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CalibratePhysics

Chapter 1

Electric Charges and Fields

CBSE · 10 subtopics

Formula SheetEvery formula this chapter can be examined on, in one table.

Constants and units CBSE expects

  • Elementary charge e=1.6×10−19 Ce = 1.6\times10^{-19}\,\text{C} (NCERT quotes 1.602192×10−19 C1.602192\times10^{-19}\,\text{C}). Electron carries −e-e, proton +e+e.
  • Permittivity of free space ε0=8.854×10−12 C2 N−1 m−2\varepsilon_0 = 8.854\times10^{-12}\,\text{C}^2\,\text{N}^{-1}\,\text{m}^{-2}; use 8.85×10−128.85\times10^{-12} in numericals.
  • Coulomb constant k=14πε0=9×109 N m2 C−2k = \dfrac{1}{4\pi\varepsilon_0} = 9\times10^{9}\,\text{N m}^2\,\text{C}^{-2}, so 1ε0=4π×9×109 N m2 C−2\dfrac{1}{\varepsilon_0} = 4\pi\times9\times10^{9}\,\text{N m}^2\,\text{C}^{-2}.
  • 1 μC=10−6 C1\,\mu\text{C} = 10^{-6}\,\text{C}; 1 mC=10−3 C1\,\text{mC} = 10^{-3}\,\text{C}; about 6×10186\times10^{18} electrons make up a charge of −1 C-1\,\text{C}.
  • Units to quote: charge in C; electric field in N C−1\text{N C}^{-1} (same as V m−1\text{V m}^{-1}); electric flux in N m2 C−1\text{N m}^2\,\text{C}^{-1} (same as V m); dipole moment in C m.
  • Charge densities: linear λ\lambda in C m−1\text{C m}^{-1}, surface σ\sigma in C m−2\text{C m}^{-2}, volume ρ\rho in C m−3\text{C m}^{-3}.
  • Ratio of electric to gravitational force between a proton and an electron, ke2G memp≈2.4×1039\dfrac{ke^2}{G\,m_e m_p}\approx 2.4\times10^{39} — a pure number, no units.

Basic properties of electric charge

FormulaSymbols, units and conditions
q=ne,n=0, ±1, ±2, …q = ne,\qquad n = 0,\ \pm1,\ \pm2,\ \ldots
  • Quantisation of charge. qq is the charge on a body, nn an integer, ee the elementary charge. Any measured free charge must be an integral multiple of ee; fractional multiples such as 3.5e3.5e are impossible.
qtotal=q1+q2+⋯+qnq_{\text{total}} = q_1+q_2+\cdots+q_n
  • Additivity. Charges add algebraically, with their own signs — charge is a scalar.
∑qbefore=∑qafter\sum q_{\text{before}} = \sum q_{\text{after}}
  • Conservation. The total charge of an isolated system is unchanged in any process; charging by friction only transfers electrons.
qgain=−neq_{\text{gain}} = -ne
  • Charge acquired by a body that gains nn electrons; a body that loses nn electrons acquires +ne+ne.

Coulomb's law

FormulaSymbols, units and conditions
F=14πε0q1q2r2=kq1q2r2F = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_2}{r^2} = k\dfrac{q_1q_2}{r^2}
  • Magnitude of the mutual electrostatic force between two point charges q1,q2q_1, q_2 separated by rr in vacuum, directed along the line joining them.
F⃗21=14πε0q1q2r212 r^21,F⃗12=−F⃗21\vec{F}_{21} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_2}{r_{21}^{2}}\,\hat{r}_{21},\qquad \vec{F}_{12} = -\vec{F}_{21}
  • Vector form. r^21\hat{r}_{21} points from q1q_1 to q2q_2. The sign of q1q2q_1q_2 automatically gives repulsion (positive product) or attraction (negative product); the pair obeys Newton's third law.
Fmedium=14πε0Kq1q2r2=FvacuumKF_{\text{medium}} = \dfrac{1}{4\pi\varepsilon_0 K}\dfrac{q_1q_2}{r^2} = \dfrac{F_{\text{vacuum}}}{K}
  • Force in a medium of dielectric constant (relative permittivity) K=εrK = \varepsilon_r. Since K>1K>1, inserting a slab of any insulator between two charges reduces the force.
q1′=q2′=q1+q22q_1' = q_2' = \dfrac{q_1+q_2}{2}
  • Charge on each of two identical conducting spheres after they are touched and separated. Use it before applying Coulomb's law again.

Forces between multiple charges (superposition)

FormulaSymbols, units and conditions
F⃗1=F⃗12+F⃗13+⋯+F⃗1n=q14πε0∑i=2nqir1i2 r^1i\vec{F}_1 = \vec{F}_{12}+\vec{F}_{13}+\cdots+\vec{F}_{1n} = \dfrac{q_1}{4\pi\varepsilon_0}\sum_{i=2}^{n}\dfrac{q_i}{r_{1i}^{2}}\,\hat{r}_{1i}
  • Principle of superposition. The force on one charge is the vector sum of the pairwise Coulomb forces, each unaffected by the presence of the others.
Fnet=F12+F22+2F1F2cos⁡αF_{\text{net}} = \sqrt{F_1^2+F_2^2+2F_1F_2\cos\alpha}
  • Parallelogram law for combining two of those forces at angle α\alpha; for two perpendicular equal forces FF this gives 2 F\sqrt{2}\,F.

Electric field

FormulaSymbols, units and conditions
E⃗=lim⁡q0→0F⃗q0,F⃗=qE⃗\vec{E} = \lim_{q_0\to 0}\dfrac{\vec{F}}{q_0},\qquad \vec{F} = q\vec{E}
  • Definition: force per unit positive test charge. The limit keeps the test charge from disturbing the source. Force on a negative charge is opposite to E⃗\vec{E}.
E⃗=14πε0qr2 r^,E=14πε0∣q∣r2\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{r^2}\,\hat{r},\qquad E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{\lvert q\rvert}{r^2}
  • Field of a point charge qq at distance rr: radially outward for q>0q>0, radially inward for q<0q<0; spherically symmetric.
E⃗=14πε0∑i=1nqiriP2 r^iP\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\sum_{i=1}^{n}\dfrac{q_i}{r_{iP}^{2}}\,\hat{r}_{iP}
  • Field at PP due to a system of nn point charges, by superposition. riPr_{iP} is the distance from qiq_i to PP and r^iP\hat{r}_{iP} the unit vector from qiq_i to PP.
q1x2=q2(d−x)2\dfrac{q_1}{x^2} = \dfrac{q_2}{(d-x)^2}
  • Null-point condition on the line joining two like charges dd apart; xx is measured from q1q_1. For unlike charges the null point lies outside the pair, beyond the smaller charge, and the condition becomes q1(d+x)2=q2x2\dfrac{q_1}{(d+x)^2} = \dfrac{q_2}{x^2}.
E=14πε0qx(r2+x2)3/2,q=λ(2πr)E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{qx}{(r^2+x^2)^{3/2}},\qquad q = \lambda(2\pi r)
  • Field on the axis of a uniformly charged thin ring of radius rr and linear charge density λ\lambda, at axial distance xx from the centre. For x≫rx\gg r it becomes 14πε0qx2\dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{x^2} — the ring behaves as a point charge; at the centre (x=0x=0) the field is zero.
a⃗=qE⃗m,v⃗=u⃗+a⃗t\vec{a} = \dfrac{q\vec{E}}{m},\qquad \vec{v} = \vec{u}+\vec{a}t
  • Motion of a charged particle in a uniform field: constant acceleration, so the Class 11 kinematic equations apply directly.
qE=mgtan⁡θqE = mg\tan\theta
  • Equilibrium of a charged bob of weight mgmg on a string making angle θ\theta with the vertical in a horizontal field EE; hence q=(mgE)tan⁡θq = \left(\dfrac{mg}{E}\right)\tan\theta.

Electric flux

FormulaSymbols, units and conditions
Δϕ=E⃗⋅ΔS⃗=E ΔScos⁡θ,ΔS⃗=ΔS n^\Delta\phi = \vec{E}\cdot\Delta\vec{S} = E\,\Delta S\cos\theta,\qquad \Delta\vec{S} = \Delta S\,\hat{n}
  • Flux through a small plane area element. θ\theta is the angle between E⃗\vec{E} and the outward normal n^\hat{n}, not between E⃗\vec{E} and the plane of the surface.
ϕ=∮SE⃗⋅dS⃗\phi = \oint_S \vec{E}\cdot d\vec{S}
  • Total flux through a surface SS; a scalar, SI unit N m2 C−1\text{N m}^2\,\text{C}^{-1} (equivalently V m). For a closed surface n^\hat{n} is the outward normal by convention.
ϕ=0when E⃗⊥n^ (θ=90∘)\phi = 0 \quad\text{when } \vec{E}\perp\hat{n}\ (\theta = 90^\circ)
  • Curved side of a coaxial cylinder in an axial field, and the sides of a Gaussian pillbox parallel to E⃗\vec{E}, contribute nothing.

