Electrostatic Potential and Capacitance

Chapter 1 gave you the electric field — a vector recipe telling you the force per unit charge at every point around a charge configuration. This chapter asks the companion question: if you actually carry a charge through that field, how much work does it cost, and where does that work go? The answer is that the Coulomb force is conservative, exactly like gravity, so the work done depends only on the start and end points, never on the path. That path-independence is the seed from which the entire chapter grows: it lets us define a scalar field, the electrostatic potential VV, whose difference between two points equals the work done per unit charge in moving between them. From that one idea the chapter builds outward in a natural sequence. First we find the potential of a single point charge and of a dipole, then of any collection of charges by superposition, then of a charged conducting shell. We learn to read potential geometrically through equipotential surfaces, always perpendicular to the field, and derive the working link E=−dV/dlE = -dV/dl that lets you move between the vector picture and the scalar picture at will. We then price out the energy stored in assembling any charge configuration, and separately the energy of a charge or a dipole sitting inside someone else's field. A close look at conductors follows — why the field inside is always zero, why charge lives only on the surface, why a hollow conductor shields its interior — and then dielectrics, the polarisable insulators that weaken an internal field without ever cancelling it. All of this converges on the chapter's most exam-tested device: the capacitor, a pair of conductors that stores charge at a controlled, safe potential. You will derive the parallel-plate formula, see how a dielectric slab boosts it, learn to collapse series and parallel networks into a single effective capacitance, and compute the energy a charged capacitor holds — the same quantity that powers a camera flash and, in reverse, tells you why an electric field itself carries energy. Everything here recurs in the very next chapter, current electricity, where capacitors and potential differences drive real circuits.

Key takeaways
  • Coulomb force is conservative, so work done moving a charge between two points is path-independent; this defines electrostatic potential energy and, per unit charge, the electrostatic potential VV.
  • Potential due to a point charge is V=14πε0QrV = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{r}, taking V=0V = 0 at infinity; a dipole's potential falls off faster, as 1/r21/r^2, and vanishes on the equatorial plane.
  • Potential obeys superposition: the potential of any charge system is the algebraic sum of the potentials of its parts, including for a uniformly charged spherical shell where V=kq/RV = kq/R everywhere inside and V=kq/rV=kq/r outside.
  • Equipotential surfaces are always perpendicular to the electric field, and E=−dVdlE = -\dfrac{dV}{dl} — the field points along the steepest decrease of potential.
  • Potential energy of a pair of charges is U=14πε0q1q2r12U = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_2}{r_{12}}; a dipole in a uniform external field has energy U(θ)=−p⃗⋅E⃗U(\theta) = -\vec p \cdot \vec E and feels a torque τ⃗=p⃗×E⃗\vec\tau = \vec p \times \vec E.
  • Inside any conductor in electrostatic equilibrium the field is zero, all excess charge sits on the surface, the whole conductor is at one potential, and a cavity inside is completely shielded from outside fields.
  • A dielectric polarises in an external field, developing bound surface charge that opposes and weakens (but never cancels) the field, characterised by a dielectric constant K>1K > 1.
  • A capacitor stores charge QQ at potential difference VV with C=Q/VC = Q/V; for a parallel plate capacitor C=ε0A/dC = \varepsilon_0 A/d in vacuum and C=Kε0A/dC = K\varepsilon_0 A/d with a dielectric filling the gap.
  • Capacitors in series add as reciprocals (1/C=∑1/Ci1/C = \sum 1/C_i, same QQ on each), capacitors in parallel add directly (C=∑CiC = \sum C_i, same VV across each), and a charged capacitor stores energy U=12QV=12CV2=Q22CU = \tfrac{1}{2}QV = \tfrac12 CV^2 = \tfrac{Q^2}{2C}, equivalent to an energy density u=12ε0E2u = \tfrac12 \varepsilon_0 E^2 in the field itself.
  • Key idea: because the Coulomb force is conservative, a scalar potential V (work per unit charge from infinity) captures everything about a charge configuration's energy, and capacitors are the practical device built on this idea — two conductors that store charge Q at potential difference V with C = Q/V, boosted by a dielectric and combined in series or parallel.
The core insight

Electrostatic potential is the work done per unit charge in bringing a test charge from infinity, it obeys superposition and is always perpendicular to equipotential surfaces with E=−dV/dlE=-dV/dl, and a capacitor packages this idea practically as C=Q/VC=Q/V, storing energy U=12CV2U=\tfrac12 CV^2 that a dielectric can boost by its dielectric constant KK.

What this chapter covers

The chapter has two connected halves. The first half (potential and potential energy) builds the scalar description of the electric field: potential energy and potential from work done, potential of a point charge and a dipole, potential of a system of charges and of a charged spherical shell, equipotential surfaces and the field-potential relation, potential energy of a system of charges, potential energy in an external field including a dipole in a uniform field, and the electrostatics of conductors (zero interior field, surface charge, constant potential, electrostatic shielding). The second half (capacitance) turns this into a device: dielectrics and polarisation, capacitors and capacitance, the parallel plate capacitor, the effect of a dielectric on capacitance, series and parallel combinations, and the energy stored in a capacitor together with the idea of energy density in the electric field. Worked examples throughout reuse NCERT's own numbering (Examples 2.1 to 2.10) so you can cross-check against your textbook.

The core ideas

From work done to potential energy

Coulomb force, like gravity, is a conservative force — the work done moving a charge between two points does not depend on the path taken, only on the endpoints. Bringing a positive test charge qq from a point RR to a point PP against the repulsive field of a source charge QQ requires an external force that does work WRPW_{RP}, and this work is stored entirely as potential energy, since removing the external force lets the field convert that stored energy back into kinetic energy.

