जहाँ पुंज चुंबक को छोड़ता है, अनुप्रस्थ विषेषण की गणना कीजिये । 10 अंक (e) यदि एक परमाणु को 0·1 weber/m² तीव्रता के चुंबकीय क्षेत्र में रखा है, तब एक इलेक्ट्रॉन जो परमाणु में l = 3 अवस्था में है की पुरस्सरण की दर एवं बल आघूर्ण की गणना कीजिये। दिया गया है कि इलेक्ट्रॉन का चुंबकीय आघूर्ण चुंबकीय क्षेत्र से 30° का कोण बनाता है। 10 अंक

Answer approach & key points

Calculate requires systematic numerical working with proper physical reasoning. Structure: (a) Apply E₁ = π²ℏ²/(2mL²) for all three cases, showing orders of magnitude comparison; (b) Complete the square for the shifted harmonic oscillator, finding new equilibrium and energy levels; (c) Solve radial Schrödinger equation for l=0 with boundary conditions at r=a; (d) Use force method or quantum expectation for Stern-Gerlach splitting; (e) Apply Larmor precession formula τ = μ×B. Allocate ~20% time each to (a), (b), (c), (d), (e) as all carry equal marks.

  • (a) Zero-point energy calculation: E₁ = π²ℏ²/(2mL²) for 100g ball (~10⁻⁶⁷ J), oxygen atom (~10⁻²¹ J), electron (~10⁻¹⁸ J); explicit comparison showing macroscopic E₁ is negligible vs thermal energy kT ~ 10⁻²¹ J at 300K
  • (b) Shifted harmonic oscillator: complete square to get H = p²/2m + ½mω²(X - qE/mω²)² - q²E²/2mω²; energy levels Eₙ = (n+½)ℏω - q²E²/2mω²; wave functions ψₙ(x) = φₙ(x - qE/mω²) where φₙ are standard HO eigenfunctions
  • (c) Spherical well: radial equation for l=0 with u(r)=rR(r); boundary conditions u(0)=0, continuity of u and u' at r=a; transcendental equation for bound states; condition for two bound states requires at least one node, giving minimum depth V₀ ≥ π²ℏ²/(8ma²)
  • (d) Stern-Gerlach: force F = μ_z(dB/dz) = ±(eℏ/2m_e)(dB/dz); classical trajectory with transverse acceleration; deflection δz = (F/m_H)(L/v)²/2 where v = √(3kT/m_H); numerical value ~0.3-0.5 mm
  • (e) Larmor precession: ω_L = g_lμ_BB/ℏ = μ_BB/ℏ for orbital moment (g_l=1); torque |τ| = μBsinθ = lμ_B·B·sin30°; precession rate ~10⁹ rad/s, torque ~10⁻²³ Nm
Q2
50M solve Quantum mechanics - spin, potential barrier and particle in a box

(a) An operator P describing the interaction of two spin 1/2 particles is P = a + bσ⃗₁·σ⃗₂, where a and b are constants, and σ⃗₁ and σ⃗₂ are Pauli matrices of the two spins. The total spin angular momentum S⃗ = S⃗₁ + S⃗₂ = 1/2 ℏ(σ⃗₁ + σ⃗₂). Show that P, S² and Sz can be measured simultaneously. 15 marks (b) Consider a stream of particles of mass m each moving in the positive x-direction with kinetic energy E towards the potential barrier V(x) = 0 for x ≤ 0, V(x) = 3E/4 for x > 0. Find the fraction of particles reflected at x = 0. 15 marks (c) Consider the potential V(x) = { 0, 0 < x < a; ∞, elsewhere } (a) Estimate the energies of the ground state as well as those of the first and the second excited states for (i) an electron enclosed in a box of size a = 10⁻¹⁰ m. (ii) a 1 g metallic sphere which is moving in a box of size a = 10 cm. (b) Discuss the importance of the Quantum effects for both of these systems. (c) Estimate the velocities of the electron and the metallic sphere using uncertainty principle. 20 marks

