Quick Recap — Charge & Coulomb's Law

  • Charge: quantized (q=neq = ne, with e=1.6×1019e = 1.6\times10^{-19} C), conserved, and additive.
  • Coulomb's law: F=kq1q2r2F = \dfrac{kq_1 q_2}{r^2}, with k=14πε0=9×109k = \dfrac{1}{4\pi\varepsilon_0} = 9\times10^9 N m2^2/C2^2 — like charges repel, unlike attract.
  • Superposition: the net force or field is the vector sum of the individual contributions.
  • Electric field: E=Fq\vec{E} = \dfrac{\vec{F}}{q}; for a point charge E=kqr2E = \dfrac{kq}{r^2} (unit N/C).
  • Field lines start on positive and end on negative charges, never cross, and are denser where the field is stronger.

Beyond-NCERT JEE Formulae

Section 1 already nails Coulomb's law and the point-charge field, so this sheet gathers the results one level up — the dipole, continuous charge distributions, field energy and the capacitor toolkit. These are the formulae that quietly decide most JEE Main electrostatics questions. Constants used below: k=14πε0=9×109k=\dfrac{1}{4\pi\varepsilon_0}=9\times10^{9} SI units and ε0=8.85×1012\varepsilon_0=8.85\times10^{-12} SI units.

1. Electric dipole (short dipole, r much greater than its size)

  • Axial (end-on) field: Eax=2kpr3E_{ax}=\dfrac{2kp}{r^{3}}, directed along p\vec{p}.
  • Equatorial (broadside) field: Eeq=kpr3E_{eq}=\dfrac{kp}{r^{3}}, directed opposite to p\vec{p}; so at equal distance the axial field is exactly twice the equatorial field.
  • At a general angle θ\theta from the axis: E=kpr31+3cos2θE=\dfrac{kp}{r^{3}}\sqrt{1+3\cos^{2}\theta}, while the potential is V=kpcosθr2V=\dfrac{kp\cos\theta}{r^{2}} — note VV carries NO factor of 2 and falls as 1r2\dfrac{1}{r^{2}}, whereas EE falls as 1r3\dfrac{1}{r^{3}}.
  • In a uniform field: torque τ=pEsinθ\tau=pE\sin\theta (as a vector τ=p×E\vec{\tau}=\vec{p}\times\vec{E}), with zero net force; potential energy U=pEcosθU=-pE\cos\theta; and the work to turn it from θ1\theta_1 to θ2\theta_2 is W=pE(cosθ1cosθ2)W=pE(\cos\theta_1-\cos\theta_2).
  • In a NON-uniform field: the two ends feel unequal forces, so besides the torque there is a net translational force F=pdEdxF=p\dfrac{dE}{dx} (aligned dipole) dragging it toward the stronger-field region.

When to use: any "short dipole", "two equal and opposite charges 2a2a apart" or "polar molecule in a field" question. [JEE Tip] The axial factor of 2 lives in the FIELD only — never smuggle it into the dipole potential. When a problem compares an axial point with an equatorial point, weigh 2rax3\dfrac{2}{r_{ax}^{3}} against 1req3\dfrac{1}{r_{eq}^{3}}, not the bare distances.

2. Fields of continuous charge distributions

  • Infinite line charge: E=2kλr=λ2πε0rE=\dfrac{2k\lambda}{r}=\dfrac{\lambda}{2\pi\varepsilon_0 r}, radial and falling as 1r\dfrac{1}{r}.
  • Infinite non-conducting sheet: E=σ2ε0E=\dfrac{\sigma}{2\varepsilon_0}, uniform and independent of distance.
  • Just outside a charged conductor: E=σε0E=\dfrac{\sigma}{\varepsilon_0} — double the sheet result, because the charge sits on one face only.
  • Uniformly charged ring on its axis: E=kQx(x2+R2)3/2E=\dfrac{kQx}{(x^{2}+R^{2})^{3/2}}, which is zero at the centre and largest at x=R2x=\dfrac{R}{\sqrt{2}}.
  • Charged conducting sphere or shell (charge Q, radius R): for r>Rr>R it acts as a point charge, E=kQr2E=\dfrac{kQ}{r^{2}} with V=kQrV=\dfrac{kQ}{r}; for r<Rr<R, E=0E=0 but V=kQRV=\dfrac{kQ}{R} stays constant (a shell is NOT at zero potential inside).