ΔU=UP−UR=WRP.(1)\Delta U = U_P - U_R = W_{RP}. \qquad (1)

where: UP,URU_P, U_R are the potential energies of the test charge at PP and RR, and WRPW_{RP} is the work done by an external agent (equal and opposite to the electric force) in moving the charge from RR to PP without giving it any net kinetic energy. Because only differences in UU ever enter physics, potential energy is defined only up to an arbitrary additive constant — the natural choice is to set U=0U=0 at infinity, which then fixes UU at any point PP as the work done bringing the charge from infinity to PP.

Electrostatic potential

Dividing potential energy by the test charge qq removes the dependence on how big a test charge you happened to use, leaving a property of the field alone: the electrostatic potential VV.

VP−VR=UP−URq.(2)V_P - V_R = \frac{U_P - U_R}{q}. \qquad (2)

where: VP,VRV_P, V_R are the potentials at PP and RR in volts (1 V=1 J/C1\ \text{V} = 1\ \text{J/C}). With V=0V=0 chosen at infinity, VV at any point is the work done by an external agent in bringing a unit positive charge from infinity to that point, without acceleration. Potential, like potential energy, is a scalar — no direction to track, only a sign and a magnitude — which is exactly what makes it so much easier to add up over many charges than the vector field E⃗\vec E.

Potential due to a point charge

Placing charge QQ at the origin and integrating the Coulomb force along a radial path from infinity to a point at distance rr gives the potential everywhere around a point charge, and this is the seed formula for the whole chapter.

V(r)=14πε0Qr.(3)V(r) = \frac{1}{4\pi\varepsilon_0}\frac{Q}{r}. \qquad (3)

where: ε0=8.85×10−12 C2N−1m−2\varepsilon_0 = 8.85\times10^{-12}\ \text{C}^2\text{N}^{-1}\text{m}^{-2} is the permittivity of free space, and rr is the distance from the charge (full derivation below). Equation (3) holds for either sign of QQ: positive charge gives positive potential everywhere, negative charge gives negative potential everywhere, consistent with V=0V=0 at infinity. Unlike the field, which falls off as 1/r21/r^2, potential falls off more gently, as 1/r1/r.

Figure
Graphs of potential varying as one over r and field varying as one over r squared for a point charge plotted against distance from the charge
Potential falls as 1/r, field falls faster, as 1/r squared distance r from the charge V and E in scaled units V(r) proportional to 1/r E(r) proportional to 1/r squared near the charge far from the charge

Potential due to an electric dipole

An electric dipole is a charge +q+q and −q-q separated by a small distance 2a2a, with dipole moment p⃗\vec p of magnitude q(2a)q(2a) pointing from −q-q to +q+q. Superposing the potentials of the two point charges and expanding for a point far from the dipole (r≫ar \gg a) gives a result strikingly different from a single charge.

V(r,θ)=14πε0pcos⁡θr2,r≫a.(4)V(r,\theta) = \frac{1}{4\pi\varepsilon_0}\frac{p\cos\theta}{r^2}, \qquad r \gg a. \qquad (4)

where: θ\theta is the angle between the position vector r⃗\vec r of the field point and the dipole moment p⃗\vec p. The dipole's potential depends not just on distance but on direction — maximum and positive on the axis toward +q+q (θ=0\theta=0), equally maximum but negative toward −q-q (θ=π\theta=\pi), and exactly zero on the equatorial plane (θ=π/2\theta=\pi/2), since the two charges are equidistant there and cancel. It also falls off as 1/r21/r^2, one power of rr faster than a single charge's 1/r1/r, because the near-cancellation of +q+q and −q-q weakens it faster with distance.

Potential due to a system of charges, and a charged spherical shell

Because potential is a scalar built from a linear operation (division by qq of a linear work integral), it inherits the superposition principle exactly as the field does, but without any vector addition to worry about.

V=14πε0(q1r1P+q2r2P+⋯+qnrnP).(5)V = \frac{1}{4\pi\varepsilon_0}\left(\frac{q_1}{r_{1P}} + \frac{q_2}{r_{2P}} + \cdots + \frac{q_n}{r_{nP}}\right). \qquad (5)

where: riPr_{iP} is the distance from the ii-th charge to the field point PP. This scalar sum is why potential is often easier to compute than the field for a complicated arrangement — no components to resolve. Applying it to a uniformly charged spherical shell of charge qq, radius RR (whose field is zero inside and behaves as a point charge outside) gives V=14πε0qrV=\frac{1}{4\pi\varepsilon_0}\frac{q}{r} for r≥Rr\ge R, and, since no work is needed through a zero field, the constant value V=14πε0qRV=\frac{1}{4\pi\varepsilon_0}\frac{q}{R} for every point inside, including the centre.

Equipotential surfaces and the field-potential relation

A surface on which VV has the same value everywhere is an equipotential surface; for a single point charge these are concentric spheres centred on the charge, and for a uniform field they are planes perpendicular to the field direction. The defining geometric fact links the scalar and vector pictures: the field is always perpendicular to the equipotential surface through any point, because any component of EE along the surface would mean work is needed to move a charge along a supposedly constant-potential surface — a contradiction.

E=−dVdl.(6)E = -\frac{dV}{dl}. \qquad (6)

where: dVdV is the change in potential over an infinitesimal displacement dldl measured normal to the equipotential surfaces. The field points in the direction potential decreases most steeply (hence the minus sign — high to low potential), and its magnitude equals the rate of that decrease per unit distance. Closely packed equipotential surfaces mean a strong field; widely spaced ones mean a weak field — like closely spaced contour lines meaning steep terrain on a map.

Figure
Two equipotential surfaces around a point charge shown as concentric circles with field lines drawn as radial arrows perpendicular to each equipotential surface and pointing from higher to lower potential
Field lines cross equipotential surfaces at right angles, pointing to lower V +Q V = V1 (near) V = V2 V = V3 (far, smaller V) field lines, always normal to each surface Closer surfaces (near the charge) mean a stronger field; wider spacing means a weaker field.

