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CLASS 12 · CHAPTER 2 · ELECTROSTATICS

DETAILED NOTES

Electrostatic Potential & Capacitance

The complete chapter, section by section: electrostatic potential, the potential of an electric dipole, equipotential surfaces, the relationship between field and potential, conductors and the Van de Graaff generator, capacitors and capacitance (including an isolated sphere), the parallel-plate derivation, dielectrics, combinations, and stored energy along with the energy density of the electric field, explained in plain language with original worked examples. For the interactive battery-connected-vs-disconnected capacitor simulation, see the concept page.

2.1 Electrostatic Potential

Just as a mass raised against gravity stores potential energy, moving a charge against an electric field stores electrostatic potential energy. The potential at a point is this stored energy per unit charge, the work needed to bring a tiny positive test charge from infinity (where potential is conventionally zero) to that point, without speeding it up:

V(r)=W∞→rq0V(r) = \dfrac{W_{\infty \to r}}{q_0}

For a single point charge QQ, carrying out this integral of the Coulomb field gives a strikingly simple result:

Potential of a point charge
V(r)=14πε0Qr=kQr\textcolor{#e08a1e}{V(r)} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{r} = \dfrac{kQ}{r}

Unlike the electric field, potential is a scalar, so the potential due to several charges is just an ordinary sum, no vector addition required:

V=∑ikqiriV = \sum_i \dfrac{kq_i}{r_i}

2.2 Potential Due to an Electric Dipole

That sum is all it takes to find the potential of an electric dipole: charges +q+q and −q-q a small distance 2a2a apart, with dipole moment of magnitude p=q×2ap = q\times2a, pointing from −q-q to +q+q. The Electric Charges and Fields notes found the dipole’s field on its axial and equatorial lines by adding two vectors. Here the job is easier: potential is a scalar, so the two contributions just add as ordinary numbers, with signs.

Put the origin O at the centre of the dipole, and pick any point P a distance rr from O, with θ\theta the angle between OP and p⃗\vec{p}. Let r1r_1 be P’s distance from +q+q, and r2r_2 its distance from −q-q. Then, from the sum above:

V=kqr1+k(−q)r2=kq(1r1−1r2)V = \dfrac{kq}{r_1} + \dfrac{k(-q)}{r_2} = kq\left(\dfrac{1}{r_1}-\dfrac{1}{r_2}\right)

2.2.1 At a general point

The charge +q+q sits a distance aa from O along p⃗\vec{p}, and −q-q sits a distance aa from O the opposite way. Apply the cosine rule to the triangle each charge makes with O and P. The angle at O is θ\theta for +q+q’s triangle and 180∘−θ180^\circ-\theta for −q-q’s, and cos⁡(180∘−θ)=−cos⁡θ\cos(180^\circ-\theta) = -\cos\theta, so:

r12=r2+a2−2arcos⁡θ,r22=r2+a2+2arcos⁡θr_1^2 = r^2 + a^2 - 2ar\cos\theta, \qquad r_2^2 = r^2 + a^2 + 2ar\cos\theta

A real dipole is tiny compared with the distances we care about, so take r≫ar \gg a. Then a2a^2 is negligible next to the other terms, and keeping only terms of first order in a/ra/r:

r12≈r2(1−2acos⁡θr),r22≈r2(1+2acos⁡θr)r_1^2 \approx r^2\left(1 - \dfrac{2a\cos\theta}{r}\right), \qquad r_2^2 \approx r^2\left(1 + \dfrac{2a\cos\theta}{r}\right)

We need 1/r11/r_1 and 1/r21/r_2, so raise each to the power −12-\tfrac{1}{2} and use the binomial approximation (1+x)n≈1+nx(1+x)^n \approx 1+nx for small xx, here with n=−12n=-\tfrac{1}{2}:

1r1=1r(1−2acos⁡θr)−1/2≈1r(1+acos⁡θr)\dfrac{1}{r_1} = \dfrac{1}{r}\left(1 - \dfrac{2a\cos\theta}{r}\right)^{-1/2} \approx \dfrac{1}{r}\left(1 + \dfrac{a\cos\theta}{r}\right)1r2=1r(1+2acos⁡θr)−1/2≈1r(1−acos⁡θr)\dfrac{1}{r_2} = \dfrac{1}{r}\left(1 + \dfrac{2a\cos\theta}{r}\right)^{-1/2} \approx \dfrac{1}{r}\left(1 - \dfrac{a\cos\theta}{r}\right)