Electric dipole

FormulaSymbols, units and conditions
p⃗=q (2a) p^,p=q×2a\vec{p} = q\,(2a)\,\hat{p},\qquad p = q\times 2a
  • Dipole moment: magnitude charge times separation, direction from −q-q to +q+q. SI unit C m. Net charge of a dipole is zero.
E⃗axial=14πε02pr(r2−a2)2 p^\vec{E}_{\text{axial}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{2pr}{(r^2-a^2)^2}\,\hat{p}
  • Exact field at an axial point, distance rr from the centre, dipole length 2a2a; directed along p⃗\vec{p}.
E⃗axial=14πε02p⃗r3(r≫a)\vec{E}_{\text{axial}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{2\vec{p}}{r^3}\qquad (r\gg a)
  • Short-dipole limit on the axis.
E⃗equatorial=−14πε0p⃗(r2+a2)3/2\vec{E}_{\text{equatorial}} = -\dfrac{1}{4\pi\varepsilon_0}\dfrac{\vec{p}}{(r^2+a^2)^{3/2}}
  • Exact field at a point on the perpendicular bisector, distance rr from the centre; antiparallel to p⃗\vec{p}.
E⃗equatorial=−14πε0p⃗r3(r≫a)\vec{E}_{\text{equatorial}} = -\dfrac{1}{4\pi\varepsilon_0}\dfrac{\vec{p}}{r^3}\qquad (r\gg a)
  • Short-dipole limit on the equatorial line.
EaxialEequatorial=2(r≫a)\dfrac{E_{\text{axial}}}{E_{\text{equatorial}}} = 2 \qquad (r\gg a)
  • Standard one-mark result: at equal distances the axial field is twice the equatorial field and oppositely directed. Both fall off as 1/r31/r^3, faster than the 1/r21/r^2 of a point charge.

Dipole in a uniform external field

FormulaSymbols, units and conditions
τ⃗=p⃗×E⃗,τ=pEsin⁡θ\vec{\tau} = \vec{p}\times\vec{E},\qquad \tau = pE\sin\theta
  • Torque on a dipole making angle θ\theta with a uniform field. τ⃗\vec{\tau} is perpendicular to both p⃗\vec{p} and E⃗\vec{E}. Maximum τ=pE\tau = pE at θ=90∘\theta = 90^\circ; zero at θ=0∘\theta = 0^\circ and 180∘180^\circ.
F⃗net=qE⃗+(−q)E⃗=0(uniform field only)\vec{F}_{\text{net}} = q\vec{E}+(-q)\vec{E} = 0 \quad\text{(uniform field only)}
  • Net force vanishes in a uniform field, so the dipole only rotates. In a non-uniform field the two forces differ and there is a net force as well as a torque — translation plus rotation.
U=−p⃗⋅E⃗=−pEcos⁡θU = -\vec{p}\cdot\vec{E} = -pE\cos\theta
  • Potential energy of a dipole in a uniform field. Umin⁡=−pEU_{\min} = -pE at θ=0∘\theta = 0^\circ (stable), U=0U = 0 at θ=90∘\theta = 90^\circ, Umax⁡=+pEU_{\max} = +pE at θ=180∘\theta = 180^\circ (unstable).
pr=p12+p22+2p1p2cos⁡αp_r = \sqrt{p_1^2+p_2^2+2p_1p_2\cos\alpha}
  • Resultant moment of two dipoles inclined at angle α\alpha; for two equal dipoles pp at 120∘120^\circ, pr=pp_r = p.

Continuous charge distribution

FormulaSymbols, units and conditions
λ=ΔQΔl,σ=ΔQΔS,ρ=ΔQΔV\lambda = \dfrac{\Delta Q}{\Delta l},\qquad \sigma = \dfrac{\Delta Q}{\Delta S},\qquad \rho = \dfrac{\Delta Q}{\Delta V}
  • Linear, surface and volume charge densities. Useful conversions: charge on length ll of a wire is λl\lambda l; on area AA of a sheet is σA\sigma A; on a shell of radius RR is q=4πR2σq = 4\pi R^2\sigma.
E⃗=14πε0∑all ΔVρ ΔVr′2 r^′\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\sum_{\text{all }\Delta V}\dfrac{\rho\,\Delta V}{r'^2}\,\hat{r}'
  • Field of a continuous distribution, by superposition over volume elements; r′r' is the distance from the element to the field point.

Gauss's law

FormulaSymbols, units and conditions
ϕ=∮SE⃗⋅dS⃗=qencε0\phi = \oint_S \vec{E}\cdot d\vec{S} = \dfrac{q_{\text{enc}}}{\varepsilon_0}
  • The total electric flux through any closed surface equals 1ε0\dfrac{1}{\varepsilon_0} times the net charge enclosed. Independent of the shape and size of the surface and of where inside the charges sit; charges outside contribute to E⃗\vec{E} but not to ϕ\phi.
ϕ=qencε0εr\phi = \dfrac{q_{\text{enc}}}{\varepsilon_0\varepsilon_r}
  • Same law when the enclosed region is filled with a medium of dielectric constant εr\varepsilon_r.
ϕface=q6ε0\phi_{\text{face}} = \dfrac{q}{6\varepsilon_0}
  • Flux through one face of a cube with a point charge qq at its centre — used whenever a charge sits at distance d/2d/2 above the centre of a square of side dd.
qenc=ε0ϕq_{\text{enc}} = \varepsilon_0\phi
  • Reading a net enclosed charge off a measured flux.

Applications of Gauss's law

FormulaSymbols, units and conditions
E=λ2πε0rE = \dfrac{\lambda}{2\pi\varepsilon_0 r}
  • Infinitely long straight uniformly charged wire, at perpendicular distance rr; radially outward for λ>0\lambda>0. E∝1rE\propto\dfrac{1}{r}.
W=qλ2πε0ln⁡r1r2W = \dfrac{q\lambda}{2\pi\varepsilon_0}\ln\dfrac{r_1}{r_2}
  • Work done in taking a charge qq from perpendicular distance r2r_2 to r1r_1 from such a wire.
E⃗=σ2ε0 n^\vec{E} = \dfrac{\sigma}{2\varepsilon_0}\,\hat{n}
  • Infinite uniformly charged plane sheet; n^\hat{n} is the outward normal on either side. Independent of distance from the sheet — away from it if σ>0\sigma>0, towards it if σ<0\sigma<0.
Ebetween=σε0,Eoutside=0E_{\text{between}} = \dfrac{\sigma}{\varepsilon_0},\qquad E_{\text{outside}} = 0
  • Two large parallel sheets carrying +σ+\sigma and −σ-\sigma: the fields add between the plates and cancel outside.
Ebetween=σ1−σ22ε0,Eoutside=σ1+σ22ε0E_{\text{between}} = \dfrac{\sigma_1-\sigma_2}{2\varepsilon_0},\qquad E_{\text{outside}} = \dfrac{\sigma_1+\sigma_2}{2\varepsilon_0}
  • Two parallel sheets with like densities σ1>σ2\sigma_1>\sigma_2: region between the sheets, and the regions beyond them.
E=q4πε0r2(r≥R),E=0(r<R)E = \dfrac{q}{4\pi\varepsilon_0 r^2}\quad (r\ge R),\qquad E = 0\quad (r<R)
  • Thin uniformly charged spherical shell of radius RR and total charge q=4πR2σq = 4\pi R^2\sigma. Outside, the shell behaves exactly as a point charge qq at the centre; inside, the field is zero everywhere.
Esurface=σε0(r=R)E_{\text{surface}} = \dfrac{\sigma}{\varepsilon_0}\qquad (r = R)
  • Value at the surface of the shell — the field jumps discontinuously from 00 to σε0\dfrac{\sigma}{\varepsilon_0} there.
E=14πε0qrR3=ρr3ε0(r<R)E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{qr}{R^3} = \dfrac{\rho r}{3\varepsilon_0}\qquad (r<R)
  • Inside a solid sphere of uniform volume charge density ρ\rho; outside it the field is again q4πε0r2\dfrac{q}{4\pi\varepsilon_0 r^2}.
E(r)=Ze4πε0(1r2−rR3)(r<R),E=0(r>R)E(r) = \dfrac{Ze}{4\pi\varepsilon_0}\left(\dfrac{1}{r^2}-\dfrac{r}{R^3}\right)\quad (r<R),\qquad E = 0\quad (r>R)
  • NCERT's early atom model: point nucleus +Ze+Ze inside a uniform negative cloud of radius RR, the whole atom neutral.
Einside conductor=0E_{\text{inside conductor}} = 0
  • Electrostatic field inside the material of any conductor is zero; all excess charge resides on the outer surface — so the charge a metallic sphere holds does not depend on whether it is hollow or solid.
σinner=−q4πr12,σouter=Q+q4πr22\sigma_{\text{inner}} = \dfrac{-q}{4\pi r_1^2},\qquad \sigma_{\text{outer}} = \dfrac{Q+q}{4\pi r_2^2}
  • Hollow conducting shell of inner radius r1r_1, outer radius r2r_2, carrying its own charge QQ, with a point charge qq at the centre of the cavity: charge −q-q is induced on the inner surface and Q+qQ+q appears on the outer surface. (For −q-q at the centre, the inner surface carries +q+q and the outer Q−qQ-q.)
E=14πε0qx2 (r<x<R),E=14πε0q+Qx2 (x>R)E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{x^2}\ (r<x<R),\qquad E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q+Q}{x^2}\ (x>R)
  • Small sphere of charge qq and radius rr inside a concentric shell of radius RR carrying QQ.
Short NotesThe chapter subtopic by subtopic, in the textbook's own order.10 subtopics
  1. 1Electric Charges1 board question
  2. 2Basic Properties of Electric Charge2 board questions
  3. 3Coulomb's Law5 board questions
  4. 4Electric Field5 board questions
  5. 5Electric Field Lines6 board questions
  6. 6Electric Flux4 board questions
  7. 7Electric Dipole4 board questions
  8. 8Dipole in a Uniform External Field11 board questions
  9. 9Gauss's Law1 board question
  10. 10Applications of Gauss's Law27 board questions
The whole chapter in brief

