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Milan Physics Page List

Milan Physics Page List

Saturday, November 29, 2025

🔬 Potential Energy - Class 12 Physics

🔬 POTENTIAL ENERGY (U)

Class 12 Physics | Complete Detailed Notes

📚 1. DEFINITION & BASIC CONCEPT

U = - ∫ F · dr

"Stored energy due to position, configuration, or state of a system"

✅ Key Properties:
  • Scalar quantity
  • Depends on position/configuration
  • Reference point arbitrary (only ΔU matters)
  • Force = -∇U (Negative gradient)

🎯 2. TYPES OF POTENTIAL ENERGY

A. Gravitational Potential Energy (U_g)

Near Earth's Surface

U_g = mgh
SymbolMeaningSI Unit
mMasskg
gAcceleration due to gravity9.8 m/s²
hHeight above referencem

Universal Gravitational PE

U_g = -GMm/r
⚡ Key Points:
  • Negative sign → Attractive force
  • U = 0 at r = ∞
  • Maximum (least negative) at infinity
ConceptFormulaUnit
Gravitational Field (g)GM/r²N/kg
Gravitational Potential (V)-GM/rJ/kg
PE of mass mmV = -GMm/rJ

B. Elastic Potential Energy (U_s)

U_s = ½kx²
📈 Graph: Parabola (U vs x)
                          U
                        ½kx²
                         │
                         └─────────→ x
                    

C. Electric Potential Energy

U = kq₁q₂/r

k = 9×10⁹ Nm²/C² | +ve (repulsive) / -ve (attractive)

🔧 3. IMPORTANT DERIVATIONS

A. Derivation of Spring PE

W = ∫₀ˣ kx dx = ½kx²

This work = Potential Energy stored

B. Relation: F = -dU/dx

SystemUF = -dU/dx
Gravitymgh-mg ✓
Spring½kx²-kx ✓

📊 4. GRAPHICAL REPRESENTATION

Potential Energy Curves
SystemU vs x GraphForce Direction
SpringParabola (U-shaped)Towards equilibrium
GravityStraight lineDownward
Stable equilibriumMinimum URestoring force
Unstable equilibriumMaximum UAway from point
💡 Work from PE Graph:
W_conservative = -ΔU
Area under F-x = ΔU

🌍 Gravity (Earth)

U = mgh
F = -mg

🌌 Gravity (Universal)

U = -GMm/r
F = -GMm/r²

🪢 Spring

U = ½kx²
F = -kx

⚡ Electric

U = kq₁q₂/r
F = kq₁q₂/r²

⚠️ 5. COMMON MISTAKES & TIPS

❌ WRONG✅ CORRECT
U = mgh (absolute)ΔU = mgΔh
PE depends on velocityOnly position
Spring PE = kx½kx²
F = dU/dxF = -dU/dx

🎯 6. NEET/JEE LEVEL QUESTIONS

Q1: Work done by gravity when body falls from height h?
Ans: W_g = -ΔU = mgh ✓
Q2: Spring constant if 2 kg mass compresses spring by 10 cm?
Ans: k = mg/x = 196 N/m

Friday, November 28, 2025

Detailed Notes: Class 12 Physics Chapter 5 - Magnetism and Matter

Detailed Notes: Class 12 Physics Chapter 5 - Magnetism and Matter

Detailed Notes: Class 12 Physics Chapter 5 - Magnetism and Matter

These notes are based on the NCERT syllabus for CBSE Class 12 Physics (updated for 2025-26). They provide in-depth explanations, derivations, formulas, and key concepts for comprehensive understanding and revision. Structured section-wise, with embedded diagrams from public educational sources for visual aid. Important formulas are highlighted, and examples/numericals hints are included where relevant.

1. Introduction to the Bar Magnet and Magnetic Dipole

1.1 Bar Magnet

A bar magnet is a rectangular piece of ferromagnetic material (e.g., steel, iron) that exhibits magnetic properties with two distinct poles: North (N) pole and South (S) pole.