Subtract them. The leading 1/r1/r terms cancel, and only the small correction terms survive:

1r1−1r2≈2acos⁡θr2\dfrac{1}{r_1} - \dfrac{1}{r_2} \approx \dfrac{2a\cos\theta}{r^2}

Multiply by kqkq and recognise q×2a=pq\times2a = p:

V≈kq⋅2acos⁡θr2=k(2aq)cos⁡θr2=kpcos⁡θr2V \approx kq\cdot\dfrac{2a\cos\theta}{r^2} = \dfrac{k(2aq)\cos\theta}{r^2} = \dfrac{kp\cos\theta}{r^2}
Potential of a dipole (r ≫ a)
V=14πε0pcos⁡θr2=k p⃗⋅r^r2\textcolor{#e08a1e}{V} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p\cos\theta}{r^2} = \dfrac{k\,\vec{p}\cdot\hat{r}}{r^2}

Two things set this apart from a single charge’s potential. It depends on direction, through cos⁡θ\cos\theta, not just on distance. And it falls off as 1/r21/r^2, a full power of rr faster than kQ/rkQ/r, for the same reason the dipole’s field falls off as 1/r31/r^3 instead of 1/r21/r^2: seen from far away, +q+q and −q-q are almost on top of each other, and their contributions very nearly cancel. The approximation gets better the farther away P is, and for an ideal point dipole (2a2a shrinking to zero while pp stays fixed) the terms we dropped vanish completely and the formula is exact.

2.2.2 On the axial line

On the axis, beyond +q+q, θ=0\theta=0 and cos⁡θ=1\cos\theta=1, so the general formula gives V=kp/r2V=kp/r^2. On the axis, though, we don’t need the approximation at all, just as with the axial field in the previous chapter: P is exactly r−ar-a from +q+q and r+ar+a from −q-q, so:

Vaxial=kq[1r−a−1r+a]=kq⋅(r+a)−(r−a)(r−a)(r+a)=kq⋅2ar2−a2V_{\text{axial}} = kq\left[\dfrac{1}{r-a}-\dfrac{1}{r+a}\right] = kq\cdot\dfrac{(r+a)-(r-a)}{(r-a)(r+a)} = kq\cdot\dfrac{2a}{r^2-a^2}

Writing q×2a=pq\times2a = p:

Vaxial=kpr2−a2  → r≫a   kpr2V_{\text{axial}} = \dfrac{kp}{r^2-a^2}\;\xrightarrow{\,r\gg a\,}\;\dfrac{kp}{r^2}

which agrees with the general formula at θ=0\theta=0. On the other side, beyond −q-q (θ=180∘\theta=180^\circ, cos⁡θ=−1\cos\theta=-1), the nearer charge is now −q-q, so the potential has the same size but is negative: −kp/(r2−a2)-kp/(r^2-a^2). There’s also a neat consistency check waiting in §2.4, which shows that the field is minus the rate of change of potential, E=−dV/drE=-dV/dr. Applying that to the exact axial potential:

Eaxial=−ddr[kpr2−a2]=−kp⋅−2r(r2−a2)2=2kpr(r2−a2)2E_{\text{axial}} = -\dfrac{d}{dr}\left[\dfrac{kp}{r^2-a^2}\right] = -kp\cdot\dfrac{-2r}{(r^2-a^2)^2} = \dfrac{2kpr}{(r^2-a^2)^2}

exactly the axial field the previous chapter found by adding vectors, now recovered from a scalar in one line.

2.2.3 On the equatorial line

On the equatorial line (the perpendicular bisector of the dipole), θ=90∘\theta=90^\circ and cos⁡θ=0\cos\theta=0, so the general formula predicts zero. Once again this is exact, not an approximation: every point on the equatorial line is equally far from both charges, r1=r2=r2+a2r_1 = r_2 = \sqrt{r^2+a^2}, so:

Vequatorial=kq(1r2+a2−1r2+a2)V_{\text{equatorial}} = kq\left(\dfrac{1}{\sqrt{r^2+a^2}}-\dfrac{1}{\sqrt{r^2+a^2}}\right)
Vequatorial=0\textcolor{#e08a1e}{V_{\text{equatorial}}} = 0

at every distance, near or far. This is a good place to see that zero potential does not mean zero field: the previous chapter found a field of kp/(r2+a2)3/2kp/(r^2+a^2)^{3/2} at these very points. There’s no contradiction. The whole equatorial plane is an equipotential surface (V=0V=0 everywhere on it), so by §2.3 the field must cross it at right angles, and it does: the equatorial field points opposite to p⃗\vec{p}, straight through the plane. Bringing a test charge in from infinity along the equatorial line takes zero work, because the field is perpendicular to the path at every step.