1.1 What electrostatics is

  • Electrostatics is the study of forces, fields and potentials due to charges at rest. Static means not changing with time.
  • Frictional electricity (a comb attracting paper, a spark from a sweater) is the everyday evidence: rubbing transfers electrons and leaves the two bodies oppositely charged.

1.2 Electric charge

  • Two kinds of charge exist. Like charges repel; unlike charges attract. The property distinguishing them is called polarity.
  • By Franklin's convention, glass rubbed with silk is positive; plastic rubbed with fur (and silk rubbed by glass) is negative.
  • A charged body attracts a light neutral body as well, by inducing charge on it — so attraction alone never proves the second body is charged, but repulsion is a sure test of charge.
  • Gold-leaf electroscope: a metal rod in a box with two thin gold leaves at the bottom. Charge given to the knob spreads onto the leaves, which repel and diverge; the divergence measures the amount of charge.
  • Charging by friction transfers electrons only. A body that loses electrons becomes positive; one that gains electrons becomes negative. No new charge is created.

1.3 Conductors and insulators

  • Conductors have charges (electrons in metals, ions in electrolytes) free to move; charge given to a conductor spreads at once over its whole surface. Metals, human and animal bodies and the earth are conductors.
  • Insulators (glass, porcelain, plastic, nylon, wood) resist the flow of charge; charge put on an insulator stays where it is put. Semiconductors are an intermediate third class.
  • A plastic comb gets electrified on rubbing but a metal spoon held in the hand does not, because charge on the metal leaks away through the body to the earth. Held by an insulating handle, the metal rod does show charging.
  • Charging by induction: bringing +Q+Q near an uncharged conductor draws a negative induced charge to the near face and leaves an equal positive charge on the far face. The net charge on the conductor stays zero — charge is only redistributed.

1.4 Basic properties of electric charge

  • Point charge: a charged body whose size is negligible compared with the distances involved, so all its charge is taken to be at one point.
  • Additivity: charges add algebraically, signs included; charge is a scalar. Total of +1,+2,−3,+4,−5+1, +2, -3, +4, -5 is −1-1.
  • Conservation: the total charge of an isolated system is constant. Charged particles may be created or destroyed (a neutron decaying to a proton plus an electron), but always in pairs of equal and opposite charge.
  • Quantisation: q=neq = ne with nn an integer and e=1.6×10−19 Ce = 1.6\times10^{-19}\,\text{C}. A charge of 3.5e3.5e is impossible. First suggested by Faraday's laws of electrolysis, demonstrated by Millikan in 1912.
  • Quantisation may be ignored at the macroscopic level: a charge of 1 μC1\,\mu\text{C} is about 101310^{13} electronic charges, so the graininess is invisible. At the microscopic level, where charges are a few tens of ee, it cannot be ignored.

1.5 Coulomb's law

  • Statement: the electrostatic force between two point charges is directly proportional to the product of their magnitudes, inversely proportional to the square of the distance between them, and acts along the line joining them.
  • F=14πε0q1q2r2F = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_2}{r^2}, with 14πε0=9×109 N m2 C−2\dfrac{1}{4\pi\varepsilon_0} = 9\times10^{9}\,\text{N m}^2\,\text{C}^{-2} and ε0=8.854×10−12 C2 N−1 m−2\varepsilon_0 = 8.854\times10^{-12}\,\text{C}^2\,\text{N}^{-1}\,\text{m}^{-2}.
  • Vector form F⃗21=14πε0q1q2r212r^21\vec{F}_{21} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_2}{r_{21}^2}\hat{r}_{21} covers both attraction and repulsion in one equation, and gives F⃗12=−F⃗21\vec{F}_{12} = -\vec{F}_{21}, in agreement with Newton's third law.
  • Definition of the coulomb that follows: 1 C1\,\text{C} is that charge which, placed 1 m1\,\text{m} from an equal charge in vacuum, is repelled with a force of 9×109 N9\times10^{9}\,\text{N}. A very large unit in practice.
  • Coulomb used a torsion balance, and got equal sub-multiples of an unknown charge by touching a charged sphere to an identical uncharged one, halving the charge each time.
  • In a medium of dielectric constant KK the force falls to F/KF/K; inserting any insulating sheet between two charges reduces the force.

1.6 Forces between multiple charges

  • Principle of superposition: the force on any one charge is the vector sum of the forces exerted on it by every other charge, taken one pair at a time, each pairwise force being unaffected by the presence of the rest.
  • F⃗1=F⃗12+F⃗13+⋯+F⃗1n\vec{F}_1 = \vec{F}_{12}+\vec{F}_{13}+\cdots+\vec{F}_{1n}; add by the parallelogram law or by resolving into components.
  • Two equal perpendicular forces FF give a resultant 2 F\sqrt{2}\,F at 45∘45^\circ — the pattern behind most three-charge MCQs.

1.7 Electric field

  • Definition: the electric field at a point is the force experienced per unit positive test charge placed there, E⃗=lim⁡q0→0F⃗q0\vec{E} = \displaystyle\lim_{q_0\to0}\dfrac{\vec{F}}{q_0}. The limit is taken so the test charge does not disturb the source charge.
  • F⃗=qE⃗\vec{F} = q\vec{E}. On a positive charge the force is along E⃗\vec{E}; on a negative charge it is opposite to E⃗\vec{E}.
  • Field of a point charge: E=14πε0∣q∣r2E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{\lvert q\rvert}{r^2}, radially outward for +q+q, radially inward for −q-q, with the same magnitude at all points of a sphere centred on the charge (spherical symmetry).
  • E⃗\vec{E} is independent of the test charge, since F⃗∝q0\vec{F}\propto q_0 and the ratio does not depend on q0q_0. It is a function of position and exists at every point of space.
  • Superposition holds for fields as it does for forces: E⃗=14πε0∑iqiriP2r^iP\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\sum_i\dfrac{q_i}{r_{iP}^2}\hat{r}_{iP}.
  • SI unit N C−1\text{N C}^{-1}, alternatively V m−1\text{V m}^{-1}.