हिंदी में पढ़ें

(a) दो प्रचक्रण 1/2 के कणों की पारस्परिक क्रिया को एक संकारक P = a + bσ⃗₁·σ⃗₂ से दर्शाया गया है जहाँ a व b स्थिरांक एवं σ⃗₁, σ⃗₂ दोनों प्रचक्रण के पाउली आव्यूह हैं। कुल प्रचक्रण कोणीय संवेग S⃗ = S⃗₁ + S⃗₂ = 1/2 ℏ(σ⃗₁ + σ⃗₂) है। दर्शाइये कि P, S² एवं Sz का एक साथ मापन किया जा सकता है। 15 अंक (b) विचार कीजिए कि m द्रव्यमान के और गतिज ऊर्जा E के कणों की एक धारा धनात्मक x-दिशा में एक विभव अवरोधक की ओर गतिमय है। V(x) = 0 for x ≤ 0, V(x) = 3E/4 for x > 0. x = 0 पर परावर्तित कणों का अंश ज्ञात कीजिए। 15 अंक (c) मान लें, विभव V(x) = { 0, 0 < x < a; ∞, बाकी सब जगह } तब (a) आर्य अवस्था तथा पहली व दूसरी उत्तेजित अवस्थाओं की ऊर्जाओं का आकलन कीजिए। जबकि (i) एक इलेक्ट्रॉन एक बाक्स के अंदर परिबद्ध है जिसका आकार a = 10⁻¹⁰ m है। (ii) 1 g की बृत्ताकार धातु जो आकार a = 10 cm के बाक्स में गतिशील है। (b) ऊपर दिये गये दोनों निकायों के लिये क्वांटम प्रभाव के महत्व की चर्चा कीजिए। (c) अनिश्चितता सिद्धांत का प्रयोग कर इलेक्ट्रॉन व बृत्ताकार धातु के वेगों का आकलन कीजिए। 20 अंक

Answer approach & key points

Solve this multi-part quantum mechanics problem by first proving the simultaneous measurability in part (a) through operator commutation, then calculating reflection coefficient in part (b) using boundary conditions, and finally computing energy levels and velocities for both quantum and classical systems in part (c). Allocate approximately 30% time to part (a), 25% to part (b), and 45% to part (c) given its higher mark weightage and computational complexity. Conclude with a comparative discussion highlighting why quantum effects dominate at atomic scales but are negligible for macroscopic objects.

  • Part (a): Prove [P, S²] = 0 and [P, Sz] = 0 using σ⃗₁·σ⃗₂ = (S²/ℏ²) - 3/2 and [S², Sz] = 0, establishing complete set of commuting observables
  • Part (b): Apply boundary conditions at x=0 for wavefunctions ψ_I = Ae^(ikx) + Be^(-ikx) and ψ_II = Ce^(ik'x) with k=√(2mE)/ℏ, k'=√(2m(E-V))/ℏ=√(2mE/4)/ℏ to find reflection coefficient R = |B/A|² = (k-k')²/(k+k')² = 1/9
  • Part (c)(i): Calculate E_n = n²π²ℏ²/(2ma²) for electron (m=9.11×10⁻³¹ kg, a=10⁻¹⁰ m): E₁≈6.02×10⁻¹⁸ J≈37.6 eV, E₂≈150.4 eV, E₃≈338.4 eV
  • Part (c)(ii): Calculate same formula for metallic sphere (m=10⁻³ kg, a=0.1 m): E₁≈5.49×10⁻⁶⁴ J, showing extremely closely spaced levels
  • Part (c)(b): Discuss quantum effects: electron shows discrete levels, zero-point energy, wave-particle duality; sphere behaves classically with continuous energy spectrum
  • Part (c)(c): Apply ΔxΔp≥ℏ/2 to estimate v_electron≈1.1×10⁶ m/s (relativistic correction may be noted) and v_sphere≈5×10⁻³¹ m/s (effectively at rest)
  • Demonstrate understanding that quantum-classical correspondence principle requires n→∞ or ℏ→0 limits
Q3
50M explain Atomic structure and spectroscopy

(a) What is vector atom model ? How the principal features of vector atom model were explained by Stern-Gerlach experiment ? (5+10=15 marks) (b) What is Lande's g factor ? Evaluate the Lande's g factor for the ³P₁ level in the 2p3s configuration of the ⁶C atom. Also calculate the splitting of the level when the atom is placed in an external magnetic field of 0·1 tesla. (5+5+5=15 marks) (c) What is Raman effect ? Explain Quantum theory of Raman effect and Rotational Structure of a Raman spectrum. (5+10+5=20 marks)