Worked example

Potential around a small dipole, in three directions

Charges of ±5.0\pm5.0 nC sit 2.0 mm apart. Find the potential at a point 10 cm from the centre of the dipole (a) in a direction at 60∘60^\circ to p⃗\vec{p}, (b) on the axis, beyond the positive charge, (c) on the equatorial line.

First the dipole moment, with 2a=2.0×10−32a = 2.0\times10^{-3} m:

p=q×2a=(5.0×10−9)(2.0×10−3)=1.0×10−11 C mp = q\times2a = (5.0\times10^{-9})(2.0\times10^{-3}) = 1.0\times10^{-11}\text{ C m}

Here r/a=100r/a = 100, comfortably in the r≫ar\gg a regime:

(a) V=kpcos⁡θr2=(8.99×109)(1.0×10−11)cos⁡60∘(0.10)2=4.50 V\text{(a)}\ V = \dfrac{kp\cos\theta}{r^2} = \dfrac{(8.99\times10^9)(1.0\times10^{-11})\cos60^\circ}{(0.10)^2} = \textcolor{#e08a1e}{4.50\text{ V}}(b) V=kpr2−a2=(8.99×109)(1.0×10−11)(0.10)2−(0.001)2=8.99 V\text{(b)}\ V = \dfrac{kp}{r^2-a^2} = \dfrac{(8.99\times10^9)(1.0\times10^{-11})}{(0.10)^2-(0.001)^2} = \textcolor{#e08a1e}{8.99\text{ V}}(c) V=0\text{(c)}\ V = \textcolor{#e08a1e}{0}

In (b), the exact formula and the kp/r2kp/r^2 approximation agree to three significant figures, since a2a^2 is only one ten-thousandth of r2r^2. For contrast, the +5.0 nC charge on its own would give kq/r=449.5kq/r = 449.5 V at the same distance, 50 times the axial value: that factor is r/(2a)=0.10/0.002r/(2a) = 0.10/0.002, a direct measure of how thoroughly the two charges cancel each other from 10 cm away.

2.3 Equipotential Surfaces

An equipotential surface is any surface on which every point has the same potential. For a single point charge, these are concentric spheres centred on the charge. Two properties worth holding onto:

  • No work is done moving a charge along an equipotential surface, since W=qΔVW = q\Delta V and ΔV=0\Delta V = 0 there.
  • The electric field is always perpendicular to an equipotential surface at every point. If it had any component along the surface, moving charge along that direction would require zero work against a nonzero force component, a contradiction.

2.4 Relation Between Field and Potential

Field and potential are two descriptions of the same underlying reality, one a vector, one a scalar, and they’re linked by a derivative. Moving a tiny distance drdr against the field changes the potential by dV=−E drdV = -E\,dr, so:

Field from potential
E=−dVdr\textcolor{#e08a1e}{E} = -\dfrac{dV}{dr}

The minus sign matters: the field always points in the direction of decreasing potential, “downhill”, the fastest. A large field doesn’t require a large potential; it requires potential to be changing rapidly with position. A region of uniformly high potential with no variation at all has zero field inside it.

Worked example

Field between two charged plates, from potential alone

Two large parallel plates are held at 0 V and 200 V, 4 mm apart. Find the field between them.

E=ΔVd=2000.004=50,000 V/mE = \dfrac{\Delta V}{d} = \dfrac{200}{0.004} = \textcolor{#e08a1e}{50{,}000\text{ V/m}}

A uniform field between parallel plates is exactly E=V/dE = V/d, the straight-line version of E=−dV/drE=-dV/dr since the potential changes at a constant rate across the gap.

2.5 Electrostatic Potential Energy

The potential energy of a pair of charges is the work done to assemble them, bringing the second charge in from infinity against the first charge’s field:

U=kq1q2r12U = \dfrac{kq_1q_2}{r_{12}}

For an electric dipole (moment pp) sitting in an external uniform field EE at angle θ\theta to it, the potential energy is:

U(θ)=−pEcos⁡θ=−p⃗⋅E⃗U(\theta) = -pE\cos\theta = -\vec{p}\cdot\vec{E}

which is minimum (most stable) when the dipole aligns with the field, and maximum when it points directly against it, exactly the torque τ=pEsin⁡θ\tau = pE\sin\theta trying to rotate it toward.

