Chapter 1 · RevisionTextbook pages 42–46

Summary, Points to Ponder & Quick Quiz

The whole chapter on one page: the textbook summary as cards, the Points to Ponder, a formula sheet with units, the mistakes that cost marks, flashcards (with the Malayalam terms), a scored board-style quiz and your study checklist.

1. The chapter in one picture

🗺️ Electric charges and fields – concept map

Read it from the centre outwards: charge → force between charges (Coulomb, superposition) → field (E = F/q₀) → field lines and flux → Gauss’s law and its three applications; a pair of opposite charges is a dipole.

2. Summary – the textbook list as cards

1Forces that build matter

Electric and magnetic forces determine the properties of atoms, molecules and bulk matter. – page 4

2Two kinds of charge

Electric charge (വൈദ്യുത ചാർജ്): like charges repel, unlike attract. Glass rubbed with silk: +; plastic rubbed with fur: − (Franklin’s convention). – page 4

3Conductors and insulators

Conductors (ചാലകം) let charge move; insulators (ഇൻസുലേറ്റർ (കുചാലകം)) do not. In metals electrons move; in electrolytes both + and − ions. – page 5

4Three properties of charge
q = ne,  e = 1.6 × 10−19 C

Quantisation (ചാർജിന്റെ ക്വാണ്ടീകരണം), additivity (ചാർജിന്റെ സങ്കലനീയത) – algebraic sum, and conservation (ചാർജ് സംരക്ഷണം) – charge is transferred, never created or destroyed. – page 6

5Coulomb’s law
F21 = k q1q2 r̂21/r212,  k = 1/4πε0 ≈ 9 × 109 N m2 C−2

Coulomb’s law (കൂളോം നിയമം); ε0 = 8.854 × 10−12 C2 N−1 m−2. – page 7

6Electric vs gravitational
ke2/(G memp) ≅ 2.4 × 1039

Between an electron and a proton the electric force is about 1039 times stronger. – page 7

7Superposition
F1 = F12 + F13 + … + F1n

Superposition principle (അധ്യാരോപണ തത്വം): each pair force is unaffected by other charges; add the forces as vectors. – page 8

8Electric field
E = F/q0;  point charge E = |q|/(4πε0r2)

Electric field (വൈദ്യുത മണ്ഡലം): radially outward for +q, inward for −q; obeys superposition. – page 9

9Field lines

Field lines (വൈദ്യുത മണ്ഡലരേഖകൾ): the tangent gives the direction of E; crowded where E is strong; uniform field – parallel, equally spaced lines. – page 10

10Properties of field lines

(i) continuous, no breaks; (ii) never cross; (iii) start on + and end on − charges – no closed loops. – page 10

11Electric dipole
p = q × 2a, from −q to +q

Electric dipole (വൈദ്യുത ദ്വിധ്രുവം) and dipole moment (ദ്വിധ്രുവ മൊമെന്റ്). – page 11

12Dipole fields
axial E = 2pr/[4πε0(r2 − a2)2] ≅ 2p/4πε0r3
equatorial E = −p/[4πε0(r2 + a2)3/2] ≅ −p/4πε0r3

Note the 1/r3 fall-off (a point charge: 1/r2). – page 11

13Dipole in a uniform field
τ = p × E,  τ = pE sin θ

Torque (ടോർക്ക് (ബലാഘൂർണം)) but no net force in a uniform field (ഏകീകൃത വൈദ്യുത മണ്ഡലം). – page 11

14Electric flux
Δφ = E·ΔS,  ΔS = ΔS n̂

Electric flux (വൈദ്യുത ഫ്ലക്സ്); for a closed surface n̂ is the outward normal. – page 10

15Gauss’s law and its uses
φ = qenc/ε0
wire λ/(2πε0r) · sheet σ/(2ε0) · shell q/(4πε0r2) outside, 0 inside