When to use: rods or wires long compared with the distance (line), broad flat plates (sheet), the field just outside any conductor, and ring-on-axis set-ups. [JEE Tip] Fix the distance law to the geometry first: a point or sphere goes as 1r2\dfrac{1}{r^{2}}, an infinite line as 1r\dfrac{1}{r}, and an infinite sheet stays constant. Forcing a line or sheet into kqr2\dfrac{kq}{r^{2}} is the commonest silent blunder.

3. Field energy and the pull on a conductor

  • Energy density stored in any electric field: u=12ε0E2u=\dfrac{1}{2}\varepsilon_0 E^{2}, measured in J/m3^3; the total field energy is U=udVU=\displaystyle\int u\,dV.
  • Electrostatic pressure — the outward force per unit area on a charged conductor's surface: P=σ22ε0=12ε0E2P=\dfrac{\sigma^{2}}{2\varepsilon_0}=\dfrac{1}{2}\varepsilon_0 E^{2}.
  • Force between capacitor plates: each plate sits in the OTHER plate's field σ2ε0\dfrac{\sigma}{2\varepsilon_0}, so F=Q22ε0A=σ2A2ε0F=\dfrac{Q^{2}}{2\varepsilon_0 A}=\dfrac{\sigma^{2}A}{2\varepsilon_0}, always attractive.

When to use: "energy stored in the field", "force needed to hold a plate", or "outward pull on a charged shell / soap film" questions. [JEE Tip] That lone factor of 12\dfrac{1}{2} is the whole game: a plate feels only the other plate's field σ2ε0\dfrac{\sigma}{2\varepsilon_0}, not the full gap field σε0\dfrac{\sigma}{\varepsilon_0}. Dropping it doubles every force-on-a-plate answer.

4. Capacitor toolkit

  • Series: 1Cs=1Ci\dfrac{1}{C_s}=\displaystyle\sum\dfrac{1}{C_i} (every capacitor holds the SAME charge). Parallel: Cp=CiC_p=\displaystyle\sum C_i (every capacitor holds the SAME voltage).
  • Stored energy: U=12CV2=12QV=Q22CU=\dfrac{1}{2}CV^{2}=\dfrac{1}{2}QV=\dfrac{Q^{2}}{2C}. Keep the battery connected and VV is fixed (use 12CV2\tfrac12 CV^{2}); once it is disconnected the charge QQ is fixed (use Q22C\dfrac{Q^{2}}{2C}).
  • Dielectric slab of thickness t in a gap d (with t less than d): C=ε0Adt+t/KC=\dfrac{\varepsilon_0 A}{d-t+t/K}. A conducting slab is the KK\to\infty limit, giving C=ε0AdtC=\dfrac{\varepsilon_0 A}{d-t}, and where it sits in the gap makes no difference.
  • Combining two charged capacitors (like plates joined): common potential V=C1V1+C2V2C1+C2V=\dfrac{C_1V_1+C_2V_2}{C_1+C_2}, with heat lost ΔU=12C1C2C1+C2(V1V2)2\Delta U=\dfrac{1}{2}\dfrac{C_1C_2}{C_1+C_2}(V_1-V_2)^{2}.

When to use: any network reduction, energy-stored question, dielectric insertion, or "two capacitors reconnected" charge-sharing problem. [JEE Tip] The sharing loss ΔU\Delta U is ALWAYS positive (energy goes into the wire and the spark) and does not depend on the wire's resistance; it vanishes only when V1=V2V_1=V_2. That sign is a quick sanity check — you can never gain energy on reconnection.

Solved Examples — Beyond-NCERT Formulae

Example 1 — Dipole: axial vs equatorial field

Problem: A short dipole has moment p=6×109p=6\times10^{-9} C m. Find its field at an axial point and at an equatorial point, each 0.200.20 m away, and their ratio. Take k=9×109k=9\times10^{9} SI units.

Formula: Eax=2kpr3E_{ax}=\dfrac{2kp}{r^{3}} and Eeq=kpr3E_{eq}=\dfrac{kp}{r^{3}}.

Working: With r3=(0.20)3=8×103r^{3}=(0.20)^{3}=8\times10^{-3} and kp=(9×109)(6×109)=54kp=(9\times10^{9})(6\times10^{-9})=54,

Eax=2×548×103=1.35×104 N/CE_{ax}=\dfrac{2\times54}{8\times10^{-3}}=1.35\times10^{4}\ \text{N/C}

Eeq=548×103=6.75×103 N/CE_{eq}=\dfrac{54}{8\times10^{-3}}=6.75\times10^{3}\ \text{N/C}

Answer: Eax=1.35×104E_{ax}=1.35\times10^{4} N/C and Eeq=6.75×103E_{eq}=6.75\times10^{3} N/C, so the ratio is EaxEeq=2\dfrac{E_{ax}}{E_{eq}}=2 exactly — the axial field is always twice the equatorial field at the same distance.