1.8 Electric field lines

  • An electric field line is a curve whose tangent at every point gives the direction of the net electric field there; an arrow fixes which of the two tangent directions is meant.
  • Magnitude is carried by the density of lines: lines crowd where the field is strong, spread out where it is weak. Only the relative density matters, since any number of lines may be drawn.
  • Because the field of a point charge falls as 1/r21/r^2 while the enclosing area grows as r2r^2, the number of lines crossing a sphere around the charge is the same at every radius — the picture is self-consistent.
  • Properties: (i) lines start on positive charges and end on negative charges, beginning or ending at infinity for a single charge; (ii) in a charge-free region they are continuous curves with no breaks; (iii) two lines can never cross; (iv) they never form closed loops.
  • No crossing, because at the crossing point the field would have two directions at once, which is absurd.
  • No closed loops, because the electrostatic field is conservative — the work done round a closed path is zero, which a closed field line would violate.
  • In a uniform field the lines are equally spaced parallel straight lines.

1.9 Electric flux

  • Electric flux through a surface is the total number of electric field lines crossing it normally: Δϕ=E⃗⋅ΔS⃗=E ΔScos⁡θ\Delta\phi = \vec{E}\cdot\Delta\vec{S} = E\,\Delta S\cos\theta, with θ\theta the angle between E⃗\vec{E} and the area vector.
  • Area is treated as a vector, ΔS⃗=ΔS n^\Delta\vec{S} = \Delta S\,\hat{n}, directed along the normal to the surface; for a closed surface the outward normal is taken, by convention.
  • Total flux ϕ=∮SE⃗⋅dS⃗\phi = \displaystyle\oint_S\vec{E}\cdot d\vec{S}. Flux is a scalar. SI unit N m2 C−1\text{N m}^2\,\text{C}^{-1} or V m.
  • ϕ\phi is maximum (ESES) when the surface is held normal to E⃗\vec{E}, and zero when the plane of the surface contains E⃗\vec{E} (θ=90∘\theta = 90^\circ).
  • A uniform field through a closed surface gives zero net flux: what enters one side leaves the other.

1.10 Electric dipole

  • An electric dipole is a pair of equal and opposite point charges +q+q and −q-q separated by a small distance 2a2a. Its total charge is zero but its field is not.
  • Dipole moment p⃗=q(2a)p^\vec{p} = q(2a)\hat{p}, magnitude 2qa2qa, directed from −q-q to +q+q along the dipole axis. Unit C m; it is a vector.
  • Axial field (short dipole): E⃗=14πε02p⃗r3\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{2\vec{p}}{r^3}, along p⃗\vec{p}.
  • Equatorial field (short dipole): E⃗=−14πε0p⃗r3\vec{E} = -\dfrac{1}{4\pi\varepsilon_0}\dfrac{\vec{p}}{r^3}, opposite to p⃗\vec{p}.
  • The dipole field falls off as 1/r31/r^3, faster than the 1/r21/r^2 of a point charge, because the two fields nearly cancel at large distance. It depends on qq and aa only through the product qaqa.
  • The field of a dipole depends on the angle between r⃗\vec{r} and p⃗\vec{p} as well as on rr — it is not spherically symmetric.

1.11 Dipole in a uniform external field

  • In a uniform field the two forces qE⃗q\vec{E} and −qE⃗-q\vec{E} are equal, opposite and non-collinear: net force zero, but they form a couple.
  • Torque τ=qE×2asin⁡θ=pEsin⁡θ\tau = qE\times 2a\sin\theta = pE\sin\theta, i.e. τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E}, directed perpendicular to the plane containing p⃗\vec{p} and E⃗\vec{E}. It tends to align p⃗\vec{p} along E⃗\vec{E}.
  • τ=0\tau = 0 at θ=0∘\theta = 0^\circ and θ=180∘\theta = 180^\circ; τ\tau is maximum, pEpE, at θ=90∘\theta = 90^\circ.
  • Potential energy U=−p⃗⋅E⃗=−pEcos⁡θU = -\vec{p}\cdot\vec{E} = -pE\cos\theta; in stable equilibrium (θ=0∘\theta=0^\circ) U=−pEU = -pE, in unstable equilibrium (θ=180∘\theta=180^\circ) U=+pEU = +pE.
  • In a non-uniform field the forces on the two charges differ in magnitude, so there is a net force as well as a torque: the dipole both translates and rotates. If p⃗\vec{p} is parallel to E⃗\vec{E} the net force is towards increasing field; if antiparallel, towards decreasing field.
  • This is why a charged comb attracts a neutral scrap of paper: the comb polarises the paper (induces a dipole moment along its own field) and its field is non-uniform, so the induced dipole is pulled towards the comb.

1.12 Continuous charge distribution

  • Where charges are too many to list, use smoothed-out densities: λ=ΔQΔl\lambda = \dfrac{\Delta Q}{\Delta l} (C m−1\text{C m}^{-1}), σ=ΔQΔS\sigma = \dfrac{\Delta Q}{\Delta S} (C m−2\text{C m}^{-2}), ρ=ΔQΔV\rho = \dfrac{\Delta Q}{\Delta V} (C m−3\text{C m}^{-3}).
  • The elements Δl\Delta l, ΔS\Delta S, ΔV\Delta V are small on the macroscopic scale but contain very many charges, so quantisation and microscopic discontinuity are averaged away.
  • The field is then found by superposing the fields of the elements: E⃗=14πε0∑ρ ΔVr′2r^′\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\displaystyle\sum\dfrac{\rho\,\Delta V}{r'^2}\hat{r}', becoming an integral in the limit.

1.13 Gauss's law

  • Statement: the total electric flux through any closed surface is 1ε0\dfrac{1}{\varepsilon_0} times the net charge enclosed by it — ∮SE⃗⋅dS⃗=qencε0\displaystyle\oint_S\vec{E}\cdot d\vec{S} = \dfrac{q_{\text{enc}}}{\varepsilon_0}.
  • It holds for any closed surface, of any shape or size, and for any field, uniform or not.
  • E⃗\vec{E} in the integral is the field of all charges, inside and outside; but only the charge inside appears on the right.
  • Zero net flux means zero net enclosed charge (a dipole inside a box gives zero flux), not necessarily zero field.
  • The chosen closed surface is called the Gaussian surface. It may be imaginary, but it must not pass through a discrete point charge, where the field is undefined.
  • Gauss's law follows from Coulomb's inverse-square law: for a sphere of radius rr around a point charge, ϕ=q4πε0r2×4πr2=qε0\phi = \dfrac{q}{4\pi\varepsilon_0 r^2}\times 4\pi r^2 = \dfrac{q}{\varepsilon_0}, independent of rr.

1.14 Applications of Gauss's law

  • Infinite straight wire, linear density λ\lambda: coaxial cylindrical Gaussian surface; E=λ2πε0rE = \dfrac{\lambda}{2\pi\varepsilon_0 r}, radial, E∝1rE\propto\dfrac{1}{r}.
  • Infinite plane sheet, surface density σ\sigma: pillbox Gaussian surface through the sheet; E=σ2ε0E = \dfrac{\sigma}{2\varepsilon_0}, normal to the sheet and independent of distance from it.
  • Thin spherical shell, radius RR, total charge qq: concentric spherical Gaussian surface; E=q4πε0r2E = \dfrac{q}{4\pi\varepsilon_0 r^2} for r≥Rr\ge R, and E=0E = 0 for r<Rr<R. Outside, the shell acts as a point charge at its centre.
  • Solid sphere of uniform volume charge density: outside, the same as a point charge; inside, E=ρr3ε0E = \dfrac{\rho r}{3\varepsilon_0}, rising linearly with rr.
  • Conductors: the field inside the material of a conductor is zero, so all excess charge sits on its outer surface, and a hollow conductor shields its interior (Faraday cage — a car body is the everyday example).
  • Cavity with a charge: qq at the centre of a cavity in a conductor induces −q-q on the inner surface and leaves qq (plus any charge already on the conductor) on the outer surface.