2.6 Conductors in Electrostatic Equilibrium

Inside a conductor in electrostatic equilibrium, the field is always exactly zero (free charges would otherwise keep moving until it is). Three consequences follow immediately:

  • The entire conductor, surface included, is one equipotential.
  • Any net charge resides entirely on the outer surface, never in the bulk.
  • Just outside the surface, the field is perpendicular to it, with magnitude E=σ/ε0E = \sigma/\varepsilon_0.

2.6.1 The Van de Graaff generator

The second consequence above, that a conductor’s net charge always ends up on its outer surface, is the whole working principle of the Van de Graaff generator, a machine that builds up potentials of around a million volts. What makes it work is a stronger version of that statement: charge placed inside a hollow conductor moves to the outer surface even when that outer surface is already at an enormous potential. To see why, we first need the potential of a charged spherical shell.

Take a thin spherical shell of radius RR carrying charge QQ spread uniformly over it, and let xx be the distance from its centre. By symmetry the field can only point radially, with the same magnitude at every point a given distance from the centre, so apply Gauss’s law (previous chapter) to an imaginary concentric sphere of radius xx. Outside the shell (x>Rx>R) that sphere encloses all of QQ; inside (x<Rx<R) it encloses nothing:

E(4πx2)=Qε0  ⇒  E=kQx2  (x>R),E(4πx2)=0  ⇒  E=0  (x<R)E(4\pi x^2) = \dfrac{Q}{\varepsilon_0} \;\Rightarrow\; E = \dfrac{kQ}{x^2}\ \ (x>R), \qquad E(4\pi x^2) = 0 \;\Rightarrow\; E = 0\ \ (x<R)

Outside, then, the field is exactly that of a point charge QQ at the centre, so bringing a test charge in from infinity to any x≥Rx \ge R takes the same work as for a point charge, and the potential there is kQ/xkQ/x, reaching kQ/RkQ/R at the surface. Inside, the field is zero, so moving the test charge around costs no further work at all: the potential stays at its surface value everywhere in the interior.

Potential of a charged spherical shell
V=kQx(x≥R),V=kQR(x≤R)V = \dfrac{kQ}{x}\quad (x \ge R), \qquad V = \dfrac{kQ}{R}\quad (x \le R)

Now place a small conducting sphere of radius rr, carrying charge qq, at the centre of a large hollow conducting shell of radius RR, carrying charge QQ. The small sphere’s charge also sits on its surface, so it is a charged shell too, and the formula above applies to both. Potential is a scalar, so each conductor’s potential is just the sum of what the two charges contribute there. The outer shell (at distance RR from the centre) gets kQ/RkQ/R from its own charge, plus kq/Rkq/R from the small sphere, since it lies outside the small sphere:

VR=kQR+kqRV_R = \dfrac{kQ}{R} + \dfrac{kq}{R}

The small sphere (at distance rr) gets kq/rkq/r from its own charge, plus kQ/RkQ/R from the outer shell, since it sits inside the shell, where the shell’s potential is the same everywhere:

Vr=kqr+kQRV_r = \dfrac{kq}{r} + \dfrac{kQ}{R}

Subtract, inner minus outer:

Vr−VR=(kqr+kQR)−(kQR+kqR)=kqr−kqRV_r - V_R = \left(\dfrac{kq}{r} + \dfrac{kQ}{R}\right) - \left(\dfrac{kQ}{R} + \dfrac{kq}{R}\right) = \dfrac{kq}{r} - \dfrac{kq}{R}
Inner sphere minus outer shell
Vr−VR=kq(1r−1R)\textcolor{#e08a1e}{V_r - V_R} = kq\left(\dfrac{1}{r}-\dfrac{1}{R}\right)

Look at what’s missing: QQ. The outer shell’s own charge raises both potentials by exactly the same amount, kQ/RkQ/R, so it cancels out of the difference. And since r<Rr<R, the bracket is always positive. So as long as the inner sphere holds any positive charge at all, it sits at a higher potential than the outer shell, however much charge the shell already carries. Join the two with a wire and positive charge flows from the inner sphere to the shell, downhill in potential, and keeps flowing until the difference is zero, which by the formula happens only when q=0q=0. Every bit of the inner charge ends up on the outer shell.