Example 2 — Dipole: torque, energy and work to rotate

Problem: A dipole of moment p=3×108p=3\times10^{-8} C m sits in a uniform field E=5×104E=5\times10^{4} N/C. Find the torque when it makes 3030^\circ with the field, and the work an external agent does to turn it from alignment (00^\circ) to 9090^\circ.

Formula: τ=pEsinθ\tau=pE\sin\theta and U=pEcosθU=-pE\cos\theta, so W=U(θ2)U(θ1)=pE(cosθ1cosθ2)W=U(\theta_2)-U(\theta_1)=pE(\cos\theta_1-\cos\theta_2).

Working: First pE=(3×108)(5×104)=1.5×103pE=(3\times10^{-8})(5\times10^{4})=1.5\times10^{-3}. Then

τ=pEsin30=(1.5×103)(0.5)=7.5×104 N m\tau=pE\sin 30^\circ=(1.5\times10^{-3})(0.5)=7.5\times10^{-4}\ \text{N m}

W=pE(cos0cos90)=(1.5×103)(10)=1.5×103 JW=pE(\cos 0^\circ-\cos 90^\circ)=(1.5\times10^{-3})(1-0)=1.5\times10^{-3}\ \text{J}

Answer: torque =7.5×104=7.5\times10^{-4} N m and work =1.5×103=1.5\times10^{-3} J =1.5=1.5 mJ. The work equals pEpE here because the dipole is turned all the way to perpendicular, where cosθ=0\cos\theta=0.

Example 3 — Field of an infinite line charge

Problem: A very long straight wire carries a uniform linear charge density λ=4×106\lambda=4\times10^{-6} C/m. Find the field at 0.200.20 m from it, and again at 0.400.40 m. Take k=9×109k=9\times10^{9} SI units.

Formula: for an infinite line, E=2kλrE=\dfrac{2k\lambda}{r} — an inverse-first-power law, not an inverse square.

Working: With 2kλ=2(9×109)(4×106)=7.2×1042k\lambda=2(9\times10^{9})(4\times10^{-6})=7.2\times10^{4},

E(0.20)=7.2×1040.20=3.6×105 N/CE(0.20)=\dfrac{7.2\times10^{4}}{0.20}=3.6\times10^{5}\ \text{N/C}

E(0.40)=7.2×1040.40=1.8×105 N/CE(0.40)=\dfrac{7.2\times10^{4}}{0.40}=1.8\times10^{5}\ \text{N/C}

Answer: 3.6×1053.6\times10^{5} N/C and 1.8×1051.8\times10^{5} N/C. Doubling the distance HALVES the field rather than quartering it — the signature of a line charge as opposed to a point charge.

Example 4 — Field of an infinite sheet and the force on a charge

Problem: A large non-conducting sheet carries a uniform surface density σ=8.85×106\sigma=8.85\times10^{-6} C/m2^2. Find the field it produces and the force it exerts on a 2 μ2\ \muC charge placed near it. Take ε0=8.85×1012\varepsilon_0=8.85\times10^{-12} SI units.

Formula: for an infinite sheet, E=σ2ε0E=\dfrac{\sigma}{2\varepsilon_0}, the same at every distance; then F=qEF=qE.

Working:

E=8.85×1062(8.85×1012)=5×105 N/CE=\dfrac{8.85\times10^{-6}}{2(8.85\times10^{-12})}=5\times10^{5}\ \text{N/C}

F=qE=(2×106)(5×105)=1.0 NF=qE=(2\times10^{-6})(5\times10^{5})=1.0\ \text{N}

Answer: E=5×105E=5\times10^{5} N/C and F=1.0F=1.0 N. Because the field is uniform, the force is the same however far the charge sits from the sheet. Had this been a conducting surface, E=σε0E=\dfrac{\sigma}{\varepsilon_0} would double both answers.

Example 5 — Energy density and electrostatic pressure

Problem: (a) At a point the electric field is E=2×106E=2\times10^{6} N/C; find the energy density there and the energy stored in 11 cm3^3 around it. (b) A charged conductor has surface density σ=8.85×106\sigma=8.85\times10^{-6} C/m2^2; find the outward electrostatic pressure on its surface. Take ε0=8.85×1012\varepsilon_0=8.85\times10^{-12} SI units.