Comparisons CBSE asks for

Point of comparisonCoulomb (electrostatic) forceGravitational force
Depends onproduct of chargesproduct of masses
Signattractive or repulsivealways attractive
Mediumreduced by factor KKunaffected by medium
Relative strengthabout 2.4×10392.4\times10^{39} times stronger for a proton-electron pairfar weaker
Point of comparisonAxial pointEquatorial point
Exact field14πε02pr(r2−a2)2\dfrac{1}{4\pi\varepsilon_0}\dfrac{2pr}{(r^2-a^2)^2}14πε0p(r2+a2)3/2\dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}}
Short dipole14πε02pr3\dfrac{1}{4\pi\varepsilon_0}\dfrac{2p}{r^3}14πε0pr3\dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^3}
Directionalong p⃗\vec{p}antiparallel to p⃗\vec{p}
Ratio at equal rr2211
OrientationStable equilibriumUnstable equilibrium
Angle θ\theta between p⃗\vec{p} and E⃗\vec{E}0∘0^\circ, p⃗\vec{p} parallel to E⃗\vec{E}180∘180^\circ, p⃗\vec{p} antiparallel to E⃗\vec{E}
Torquezerozero
Potential energy−pE-pE, minimum+pE+pE, maximum
On small displacementrestoring torque returns ittorque turns it further away
DistributionFieldDependence on distance
Point chargeq4πε0r2\dfrac{q}{4\pi\varepsilon_0 r^2}E∝1r2E\propto\dfrac{1}{r^2}
Short dipole2p4πε0r3\dfrac{2p}{4\pi\varepsilon_0 r^3} on axisE∝1r3E\propto\dfrac{1}{r^3}
Infinite line chargeλ2πε0r\dfrac{\lambda}{2\pi\varepsilon_0 r}E∝1rE\propto\dfrac{1}{r}
Infinite plane sheetσ2ε0\dfrac{\sigma}{2\varepsilon_0}independent of distance
Spherical shell, outsideq4πε0r2\dfrac{q}{4\pi\varepsilon_0 r^2}E∝1r2E\propto\dfrac{1}{r^2}
Spherical shell, inside00zero everywhere
BehaviourUniform fieldNon-uniform field
Net force on dipolezeronon-zero
Torque on dipolepEsin⁡θpE\sin\thetagenerally non-zero
Resulting motionrotation onlytranslation and rotation

Graphs to be able to draw

  • Field of an infinite line charge: EE against rr is a rectangular hyperbola, E∝1/rE\propto1/r, falling steeply and tending to zero.
  • Field of a spherical shell: E=0E = 0 from the centre out to r=Rr = R, then a vertical jump to σε0\dfrac{\sigma}{\varepsilon_0} at r=Rr = R, then a 1/r21/r^2 decay for r>Rr>R.
  • Field of a uniformly charged solid sphere: a straight line rising from the origin, E∝rE\propto r, up to r=Rr = R, then a 1/r21/r^2 decay.
  • Field of a short dipole: EE against rr falls as 1/r31/r^3 — steeper than the point-charge curve drawn on the same axes.
  • Field of an infinite plane sheet: a horizontal line, EE constant on both sides.

Standard diagrams described in words

  • Field lines of a single +q+q: straight lines radiating outward in all directions; for −q-q, the same lines directed inward.
  • Two equal positive charges: lines curve away from each other, with a neutral point midway on the line joining them where no line passes.
  • Dipole (+q+q and −q-q): lines leave +q+q, curve round and terminate on −q-q, densest along the axis between the charges; the equatorial plane carries lines running from the +q+q side to the −q-q side.
  • Point charge +q+q near an uncharged conducting plate: lines radiate from +q+q and bend so as to strike the near face of the plate at right angles, that face carrying an induced negative charge. For −q-q the lines run in the reverse sense, into the charge, leaving induced positive charge on the near face. Field lines always meet a conductor's surface normally.
  • Gaussian surface for a line charge: a cylinder of radius rr and length ll drawn coaxially with the wire — flux only through the curved side, area 2πrl2\pi rl.
  • Gaussian surface for a plane sheet: a cylinder or box pierced through the sheet, with its two flat faces of area AA parallel to the sheet, one on each side — flux EAEA through each face, none through the curved side.
  • Gaussian surface for a shell: a sphere concentric with the shell, of radius rr greater than RR for the outside field and less than RR for the inside field.

Traps that cost marks

  • The angle in ϕ=EScos⁡θ\phi = ES\cos\theta is between E⃗\vec{E} and the normal to the surface. If the question gives the angle the plane makes with the field, use 90∘90^\circ minus that angle. A plane at 30∘30^\circ to E⃗\vec{E} means θ=60∘\theta = 60^\circ.
  • Flux is a scalar. Never quote a direction for it, only a sign.
  • Only enclosed charge counts in Gauss's law; a charge just outside the surface contributes nothing to the flux even though it does contribute to E⃗\vec{E} on the surface.
  • Increasing the size of a Gaussian surface leaves the flux unchanged, provided the enclosed charge is unchanged.
  • Zero flux means zero net enclosed charge — it does not mean the field inside is zero.
  • p⃗\vec{p} points from −q-q to +q+q, the opposite sense to the field between the charges. Marking it the other way loses the direction mark.
  • Use the exact dipole formulas unless the question says short dipole or r≫ar\gg a; state the approximation explicitly when you drop a2a^2.
  • The equatorial field is antiparallel to p⃗\vec{p}. Writing it along p⃗\vec{p} loses a mark even if the magnitude is right.
  • A dipole in a uniform field has zero net force. Writing "force =pE= pE" is a standard error.
  • After two identical conductors touch, each carries q1+q22\dfrac{q_1+q_2}{2} — with signs. −Q-Q and +3Q+3Q become +Q+Q each, and the force becomes repulsive.
  • Charge is quantised: any option offering 3.5e3.5e is impossible, however well the total adds up.
  • E=σ2ε0E = \dfrac{\sigma}{2\varepsilon_0} for a single sheet but σε0\dfrac{\sigma}{\varepsilon_0} between two oppositely charged sheets. Keep the factor of two straight.
  • For several sheets, add the contributions as signed vectors: each positive sheet pushes away from itself on both sides, each negative sheet pulls towards itself on both sides.
  • Inside a conductor E=0E = 0, but inside a cavity that contains a charge the field is not zero.
  • Attraction does not prove a body is charged — a neutral body is attracted by induction. Only repulsion is a sure test.
  • Field lines never cross and never close on themselves; they must also be drawn perpendicular to any conducting surface.
  • Convert centimetres to metres before substituting: an area of 10 cm×10 cm10\,\text{cm}\times10\,\text{cm} is 10−2 m210^{-2}\,\text{m}^2, not 100100.
Solved Numerical ExamplesWorked numericals to attempt first, each with a hint before the full solution.Coming soon

These are being added chapter by chapter. They are solved numericals from the prescribed book and the reference guides — not previous board questions, which live under Practice — so that you can work through the method before meeting it in a real paper.

Important DerivationsEvery derive / obtain / prove question in this chapter.19
  1. 1
    Derivation 1
    A thin circular ring of radius rr is charged uniformly so that its linear charge density becomes λ\lambda. Derive an expression for the electric field at a point PP at a distance xx from it along the axis of the ring. Hence, prove that at large distances (x≫r)(x \gg r), the ring behaves as a point charge.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, 2020, Ev · Section E, 5 marks

    Show the derivation

    Consider an elementary charge dq=λ dldq = \lambda\,dl on the ring, where dldl is an elementary length. The distance from this element to the axial point PP is r2+x2\sqrt{r^2+x^2}. The field due to dqdq at PP is dE=dq4πε0(r2+x2)dE = \dfrac{dq}{4\pi\varepsilon_0(r^2+x^2)}, resolved into dExdE_x (along the axis) and dEydE_y (perpendicular to it). By symmetry, the perpendicular components cancel around the ring and only the axial components add: dEx=dEcos⁡θ=λ x dl4πε0(r2+x2)3/2dE_x = dE\cos\theta = \dfrac{\lambda\,x\,dl}{4\pi\varepsilon_0(r^2+x^2)^{3/2}} ∴ Ex=∫dEcos⁡θ=∫λ x dl4πε0(r2+x2)3/2=14πε0xλl(r2+x2)3/2\therefore\ E_x = \displaystyle\int dE\cos\theta = \int\dfrac{\lambda\,x\,dl}{4\pi\varepsilon_0(r^2+x^2)^{3/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{x\lambda l}{(r^2+x^2)^{3/2}} where l=2πrl = 2\pi r is the circumference (total charge q=λlq=\lambda l), so E=14πε0xq(r2+x2)3/2E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{xq}{(r^2+x^2)^{3/2}} When x≫rx \gg r: (r2+x2)3/2≈x3(r^2+x^2)^{3/2} \approx x^3, so E=14πε0xqx3=14πε0qx2E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{xq}{x^3} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{x^2} which is exactly the field of a point charge qq at distance xx — hence at large distances, the ring behaves as a point charge.