  • Key Properties:
    • Like poles repel, unlike poles attract (Coulomb's inverse square law applies).
    • Poles always occur in pairs; isolated poles (monopoles) do not exist.
    • Magnetic length (2ℓ): Distance between the two effective poles, slightly less than the geometric length (2L), typically ℓ ≈ 0.9L due to pole contraction.
  • Neutral Points: Points where the net magnetic field is zero, e.g., on the equatorial line in an external uniform field.

Diagram: Bar Magnet Poles and Magnetic Length (NCERT Fig. 5.1)

Bar magnet with field lines

Description: Rectangular bar magnet with N pole on left, S on right. Geometric length 2L, magnetic length 2ℓ (ℓ ≈ 0.9L). Dipole moment M from S to N.

Reference: Wikimedia Commons (public domain). More at BYJU'S.

1.2 Magnetic Dipole

A magnetic dipole consists of two equal and opposite magnetic poles separated by a small distance (2ℓ).

  • Magnetic Dipole Moment (M): Vector quantity pointing from S to N pole.
    • Magnitude: \[ M = m \times 2\ell \], where m is pole strength (SI unit: A·m).
    • For a current-carrying loop: \[ \vec{M} = I \vec{A} \], where I is current, A is area vector (perpendicular to plane, right-hand rule).
    • SI Unit: A·m² or J/T (joule per tesla).
  • Equivalence: A bar magnet behaves like a current loop (or solenoid) for far-field approximations.

Example: A bar magnet with pole strength 0.5 A·m and magnetic length 0.1 m has M = 0.05 A·m².

2. Coulomb's Law in Magnetism

Statement: The force between two magnetic poles is directly proportional to their pole strengths and inversely proportional to the square of the distance between them.

  • Formula: \[ F = \frac{\mu_0}{4\pi} \frac{m_1 m_2}{r^2} \]
    • Attractive if poles are unlike; repulsive if like.
    • \[ \frac{\mu_0}{4\pi} = 10^{-7} \] T·m/A (permeability of free space constant).
  • Derivation Insight: Analogous to electrostatic Coulomb's law, but magnetic (no negative poles, hence no isolated monopoles).
  • Limitations: Valid only in vacuum; ignores material effects.

Numerical Hint: Calculate force between two poles m = 10 A·m at r = 0.1 m: F ≈ 10^{-5} N (repulsive if same poles).

3. Magnetic Field Lines

Definition: Imaginary lines representing the direction and strength of the magnetic field (B).

  • Properties:
    1. Form closed continuous loops (emerge from N, enter S outside; opposite inside).
    2. Direction: Tangent to the line gives \(\vec{B}\) direction (from N to S outside).
    3. Density: Higher density indicates stronger field.
    4. Never intersect (unique direction at a point).
    5. No two lines begin/end at same point (no monopoles).
  • For Bar Magnet: Crowded near poles (strong field); sparse in equatorial region.
  • For Current Loop: Similar to bar magnet; field reverses inside the loop.

Diagram: Magnetic Field Lines Around Bar Magnet (NCERT Fig. 5.2)

Magnetic field lines around bar magnet

Description: Curved lines emerge from N pole, enter S pole, forming closed loops. Dense near poles, sparse equatorially. Inside: S to N.

Reference: Wikimedia Commons. Video at YouTube.

4. Magnetic Field on the Axis and Equatorial Line of a Magnetic Dipole (Bar Magnet)

4.1 Axial Position (End-on)

Point on the axis, distance d from center (d >> ℓ).

  • Field (B_A): \[ B_A = \frac{\mu_0}{4\pi} \frac{2M}{d^3} \]
    • Direction: Along the axis, away from N pole (parallel to M).
  • Derivation: Superposition of fields from two poles; approximates to dipole for large d.

