Class 12 CBSE Physics – Targeted Revision Session

Weak-to-Strong Chapter Walk-through

Roadmap: decode the 2024-25 sample paper, flag your weak concepts, and practise targeted problems to convert them into scoring strengths.

Sample paper snapshot – 33 questions, 5 sections (A–E), 70 marks, 3 h: our plan mirrors this pattern.

Source: CBSE Physics Sample Question Paper 2024-25 (Code 042)

Chapter-wise Question Distribution & Your Strength

Revision Roadmap

More questions mean higher exam weightage. Target “low” chapters first, consolidate “med”, then polish “high”.

Chapter # Qs Strength
Electric Charges & Fields 3 Low
Moving Charges & Magnetism 3 Low
Alternating Current 1 Low
Wave Optics 3 Low
Nuclei 2 Low
Electrostatic Potential & Capacitance 2 Med
Magnetism & Matter 1 Med
Electromagnetic Waves 2 Med
Dual Nature of Radiation & Matter 3 Med
Semiconductor Electronics 2 Med
Current Electricity 4 High
Electromagnetic Induction 2 High
Ray Optics & Optical Instruments 3 High
Atoms 2 High

Electric Charges & Fields – Tough Question

Gauss’s Law • Infinite Line Charge

Gauss’s theorem: Net electric flux through a closed surface equals enclosed charge divided by \( \varepsilon_0 \). 1. Gaussian surface — coaxial cylinder of radius \( r \) and length \( L \). 2. Flux evaluation — \( E \) is radial & uniform on curved area; ends contribute zero, so \( \Phi_E = E(2\pi rL) \). 3. Apply law — \( E(2\pi rL) = \lambda L/\varepsilon_0 \). Result: \( E(r) = \dfrac{\lambda}{2\pi \varepsilon_0 r} \).

Pitfalls: choosing a spherical surface breaks symmetry; remember no flux through end-caps.

Moving Charges & Magnetism – Tough Question

Magnetic Force Balance

A 10 g ball carrying +10 mC slides freely inside a vertical, frictionless tube. The tube is moved horizontally from east to west through a uniform 2 T magnetic field. Find (i) the minimum tube speed that keeps the ball stationary relative to the tube, and (ii) the direction of the magnetic field.

  1. Force balance: set \(qvB = mg\) so magnetic force equals weight.
  2. Solve speed: \(v = \dfrac{mg}{qB} = \dfrac{0.01\,\text{kg}\times 9.8}{0.01\,\text{C}\times 2\,\text{T}} \approx 4.9\ \text{m s}^{-1}\).
  3. Direction: Right-hand rule → with \(v\) west and \(F\) up, \(B\) must point south.

Key idea: \(F = qvB\) for motion ⟂ \(B\).

Important formula: \(F = qvB = mg\)

Alternating Current – Tough Question

New \(V_L\) after Short

Question: In a series LCR circuit \(V_R = V_C = V_L = 10\,\text{V}\) (resonance). The capacitor is short-circuited. Find the new voltage across the inductor.

Hints
1. Resonance ⇒ \(X_L = X_C\) and \(R = X_L\).
2. Without the capacitor, \(Z = \sqrt{R^{2}+X_L^{2}} = R\sqrt{2}\); current becomes \(I/\sqrt{2}\).
3. Hence \(V_L = IX_L/\sqrt{2} = 10/\sqrt{2} ≈ 7.1 V\).

Answer: \(10/\sqrt{2}\,\text{V}\).

Pitfalls: assuming current unchanged or forgetting \(V_C = 0\) after the short.

Key relation: \(Z = \sqrt{R^{2}+(\omega L)^{2}}\)

Wave Optics – Tough Question

Dual-wavelength YDSE

Q. In a Young’s double-slit set-up using λ1 = 400 nm and λ2 = 600 nm, find the smallest distance y from the central maximum where a common dark fringe appears.

Key relation \( \Delta = m\lambda_1 = \left(m+\tfrac{1}{2}\right)\lambda_2 \)

  • Apply the condition above to obtain the least positive integer \( m \).
  • Calculate the corresponding path difference \( \Delta \).
  • Translate to screen position: \( y = \dfrac{\Delta D}{d} \) (standard YDSE geometry).