A Van de Graaff generator is built around exactly this arrangement. A large hollow metal sphere, the dome, sits on top of a tall insulating column. An insulating belt, driven by a motor, loops over two pulleys, one at the base and one inside the dome. Near the bottom pulley, a comb of sharp metal points connected to a high-voltage supply sprays positive charge onto the belt (sharp points concentrate the field enough to ionise the air right next to them, which is what lets charge leap across). The belt carries this charge up into the dome, where a second comb, connected to the dome, collects it. Because that hand-off happens inside the dome, the collected charge plays the role of qq above: it moves straight to the outer surface, however high the dome’s potential has already climbed. The belt keeps delivering charge, and the dome’s potential, kQ/RkQ/R by the shell formula, keeps rising as QQ grows.

The energy isn’t free, of course. Outside the dome, the positive charge on the belt is repelled by the dome’s positive charge, so the motor has to do work hauling each bit of charge upward against that repulsion, and that work is what ends up stored as electrostatic potential energy. Only inside the dome, where the dome’s own field vanishes, does the final hand-off cost nothing.

What finally stops the potential rising is the air around the dome. At the surface of a charged sphere the field is the point-charge field at x=Rx=R, E=kQ/R2E = kQ/R^2, while the potential is V=kQ/RV = kQ/R, so the two are tied together:

VE=kQ/RkQ/R2=R⇒V=ER\dfrac{V}{E} = \dfrac{kQ/R}{kQ/R^2} = R \quad\Rightarrow\quad V = ER

Air stops insulating once the field reaches its dielectric strength, about 3×1063\times10^6 V/m, and the dome then leaks charge away through sparks. So the highest potential a dome can hold is Vmax⁡=Emax⁡RV_{\max} = E_{\max}R, which grows with the radius: that is why Van de Graaff generators are built with large, smoothly rounded domes, with no sharp edges for breakdown to start from. The million-volt potentials they reach are used to accelerate charged particles, such as protons, to the high energies needed for experiments in nuclear physics.

Worked example

Charge always flows outward, whatever the dome already holds

A small metal sphere of radius 4.0 cm carrying +3.0 nC sits at the centre of a hollow metal dome of radius 40 cm that already carries +2.0 µC. (a) Find the potential of each and the difference between them. (b) What is the highest potential this dome can reach before the surrounding air breaks down, taking Emax⁡=3.0×106E_{\max} = 3.0\times10^6 V/m?

(a) The three separate contributions first:

kQR=(8.99×109)(2.0×10−6)0.40=44,950 V,kqR=(8.99×109)(3.0×10−9)0.40=67.4 V\dfrac{kQ}{R} = \dfrac{(8.99\times10^9)(2.0\times10^{-6})}{0.40} = 44{,}950\text{ V}, \qquad \dfrac{kq}{R} = \dfrac{(8.99\times10^9)(3.0\times10^{-9})}{0.40} = 67.4\text{ V}kqr=(8.99×109)(3.0×10−9)0.040=674 V\dfrac{kq}{r} = \dfrac{(8.99\times10^9)(3.0\times10^{-9})}{0.040} = 674\text{ V}VR=44,950+67.4≈4.502×104 V,Vr=674+44,950≈4.562×104 VV_R = 44{,}950 + 67.4 \approx \textcolor{#e08a1e}{4.502\times10^4\text{ V}}, \qquad V_r = 674 + 44{,}950 \approx \textcolor{#e08a1e}{4.562\times10^4\text{ V}}Vr−VR=kq(1r−1R)=(8.99×109)(3.0×10−9)(10.040−10.40)≈607 VV_r - V_R = kq\left(\dfrac{1}{r}-\dfrac{1}{R}\right) = (8.99\times10^9)(3.0\times10^{-9})\left(\dfrac{1}{0.040}-\dfrac{1}{0.40}\right) \approx \textcolor{#e08a1e}{607\text{ V}}

Doubling the dome’s charge to 4.0 µC would add another 44,950 V to both potentials, and leave the 607 V gap untouched: the inner charge would still flow outward.

(b) Vmax⁡=Emax⁡R=(3.0×106)(0.40)=1.20×106 V\text{(b)}\ V_{\max} = E_{\max}R = (3.0\times10^6)(0.40) = \textcolor{#e08a1e}{1.20\times10^6\text{ V}}

The dome is at about 45 kV now, so the belt could keep feeding it until roughly 1.2 MV, nearly 27 times higher, before sparks start bleeding the charge away.