हिंदी में पढ़ें

(a) परमाणु का सदिश मॉडल क्या है ? सदिश परमाणु मॉडल की प्रमुख विशेषताओं की स्टर्न-गर्लाक प्रयोग द्वारा किस प्रकार व्याख्या की गई थी ? (5+10=15) (b) लैंडे g फैक्टर क्या है ? ⁶C परमाणु के 2p3s विन्यास के ³P₁ स्तर के लिए लैंडे g फैक्टर का मूल्यांकन कीजिए । जब परमाणु को 0·1 tesla के बाह्य चुंबकीय क्षेत्र में रखा जाये तो स्तर के विभाजन की भी गणना करें । (5+5+5=15) (c) रमन प्रभाव क्या है ? रमन प्रभाव के क्वांटम सिद्धांत एवं रमन वर्णक्रम (स्पेक्ट्रम) की घूर्णी संरचना की व्याख्या कीजिये । (5+10+5=20)

Answer approach & key points

Begin with a brief introduction linking atomic structure to spectroscopic phenomena. For part (a), spend ~30% time explaining vector atom model concepts and Stern-Gerlach experimental validation. For part (b), allocate ~30% to deriving Landé g-factor with proper LS coupling for ³P₁ state and calculating Zeeman splitting. For part (c), dedicate ~40% to quantum theory of Raman effect with rotational energy level diagrams. Conclude by emphasizing how these three phenomena collectively demonstrate space quantization and quantum mechanical treatment of atomic systems.

  • Part (a): Vector atom model with orbital (L), spin (S) and total (J) angular momentum vectors; Stern-Gerlach experiment showing space quantization and electron spin discovery through Ag beam splitting
  • Part (a): Explanation of how Stern-Gerlach results confirmed quantization of magnetic moment and existence of spin angular momentum, resolving Bohr-Sommerfeld model limitations
  • Part (b): Landé g-factor formula derivation for LS coupling: g_J = 1 + [J(J+1) + S(S+1) - L(L+1)]/[2J(J+1)]; calculation for ³P₁ (L=1, S=1, J=1) yielding g_J = 3/2
  • Part (b): Zeeman energy shift ΔE = μ_B·g_J·B·m_J with m_J = -1,0,+1; numerical evaluation for B=0.1 T giving splitting of ±9.27×10⁻²⁴ J or ±5.79×10⁻⁵ eV
  • Part (c): Raman effect as inelastic light scattering with Stokes/anti-Stokes lines; quantum theory involving virtual energy levels and polarizability tensor
  • Part (c): Rotational Raman spectrum showing ΔJ = ±2 selection rule, spacing of 4B, and alternating intensity due to nuclear spin statistics (relevant for homonuclear molecules like N₂, O₂)
  • Part (c): Distinction between Rayleigh, Stokes and anti-Stokes lines with energy level diagram showing rotational transitions
Q4
50M solve Quantum mechanics and NMR

(a) A particle constrained to move along x-axis in the domain 0 ≤ x ≤ L has a wave function ψ(x) = sin(nπx/L), where n is an integer. Normalize the wave function and evaluate the expectation value of momentum of the particle. (15 marks) (b) Evaluate the most probable distance of the electron of the hydrogen atom in its 2p state. What is the radial probability density at that distance ? (15 marks) (c) What is nuclear magnetic resonance ? Explain its working principle and use in magnetic resonance imaging systems. (5+5+10=20 marks)

हिंदी में पढ़ें

(a) x-अक्ष के अनुदिश गतिशील और 0 ≤ x ≤ L प्रांत (डोमेन) में प्रतिबंधित एक कण का तरंगफलन ψ(x) = sin(nπx/L) है; जहाँ n एक पूर्णांक है । तरंगफलन का प्रसामान्यीकरण कीजिये और कणके संवेग के प्रत्याशा मान का मूल्यांकन कीजिये । (15) (b) हाइड्रोजन परमाणु की 2p अवस्था के इलेक्ट्रॉन के लिए सबसे संभावित दूरी का मूल्यांकन कीजिये । इस दूरी पर त्रिज्य प्रायिकता घनत्व क्या है ? (15) (c) नाभिकीय चुंबकीय अनुनाद क्या है ? इसके कार्यकारी सिद्धांत और चुंबकीय अनुनाद इमेजिंग प्रणाली में इसके उपयोग का वर्णन कीजिये । (5+5+10=20)

Answer approach & key points

Solve this multi-part numerical-cum-descriptive question by allocating approximately 30% time to part (a) on particle-in-a-box normalization and momentum expectation, 30% to part (b) on hydrogen 2p state radial probability, and 40% to part (c) on NMR principles and MRI applications. Begin each part with the relevant formula, show complete derivation steps, and conclude with physical interpretation—especially connecting MRI to healthcare applications in Indian context like AIIMS Delhi's advanced imaging facilities.