Gauss’s law (ഗോസ് നിയമം), easiest with symmetry. – page 12, page 13

3. Points to Ponder

  1. Why does the nucleus hold together? The protons repel, but the strong force (range about 10−14 m – the size of a nucleus) holds them; quantum mechanics keeps electrons out of the nucleus.
  2. Gravity vs electricity: both follow the inverse square law (വിപരീത വർഗ നിയമം), but gravity is only attractive while electric forces of + and − charges can cancel – so the weaker gravity dominates on large scales.
  3. k is not arbitrary in SI: the ampere is defined magnetically and 1 C = 1 A s, so k ≈ 9 × 109 N m2 C−2.
  4. Why is 1 C so large? Because it is set by magnetic forces, which are much weaker than electric ones; 1 C is too big a unit for electrostatics (we use μC, nC).
  5. Additivity is not obvious – it holds because charge is a scalar (അദിശം), with no direction.
  6. Charge is invariant – the same in frames moving relative to each other (kinetic energy, for example, is not). go further
  7. Conservation is a separate property: invariance in time. A scalar need not be conserved (kinetic energy in an inelastic collision); a vector can be (angular momentum).
  8. Quantisation of charge is a basic, unexplained law of nature – there is no such law for mass.
  9. Superposition is not just vector addition: a pair force is not changed by other charges, and there are no extra three-body forces.
  10. The field of discrete charges is not defined at the charges; for a volume distribution it is defined everywhere; across a charged surface it jumps.
  11. A configuration with zero total charge (a dipole) still has a field – it just falls faster than 1/r2 far away.

4. Formula sheet with units

📐 Constants

e = 1.6 × 10−19 C · k = 1/(4πε0) = 9 × 109 N m2 C−2 · ε0 = 8.854 × 10−12 C2 N−1 m−2
1 μC = 10−6 C · 1 nC = 10−9 C · 1 C ≈ 6.25 × 1018 electrons

📐 Formulas

QuantityFormulaSI unitRemember
Quantisationq = neCn = 0, ±1, ±2, …
Coulomb forceF = kq1q2/r2Npoint charges at rest; along the line joining them
SuperpositionF1 = Σ F1iNvector sum
Electric fieldE = F/q0N C−1 (= V m−1)force on a unit + test charge
Point chargeE = kq/r2N C−1outward for +q, inward for −q
Force on a chargeF = qENopposite to E for a negative charge
FluxΔφ = E ΔS cos θN m2 C−1 (= V m)θ between E and the normal
Dipole momentp = q × 2aC mfrom −q to +q
Dipole – axialE = 2kp/r3N C−1along p (r ≫ a)
Dipole – equatorialE = kp/r3N C−1opposite to p (r ≫ a)
Torque on a dipoleτ = pE sin θN mτ = p × E; net force 0 in a uniform field
Charge densitiesλ = Q/l, σ = Q/S, ρ = Q/VC m−1, C m−2, C m−3linear, surface, volume
Gauss’s law∮ E·dS = qenc/ε0N m2 C−1any closed surface; E due to all charges
Infinite line chargeE = λ/(2πε0r)N C−1E ∝ 1/r, radial
Infinite plane sheetE = σ/(2ε0)N C−1independent of distance
Spherical shellE = kq/r2 (r ≥ R); E = 0 (r < R)N C−1q = 4πR2σ
Charged conductorE = σ/ε0 just outside; 0 insideN C−1electrostatic shielding

📏 Physical quantities (textbook table)

QuantitySymbolDimensionsUnit
Vector area elementΔS[L2]m2
Electric fieldE[MLT−3A−1]V m−1
Electric fluxφ[ML3T−3A−1]V m
Dipole momentp[LTA]C m
Linear / surface / volume charge densityλ / σ / ρ[L−1TA] / [L−2TA] / [L−3TA]C m−1 / C m−2 / C m−3
⚠️ Common mistakes

5. Flashcards

Click a card to flip it. The Malayalam cards show the technical term first.

6. Scored board-style quiz

Answer all sixteen, then press Check my answers. Each wrong answer shows the page to revise. For number answers type only the number in the unit shown.

Your score appears below.

7. Your study checklist

Ticks come from “Mark this page as completed” at the bottom of each page.

🧭 Ready?

Next: the model question paper (70 marks) ▶ – write it on paper with a timer first, then check with the solved paper.