Pitfalls: mix-ups between bright & dark criteria, forgetting to convert nm to metres.

Nuclei – Tough Question

Binding-Energy Curve Insight

Question: Using the binding-energy per nucleon curve, decide which nucleus—W(190), X(90), Y(60) or Z(30)—is most likely to (i) undergo fission and (ii) undergo fusion. Give a brief reason.

  • Hint 1 – Curve Slope: For A > 120 the curve falls; such heavy nuclei release energy by splitting.
  • Hint 2 – Light Nuclei: Very light nuclei (A < 10) lie low on the curve; they gain energy by combining.
  • Hint 3 – Apply Values: W (190) is heavy ⇒ fission. Z (30) is light ⇒ fusion.

Energy is released whenever a nucleus moves toward the curve’s peak at A≈60. Don’t confuse total binding energy with binding energy per nucleon.

Electrostatic Potential & Capacitance – Tough Question

Dielectric vs Metal Slab

Problem  A parallel-plate capacitor (plate area \(A\), gap \(d\)) receives
(i) a dielectric slab of thickness \(t\) and permittivity \(\kappa\),
(ii) a conducting slab of thickness \(t\) ( \(t<d\) ).
Derive \(C\) in each case and state which insertion increases capacitance more.

Hint 1  Model dielectric case as two series sections:
air gaps \((d-t)\) and dielectric slab \(t/\kappa\).
Hint 2  Equivalent capacitance
\(C_{\text{dielectric}}=\dfrac{\varepsilon_0A}{d-t+t/\kappa}\).
Hint 3  In a metal, \(E=0\); effective separation becomes \(d-t\), so
\(C_{\text{metal}}=\dfrac{\varepsilon_0A}{d-t}\).

Because \(d-t < d-t+t/\kappa\), we get \(C_{\text{metal}} > C_{\text{dielectric}}\).

⚠︎ Common slips: adding capacitances in parallel, omitting \(\kappa\).

Capacitance grows as the effective plate separation shrinks.

Source: CBSE Physics Sample Question Paper (2024 – 25)

Magnetism & Matter – Conceptual Question

Field Ratio at \(a/2\) Below & Above

A solid wire of radius \(a\) carries uniform current \(I\).
Find \(\displaystyle \frac{B_{\,a/2\;{\text{below}}}}{B_{\,a/2\;{\text{above}}}}\).

Hints
1. Ampère’s law → \(B_{\text{in}}=\mu_0 I r /(2\pi a^{2})\), \(B_{\text{out}}=\mu_0 I /(2\pi r)\).
2. Radii: inside point \(r=a/2\); outside point \(r=1.5a\).
3. Ratio \(= (a/2)/(1.5a)=1/3\).

Expected answer : \(1:3\).

Watch for mixing inside/outside formulas or using surface distances instead of center distances. Remember: inside \(B\propto r\); outside \(B\propto 1/r\).

Source: CBSE Physics Sample Paper 2024 – Q3

Electromagnetic Waves – Tough Question

Spectrum Production Match

Match each electromagnetic wave with its typical production mechanism: Infra-red, Radio, Light and Microwave.

Hints

  • IR – vibrations of atoms or molecules.
  • Radio – oscillating electrons in aerial/LC circuit.
  • Light – electronic transitions between atomic levels.
  • Microwave – klystron or maser action.
  • Map each wave to one source only; don’t mix IR with microwave.
  • Remember: production process follows the wave’s frequency range.

Dual Nature – Tough Question

Interpret the I–V Curves

Task → From the three photoelectric I–V plots (A, B, C), rank the incident beams by intensity and by frequency.

Hint 1: Higher saturation current ⇒ higher intensity.
Hint 2: More negative stopping potential ⇒ higher photon frequency (energy).
Hint 3: Compare both features to classify A, B, C.

Pitfall – Stopping potential is independent of intensity.

Einstein’s Photoelectric Equation: \(eV_0 = h\nu - \phi\).  Thus \(K_{\text{max}} = eV_0\).