  2. 2
    Derivation 2
    Consider a system of nn charges q1,q2,…,qnq_1, q_2, \ldots, q_n with position vectors r⃗1,r⃗2,r⃗3,…,r⃗n\vec{r}_1, \vec{r}_2, \vec{r}_3, \ldots, \vec{r}_n relative to some origin OO. Deduce the expression for the net electric field E⃗\vec{E} at a point PP with position vector r⃗P\vec{r}_P due to this system of charges.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, Foreign 2015 · Section E, 5 marks

    Show the derivation

    According to Coulomb's law, the force on a test charge q0q_0 placed at PP due to charge q1q_1 is F⃗1=14πε0q1q0r1P2r^1P\vec{F}_1 = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_0}{r_{1P}^2}\hat{r}_{1P} where r^1P\hat{r}_{1P} is the unit vector from q1q_1 to PP and r1Pr_{1P} is the distance between them. The electric field at PP due to q1q_1 is E⃗1=F⃗1q0=14πε0q1r1P2r^1P\vec{E}_1 = \dfrac{\vec{F}_1}{q_0} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1}{r_{1P}^2}\hat{r}_{1P} Similarly, the field due to q2q_2 is E⃗2=14πε0q2r2P2r^2P\vec{E}_2 = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_2}{r_{2P}^2}\hat{r}_{2P}, and so on. By the principle of superposition, the net field at PP is E⃗=E⃗1+E⃗2+…+E⃗n=14πε0∑i=1nqiriP2r^iP\vec{E} = \vec{E}_1+\vec{E}_2+\ldots+\vec{E}_n = \dfrac{1}{4\pi\varepsilon_0}\displaystyle\sum_{i=1}^{n}\dfrac{q_i}{r_{iP}^2}\hat{r}_{iP}

  3. 3
    Derivation 3
    Obtain the expression for the electric field at a point on the equatorial line of an electric dipole.

    Asked in: CBSE Class 12 Physics — SA · 2019C · Section B, 2 marks

    Show the derivation

    The strength of an electric dipole is measured by its dipole moment, p⃗=q(2a)\vec{p} = q(2a), directed from the negative to the positive charge along the line joining them (2a2a = separation). Consider a point PP on the perpendicular bisector (equatorial line), at distance rr from the centre. The fields EPAE_{PA} (due to −q-q) and EPBE_{PB} (due to +q+q) are equal in magnitude (EPA=EPB=14πε0qr2+a2E_{PA}=E_{PB}=\dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{r^2+a^2}); their components perpendicular to p⃗\vec{p} cancel, and the components along −p⃗-\vec{p} add: Enet=2EPAcos⁡θE_{net} = 2E_{PA}\cos\theta, where cos⁡θ=a(r2+a2)1/2\cos\theta = \dfrac{a}{(r^2+a^2)^{1/2}} Enet=14πε0q⋅2a(r2+a2)3/2=14πε0p(r2+a2)3/2E_{net} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q\cdot2a}{(r^2+a^2)^{3/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}} directed antiparallel to p⃗\vec{p}. For a short dipole (r≫ar \gg a): E=14πε0pr3E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^3}, or in vector form, E⃗=14πε0−p⃗r3\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{-\vec{p}}{r^3}

  4. 4
    Derivation 4
    Derive an expression for the electric field due to a dipole of dipole moment p⃗\vec{p} at a point on its perpendicular bisector (equatorial line).

    Asked in: CBSE Class 12 Physics — SA · 2/3, Delhi 2019, 2017 · Section C, 3 marks

    Show the derivation

    (Same derivation as Q26.) Electric field on the equatorial line at any point on the perpendicular bisector of the dipole, at distance rr from its centre: Enet=EPAcos⁡θ+EPBcos⁡θ=2EPAcos⁡θE_{net} = E_{PA}\cos\theta+E_{PB}\cos\theta = 2E_{PA}\cos\theta (EPA=EPBE_{PA}=E_{PB}, vertical components cancel) Enet=14πε0q⋅2a(r2+a2)3/2=14πε0p(r2+a2)3/2E_{net} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q\cdot2a}{(r^2+a^2)^{3/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}} directed antiparallel to p⃗\vec{p}. For a short dipole (r≫a)(r \gg a): E=14πε0pr3E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^3}

  5. 5
    Derivation 5
    (a) Derive an expression for the electric field EE due to a dipole of length '2a2a' at a point distant rr from the centre of the dipole on the axial line. (b) Draw a graph of EE versus rr for r≫ar \gg a.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, AI 2017, An · Section E, 5 marks

    Show the derivation

    (a) Consider a dipole with charges +q+q (at distance r−ar-a) and −q-q (at distance r+ar+a) from an axial point PP, with dipole moment p⃗\vec{p} pointing from −q-q to +q+q. Field due to −q-q at PP: E⃗−q=−q4πε0(r+a)2p^\vec{E}_{-q} = \dfrac{-q}{4\pi\varepsilon_0(r+a)^2}\hat{p} (towards −q-q, i.e. left) Field due to +q+q at PP: E⃗+q=q4πε0(r−a)2p^\vec{E}_{+q} = \dfrac{q}{4\pi\varepsilon_0(r-a)^2}\hat{p} (towards right) Resultant field: E⃗axial=E⃗+q+E⃗−q=q4πε0[1(r−a)2−1(r+a)2]p^\vec{E}_{axial} = \vec{E}_{+q}+\vec{E}_{-q} = \dfrac{q}{4\pi\varepsilon_0}\left[\dfrac{1}{(r-a)^2}-\dfrac{1}{(r+a)^2}\right]\hat{p} =q4πε0⋅4ar(r2−a2)2p^=14πε0⋅2pr(r2−a2)2p^= \dfrac{q}{4\pi\varepsilon_0}\cdot\dfrac{4ar}{(r^2-a^2)^2}\hat{p} = \dfrac{1}{4\pi\varepsilon_0}\cdot\dfrac{2pr}{(r^2-a^2)^2}\hat{p} (using p=q⋅2ap=q\cdot2a) For r≫ar \gg a, a2a^2 can be neglected compared to r2r^2: E⃗axial=14πε0⋅2p⃗r3\vec{E}_{axial} = \dfrac{1}{4\pi\varepsilon_0}\cdot\dfrac{2\vec{p}}{r^3} (directed along +p^+\hat{p}) (b) EE falls off as 1/r31/r^3: a steep monotonically decreasing curve of EE against rr, approaching zero as rr increases.

  6. 6
    Derivation 6
    An electric dipole of dipole moment p⃗\vec{p} consists of point charges +q+q and −q-q separated by a distance 2a2a apart. Deduce the expression for the electric field E⃗\vec{E} due to the dipole at a distance xx from the centre of the dipole on its axial line, in terms of the dipole moment p⃗\vec{p}. Hence show that in the limit x≫ax \gg a, E⃗→2p⃗/(4πε0x3)\vec{E} \to 2\vec{p}/(4\pi\varepsilon_0 x^3).

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, Delhi 2015, Ev · Section E, 5 marks

    Show the derivation

    (Same derivation as Q28, with rr replaced by xx.) Field at an axial point at distance xx from the centre: E⃗axial=q4πε0[1(x−a)2−1(x+a)2]p^=14πε0⋅2px(x2−a2)2p^\vec{E}_{axial} = \dfrac{q}{4\pi\varepsilon_0}\left[\dfrac{1}{(x-a)^2}-\dfrac{1}{(x+a)^2}\right]\hat{p} = \dfrac{1}{4\pi\varepsilon_0}\cdot\dfrac{2px}{(x^2-a^2)^2}\hat{p} For x≫ax \gg a, a2a^2 is negligible compared to x2x^2: E⃗→14πε0⋅2p⃗x3\vec{E} \to \dfrac{1}{4\pi\varepsilon_0}\cdot\dfrac{2\vec{p}}{x^3} — as required.

  7. 7
    Derivation 7
    Derive the expression for the torque acting on an electric dipole, when it is held in a uniform electric field. Identify the orientation of the dipole in the electric field, in which it attains a stable equilibrium.

    Asked in: CBSE Class 12 Physics — SA · 2020 · Section B, 2 marks

    Show the derivation

    When an electric dipole (+q+q at AA, −q-q at BB, separation 2a2a) is placed in a uniform field E⃗\vec{E} making angle θ\theta with p⃗\vec{p}, the two charges experience equal and opposite forces qEqE, which cancel — so the net force is zero. However, these forces are not collinear, so they constitute a couple. Torque == magnitude of either force ×\times perpendicular distance between the lines of action =qE×(2asin⁡θ)=(q⋅2a)Esin⁡θ= qE\times(2a\sin\theta) = (q\cdot2a)E\sin\theta ∴ τ=pEsin⁡θ\therefore\ \tau = pE\sin\theta, or in vector form, τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E} Stable equilibrium: when θ=0°\theta = 0° (i.e., p⃗\vec{p} parallel to E⃗\vec{E}), τ=0\tau = 0 and any small angular displacement produces a restoring torque bringing the dipole back — this is the position of stable equilibrium.