Potential energy of a system of charges

Building up a configuration of point charges from infinity, one at a time, costs no work for the first charge (nothing else is there yet), but every subsequent charge must be moved through the potential created by all the charges already in place. Summing this over all pairs gives the total electrostatic potential energy of the configuration, independent of the order of assembly because the Coulomb force is conservative.

U=14πε0(q1q2r12+q1q3r13+q2q3r23+⋯ ).(7)U = \frac{1}{4\pi\varepsilon_0}\left(\frac{q_1q_2}{r_{12}} + \frac{q_1q_3}{r_{13}} + \frac{q_2q_3}{r_{23}} + \cdots\right). \qquad (7)

where: the sum runs over every distinct pair of charges, and rijr_{ij} is the distance between charges ii and jj. Same-sign charges give positive energy (work was needed against repulsion to bring them together); opposite signs give negative energy (the attractive force did positive work, so an external agent had to hold them back with negative work). The same expression applies term by term for any number of charges — square corners, hexagon vertices, whatever arrangement a problem gives you.

Potential energy in an external field, and the dipole case

A related but distinct question: given an external field EE (or potential VV) produced by sources we are not tracking, what is the potential energy of a charge qq placed inside it? By the very definition of potential, the answer is immediate, and extending it to a dipole reveals the origin of the torque you met in Chapter 1.

U=qV(r⃗),U(θ)=−p⃗⋅E⃗=−pEcos⁡θ.(8)U = qV(\vec r), \qquad U(\theta) = -\vec p \cdot \vec E = -pE\cos\theta. \qquad (8)

where: the first form gives the energy of a charge qq at r⃗\vec r in an external potential V(r⃗)V(\vec r); the second gives a dipole of moment pp at angle θ\theta to a uniform field EE, with zero energy chosen at θ=π/2\theta=\pi/2. Energy is lowest (−pE-pE) when aligned with the field, highest (+pE+pE) when anti-aligned, and the torque τ⃗=p⃗×E⃗\vec\tau=\vec p\times\vec E from Chapter 1 is exactly what rotates the dipole downhill toward this minimum — aligned is stable, anti-aligned is not.

Electrostatics of conductors

A conductor's free electrons redistribute themselves until electrostatic equilibrium is reached, enforcing a short, memorable list of results examiners test relentlessly. Inside a conductor the field is always zero (otherwise free charges would still be drifting); excess charge resides only on the outer surface (Gauss's law on any interior volume gives zero enclosed charge, since the field on its boundary is zero); the whole conductor sits at one constant potential (zero field means zero work to move a test charge inside or on it); and just outside a charged surface the field is normal to it, fixed by the local surface charge density.

E⃗=σε0n^.(9)\vec E = \frac{\sigma}{\varepsilon_0}\hat n. \qquad (9)

where: σ\sigma is the surface charge density at that point and n^\hat n is the outward unit normal. A further consequence, electrostatic shielding, is that a charge-free cavity inside any conductor has exactly zero field inside it, whatever charge sits on the conductor or whatever external field surrounds it — the reason sensitive electronics are built inside metal enclosures (Faraday cages).

Dielectrics, polarisation, and the capacitor

Dielectrics are insulators with no free charge carriers; placed in an external field, they cannot cancel the field the way a conductor does, but they weaken it. Non-polar molecules (like O2_2) develop an induced dipole moment as the field stretches apart their charge centres; polar molecules (like H2_2O), already carrying a permanent dipole moment, instead align with the field against thermal disruption. Either way the dielectric develops a net dipole moment per unit volume, the polarisation P=ε0χeEP=\varepsilon_0\chi_e E, equivalent to induced bound surface charges ±σP\pm\sigma_P on its two faces, producing a field opposing (but not cancelling) the external one. This weakened-but-not-cancelled internal field is exactly what makes a capacitor — two conductors carrying charges +Q+Q and −Q-Q, separated by an insulator — a practical way to store charge safely at a controlled, low potential difference.

C=QV.(10)C = \frac{Q}{V}. \qquad (10)

where: QQ is the magnitude of charge on either conductor, VV is the potential difference between them, and CC, the capacitance, depends purely on geometry (shape, size, separation) and the dielectric between them — never on QQ or VV themselves, since doubling QQ doubles both the field and VV in proportion. The SI unit is the farad, 1 F=1 C V−11\ \text{F}=1\ \text{C}\,\text{V}^{-1}; a farad is an enormous unit (a 1 F capacitor with a 1 cm gap would need plates roughly 30 km on a side), so practical capacitances are quoted in microfarads, nanofarads or picofarads (pF=10−12 F\text{pF}=10^{-12}\,\text{F}).

The parallel plate capacitor and the effect of a dielectric

For two large parallel plates of area AA separated by a small distance dd (so d2≪Ad^2 \ll A and fringing at the edges can be ignored), the fields of the two oppositely charged sheets cancel outside the plates and add uniformly between them, giving a capacitance that depends only on geometry and on whatever fills the gap.

Cvac=ε0Ad,Cdielectric=Kε0Ad=KCvac.(11)C_{\text{vac}} = \frac{\varepsilon_0 A}{d}, \qquad C_{\text{dielectric}} = \frac{K\varepsilon_0 A}{d} = KC_{\text{vac}}. \qquad (11)

where: KK is the dielectric constant of whatever fills the gap (K=1K=1 for vacuum, K>1K>1 for every real dielectric). The dielectric's induced bound charge σP\sigma_P partially cancels the free charge's field, so for the same free charge QQ, the field and hence VV inside drop by the factor KK, and since C=Q/VC=Q/V, a smaller VV for the same QQ means a larger CC. This is why real capacitors sandwich a dielectric between their plates — it multiplies the capacitance for the same size, and raises the breakdown voltage too.

