Physics by Lamhi: Not Your Boring Physics

CLASS 12 · CHAPTER 1 · ELECTROSTATICS

QUICK REVISION

Electric Charges and Fields

Every key result from this chapter, boxed and ready for a last look before the exam. No derivations here, just what to recall and when to use it — for the full explanation, see the detailed notes.

1. Charge — Basic Properties

Quantisation of charge
q=ne,n=0,±1,±2,…q = ne,\qquad n = 0,\pm1,\pm2,\ldots

e≈1.6×10−19 Ce \approx 1.6\times10^{-19}\text{ C} — a charge of 1.5e1.5e never occurs.

  • Additive: total charge is the algebraic sum q1+q2+⋯+qnq_1+q_2+\cdots+q_n.
  • Conserved: total charge of an isolated system cannot change; rubbing only transfers electrons.

2. Coulomb's Law

F=kq1q2r2F = k\dfrac{q_1q_2}{r^2}

k=14πε0≈8.99×109 N m2C−2k = \dfrac{1}{4\pi\varepsilon_0} \approx 8.99\times10^9\text{ N m}^2\text{C}^{-2} (often rounded to 9×1099\times10^9); ε0≈8.85×10−12 C2N−1m−2\varepsilon_0 \approx 8.85\times10^{-12}\text{ C}^2\text{N}^{-1}\text{m}^{-2}.

F12=kq1q2r2 r^21\mathbf{F}_{12} = k\dfrac{q_1q_2}{r^2}\,\hat{r}_{21}

Like charges → repulsive (points away from source); unlike → attractive (points toward source). Newton’s third law: F21=−F12\mathbf{F}_{21} = -\mathbf{F}_{12}.

3. Electric Field and Superposition

Electric field (force per unit test charge)
E=Fq0\mathbf{E} = \dfrac{\mathbf{F}}{q_0}

Field of a single point charge QQ:

E=kQr2r^\mathbf{E} = k\dfrac{Q}{r^2}\hat{r}

Radially outward if Q>0Q>0, inward if Q<0Q<0.

Principle of superposition
E=E1+E2+⋯+En\mathbf{E} = \mathbf{E}_1 + \mathbf{E}_2 + \cdots + \mathbf{E}_n

Vector sum — each charge contributes as if the others weren’t there.

4. Field Lines and Electric Flux

  • Start on positive charge (or infinity), end on negative charge (or infinity); never closed loops.
  • Two field lines never cross.
  • Closer lines ⇒ stronger field; spread apart ⇒ weaker.
Flux through a flat area (uniform field)
ΔΦ=E⋅ΔA=E ΔAcos⁡θ\Delta\Phi = \mathbf{E}\cdot\Delta\mathbf{A} = E\,\Delta A\cos\theta
Flux through any surface
Φ=∮E⋅dA\Phi = \oint \mathbf{E}\cdot d\mathbf{A}

5. Electric Dipole

Dipole moment
p=q(2a) p^\mathbf{p} = q(2a)\,\hat{p}

Directed from −q-q to +q+q; magnitude p=q×2ap = q\times2a.

Axial field (r≫a)
Eaxial=2kpr(r2−a2)2  → r≫a   2kpr3E_{\text{axial}} = \dfrac{2kpr}{(r^2-a^2)^2}\;\xrightarrow{\,r\gg a\,}\;\dfrac{2kp}{r^3}
Equatorial field (r≫a)
Eequatorial=kp(r2+a2)3/2  → r≫a   kpr3E_{\text{equatorial}} = \dfrac{kp}{(r^2+a^2)^{3/2}}\;\xrightarrow{\,r\gg a\,}\;\dfrac{kp}{r^3}

Equatorial field points opposite to p\mathbf{p}, exactly half the axial magnitude at the same rr. Dipole field falls off as 1/r31/r^3 — a full power faster than a single charge’s 1/r21/r^2.

6. Torque on a Dipole in a Uniform Field

Net force on a dipole in a uniform field is always zero; the two equal, opposite forces form a couple.

Torque
τ=pEsin⁡θ,τ=p×E\tau = pE\sin\theta, \qquad \boldsymbol{\tau} = \mathbf{p}\times\mathbf{E}
  1. θ=0\theta = 0 (p\mathbf{p} aligned with E\mathbf{E}): stable equilibrium, τ=0\tau=0.
  2. θ=180∘\theta = 180^\circ (p\mathbf{p} anti-aligned): unstable equilibrium, τ=0\tau=0.

7. Gauss's Law

Gauss's law
∮E⋅dA=qencε0\oint \mathbf{E}\cdot d\mathbf{A} = \dfrac{q_{\text{enc}}}{\varepsilon_0}

Depends only on enclosed charge — independent of the surface’s shape/size, where inside the charge sits, and any charge outside (its net flux contribution is zero).

8. Gauss's Law — Standard Applications

  1. Infinite line charge (linear density λ\lambda): E=λ2πε0r=2kλrE = \dfrac{\lambda}{2\pi\varepsilon_0 r} = \dfrac{2k\lambda}{r} — falls off as 1/r1/r.
  2. Infinite plane sheet (surface density σ\sigma): E=σ2ε0E = \dfrac{\sigma}{2\varepsilon_0} — constant, independent of distance from the sheet.

Full derivations and worked examples: detailed notes →