Formula: energy density u=12ε0E2u=\tfrac12\varepsilon_0 E^{2}; electrostatic pressure P=σ22ε0=12ε0Es2P=\dfrac{\sigma^{2}}{2\varepsilon_0}=\tfrac12\varepsilon_0 E_{s}^{2}, where EsE_s is the field just outside.

Working (a):

u=12(8.85×1012)(2×106)2=17.7 J/m3u=\tfrac12(8.85\times10^{-12})(2\times10^{6})^{2}=17.7\ \text{J/m}^3

In a volume of 11 cm3^3, i.e. 1×1061\times10^{-6} m3^3, the stored energy is U=uV=17.7×106U=uV=17.7\times10^{-6} J =17.7 μ=17.7\ \muJ.

Working (b): the field just outside is Es=σε0=1×106E_s=\dfrac{\sigma}{\varepsilon_0}=1\times10^{6} N/C, so

P=(8.85×106)22(8.85×1012)=4.425 N/m2P=\dfrac{(8.85\times10^{-6})^{2}}{2(8.85\times10^{-12})}=4.425\ \text{N/m}^2

Answer: (a) u=17.7u=17.7 J/m3^3 and U=17.7 μU=17.7\ \muJ; (b) P=4.425P=4.425 N/m2^2. The one expression 12ε0E2\tfrac12\varepsilon_0 E^{2} serves both as an energy per unit volume and as a force per unit area.

Example 6 — Capacitor combination and stored energy

Problem: A 4 μ4\ \muF and a 12 μ12\ \muF capacitor are joined in series, and that pair is placed in parallel with a 5 μ5\ \muF capacitor across a 5050 V supply. Find the equivalent capacitance, the total charge drawn and the total energy stored.

Formula: series Cs=C1C2C1+C2C_s=\dfrac{C_1C_2}{C_1+C_2}; parallel adds; then Q=CeqVQ=C_{eq}V and U=12CeqV2U=\tfrac12 C_{eq}V^{2}.

Working: the series pair is

Cs=4×124+12=4816=3 μFC_s=\dfrac{4\times12}{4+12}=\dfrac{48}{16}=3\ \mu\text{F}

In parallel with 5 μ5\ \muF, Ceq=3+5=8 μC_{eq}=3+5=8\ \muF. Then

Q=CeqV=(8×106)(50)=4×104 C=400 μCQ=C_{eq}V=(8\times10^{-6})(50)=4\times10^{-4}\ \text{C}=400\ \mu\text{C}

U=12CeqV2=12(8×106)(50)2=1.0×102 J=10 mJU=\tfrac12 C_{eq}V^{2}=\tfrac12(8\times10^{-6})(50)^{2}=1.0\times10^{-2}\ \text{J}=10\ \text{mJ}

Answer: Ceq=8 μC_{eq}=8\ \muF, Q=400 μQ=400\ \muC and U=10U=10 mJ. Reduce the network in stages — the series pair first, then the parallel step — and apply Q=CeqVQ=C_{eq}V only to the final single capacitance.

Example 7 — Charge sharing and the energy lost

Problem: A 2 μ2\ \muF capacitor charged to 100100 V is connected, positive plate to positive plate, across a 3 μ3\ \muF capacitor charged to 5050 V. Find the common potential and the heat dissipated.

Formula: common potential V=C1V1+C2V2C1+C2V=\dfrac{C_1V_1+C_2V_2}{C_1+C_2}; heat lost ΔU=12C1C2C1+C2(V1V2)2\Delta U=\dfrac{1}{2}\dfrac{C_1C_2}{C_1+C_2}(V_1-V_2)^{2}.

Working:

V=(2)(100)+(3)(50)2+3=3505=70 VV=\dfrac{(2)(100)+(3)(50)}{2+3}=\dfrac{350}{5}=70\ \text{V}

ΔU=12(2×106)(3×106)5×106(10050)2=12(1.2×106)(2500)=1.5×103 J\Delta U=\tfrac12\cdot\dfrac{(2\times10^{-6})(3\times10^{-6})}{5\times10^{-6}}(100-50)^{2}=\tfrac12(1.2\times10^{-6})(2500)=1.5\times10^{-3}\ \text{J}

Answer: common potential 7070 V and heat lost 1.51.5 mJ. As a check, Ui=12(2×106)(100)2+12(3×106)(50)2=13.75U_i=\tfrac12(2\times10^{-6})(100)^{2}+\tfrac12(3\times10^{-6})(50)^{2}=13.75 mJ falls to Uf=12(5×106)(70)2=12.25U_f=\tfrac12(5\times10^{-6})(70)^{2}=12.25 mJ, a drop of 1.51.5 mJ — the stored energy always falls on reconnection, never rises.