Combining capacitors: series and parallel

Real circuits rarely use one capacitor alone, so the chapter gives two combination rules, mirror images of the series and parallel rules you will meet for resistors in the very next chapter (though with the two roles of QQ and VV swapped).

series: 1C=1C1+1C2+⋯ ;parallel: C=C1+C2+⋯ .(12)\text{series: } \frac{1}{C} = \frac{1}{C_1} + \frac{1}{C_2} + \cdots; \qquad \text{parallel: } C = C_1 + C_2 + \cdots. \qquad (12)

where: in a series combination, charge QQ has nowhere else to go, so every capacitor carries the same charge QQ while potential splits across them, V=V1+V2+⋯V=V_1+V_2+\cdots, producing the reciprocal-sum rule; in a parallel combination, every capacitor shares the same VV while charge splits, Q=Q1+Q2+⋯Q=Q_1+Q_2+\cdots, giving the direct-sum rule. Quick sanity check: series always gives a smaller net capacitance than the smallest individual one; parallel always gives a larger one than the largest.

Energy stored in a capacitor

Charging a capacitor means moving charge, bit by bit, from one plate to the other against a growing potential difference; integrating the work done at each infinitesimal step gives the total energy stored, which can be written in three equivalent forms depending on which two of QQ, VV, CC a problem gives you.

U=12QV=12CV2=Q22C.(13)U = \frac{1}{2}QV = \frac{1}{2}CV^2 = \frac{Q^2}{2C}. \qquad (13)

where: QQ is the final charge and VV the final potential difference. This energy is not lost when the capacitor is disconnected — it stays stored, ready to be released, which is why a capacitor (unlike a resistor) can power a sudden discharge, as in a camera flash. Rewriting the parallel-plate case using the field E=σ/ε0E=\sigma/\varepsilon_0 shows the energy can equally be thought of as stored in the field itself, occupying volume AdAd at a density u=12ε0E2u=\tfrac12\varepsilon_0 E^2 — derived here for a parallel plate capacitor, but true in general for any electric field.

Derivations

Derivation APotential due to a point charge

The goal is to derive Equation (3), the potential at distance rr from a point charge QQ, directly from the definition of potential as work done per unit charge bringing a test charge from infinity — the single integral every other potential formula in this chapter descends from. We place QQ at the origin, take Q>0Q>0 for definiteness (the result holds for either sign), and bring a unit positive test charge along a radial path from infinity to the field point PP at distance rr.

Step 1. At an intermediate point on the path, a distance r′r' from QQ, the electrostatic force on a unit positive test charge is Q4πε0r′2\dfrac{Q}{4\pi\varepsilon_0 r'^2} directed radially outward, away from QQ. To move the test charge inward, without accelerating it, an external agent must apply a force equal and opposite to this, i.e. directed inward, of the same magnitude.

Step 2. The work done by the external force over a small inward step Δr′\Delta r' (note Δr′<0\Delta r' < 0 since r′r' is decreasing toward PP) is ΔW=−Q4πε0r′2Δr′\Delta W = -\dfrac{Q}{4\pi\varepsilon_0 r'^2}\Delta r'. The minus sign is essential bookkeeping: since Δr′\Delta r' is negative, this makes ΔW\Delta W positive, correctly recording that positive work is being done against the repulsive force.

Step 3. Summing (integrating) these small contributions from r′=∞r' = \infty down to r′=rr' = r gives the total work done by the external agent, W=−∫∞rQ4πε0r′2 dr′=Q4πε0[1r′]∞r=Q4πε0(1r−0)=Q4πε0rW = -\displaystyle\int_{\infty}^{r} \frac{Q}{4\pi\varepsilon_0 r'^2}\,dr' = \frac{Q}{4\pi\varepsilon_0}\left[\frac{1}{r'}\right]_{\infty}^{r} = \frac{Q}{4\pi\varepsilon_0}\left(\frac{1}{r} - 0\right) = \frac{Q}{4\pi\varepsilon_0 r}. The upper limit contributes 1/r1/r and the lower limit at infinity contributes zero, since 1/r′→01/r' \to 0 as r′→∞r' \to \infty.

Step 4. By definition, this total work done per unit test charge is the potential at PP: V(r)=14πε0QrV(r) = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{r}, exactly Equation (3). Although derived here for Q>0Q>0, the algebra carries through unchanged for Q<0Q<0: the force is then attractive, the work done by the external agent (which must now hold the charge back rather than push it in) comes out negative, and V(r)V(r) correctly comes out negative too — the formula needs no separate case for sign. Verified: as r′→∞r'\to\infty, 1/r′→01/r'\to0 so the lower limit vanishes cleanly; the dimensions of Q4πε0r\frac{Q}{4\pi\varepsilon_0 r} reduce to J C−1=V\text{J}\,\text{C}^{-1}=\text{V}, confirming a potential.

Go deeper · Derivation B · 1 minPotential due to a short electric dipole
Derivation BPotential due to a short electric dipole

The goal is to derive Equation (4), the far-field potential of a dipole of moment p=q(2a)p=q(2a) at a point PP making angle θ\theta with the dipole axis, using nothing beyond superposition of two point-charge potentials and the binomial approximation for r≫ar\gg a — the approximation that recurs whenever "far field of a dipole" appears on an exam. Place the dipole's centre at the origin, +q+q and −q-q each a distance aa from it along the axis, and let r1,r2r_1,r_2 be the distances from +q+q and −q-q to the field point PP.

Step 1. By superposition, the potential at PP is simply the sum of the potentials of the two point charges: V=14πε0(qr1−qr2)V = \dfrac{1}{4\pi\varepsilon_0}\left(\dfrac{q}{r_1} - \dfrac{q}{r_2}\right). Everything now reduces to finding r1r_1 and r2r_2 in terms of rr, aa and θ\theta.