2.7 Capacitors and Capacitance

A capacitor is any pair of conductors that can store equal and opposite charges, separated by an insulator. Experimentally, the charge stored is always directly proportional to the potential difference applied, and the constant of proportionality, which depends only on the geometry, is called the capacitance:

Capacitance
C=QV\textcolor{#e08a1e}{C} = \dfrac{Q}{V}

with SI unit the farad (F), 1 F = 1 C/V, an enormous unit in practice, real capacitors are usually rated in microfarads (µF) or picofarads (pF).

2.7.1 Capacitance of an isolated spherical conductor

A capacitor doesn’t strictly need two conductors side by side. A single isolated conductor can store charge too, and it still has a capacitance: treat the “second plate” as being at infinity, where the potential is zero, so the potential difference VV in C=Q/VC=Q/V is just the conductor’s own potential.

Take a conducting sphere of radius RR carrying charge QQ. All of that charge sits on its outer surface (§2.6), spread uniformly by symmetry, so it is exactly the charged shell of §2.6.1, and the whole sphere, surface and interior alike, sits at the shell’s surface potential. (A solid sphere and a hollow one behave identically for the same reason: the charge is on the surface either way.)

V=14πε0QRV = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{R}

Substitute this into C=Q/VC = Q/V:

C=QV=Q  Q/(4πε0R)  =Q×4πε0RQC = \dfrac{Q}{V} = \dfrac{Q}{\;Q/(4\pi\varepsilon_0 R)\;} = Q\times\dfrac{4\pi\varepsilon_0 R}{Q}
Capacitance of an isolated sphere
C=4πε0R\textcolor{#e08a1e}{C} = 4\pi\varepsilon_0 R

The charge QQ cancels, just as §2.7 promised: capacitance depends only on geometry, and here the geometry is a single length, the radius. A sphere twice as large holds twice the charge at the same potential, so it has twice the capacitance.

Worked example

A metal sphere as a capacitor, and how big a farad really is

A metal sphere of radius 15 cm stands on an insulating support. Find (a) its capacitance, and (b) the charge it holds when it is charged to a potential of 30 kV.

(a) C=4πε0R=4π(8.85×10−12)(0.15)≈1.67×10−11 F=16.7 pF\text{(a)}\ C = 4\pi\varepsilon_0 R = 4\pi(8.85\times10^{-12})(0.15) \approx 1.67\times10^{-11}\text{ F} = \textcolor{#e08a1e}{16.7\text{ pF}}(b) Q=CV=(1.668×10−11)(3.0×104)≈5.00×10−7 C\text{(b)}\ Q = CV = (1.668\times10^{-11})(3.0\times10^{4}) \approx \textcolor{#e08a1e}{5.00\times10^{-7}\text{ C}}

Only about half a microcoulomb, even at 30 kV. To get a feel for the farad, try the whole Earth as the sphere (R=6.4×106R = 6.4\times10^6 m): C=4π(8.85×10−12)(6.4×106)≈7.12×10−4C = 4\pi(8.85\times10^{-12})(6.4\times10^6) \approx 7.12\times10^{-4} F, about 712 µF. A planet-sized conductor still falls well short of a single farad.

2.8 The Parallel-Plate Capacitor

For two large plates of area AA, separated by a small gap dd, carrying charges +Q+Q and −Q-Q, Gauss’s law gives a uniform field between them, E=σ/ε0=Q/(ε0A)E = \sigma/\varepsilon_0 = Q/(\varepsilon_0 A). Integrating V=EdV = Ed across the gap and substituting into C=Q/VC=Q/V:

Parallel-plate capacitance
C=ε0AdC = \dfrac{\varepsilon_0 A}{d}

Capacitance depends only on the plates’ area and separation, never on how much charge happens to be on them, exactly the same way a cup’s volume doesn’t depend on how much water is currently in it.

2.8.1 The connected-vs-disconnected distinction

What happens when dd changes depends entirely on whether a battery is still attached:

  • Battery connected: VV is held fixed by the battery. As dd grows, CC falls, so Q=CVQ=CV falls too (charge flows back through the battery), and with it E=V/dE=V/d and the stored energy.
  • Battery disconnected: QQ is trapped, fixed. Since E=Q/(ε0A)E=Q/(\varepsilon_0 A) depends only on the charge density, the field cannot change as dd grows. But V=EdV=Ed with EE fixed and dd growing means VV climbs in direct proportion. The concept page’s simulation shows exactly this, see the interactive capacitor for the live version.