Semiconductor Electronics – Tough Question

P-Type Band Diagram & Circuit

Question : Draw energy-band diagrams for a P-type semiconductor at 0 K and room temperature. Decide if the bulb glows when the switch is (a) open, (b) closed in the ideal-diode circuit.

Hints
• 0 K: Fermi level lies just above valence band, near acceptor level.
• Room T: holes populate valence band; \(E_F\) rises slightly.
• Switch open — diode reverse-biased; circuit broken; bulb off.
• Switch closed — diode forward-biased; current flows; bulb on.

Watch out : Misplacing \(E_F\) in conduction band or assuming reverse leakage in an ideal diode.

P-N Junction: Forward bias lowers the depletion barrier, allowing majority carriers to conduct.

Current Electricity – Tough Question

Temperature-Dependent Resistance

A heating element on a 100 V battery (internal resistance 1 Ω) draws 10 A at 20 °C. After warming to 320 °C, find the power dissipated inside the battery. Temperature coefficient α = 3.7 × 10−4 °C−1.

  • Hint 1: Hot resistance   \(R_h = R_{20}[1 + \alpha\,\Delta T]\)
  • Hint 2: Steady current   \(I = \dfrac{V}{r + R_h}\)
  • Hint 3: Battery loss   \(P_{int} = I^{2}r\)

Remember: apply α only to the element, not to the constant internal resistance. Power lost inside a source is always \(I^{2}r\).

Key formula: \(R_T = R_0(1 + \alpha\,\Delta T)\)

Electromagnetic Induction – Tough Question

A.C. Generator: Instantaneous EMF

Question – Derive the instantaneous emf induced in an N-turn coil of area A rotating with angular speed \( \omega \) in a uniform field \( B \).

1. Magnetic flux: \( \Phi = N B A \cos \theta \), where \( \theta = \omega t \). 2. Faraday’s law: \( e = -\dfrac{d\Phi}{dt} \). 3. Differentiate ⇒ \( e = N B A \omega \sin \omega t \). Peak value: \( e_{\text{max}} = N B A \omega \). Negative sign shows Lenz’s law; we usually quote magnitude only.

Energy comes from the mechanical work done by the prime mover rotating the coil.

Ray Optics – Tough Question

Cassegrain Telescope Imaging

Task: Draw a ray diagram of a Cassegrain telescope and state two advantages over a refractor.

• Primary concave and secondary convex mirrors fold the optical path.
• Secondary reflects rays through the central hole in the primary to the final focus.
• Advantages: no chromatic aberration; long focal length with a short, light tube.

Avoid: forgetting the hole in the primary mirror or claiming lower spherical aberration without proof.

Source: CBSE Physics SQP 2024-25 Q24

Atoms – Tough Question

Hydrogen Emission Line Puzzle

A discharge lamp contains an enormous number of hydrogen atoms. Each one-electron atom can be excited to different quantum levels. When electrons in different atoms return to lower levels, they emit photons with energies equal to the level gaps, \(E = 13.6\,\text{eV}\,(1/n_f^{2} - 1/n_i^{2})\). The many possible \(n_i \rightarrow n_f\) transitions across the ensemble create the full set of discrete spectral lines, even though every atom supplies only one electron.

Common mistake: imagining one electron makes all lines at once. In reality, many atoms, each in a single state, together produce the spectrum.

Key Takeaways

Quick Recap

• Exploit symmetry before using Gauss’s or Ampere’s law.
• Levitation needs \(qvB = mg\).
• At resonance \(V_L = V_C\); shorting \(C\) changes impedance.
• Interference minima: path difference = \((m+\tfrac12)\lambda\).
• Peak energy release near \(A \approx 60\).
• Capacitance rises as effective gap shrinks.
• Wire field: \(B \propto r\) inside, \(B \propto 1/r\) outside.
• Photon energy shifts stopping potential, not saturation current.
• Forward bias narrows depletion layer, enabling current.
• I²R losses heat conductors—monitor current.
• Generator emf \(e_{\text{max}} = NBA\omega\); mechanical work → electricity.
• Reflecting telescopes avoid chromatic aberration and stay compact.
• Many atoms yield multiple spectral lines, not one electron.

Next steps: revisit weaker chapters first, then drill derivations and numericals daily.