Step 2. By the law of cosines applied to the two small triangles formed by the charges, the origin, and PP: r12=r2+a2−2arcos⁡θr_1^2 = r^2 + a^2 - 2ar\cos\theta and r22=r2+a2+2arcos⁡θr_2^2 = r^2 + a^2 + 2ar\cos\theta. For r≫ar \gg a, the a2a^2 term is negligible next to the others, so r12≈r2(1−2acos⁡θr)r_1^2 \approx r^2\left(1 - \dfrac{2a\cos\theta}{r}\right) and r22≈r2(1+2acos⁡θr)r_2^2 \approx r^2\left(1 + \dfrac{2a\cos\theta}{r}\right), keeping only first order in a/ra/r.

Step 3. Taking 1/r11/r_1 and 1/r21/r_2 means raising each bracket to the power −1/2-1/2; the binomial expansion (1+x)−1/2≈1−x/2(1+x)^{-1/2} \approx 1 - x/2 for small xx gives 1r1≈1r(1+acos⁡θr)\dfrac{1}{r_1} \approx \dfrac{1}{r}\left(1 + \dfrac{a\cos\theta}{r}\right) and 1r2≈1r(1−acos⁡θr)\dfrac{1}{r_2} \approx \dfrac{1}{r}\left(1 - \dfrac{a\cos\theta}{r}\right), again keeping only first order in a/ra/r.

Step 4. Substituting into Step 1: V=q4πε0[1r(1+acos⁡θr)−1r(1−acos⁡θr)]=q4πε0⋅2acos⁡θr2V = \dfrac{q}{4\pi\varepsilon_0}\left[\dfrac{1}{r}\left(1+\dfrac{a\cos\theta}{r}\right) - \dfrac{1}{r}\left(1-\dfrac{a\cos\theta}{r}\right)\right] = \dfrac{q}{4\pi\varepsilon_0}\cdot\dfrac{2a\cos\theta}{r^2}. Writing p=2qap = 2qa for the dipole moment gives V=14πε0pcos⁡θr2V = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p\cos\theta}{r^2}, exactly Equation (4).

Step 5. Read off the two special cases directly: on the axis toward +q+q, θ=0\theta=0 so V=14πε0pr2V = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^2}, its largest positive value; on the equatorial plane, θ=π/2\theta = \pi/2 so cos⁡θ=0\cos\theta = 0 and V=0V=0 identically, confirming by direct calculation what symmetry already suggested — equidistant +q+q and −q-q contribute equal and opposite potential there. Verified: at θ=0\theta=0, V=p4πε0r2V=\dfrac{p}{4\pi\varepsilon_0 r^2}, matching the axial result; at θ=π/2\theta=\pi/2, V=0V=0 as expected on physical grounds.

Go deeper · Derivation C · 1 minCapacitance of a parallel plate capacitor
Derivation CCapacitance of a parallel plate capacitor

The goal is to derive Equation (11), C=ε0A/dC = \varepsilon_0 A/d for a vacuum-filled parallel plate capacitor, starting from the known field of an infinite charged sheet and building up the field between two oppositely charged plates, then converting field to potential difference and finally to capacitance — the single most exam-tested derivation in this chapter. Let each plate have area AA, separation dd with d2≪Ad^2 \ll A so edge effects (fringing) can be ignored, and surface charge densities +σ+\sigma on plate 1 and −σ-\sigma on plate 2, with σ=Q/A\sigma = Q/A.

Step 1. Each charged plate, treated as an infinite sheet, produces a field of magnitude σ/2ε0\sigma/2\varepsilon_0 pointing away from itself (for the positive plate) or toward itself (for the negative plate), uniform on either side of the sheet. In the region outside both plates (above plate 1, or below plate 2), the two fields point in opposite directions and are equal in magnitude, so they cancel exactly: Eoutside=σ2ε0−σ2ε0=0E_{\text{outside}} = \dfrac{\sigma}{2\varepsilon_0} - \dfrac{\sigma}{2\varepsilon_0} = 0.

Step 2. In the region between the plates, the field from plate 1 (pointing away from the positive plate, i.e. toward plate 2) and the field from plate 2 (pointing toward the negative plate, i.e. also toward plate 2's side, meaning away from plate 1 on this side) point in the same direction, so they add: E=σ2ε0+σ2ε0=σε0=Qε0AE = \dfrac{\sigma}{2\varepsilon_0} + \dfrac{\sigma}{2\varepsilon_0} = \dfrac{\sigma}{\varepsilon_0} = \dfrac{Q}{\varepsilon_0 A}. The field is confined entirely to the gap between the plates and is uniform there.

Step 3. Since the field between the plates is uniform, the potential difference is simply field times separation: V=Ed=Qε0A⋅d=Qdε0AV = Ed = \dfrac{Q}{\varepsilon_0 A}\cdot d = \dfrac{Qd}{\varepsilon_0 A}. This is the work per unit charge to cross the gap against the uniform field.

Step 4. Capacitance is defined as C=Q/VC = Q/V; substituting Step 3 and cancelling the common factor QQ: C=QQd/(ε0A)=ε0AdC = \dfrac{Q}{Qd/(\varepsilon_0 A)} = \dfrac{\varepsilon_0 A}{d}, exactly Equation (11) with K=1K=1. Notice that QQ cancels completely, confirming that CC depends only on geometry (AA, dd) and the medium (ε0\varepsilon_0), never on how much charge happens to be on the plates. Verified: for A=1 m2A=1\ \text{m}^2, d=1 mmd=1\ \text{mm}, C=(8.85×10−12)(1)/(10−3)=8.85×10−9 F≈8.85 nFC=(8.85\times10^{-12})(1)/(10^{-3})=8.85\times10^{-9}\ \text{F}\approx8.85\ \text{nF}, matching the textbook's own numerical check.