  • Part (a): Normalization constant A = √(2/L) obtained by integrating |ψ|² from 0 to L; momentum expectation value ⟨p⟩ = 0 shown via direct integration or operator method
  • Part (a): Recognition that ⟨p⟩ = 0 reflects stationary state with equal probability of left/right motion, or explicit calculation using p̂ = -iℏ(d/dx)
  • Part (b): Radial wave function R₂₁(r) ∝ r·exp(-r/2a₀) for 2p state; radial probability density P(r) = r²|R₂₁|² ∝ r⁴exp(-r/a₀)
  • Part (b): Most probable distance r_mp = 4a₀ obtained by dP/dr = 0; maximum probability density value P(r_mp) = (1/24a₀)·(4/e)⁴ or equivalent simplified form
  • Part (c): NMR defined as resonant absorption of RF radiation by nuclear spins in magnetic field; working principle involving Zeeman splitting, Larmor precession, and resonance condition ω = γB₀
  • Part (c): MRI working: gradient coils for spatial encoding, RF pulses for excitation, detection of FID signals; T₁/T₂ contrast for tissue differentiation; Indian relevance: indigenous MRI development at BARC, widespread diagnostic use for cancer and neurological disorders

B

Q5
50M Compulsory derive Particle physics, nuclear decay, reciprocal lattice, semiconductor Fermi level

(a) How could you establish that $\nu_e$ and $\bar{\nu}_e$ are two different particles ? 10 marks (b) What is the age of a fossil that contains 6 g of carbon $^{14}C$ and has a decay rate of 27 decays per minute ? Given : Ratio $\frac{^{14}C}{^{12}C}$=$1.3\times10^{-13}$, Half life $(T_{1/2})$ of $^{14}C$ = 5730 yrs. 10 marks (c) Name the interactions via which the above nuclear decays occur : (i) $K^+ \longrightarrow \Pi^+ + \Pi^+ + \Pi^-$ (ii) $\Pi^+ + p \longrightarrow \Pi^+ + \Pi^+ + n$ (iii) $\Pi^+ + p \longrightarrow \Delta^{++} \longrightarrow \Pi^+ + p$ (iv) $\Sigma^\circ \longrightarrow \Lambda^\circ + \gamma$ (v) $\Sigma^+ \longrightarrow \Lambda^\circ + e^+ + \nu_e$ (vi) $K^- + p \longrightarrow K^+ + K^\circ + \Omega^-$ (vii) $\Pi^\circ \longrightarrow \gamma + e^+ + e^-$ (viii) $\Sigma^- \longrightarrow n + e^- + \bar{\nu}_e$ (ix) $\Lambda^\circ \longrightarrow p + e^- + \bar{\nu}_e$ (x) $e^+ + e^- \longrightarrow \gamma + \gamma$ 10 marks (d) Derive diffraction conditions using reciprocal lattice concept. What are these conditions known as ? 10 marks (e) Show that the Fermi level shifts upward, closer to the conduction band in an n-type semiconductor and shifts downward, closer to the valence band in a p-type semiconductor. 10 marks