  8. 8
    Derivation 8
    (a) Obtain the expression for the torque τ⃗\vec{\tau} experienced by an electric dipole of dipole moment p⃗\vec{p} in a uniform electric field E⃗\vec{E}. (b) What will happen if the field were not uniform?

    Asked in: CBSE Class 12 Physics — Long Answer · Delhi 2017 · Section E, 5 marks

    Show the derivation

    (a) (Same derivation as Q33.) When a dipole is placed in a uniform field, the two equal and opposite forces qEqE on its charges cancel (net force zero), but being non-collinear they produce a torque: τ=Fr⊥=qE⋅2asin⁡θ=(q⋅2a)Esin⁡θ\tau = Fr_\perp = qE\cdot2a\sin\theta = (q\cdot2a)E\sin\theta, i.e., τ=pEsin⁡θ\tau = pE\sin\theta, or τ⃗=p⃗×E⃗\vec{\tau}=\vec{p}\times\vec{E} — this torque tends to align the dipole along the field direction. (b) If the field is not uniform, the forces on the two charges no longer cancel exactly, so the dipole experiences a net force in addition to the torque, and undergoes both translational and rotational motion.

  9. 9
    Derivation 9
    An electric dipole of dipole moment p⃗\vec{p} is placed in a uniform electric field E⃗\vec{E}. Obtain the expression for the torque τ⃗\vec{\tau} experienced by the dipole. Identify two pairs of perpendicular vectors in the expression.

    Asked in: CBSE Class 12 Physics — Long Answer · Delhi 2015C, Cr · Section E, 5 marks

    Show the derivation

    (Same derivation as Q33/36.) τ=pEsin⁡θ\tau = pE\sin\theta, or in vector form, τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E}. Since τ⃗\vec{\tau} is the cross product of p⃗\vec{p} and E⃗\vec{E}, it is perpendicular to both. The two pairs of perpendicular vectors are: (i) (τ⃗,p⃗)(\vec{\tau},\vec{p}) and (ii) (τ⃗,E⃗)(\vec{\tau},\vec{E}).

  10. 10
    Derivation 10
    (a) Define electric flux. Is it a scalar or a vector quantity? A point charge qq is at a distance of d/2d/2 directly above the centre of a square of side dd. Use Gauss's law to obtain the expression for the electric flux through the square. (b) If the point charge is now moved to a distance 'dd' from the centre of the square and the side of the square is doubled, explain how the electric flux will be affected.

    Asked in: CBSE Class 12 Physics — Long Answer · 2018, An · Section E, 5 marks

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    (a) Electric flux linked with a surface is the number of electric lines of force cutting through it normally; it is a scalar quantity: ϕ=∫SE⃗⋅dS⃗\phi = \displaystyle\int_S\vec{E}\cdot d\vec{S}. Imagine the given square as one face of a cube of edge dd. Since the charge qq is at distance d/2d/2 directly above the centre of the square, it lies at the centre of this imaginary cube, so by Gauss's theorem, the electric flux linked with the whole cube is ϕ=qε0\phi = \dfrac{q}{\varepsilon_0}. By symmetry, this flux is divided equally among the cube's 6 faces, so the flux through the given square is ϕsq=ϕ6=q6ε0\phi_{sq} = \dfrac{\phi}{6} = \dfrac{q}{6\varepsilon_0}. (b) Now the distance of the charge from the plane doubles (dd) and the side of the square also doubles (2d2d), so the same symmetry holds with a cube of side 2d2d — the charge again sits at the centre of an (enlarged) imaginary cube. Hence the flux through the square is unaffected: ϕsq=q6ε0\phi_{sq} = \dfrac{q}{6\varepsilon_0}, unchanged.

  11. 11
    Derivation 11
    Consider two hollow concentric spheres, S1S_1 and S2S_2, enclosing charges 2Q2Q and 4Q4Q respectively as shown in the figure. (i) Find the ratio of the electric flux through them. (ii) How will the electric flux through the sphere S1S_1 change if a medium of dielectric constant 'εr\varepsilon_r' is introduced in the space inside S1S_1 in place of air? Deduce the necessary expression.

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2014, Ap · Section E, 5 marks

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    (i) Charge enclosed by S1S_1 is 2Q2Q, so flux ϕ1=2Qε0\phi_1 = \dfrac{2Q}{\varepsilon_0}. Charge enclosed by S2S_2 is 2Q+4Q=6Q2Q+4Q=6Q, so flux ϕ2=6Qε0\phi_2 = \dfrac{6Q}{\varepsilon_0}. Ratio, ϕ1:ϕ2=2:6=1:3\phi_1:\phi_2 = 2:6 = 1:3 (ii) When a medium of dielectric constant εr\varepsilon_r is introduced inside S1S_1, the flux through S1S_1 becomes ϕ1′=2Qε0εr\phi_1' = \dfrac{2Q}{\varepsilon_0\varepsilon_r}.

  12. 12
    Derivation 12
    Apply Gauss's law to show that for a charged spherical shell, the electric field outside the shell is as if the entire charge were concentrated at the centre.

    Asked in: CBSE Class 12 Physics — SA · AI 2019, R · Section B, 2 marks

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    Consider a spherical Gaussian surface of radius rr (r>Rr>R, the shell's radius), concentric with the shell. By symmetry, E⃗\vec{E} is radial and has the same magnitude at every point of this surface. Using Gauss's theorem at point PP on this surface: ∮E⃗⋅ds⃗=Qε0\displaystyle\oint\vec{E}\cdot d\vec{s} = \dfrac{Q}{\varepsilon_0} ∫E 4πr2cos⁡0°=Qε0\displaystyle\int E\,4\pi r^2\cos0° = \dfrac{Q}{\varepsilon_0} (EE is constant over the surface) E=Q4πε0r2E = \dfrac{Q}{4\pi\varepsilon_0 r^2} This is exactly the field of a point charge QQ placed at the centre — hence the field outside a uniformly charged spherical shell is as if the entire charge were concentrated at its centre.

  13. 13
    Derivation 13
    (a) An infinitely long thin straight wire has a uniform linear charge density λ\lambda. Obtain the expression for the electric field (E)(E) at a point lying at a distance xx from the wire, using Gauss' law. (b) Show graphically the variation of this electric field EE as a function of distance xx from the wire.

    Asked in: CBSE Class 12 Physics — Long Answer · 2020 · Section E, 5 marks

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    (a) Consider a cylindrical Gaussian surface SS of radius xx and length ll, coaxial with the charged wire. The flux through the two flat circular ends is zero (field is perpendicular to their normal), and through the curved surface: ϕ=∮E⃗⋅dS⃗=∫E dScos⁡90°+∫E dScos⁡0°+∫E dScos⁡90°=E⋅2πxl\phi = \displaystyle\oint\vec{E}\cdot d\vec{S} = \int E\,dS\cos90°+\int E\,dS\cos0°+\int E\,dS\cos90° = E\cdot2\pi xl By Gauss's theorem, ϕ=qε0=λlε0\phi = \dfrac{q}{\varepsilon_0} = \dfrac{\lambda l}{\varepsilon_0} (charge enclosed on length ll is λl\lambda l). ∴ E×2πxl=λlε0 ⇒ E=λ2πε0x\therefore\ E\times2\pi xl = \dfrac{\lambda l}{\varepsilon_0} \ \Rightarrow\ E = \dfrac{\lambda}{2\pi\varepsilon_0 x}, directed radially outward from the wire. (b) Since E∝1xE \propto \dfrac{1}{x}, the graph of EE vs xx is a rectangular-hyperbola-like curve, steeply decreasing and approaching zero as xx increases.

  14. 14
    Derivation 14
    A hollow conducting sphere of inner radius r1r_1 and outer radius r2r_2 has a charge QQ on its surface. A point charge −q-q is also placed at the centre of the sphere. (a) What is the surface charge density on the (i) inner and (ii) outer surface of the sphere? (b) Use Gauss' law of electrostatics to obtain the expression for the electric field at a point lying outside the sphere.