Diagram: Axial (End-on) Position (NCERT Fig. 5.3)

Axial magnetic field of bar magnet

Description: Point P on axis at d from center; B_axial parallel to M, from N outward.

Reference: Wikimedia Commons. See Vedantu PDF.

4.2 Equatorial Position (Broadside-on)

Point on perpendicular bisector, distance d from center (d >> ℓ).

  • Field (B_E): \[ B_E = \frac{\mu_0}{4\pi} \frac{M}{d^3} = \frac{1}{2} B_A \]
    • Direction: Parallel to axis but opposite to M (towards S pole).
  • Comparison: B_A = 2 B_E; both decrease as 1/d³.

Diagram: Equatorial (Broadside-on) Position (NCERT Fig. 5.4)

Equatorial magnetic field of bar magnet

Description: Point P on bisector; B_equatorial anti-parallel to M.

Reference: Wikimedia Commons.

Neutral Point: On equatorial line, where external B cancels bar magnet's B_E.

Numerical Hint: For M = 1 A·m², d = 0.1 m, B_A ≈ 2 × 10^{-5} T.

5. Magnetic Dipole in a Uniform Magnetic Field

5.1 Torque on a Dipole

A dipole in uniform \(\vec{B}\) experiences no net force (equal/opposite on poles) but a couple (torque).

  • Formula: \[ \vec{\tau} = \vec{M} \times \vec{B} \]
    • Magnitude: \[ \tau = MB \sin \theta \] (θ = angle between M and B).
    • Direction: Perpendicular to plane of M and B; tends to align M with B.
  • Stable Equilibrium: θ = 0° (τ = 0, minimum energy).
  • Unstable Equilibrium: θ = 180°.

Diagram: Torque on Dipole in Uniform Field (NCERT Fig. 5.7)

Torque on magnetic dipole

Description: Dipole M at angle θ to B; torque τ perpendicular, aligning M with B.

Reference: Wikimedia Commons.

5.2 Potential Energy

  • Formula: \[ U = -\vec{M} \cdot \vec{B} = -MB \cos \theta \]
    • Minimum at θ = 0° (stable); maximum at θ = 180° (unstable); zero at θ = 90°.
  • Work Done to rotate from θ₁ to θ₂: \[ W = MB (\cos \theta_1 - \cos \theta_2) \].

5.3 Oscillation of a Freely Suspended Magnet

Small angular displacement: Performs SHM in Earth's horizontal field B_H.

  • Time Period: \[ T = 2\pi \sqrt{\frac{I}{MB_H}} \]
    • I = moment of inertia about suspension point.
  • Application: Vibration magnetometer measures M and B_H.
  • Derivation Insight: τ = -MB_H sinθ ≈ -MB_H θ (small θ); like torsional pendulum.

6. Moving Coil Galvanometer and Earth's Magnetism (Connection)

In vibration magnetometer, T helps find M = (4π² I)/(T² B_H).

Earth's field used as uniform B.

7. The Moving Coil Galvanometer (Brief Link to Chapter)

Though in Chapter 4, relevant here: Torque τ = N I A B sinθ aligns with dipole torque.

8. Gauss's Law for Magnetism

Statement: The surface integral of \(\vec{B}\) over any closed surface is zero.

  • Formula: \[ \oint \vec{B} \cdot d\vec{A} = 0 \]
  • Implication: Magnetic field lines form closed loops; no net flux (no monopoles).
  • Analogy with Electrostatics:
ElectrostaticsMagnetism
\[ \oint \vec{E} \cdot d\vec{A} = \frac{q}{\epsilon_0} \]\[ \oint \vec{B} \cdot d\vec{A} = 0 \]
Isolated charges existNo isolated poles

9. Earth's Magnetism

9.1 Earth's Magnetic Field

Earth acts like a giant bar magnet (dipole moment ≈ 8 × 10²² A·m², confirmed as of 2025), but actually due to dynamo effect (molten core currents).

Total Field (B): Varies (weaker at equator ~0.3 × 10^{-4} T; stronger at poles ~0.6 × 10^{-4} T).