हिंदी में पढ़ें

(a) आप किस प्रकार स्थापित करेंगे कि $\nu_e$ एवं $\bar{\nu}_e$ दो विभिन्न प्रकार के कण हैं ? 10 (b) जिस जीवाश्म में 6 g कार्बन $^{14}C$ है एवं उसकी क्षय दर 27 क्षय प्रति मिनट है, उसकी आयु क्या है ? दिया गया है : $\frac{^{14}C}{^{12}C}$ का अनुपात=$1.3\times10^{-13}$, $^{14}C$ की अर्ध-आयु $(T_{1/2})$ = 5730 वर्ष । 10 (c) उन अन्योन्य क्रियाओं को नामित कीजिए जिनके द्वारा निम्नलिखित नाभिकीय क्षय घटित होते हैं : (i) $K^+ \longrightarrow \Pi^+ + \Pi^+ + \Pi^-$ (ii) $\Pi^+ + p \longrightarrow \Pi^+ + \Pi^+ + n$ (iii) $\Pi^+ + p \longrightarrow \Delta^{++} \longrightarrow \Pi^+ + p$ (iv) $\Sigma^\circ \longrightarrow \Lambda^\circ + \gamma$ (v) $\Sigma^+ \longrightarrow \Lambda^\circ + e^+ + \nu_e$ (vi) $K^- + p \longrightarrow K^+ + K^\circ + \Omega^-$ (vii) $\Pi^\circ \longrightarrow \gamma + e^+ + e^-$ (viii) $\Sigma^- \longrightarrow n + e^- + \bar{\nu}_e$ (ix) $\Lambda^\circ \longrightarrow p + e^- + \bar{\nu}_e$ (x) $e^+ + e^- \longrightarrow \gamma + \gamma$ 10 (d) व्युत्क्रम जालक अवधारणा का उपयोग करके विवर्तन की शर्तों की व्युत्पत्ति कीजिये । इन शर्तों को किस रूप में जाना जाता है ? 10 (e) दर्शाइए कि फर्मी स्तर n-प्रकार के अर्धचालक में ऊपर की तरफ चालन बैंड के नजदीक विस्थापित होता है और p-प्रकार के अर्धचालक में नीचे की तरफ संयोजकता बैंड के नजदीक विस्थापित होता है । 10

Answer approach & key points

Begin with a brief introduction acknowledging the breadth from particle physics to solid state physics. For part (a), explain helicity, lepton number conservation, and scattering experiments; for (b), set up the radioactive decay equation and solve for age; for (c), classify all ten reactions by interaction type using conservation laws; for (d), derive Laue conditions from reciprocal lattice vectors; for (e), use charge neutrality and mass action law to show Fermi level shifts. Allocate time proportionally: ~15% each for (a), (b), (c), and 20% each for (d) and (e) due to derivations required.

  • (a) Distinguishing νₑ and ν̄ₑ: helicity differences, lepton number conservation (Lₑ = +1 vs −1), and experimental evidence from inverse beta decay (ν̄ₑ + p → n + e⁺) vs (νₑ + n → p + e⁻)
  • (b) Age calculation: determine initial ¹⁴C mass from given ratio, apply N = N₀e^(-λt) with λ = ln(2)/T₁/₂, relate activity A = λN, solve for t ≈ 11,400 years
  • (c) Interaction classification: (i) Weak, (ii) Strong, (iii) Strong (resonance formation), (iv) Electromagnetic, (v) Weak, (vi) Weak (strangeness changing), (vii) Electromagnetic, (viii) Weak, (ix) Weak, (x) Electromagnetic
  • (d) Reciprocal lattice derivation: define reciprocal basis vectors b₁, b₂, b₃, show scattering vector Δk = G (reciprocal lattice vector), derive Laue conditions k·G = G²/2 or equivalently 2k·G = G²
  • (e) Fermi level shifts: for n-type, n = N_D⁺ + nᵢ²/n, show E_F moves toward E_C; for p-type, p = N_A⁻ + nᵢ²/p, show E_F moves toward E_V using charge neutrality and mass action law
Q6
50M derive Rutherford scattering, nuclear structure, nuclear forces and meson theory

(a) Establish the Rutherford's scattering cross section formula for α-particle by considering the standard assumptions and symbols. 20 marks (b) By assuming the nucleus as a cubical box of length equal to the nuclear diameter 10⁻¹² cm, calculate the kinetic energy of the highest level occupied nucleon of iron-56 nucleus. 15 marks (c) What do you understand by nuclear forces ? Explain meson theory of exchange forces. 5+10=15 marks

हिंदी में पढ़ें

(a) मानक अभिधारणाओं एवं प्रतीकों को लेकर α-कणों के लिए रदरफोर्ड के प्रकीर्णन परिछेत्र के सूत्र को स्थापित कीजिए । 20 (b) नाभिक को नाभिक व्यास 10⁻¹² cm के समतुल्य लम्बाई का एक घनीय बॉक्स मान कर उच्चतम स्तर पर अधिष्ठित आयरन-56 नाभिक के न्यूक्लिऑन की गतिज ऊर्जा की गणना कीजिये । 15 (c) नाभिकीय बलों से आप क्या समझते हैं ? विनिमय बलों के मेसॉन सिद्धांत की व्याख्या कीजिये । 5+10=15