Go deeper · Derivation D · 1 minEnergy stored in a charged capacitor
Derivation DEnergy stored in a charged capacitor

The goal is to derive Equation (13), U=Q2/2CU = Q^2/2C, by tracking the work done during the process of charging a capacitor rather than just quoting the final formula — because the charge on the plates, and hence the potential difference resisting further charging, both grow as the capacitor charges, so the work per unit charge transferred is not constant and must be integrated. Start with two uncharged conductors and imagine transferring positive charge from conductor 2 to conductor 1, bit by bit, until conductor 1 holds the final charge QQ (and conductor 2, by charge conservation, holds −Q-Q).

Step 1. At an intermediate stage, when conductor 1 already holds charge Q′Q' (and conductor 2 holds −Q′-Q'), the potential difference between them is V′=Q′/CV' = Q'/C, using the very definition of capacitance applied at this intermediate charge value.

Step 2. Moving a further small charge δQ′\delta Q' from conductor 2 to conductor 1 requires work δW=V′ δQ′=Q′C δQ′\delta W = V'\,\delta Q' = \dfrac{Q'}{C}\,\delta Q', since at every stage conductor 1 sits at the higher potential and work must be done against this potential difference to add more positive charge there.

Step 3. Summing (integrating) this from Q′=0Q' = 0 (start, both plates uncharged) to Q′=QQ' = Q (final charge) gives the total work done, which becomes the stored energy: U=∫0QQ′C dQ′=1C[Q′22]0Q=Q22CU = \displaystyle\int_0^{Q} \frac{Q'}{C}\,dQ' = \frac{1}{C}\left[\frac{Q'^2}{2}\right]_0^{Q} = \frac{Q^2}{2C}. The key feature making this an integral rather than simple multiplication is that V′=Q′/CV' = Q'/C itself grows as charge accumulates — the last bit of charge transferred costs far more work than the first bit.

Step 4. Using Q=CVQ=CV converts this into the two other familiar forms: U=Q22C=(CV)22C=12CV2=12QVU = \dfrac{Q^2}{2C} = \dfrac{(CV)^2}{2C} = \dfrac{1}{2}CV^2 = \dfrac{1}{2}QV, exactly Equation (13). Note the missing factor of 12\tfrac12 compared to the naive (and wrong) guess U=QVU = QV — that guess would be the work to move the entire charge QQ through the final, full potential difference VV in one step, which overcounts because most of the charge was actually moved when the potential difference was still smaller. Verified: for a 900 pF900\ \text{pF} capacitor charged to 100 V100\ \text{V}, Q=CV=9×10−8 CQ=CV=9\times10^{-8}\ \text{C} and U=12QV=4.5×10−6 JU=\tfrac12 QV=4.5\times10^{-6}\ \text{J}, matching NCERT Example 2.10(a) exactly.

Worked examples

Board level - potential and work done bringing a charge from infinity

Calculate the potential at a point PP due to a charge of 4×10−7 C4\times10^{-7}\ \text{C} located 9 cm9\ \text{cm} away. Hence find the work done in bringing a charge of 2×10−9 C2\times10^{-9}\ \text{C} from infinity to PP.

Step 1. Apply the point-charge formula, Equation (3), with Q=4×10−7 CQ = 4\times10^{-7}\ \text{C} and r=9×10−2 mr = 9\times10^{-2}\ \text{m}: V=14πε0Qr=(9×109)4×10−79×10−2=4×104 VV = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{r} = (9\times10^{9})\dfrac{4\times10^{-7}}{9\times10^{-2}} = 4\times10^{4}\ \text{V}.

Step 2. Work done bringing charge q=2×10−9 Cq = 2\times10^{-9}\ \text{C} from infinity to PP uses W=qVW = qV directly, since VV is by definition the work per unit charge: W=(2×10−9)(4×104)=8×10−5 JW = (2\times10^{-9})(4\times10^4) = 8\times10^{-5}\ \text{J}.

Step 3. This work is path-independent, since electrostatic force is conservative: any infinitesimal path splits into a component along rr (which does work) and a component perpendicular to rr (which does zero work, since the force is radial). Answer: V=4×104 VV = 4\times10^4\ \text{V} and W=8×10−5 JW = 8\times10^{-5}\ \text{J}, independent of the path taken.

Board level - equivalent capacitance and charge in a mixed network

A network of four 10 μF10\ \mu\text{F} capacitors is connected to a 500 V500\ \text{V} supply: three of them, C1,C2,C3C_1, C_2, C_3, are in series with each other, and this series group is in parallel with the fourth, C4C_4. Find the equivalent capacitance and the charge on each capacitor.

Step 1. Combine the series group first, using Equation (12): 1C′=1C1+1C2+1C3=110+110+110=310 μF−1\dfrac{1}{C'} = \dfrac{1}{C_1}+\dfrac{1}{C_2}+\dfrac{1}{C_3} = \dfrac{1}{10}+\dfrac{1}{10}+\dfrac{1}{10} = \dfrac{3}{10}\ \mu\text{F}^{-1}, so C′=103 μF≈3.33 μFC' = \dfrac{10}{3}\ \mu\text{F} \approx 3.33\ \mu\text{F}.

Step 2. This series group C′C' sits in parallel with C4=10 μFC_4 = 10\ \mu\text{F}, so the total is a direct sum: C=C′+C4=3.33+10=13.3 μFC = C' + C_4 = 3.33 + 10 = 13.3\ \mu\text{F}.

Step 3. In the series branch, the same charge QQ flows through C1C_1, C2C_2, C3C_3; the potential drop across the branch is the full 500 V500\ \text{V}, so Q=C′×500=1.7×10−3 CQ = C'\times500 = 1.7\times10^{-3}\ \text{C} on each. The parallel branch C4C_4 sees 500 V500\ \text{V} directly, so Q4=C4×500=5.0×10−3 CQ_4 = C_4\times500 = 5.0\times10^{-3}\ \text{C}. Answer: equivalent capacitance 13.3 μF\mathbf{13.3\ \mu F}; charge on each of C1,C2,C3C_1, C_2, C_3 is 1.7×10−3 C\mathbf{1.7\times10^{-3}\ C}, and on C4C_4 is 5.0×10−3 C\mathbf{5.0\times10^{-3}\ C}.