9.2 Magnetic Elements

  • Declination (δ or θ): Angle between magnetic meridian (compass N) and geographic meridian (true N). Varies (0° at agonic line).
  • Inclination or Dip Angle (δ): Angle between total B and horizontal plane.
    • At magnetic equator: δ = 0° (B horizontal).
    • At magnetic poles: δ = 90° (B vertical).
  • Horizontal Component (B_H): \[ B_H = B \cos \delta \] (used in compasses).
  • Vertical Component (B_V): \[ B_V = B \sin \delta \].
  • Relations: \[ B = \frac{B_H}{\cos \delta} = B_H \sqrt{1 + \tan^2 \delta} \]; \[ \tan \delta = \frac{B_V}{B_H} \].
  • Average B_H ≈ 0.3–0.6 × 10^{-4} T (India: ~0.4 × 10^{-4} T).

Diagram: Earth's Magnetic Elements (Declination & Dip)

Earth's magnetic dip and declination diagram

Description: Compass showing declination θ; dip circle for inclination δ. B_H horizontal, B_V vertical.

Example: If δ = 30°, B_H = 0.3 × 10^{-4} T, then B_V ≈ 0.17 × 10^{-4} T; B ≈ 0.35 × 10^{-4} T.

Reference: Wikimedia Commons.

9.3 Measurement

  • Deflection Magnetometer: Measures B_H, M (tan A/B positions).
  • Vibration Magnetometer: Measures M, B_H via T.

10. Magnetism and Magnetic Properties of Materials

10.1 Basic Relations

  • Magnetic Field (B): Total field inside material.
  • Magnetizing Field (H): External field causing magnetization (SI unit: A/m).
  • Magnetization (M): Magnetic moment per unit volume (SI unit: A/m).
  • Key Relation: \[ \vec{B} = \mu_0 (\vec{H} + \vec{M}) \]
  • Relative Permeability (μ_r): \[ \mu_r = \frac{B}{\mu_0 H} = 1 + \frac{M}{H} \]
  • Magnetic Susceptibility (χ_m): \[ \chi_m = \frac{M}{H} \] (dimensionless).
    • μ_r = 1 + χ_m.

10.2 Classification of Materials

Materials classified based on response to external H:

Typeχ_m Valueμ_r ValueBehaviorExamplesExplanation
DiamagneticNegative, small (~ -10^{-5})< 1Weakly repelled; field lines expelled (Meissner effect in superconductors).Bi, Cu, H₂O, Au, AgInduced M opposes H (Lenz's law); all materials show this weakly.
ParamagneticPositive, small (~ 10^{-5})>1, close to 1Weakly attracted; aligns with field.Al, Cr, O₂, Pt, MgAtomic dipoles align with H; disordered without field. Follows Curie's Law: \[ \chi_m = \frac{C}{T} \] (C = Curie constant).
FerromagneticPositive, large (~10²–10⁶)>>1Strongly attracted; retains magnetism (domains align).Fe, Ni, Co, GdDomain structure; hysteresis; Curie temperature (T_C) above which becomes paramagnetic.
  • Diamagnetism: Temperature independent; universal.
  • Paramagnetism: Inverse to T.
  • Ferromagnetism: Complex; Weiss theory (internal fields).

10.3 Hysteresis Loop

B-H Curve: Plot of B vs H; loop shows lag (hysteresis).

  • Retentivity (Residual Magnetism): B at H=0.
  • Coercivity: Reverse H to make B=0.

Soft Magnets (e.g., soft iron): Narrow loop (low coercivity, low retentivity) – for electromagnets.

Hard Magnets (e.g., steel): Wide loop (high coercivity, high retentivity) – for permanent magnets.

Energy Loss: Area of loop = energy dissipated per cycle (as heat).

Diagram: Hysteresis Loop

Hysteresis loop diagram

Description: B vs H plot; S-shaped initial curve, closed loop on cycling. Shows saturation, retentivity, coercivity.