Answer approach & key points

Derive the Rutherford differential cross-section formula in part (a) by setting up the scattering geometry, applying Coulomb's law, and integrating to obtain the solid angle dependence. For part (b), apply the particle-in-a-box quantum mechanical model with appropriate boundary conditions to calculate the Fermi energy for Fe-56 nucleons. In part (c), define nuclear forces with their key characteristics, then explain Yukawa's meson exchange theory with mass-energy relation and range estimation. Allocate approximately 40% effort to (a), 30% to (b), and 30% to (c) based on mark distribution.

  • Part (a): Coulomb scattering geometry with impact parameter b, scattering angle θ, and hyperbolic trajectory; derivation of relation b = (kZe²/2E)cot(θ/2); differential cross-section dσ/dΩ = (kZe²/4E)²cosec⁴(θ/2); assumptions: point charge nucleus, single scattering, non-relativistic α-particles, neglect of electron screening
  • Part (a): Integration over solid angle to show total cross-section divergence, physical significance of Rutherford formula validation through Geiger-Marsden experiments at Manchester
  • Part (b): Particle in a 3D cubic box energy levels E = (h²/8mL²)(nx²+ny²+nz²); nuclear diameter L = 10⁻¹² cm; neutron and proton as spin-½ fermions with degeneracy g=2; Fermi momentum and energy calculation for A=56, Z=26, N=30
  • Part (b): Numerical computation with ħc = 197 MeV-fm, nucleon mass ≈ 938 MeV/c², proper unit conversion from cm to fm; comparison with empirical nuclear Fermi energy ~38 MeV
  • Part (c): Nuclear force characteristics: short-range (~1-3 fm), spin-dependent, charge-independent, saturated, non-central tensor component; contrast with Coulomb force
  • Part (c): Yukawa meson theory: virtual particle exchange, uncertainty principle ΔE·Δt ≈ ħ, meson mass mπ from range R ≈ ħ/mπc ≈ 1.4 fm giving mπ ≈ 140 MeV/c²; prediction of π-meson later discovered in cosmic rays by Powell (1950 Nobel Prize)
Q7
50M explain Diamagnetism, Debye theory, Wien-Bridge oscillator

(a) Explain classical theory of diamagnetism. Show that the susceptibility of diamagnetic substances is directly proportional to the atomic number. Why all the electrons in an atom contribute to diamagnetism ? 5+8+2=15 (b) Derive an expression for the specific heat of a solid based on the Debye theory and show how it agrees with the experimental values. What is the most important assumption of Debye theory in comparison to Einstein theory ? Is there any drawback of Debye theory ? 15+3+2=20 (c) With a neat circuit diagram, explain the working of Wien-Bridge oscillator. 15

हिंदी में पढ़ें

(a) प्रतिचुंबकत्व के चिरप्रतिष्ठित सिद्धांत की व्याख्या कीजिए । दर्शाइए कि प्रतिचुंबकीय पदार्थों की प्रवृत्ति सीधे परमाणु संख्या के समानुपाती होती है । एक परमाणु के सभी इलेक्ट्रॉन प्रतिचुंबकत्व में योगदान क्यों करते हैं ? 5+8+2=15 (b) डिबाई सिद्धांत से एक ठोस पदार्थ की विशिष्ट ऊष्मा के लिए व्यंजक प्राप्त करें और दिखाइए कि प्रायोगिक मानों से यह कितना संगत है । आइंस्टाइन सिद्धांत की तुलना में डिबाई सिद्धांत में सबसे महत्वपूर्ण अभिधारणा क्या है ? डिबाई सिद्धांत में क्या कोई कमी है ? 15+3+2=20 (c) एक स्पष्ट परिपथ आरेख के साथ वीन-ब्रिज दोलक की कार्य प्रणाली की व्याख्या कीजिए । 15

Answer approach & key points

The directive 'explain' demands clear exposition with logical flow across all three parts. Allocate approximately 30% time/words to part (a) on diamagnetism (15 marks), 40% to part (b) on Debye theory (20 marks), and 30% to part (c) on Wien-Bridge oscillator (15 marks). Structure: begin each part with defining the core concept, proceed through derivations with intermediate steps shown, and conclude with physical significance and limitations.