Competitive level (JEE / NEET) - energy "lost" when a charged capacitor shares charge with an uncharged one

A 600 pF600\ \text{pF} capacitor is charged by a 200 V200\ \text{V} supply, then disconnected from the supply and connected to another uncharged 600 pF600\ \text{pF} capacitor. How much electrostatic energy is lost in the process, and where does it go?

Step 1. Initial charge and energy on the first capacitor before connection: Q=CV=(600×10−12)(200)=1.2×10−7 CQ = CV = (600\times10^{-12})(200) = 1.2\times10^{-7}\ \text{C}, and initial energy Ui=12CV2=12(600×10−12)(200)2=1.2×10−5 JU_i = \tfrac12 CV^2 = \tfrac12(600\times10^{-12})(200)^2 = 1.2\times10^{-5}\ \text{J}.

Step 2. When connected, charge QQ redistributes between the two equal capacitors until both reach the same common potential V′V'; by charge conservation the total charge QQ splits equally, so each capacitor ends with Q/2Q/2, and since both have the same capacitance CC, the common potential is V′=Q/2C=V2=100 VV' = \dfrac{Q/2}{C} = \dfrac{V}{2} = 100\ \text{V}.

Step 3. Final energy is the sum over both capacitors, now each at C=600 pFC=600\ \text{pF} and V′=100 VV'=100\ \text{V}: Uf=2×12CV′2=CV′2=(600×10−12)(100)2=6×10−6 JU_f = 2\times\tfrac12 C V'^2 = C V'^2 = (600\times10^{-12})(100)^2 = 6\times10^{-6}\ \text{J}. Alternatively, using the equivalent parallel capacitance 2C2C at V′V': Uf=12(2C)(V′)2U_f = \tfrac12(2C)(V')^2, the same result.

Step 4. Energy lost is ΔU=Ui−Uf=1.2×10−5−6×10−6=6×10−6 J\Delta U = U_i - U_f = 1.2\times10^{-5} - 6\times10^{-6} = 6\times10^{-6}\ \text{J}, exactly half the initial energy. No charge is lost, but energy is lost because a transient current flows briefly while the potentials equalise, dissipating energy as heat in the wires (and briefly as radiation). Answer: energy lost is 6×10−6\mathbf{6\times10^{-6}} J, exactly half the original 1.2×10−51.2\times10^{-5} J, dissipated as heat during the brief redistribution current. Timing note: under two minutes if you remember the shortcut. For two equal capacitors sharing charge, the common potential is always the average of what each would have alone (here, average of 200 V200\ \text{V} and 0 V0\ \text{V} is 100 V100\ \text{V}), and the general result for any two capacitors C1C_1 (charged to V1V_1) connected to C2C_2 (charged to V2V_2) is ΔU=C1C22(C1+C2)(V1−V2)2\Delta U = \dfrac{C_1C_2}{2(C_1+C_2)}(V_1-V_2)^2 — memorising this formula turns a multi-step problem into a single substitution, a favourite JEE shortcut.

Competitive level (JEE / NEET) - capacitance with a partial dielectric slab

A parallel plate capacitor with plate separation dd has a dielectric slab of dielectric constant KK inserted between the plates, but the slab's thickness is only 34d\tfrac34 d (it does not fill the whole gap). Find the new capacitance in terms of the vacuum capacitance C0C_0.

Step 1. Split the gap into two regions in series: a dielectric-filled region of thickness t=34dt=\tfrac34 d where the field is reduced to E=E0/KE = E_0/K (with E0=V0/dE_0 = V_0/d the vacuum-case field), and a vacuum region of thickness d−t=14dd-t = \tfrac14 d where the field remains the full E0E_0.

Step 2. The total potential difference is the field times distance, summed over the two regions: V=E0(14d)+E0K(34d)=E0d(14+34K)=E0d⋅K+34KV = E_0\left(\dfrac14 d\right) + \dfrac{E_0}{K}\left(\dfrac34 d\right) = E_0 d\left(\dfrac14 + \dfrac{3}{4K}\right) = E_0 d\cdot\dfrac{K+3}{4K}. Recognising E0d=V0E_0 d = V_0, this is V=V0⋅K+34KV = V_0\cdot\dfrac{K+3}{4K}.

Step 3. The free charge Q0Q_0 on the plates is unchanged by inserting the slab (nothing was connected or disconnected during insertion in this idealisation), so the new capacitance is C=Q0V=Q0V0⋅K+34K=4KK+3⋅Q0V0=4KK+3 C0C = \dfrac{Q_0}{V} = \dfrac{Q_0}{V_0\cdot\frac{K+3}{4K}} = \dfrac{4K}{K+3}\cdot\dfrac{Q_0}{V_0} = \dfrac{4K}{K+3}\,C_0.

Step 4. Sanity-check the limits: if K→1K \to 1 (slab is effectively vacuum), C→44C0=C0C \to \dfrac{4}{4}C_0 = C_0 as it must; if t→dt\to d (slab fills the whole gap, the special case in the chapter's own derivation of C=KC0C=KC_0), a similar calculation with t=dt=d collapses cleanly to C=KC0C=KC_0, confirming the partial-slab method reduces correctly to the full-slab formula. Answer: C=4KK+3 C0\mathbf{C = \dfrac{4K}{K+3}\,C_0}. Timing note: about ninety seconds once you recognise the pattern. The general method — split the gap into series regions of uniform field, sum V=∑EidiV = \sum E_i d_i, then use C=Q0/VC=Q_0/V — handles any combination of slabs and air gaps a JEE question throws at you, including multiple slabs of different KK stacked in the same gap; always check the K→1K\to1 and full-thickness limits as a thirty-second safety net before committing to an answer.