Reference: Wikimedia Commons.

11. Permanent Magnets and Electromagnets

11.1 Permanent Magnets

Made from hard ferromagnetic materials (high coercivity); retain M without external H.

  • Materials: Alnico, CrCo, ferrites.
  • Demagnetization Methods: Heating above T_C, hammering, AC field.
  • Limitations: Lose strength over time; cannot vary strength.

11.2 Electromagnets

Temporary magnets using soft iron core in solenoid; strength varies with I.

  • Advantages: Variable strength/polarity; no residual magnetism; stronger than permanent.
  • Formula for Field: \[ B = \mu_0 n I \] (inside solenoid).

Choice: Permanent for steady fields (e.g., fridge magnets); electromagnets for cranes, MRI.

Important Formulas Summary Table

ConceptFormulaKey Notes
Dipole Moment\[ M = m \cdot 2\ell = I A \]Vector from S to N
Force Between Poles\[ F = \frac{\mu_0}{4\pi} \frac{m_1 m_2}{r^2} \]Attractive for unlike poles
Axial Field\[ B_A = \frac{\mu_0}{4\pi} \frac{2M}{d^3} \]Parallel to M
Equatorial Field\[ B_E = \frac{\mu_0}{4\pi} \frac{M}{d^3} \]Anti-parallel to M
Torque\[ \tau = M B \sin \theta \]Aligns M with B
Potential Energy\[ U = - M B \cos \theta \]Min at θ=0°
Oscillation Period\[ T = 2\pi \sqrt{\frac{I}{M B_H}} \]SHM for small θ
Earth's Components\[ B_H = B \cos \delta \], \[ B_V = B \sin \delta \]tan δ = B_V / B_H
B-H Relation\[ B = \mu_0 (H + M) \], \[ \chi_m = M/H \]μ_r = 1 + χ_m

Tips for Exams

  • Derivations: Practice axial/equatorial fields, torque from forces.
  • Numericals: Focus on B calculations, T for oscillations, susceptibility.
  • Conceptual: Explain why no monopoles, hysteresis importance.
  • Diagrams: Draw field lines, hysteresis loop, dip circle.
  • MCQs: Common on properties, classifications, Earth's elements.

For practice questions, refer to NCERT exercises. These notes cover 100% of the chapter for boards/JEE. Updated values confirmed for 2025. If you need Hindi version or expansions, let me know!

Sunday, November 23, 2025

Magnetic Field & Magnetisation - Curie's Law

Magnetic Field & Magnetisation – Colorful Notes

Magnetic Field & Magnetisation
and Curie’s Law

1. Magnetic Field and Magnetisation

Material ke andar effective magnetic field B ka formula:

B = μ₀ (H + M)

Where:

  • B = Magnetic field (Tesla)
  • H = Magnetising field (A/m)
  • M = Magnetisation
  • μ₀ = 4π × 10⁻⁷ T·m/A

Magnetisation & Susceptibility

M = χ H

Substitute M = χH inside B = μ₀(H + M):

B = μ₀H(1 + χ)

Thus permeability:

μ = μ₀(1 + χ)

So,

B = μH
Example 1: Calculate B

Given: χ = 0.004, H = 1000 A/m

1) Magnetisation:

M = χH = 0.004 × 1000 = 4 A/m

2) Magnetic Field:

B = μ₀(H + M) = 4π × 10⁻⁷ × 1004 ≈ 1.26 × 10⁻³ T

2. Curie’s Law

Paramagnetic materials ke liye:

χ = C / T

Temperature ↑ → Susceptibility ↓

Example 2: Curie’s Law

Given: C = 0.8 K

At T₁ = 200 K:

χ₁ = 0.8 / 200 = 0.004

At T₂ = 400 K:

χ₂ = 0.8 / 400 = 0.002

Result: Temperature doubles → χ half.

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