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2020 · Section E, 5 marks

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    (a) By induction, charge +q+q is induced on the inner surface (to neutralise the field inside the conductor due to −q-q at the centre), so the inner surface charge is +q+q: σinner=q4πr12\sigma_{inner} = \dfrac{q}{4\pi r_1^2} Charge conservation: total charge on the conductor is QQ, so the outer surface carries (Q−q)(Q-q): σouter=Q−q4πr22\sigma_{outer} = \dfrac{Q-q}{4\pi r_2^2} (b) For a point outside the sphere at distance x>r2x>r_2, using a spherical Gaussian surface, the total charge enclosed is (Q−q)+q−q=Q−q(Q-q)+q-q = Q-q... more directly, the net charge enclosed is (−q)+Q=Q−q(-q)+Q = Q-q: ∮E⃗⋅dS⃗=Q−qε0 ⇒ E×4πx2=Q−qε0\displaystyle\oint\vec{E}\cdot d\vec{S} = \dfrac{Q-q}{\varepsilon_0} \ \Rightarrow\ E\times4\pi x^2 = \dfrac{Q-q}{\varepsilon_0} E=14πε0Q−qx2E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q-q}{x^2}

  15. 15
    Derivation 15
    State Gauss's law on electrostatics and derive an expression for the electric field due to a long straight thin uniformly charged wire (linear charge density λ\lambda) at a point lying at a distance rr from the wire.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, 2020 · Section E, 5 marks

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    Gauss's law: the total flux over a closed surface SS in vacuum is 1ε0\dfrac{1}{\varepsilon_0} times the total charge enclosed by that surface: ϕ=∮SE⃗⋅dS⃗=qenclosedε0\phi = \displaystyle\oint_S\vec{E}\cdot d\vec{S} = \dfrac{q_{enclosed}}{\varepsilon_0} (Derivation, same as Q57(a).) Using a coaxial cylindrical Gaussian surface of radius rr and length ll: flux through the flat ends is zero, and through the curved surface ϕ=E×2πrl\phi = E\times2\pi rl. By Gauss's theorem, ϕ=λlε0\phi = \dfrac{\lambda l}{\varepsilon_0}, so E×2πrl=λlε0 ⇒ E=λ2πε0rE\times2\pi rl = \dfrac{\lambda l}{\varepsilon_0} \ \Rightarrow\ E = \dfrac{\lambda}{2\pi\varepsilon_0 r}, directed radially outward (for λ>0\lambda>0).

  16. 16
    Derivation 16
    Using Gauss law, derive an expression for electric field due to a spherical shell of uniform charge distribution σ\sigma and radius RR at a point lying at a distance xx from the centre of the shell, such that (i) 0<x<R0<x<R, and (ii) x>Rx>R. OR Use Gauss's law to show that due to a uniformly charged spherical shell of radius RR, the electric field at any point situated outside the shell at a distance rr from its centre is equal to the electric field at the same point when the entire charge on the shell were concentrated at its centre. Also plot the graph showing the variation of electric field with rr, for r≤Rr\le R and r≥Rr\ge R.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, 2020 · Section E, 5 marks

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    (i) For a point inside the shell (x<Rx<R), a spherical Gaussian surface of radius xx encloses no charge (all the charge q=σ×4πR2q=\sigma\times4\pi R^2 resides on the shell of radius R>xR>x). By Gauss's law, E×4πx2=0 ⇒ E=0E\times4\pi x^2 = 0 \ \Rightarrow\ E=0. (ii) For a point outside the shell (x>Rx>R), take a concentric spherical Gaussian surface of radius xx. By symmetry E⃗\vec{E} is radial and uniform over this surface: ∮E⃗⋅dS⃗=E×4πx2\displaystyle\oint\vec{E}\cdot d\vec{S} = E\times4\pi x^2 Charge enclosed =σ×4πR2=q= \sigma\times4\pi R^2 = q (total charge on shell), so by Gauss's law: E×4πx2=σ×4πR2ε0=qε0E\times4\pi x^2 = \dfrac{\sigma\times4\pi R^2}{\varepsilon_0} = \dfrac{q}{\varepsilon_0} E=q4πε0x2E = \dfrac{q}{4\pi\varepsilon_0 x^2}, or vectorially, E⃗=14πε0qx2r^\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{x^2}\hat{r} — identical to the field of the entire charge qq concentrated at the centre, confirming the required result. The graph of EE vs rr is zero for r<Rr<R, and falls off as E∝1/r2E\propto1/r^2 for r>Rr>R (with a discontinuous jump to σ/ε0\sigma/\varepsilon_0 exactly at r=Rr=R).

  17. 17
    Derivation 17
    (a) Use Gauss' law to derive the expression for the electric field (E⃗)(\vec{E}) due to a straight uniformly charged infinite line of charge density λ C m−1\lambda\,\text{C m}^{-1}. (b) Draw a graph to show the variation of EE with perpendicular distance rr from the line of charge. (c) Find the work done in bringing a charge qq from perpendicular distance r1r_1 to r2 (r2>r1)r_2\,(r_2>r_1).

    Asked in: CBSE Class 12 Physics — Long Answer · 2018 · Section E, 5 marks

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    (a),(b) (Same derivation as Q57/60.) E=λ2πε0rE = \dfrac{\lambda}{2\pi\varepsilon_0 r}, directed radially outward; E∝1/rE \propto 1/r, so the graph is a steadily decreasing curve. (c) Work done in moving charge qq from r2r_2 to r1r_1 (against/along the field): W=∫r2r1F⃗⋅dr⃗=∫r2r1qλ2πε0rdrcos⁡0°=qλ2πε0∫r2r1drrW = \displaystyle\int_{r_2}^{r_1}\vec{F}\cdot d\vec{r} = \int_{r_2}^{r_1}\dfrac{q\lambda}{2\pi\varepsilon_0 r}dr\cos0° = \dfrac{q\lambda}{2\pi\varepsilon_0}\int_{r_2}^{r_1}\dfrac{dr}{r} =qλ2πε0[ln⁡r]r2r1=qλ2πε0ln⁡r1r2= \dfrac{q\lambda}{2\pi\varepsilon_0}[\ln r]_{r_2}^{r_1} = \dfrac{q\lambda}{2\pi\varepsilon_0}\ln\dfrac{r_1}{r_2}

  18. 18
    Derivation 18
    Use Gauss's law to prove that the electric field inside a uniformly charged spherical shell is zero.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, AI 2015 · Section E, 5 marks

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    (Same as the r<Rr<R case of Q61.) For a point PP inside the shell, take a concentric spherical Gaussian surface of radius r<Rr<R through PP. Since all the charge qq resides on the shell of radius RR (outside this Gaussian surface), the charge enclosed by this surface is zero. By Gauss's law, E×4πr2=0ε0=0 ⇒ E=0E\times4\pi r^2 = \dfrac{0}{\varepsilon_0} = 0 \ \Rightarrow\ E=0 Hence the electric field at every point inside a uniformly charged spherical shell is zero.

  19. 19
    Derivation 19
    A small conducting sphere of radius 'rr' carrying a charge +q+q is surrounded by a large concentric conducting shell of radius RR on which a charge +Q+Q is placed. Using Gauss's law, derive the expressions for the electric field at a point 'xx' (i) between the sphere and the shell (r<x<R)(r<x<R), and (ii) outside the spherical shell.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, Foreign 2015, An · Section E, 5 marks

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    Consider a Gaussian spherical surface of radius xx, centred at OO. Total flux through this surface: ϕ=∮E ds=E∮ds=E×4πx2\phi = \displaystyle\oint E\,ds = E\oint ds = E\times4\pi x^2 ...(i) (since ∮ds=4πx2\oint ds = 4\pi x^2) By Gauss's theorem, ϕ=qenclosedε0\phi = \dfrac{q_{enclosed}}{\varepsilon_0} ...(ii) (i) For r<x<Rr<x<R: the Gaussian surface encloses only the inner sphere's charge, qenclosed=qq_{enclosed}=q. From (i) and (ii): E×4πx2=qε0 ⇒ E=q4πε0x2E\times4\pi x^2 = \dfrac{q}{\varepsilon_0} \ \Rightarrow\ E = \dfrac{q}{4\pi\varepsilon_0 x^2} (ii) For x>Rx>R (outside the shell): the Gaussian surface encloses both charges, qenclosed=q+Qq_{enclosed}=q+Q. From (i) and (ii): E×4πx2=q+Qε0 ⇒ E=q+Q4πε0x2E\times4\pi x^2 = \dfrac{q+Q}{\varepsilon_0} \ \Rightarrow\ E = \dfrac{q+Q}{4\pi\varepsilon_0 x^2}

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