Common traps

Confusing electric field and electric potential is the single most common source of errors — a point can have zero field but nonzero potential (the centre of two equal like charges) or zero potential but nonzero field (between a +3q+3q and a −2q-2q charge where potentials cancel but the field does not, Example 2.2). Always ask which quantity a question wants. Writing V=EdV = Ed as if it applies everywhere is another frequent slip — it holds only for a uniform field between parallel plates; for a point charge or any non-uniform field, go back to E=−dV/dlE=-dV/dl or integrate. Forgetting the factor of 12\tfrac12 in energy formulas is common under time pressure — students write U=QVU=QV instead of U=12QVU=\tfrac12 QV, forgetting that charge was moved gradually against a growing potential, not all at once against the final value. Assuming both charge and energy are conserved when two capacitors are connected is a related mistake — charge is always conserved, but energy is generally not (Worked example 3); do not assume Ui=UfU_i=U_f just because nothing was "lost" in the everyday sense. Mixing up series and parallel rules for capacitors with the resistor rules of the next chapter trips up many students, since the roles are swapped: capacitors in series share the same charge, capacitors in parallel share the same voltage. Believing a dielectric cancels the field, rather than merely weakening it by the factor KK, is a conceptual error worth flagging — a dielectric is not a conductor. Assuming a charged conductor's potential equals its field is a subtle Assertion-Reasoning trap — the field can be strong right at a highly charged surface while the potential is a modest, finite number; the two are related by geometry, not interchangeable.

You should be able to…

  • Define electrostatic potential energy and electrostatic potential from first principles, and explain why both are defined only up to an arbitrary additive constant.
  • Write down and apply the potential of a point charge, a dipole, and a system of point charges, including the special case of a uniformly charged spherical shell inside and outside.
  • Sketch equipotential surfaces for a point charge, a uniform field, and a dipole, and correctly state and use the relation E=−dV/dlE=-dV/dl.
  • Compute the potential energy of a system of point charges, and separately the potential energy of a charge or a dipole placed in an external field.
  • State all five key electrostatic properties of a conductor in equilibrium, and explain electrostatic shielding.
  • Explain, at the molecular level, how polar and non-polar dielectrics polarise in an external field and why this weakens (without cancelling) the internal field.
  • Derive the capacitance of a parallel plate capacitor, both with vacuum and with a dielectric filling all or part of the gap.
  • Reduce any series-parallel network of capacitors to a single equivalent capacitance, and find the charge and voltage on each individual capacitor within it.
  • Compute the energy stored in a charged capacitor in all three equivalent forms, and explain the energy density interpretation of the electric field.
  • Correctly diagnose, in a mixed problem, whether a question is really asking about field, potential, potential energy, or capacitance — and avoid substituting one for another.

Ask the tutor: Want to work through a mixed series-parallel capacitor network with a dielectric slab in one branch, step by step, using your own numbers?

If the electric field inside a conductor is always zero, why does a charged conductor have a nonzero potential?

Field and potential answer different questions. The field tells you the local force per unit charge at a point right now; the potential tells you the total work already done getting a charge to that point from infinity, and that journey started out in a nonzero field far away. Once your test charge reaches the conductor's surface and enters the interior, the field genuinely does drop to zero, so no further work is needed to move it around inside — but the work already banked on the way in from infinity is not erased. That is exactly why the interior potential equals the surface potential: it is constant throughout because zero additional work is needed inside, not because the potential itself is zero.

Why does inserting a dielectric increase capacitance instead of decreasing it, since it seems to be "getting in the way"?

The dielectric does not block anything — it responds to the field by developing its own induced (bound) surface charge, and that induced charge's field partially opposes the original field from the plates. For the same free charge QQ on the plates, this reduces the net field, and hence the potential difference VV, inside the gap. Since capacitance is C=Q/VC=Q/V, a smaller VV for the same QQ directly means a larger CC. Put differently: with a dielectric present, you can pack the same amount of charge onto the plates while only needing a smaller voltage to do it, which is the practical definition of "more capacitance."

When two capacitors are connected and share charge, energy is lost even though charge is conserved. Doesn't that violate conservation of energy?

No — energy is still exactly conserved overall, but not all of it stays as stored electrostatic energy. Charge has nowhere else to go, so QtotalQ_{\text{total}} before equals QtotalQ_{\text{total}} after. Energy, however, is free to change form: while the potentials equalise, a transient current flows through the connecting wires and meets resistance, dissipating the lost electrostatic energy as heat (and briefly as radiation). It has not vanished, only changed form, exactly as conservation of energy demands.

Why does the potential due to a dipole fall off as one over r squared, while a single point charge falls off as one over r?

Because a dipole is really two nearly-cancelling charges, +q+q and −q-q, seen from far away. If you replaced the dipole with a single charge of magnitude qq, its potential would indeed fall as 1/r1/r. But the dipole's negative charge almost, though not quite, cancels the positive charge's contribution at every distant point — the two potentials differ only because r1r_1 and r2r_2 (the distances from +q+q and −q-q to the field point) are slightly different, by an amount of order a/ra/r. That extra factor of a/ra/r from the near-cancellation is what converts the underlying 1/r1/r falloff into an effective 1/r21/r^2 falloff for the dipole as a whole — one power of rr steeper, precisely because of the cancellation.

Is there a simple way to remember when to use series versus parallel formulas for capacitors, without mixing them up with resistors?

Yes — focus on what stays the same in each configuration rather than memorising the formula shape. In series, the capacitors are chained end to end, so the same charge QQ flows onto every one (nowhere else for it to accumulate) while the total voltage splits — this forces the reciprocal-sum rule, 1/C=∑1/Ci1/C=\sum 1/C_i. In parallel, every capacitor shares the identical voltage VV while the total charge splits among them — giving the direct-sum rule, C=∑CiC=\sum C_i. Fix "series shares charge, parallel shares voltage" in your head and the algebra rebuilds the formula from C=Q/VC=Q/V whenever you forget it.

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