2.9 Dielectrics

Filling the gap between the plates with an insulating material (a dielectric) always increases capacitance, by a factor called the dielectric constant KK (also written εr\varepsilon_r):

Cdielectric=Kε0Ad=KCvacuumC_{dielectric} = K\varepsilon_0\dfrac{A}{d} = KC_{vacuum}

The mechanism: the external field polarises the dielectric’s molecules, producing an induced field that opposes and partially cancels the original field inside the material, so a given charge now produces a smaller net field, and therefore a smaller voltage for the same charge, which by C=Q/VC=Q/V means a larger CC.

2.10 Combinations of Capacitors

2.10.1 Series

Same charge QQ sits on every capacitor in the chain; voltages add:

1Cseries=1C1+1C2+⋯\dfrac{1}{C_{series}} = \dfrac{1}{C_1}+\dfrac{1}{C_2}+\cdots

always smaller than the smallest individual capacitance, the same combination rule as resistors in parallel.

2.10.2 Parallel

Same voltage VV across every capacitor; charges add:

Cparallel=C1+C2+⋯C_{parallel} = C_1+C_2+\cdots

always larger than the largest individual capacitance, more plate area effectively available to store charge.

Worked example

Two capacitors, both ways

A 2 µF and a 3 µF capacitor are combined (a) in series, (b) in parallel. Find the equivalent capacitance each way.

(a) 1Cs=12+13=56  ⇒  Cs=1.2 μF\text{(a)}\ \dfrac{1}{C_s} = \dfrac{1}{2}+\dfrac{1}{3} = \dfrac{5}{6} \;\Rightarrow\; C_s = \textcolor{#e08a1e}{1.2\ \mu\text{F}}(b) Cp=2+3=5 μF\text{(b)}\ C_p = 2+3 = \textcolor{#e08a1e}{5\ \mu\text{F}}

Series always lands below the smaller value (1.2 < 2); parallel always lands above the larger value (5 > 3).

2.11 Energy Stored in a Capacitor

Charging a capacitor means pushing charge onto a plate against an opposing voltage that itself grows as charge builds up, so the energy isn’t simply QVQV, it’s the area under the Q-V graph, a triangle, giving a factor of 12\tfrac{1}{2}:

Energy stored
U=12QV=12CV2=Q22CU = \dfrac{1}{2}QV = \dfrac{1}{2}CV^2 = \dfrac{Q^2}{2C}

Worked example

Energy in a charged capacitor

A 10 µF capacitor is charged to 200 V. Find the energy stored.

U=12CV2=12(10×10−6)(200)2=0.2 JU = \dfrac{1}{2}CV^2 = \dfrac{1}{2}(10\times10^{-6})(200)^2 = \textcolor{#e08a1e}{0.2\text{ J}}

2.11.1 Energy density of the electric field

Where, physically, is that energy? A powerful way to answer is to say it is stored in the electric field itself, in the space between the plates where the field exists. To see why that picture works, take a parallel-plate capacitor (plate area AA, gap dd) and rewrite its stored energy entirely in terms of the field EE between the plates. Start from

U=12CV2U = \dfrac{1}{2}CV^2

and substitute the two parallel-plate results from §2.8, the capacitance C=ε0A/dC = \varepsilon_0 A/d and the uniform-field relation V=EdV = Ed:

U=12(ε0Ad)(Ed)2=12⋅ε0Ad⋅E2d2=12ε0E2 (Ad)U = \dfrac{1}{2}\left(\dfrac{\varepsilon_0 A}{d}\right)(Ed)^2 = \dfrac{1}{2}\cdot\dfrac{\varepsilon_0 A}{d}\cdot E^2d^2 = \dfrac{1}{2}\varepsilon_0E^2\,(Ad)

One factor of dd cancels, and what is left multiplying 12ε0E2\tfrac{1}{2}\varepsilon_0E^2 is AdAd, the volume of the region between the plates, which is precisely the region where the field lives (outside an ideal parallel-plate capacitor the field is zero). Divide the energy by that volume to get the energy per unit volume, the energy density uu:

u=UAd=12ε0E2 (Ad)Adu = \dfrac{U}{Ad} = \dfrac{\tfrac{1}{2}\varepsilon_0E^2\,(Ad)}{Ad}
Energy density of the electric field
u=12ε0E2\textcolor{#e08a1e}{u} = \dfrac{1}{2}\varepsilon_0E^2