  • Part (a): Larmor precession explanation, derivation of χ = -μ₀NZe²⟨r²⟩/(6mₑ), proportionality to Z via electron count, and explanation of why all electrons contribute (closed shells, no net paramagnetism)
  • Part (b): Debye frequency distribution g(ω) ∝ ω², derivation of Cᵥ = 9R(T/θ_D)³∫₀^(θ_D/T) x⁴eˣ/(eˣ-1)²dx, T³ law at low T and Dulong-Petit at high T, comparison with Einstein's single frequency assumption
  • Part (c): Wien-Bridge circuit with four resistors and two capacitors, frequency formula f = 1/(2πRC), Barkhausen criterion (R₃/R₄ = 2), amplitude stabilization via lamp or diodes
  • Debye theory assumption: continuous spectrum of frequencies up to ω_D vs Einstein's single ω_E; Debye's acoustic phonon approximation
  • Drawbacks of Debye theory: fails at intermediate temperatures, neglects optical phonons, assumes isotropic solids and linear dispersion
  • Experimental verification: specific heat data for copper, lead, diamond showing T³ region and Debye temperature extraction
Q8
50M explain Nuclear reactor, superconductivity, operational amplifier

(a) What do you understand by the critical size of a reactor ? Explain the main features of nuclear reactors. 5+15=20 (b) What is superconductivity ? Explain Meissner effect. Why superconductors should be a diamagnetic material ? 15 (c) (i) Determine the input and output impedances of the amplifier in given figure. The op-amp datasheet gives Z_in = 2 MΩ, Z_out = 75 Ω and A_OL = 200,000 (open loop voltage gain). 10 (ii) Find the closed-loop voltage gain. 5

हिंदी में पढ़ें

(a) रिएक्टर के क्रांतिक आकार से आप का क्या अभिप्राय है ? नाभिकीय रिएक्टरों की मुख्य विशेषताओं का वर्णन कीजिए । 5+15=20 (b) अतिचालकता क्या है ? माइसनर प्रभाव की व्याख्या कीजिए । अतिचालक पदार्थ क्यों एक प्रतिचुंबकीय पदार्थ होते हैं ? 15 (c) (i) दर्शाए गए चित्र में प्रवर्धक का निवेशी और निर्गत प्रतिबाधाओं का मान निर्धारित कीजिए । संक्रियात्मक प्रवर्धक के डेटाशीट के अनुसार Z_in = 2 MΩ, Z_out = 75 Ω और A_OL (खुला पाश वोल्टता गेन) = 200,000 है । 10 (ii) संयुक्त पाश वोल्टता गेन का मान प्राप्त कीजिए । 5

Answer approach & key points

The directive 'explain' demands clear conceptual exposition with logical reasoning. Allocate approximately 40% effort to part (a) given its 20 marks, 30% to part (b) for 15 marks, and 30% combined to part (c)(i) and (ii) for 15 marks. Structure: begin with reactor physics fundamentals, transition to superconductivity phenomena, then conclude with systematic op-amp circuit analysis using negative feedback principles.

  • Critical size definition: minimum dimensions for self-sustaining chain reaction where neutron production equals losses (multiplication factor k=1); mention critical mass and critical volume relationship
  • Nuclear reactor main features: fuel (enriched U-235/Pu-239), moderator (heavy water/graphite in Indian PHWRs), control rods (Cd/B), coolant, shielding; reference Indian reactors like Dhruva or CIRUS
  • Superconductivity: zero DC resistance below critical temperature Tc; Meissner effect as perfect diamagnetism with expulsion of magnetic field (B=0 inside); Type-I vs Type-II distinction
  • Diamagnetic necessity: superconductors must expel magnetic flux to maintain zero resistance state; London penetration depth and thermodynamic argument for free energy minimization
  • Op-amp input impedance with feedback: Z_in(CL) = Z_in(OL)[1+βA_OL] for non-inverting; output impedance reduction by factor (1+βA_OL)
  • Closed-loop gain derivation: A_CL = A_OL/(1+βA_OL) ≈ 1/β for large A_OL; identify feedback network β from resistor configuration
  • Numerical calculation: substitute given values Z_in=2MΩ, Z_out=75Ω, A_OL=200,000 with appropriate β determination from implied circuit topology

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