measured in J/m³ (a quick check: ε0E2\varepsilon_0E^2 has units C2N−1m−2×N2C−2=N/m2=J/m3\text{C}^2\text{N}^{-1}\text{m}^{-2}\times\text{N}^2\text{C}^{-2} = \text{N/m}^2 = \text{J/m}^3). The plate area and the gap have cancelled out completely: the result depends only on the field strength at that spot. That is what makes it more than a fact about capacitors. Any electric field, however non-uniform, can be chopped into boxes small enough that the field across each one is effectively uniform, with two opposite faces lying along equipotential surfaces, and each such box behaves like a miniature parallel-plate capacitor holding 12ε0E2\tfrac{1}{2}\varepsilon_0E^2 of energy per unit volume. So wherever there is an electric field, between capacitor plates, around a charged sphere, or in empty space, energy is stored at a density of 12ε0E2\tfrac{1}{2}\varepsilon_0E^2.

Worked example

Two routes to the same stored energy

A parallel-plate capacitor has plates of area 200 cm² separated by 1.5 mm of air, and is connected to a 300 V supply. Find the field between the plates and the energy density there, use it to get the total stored energy, and check the answer against 12CV2\tfrac{1}{2}CV^2.

Field and energy density, with A=0.020A = 0.020 m² and d=1.5×10−3d = 1.5\times10^{-3} m:

E=Vd=3001.5×10−3=2.0×105 V/mE = \dfrac{V}{d} = \dfrac{300}{1.5\times10^{-3}} = 2.0\times10^5\text{ V/m}u=12ε0E2=12(8.85×10−12)(2.0×105)2=0.177 J/m3u = \dfrac{1}{2}\varepsilon_0E^2 = \dfrac{1}{2}(8.85\times10^{-12})(2.0\times10^5)^2 = \textcolor{#e08a1e}{0.177\text{ J/m}^3}

Multiply by the volume between the plates:

U=u (Ad)=(0.177)(0.020×1.5×10−3)=(0.177)(3.0×10−5)=5.31×10−6 JU = u\,(Ad) = (0.177)(0.020\times1.5\times10^{-3}) = (0.177)(3.0\times10^{-5}) = \textcolor{#e08a1e}{5.31\times10^{-6}\text{ J}}

Now the capacitor route:

C=ε0Ad=(8.85×10−12)(0.020)1.5×10−3=1.18×10−10 FC = \dfrac{\varepsilon_0 A}{d} = \dfrac{(8.85\times10^{-12})(0.020)}{1.5\times10^{-3}} = 1.18\times10^{-10}\text{ F}U=12CV2=12(1.18×10−10)(300)2=5.31×10−6 JU = \dfrac{1}{2}CV^2 = \dfrac{1}{2}(1.18\times10^{-10})(300)^2 = \textcolor{#e08a1e}{5.31\times10^{-6}\text{ J}}

The same answer both ways, as it has to be: they are the same calculation, just bookkept differently, once as “energy on the capacitor” and once as “energy in the field”.

— From the NCERT exercises

A classic exercise question from the chapter, with an original worked solution.

NCERT Exercise 2.11

A 600 pF capacitor is charged by a 200 V supply. It is then disconnected from the supply and connected to another uncharged 600 pF capacitor. How much electrostatic energy is lost in the process?

Solution

Initial charge and energy, on the first capacitor alone:

Q0=CV0=(600×10−12)(200)=1.2×10−7 CQ_0 = C V_0 = (600\times10^{-12})(200) = 1.2\times10^{-7}\text{ C}Ui=12CV02=12(600×10−12)(200)2=1.2×10−5 JU_i = \dfrac{1}{2}C V_0^2 = \dfrac{1}{2}(600\times10^{-12})(200)^2 = 1.2\times10^{-5}\text{ J}

Connecting an identical uncharged capacitor shares the same total charge equally (both have equal CC), so each ends up at half the original voltage, 100 V, across double the capacitance:

Uf=12(2C)(100)2=12(1200×10−12)(100)2=6×10−6 JU_f = \dfrac{1}{2}(2C)(100)^2 = \dfrac{1}{2}(1200\times10^{-12})(100)^2 = 6\times10^{-6}\text{ J}ΔU=Ui−Uf=1.2×10−5−0.6×10−5=6×10−6 J lost\Delta U = U_i - U_f = 1.2\times10^{-5} - 0.6\times10^{-5} = \textcolor{#e08a1e}{6\times10^{-6}\text{ J lost}}

This energy doesn’t vanish, it’s dissipated as heat and a brief spark in the connecting wires, which have some resistance even though it’s never mentioned in the problem.

Want the interactive version instead? Try the capacitor simulation → or take a practice paper →
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