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Capacitors and Dielectrics

A conductor at electrostatic equilibrium is an equipotential surface. If you put charge QQ on a fixed isolated conductor, its potential relative to infinity is proportional to QQ, because electrostatics is linear. Thus we can define a value of capacitance:

C=ΔQΔV.C=\frac{\Delta Q}{\Delta V}.

Capacitance measures how much charge a geometry can store per volt. It depends only on the geometry and the material between conductors, not on the particular value of QQ or ΔV\Delta V. The sign convention is usually: QQ means the positive charge on one conductor and ΔV\Delta V means the potential of that positive conductor minus the other conductor, so C>0C>0.

For a single isolated conducting sphere of radius RR,

V=kQR⟹C=4πε0R.V=\frac{kQ}{R} \qquad\Longrightarrow\qquad C=4\pi\varepsilon_0R.

Most devices use two conductors carrying equal and opposite charges +Q+Q and −Q-Q. The electric field is mostly trapped between them, which makes the stored energy useful and controllable.

For two large parallel conducting plates of area AA separated by distance dd (ignoring edge fringing), the field between the two plates is approximately uniform:

E=σε0=Qε0A.E=\frac{\sigma}{\varepsilon_0}=\frac{Q}{\varepsilon_0 A}.

The potential difference is therefore

ΔV=Ed=Qdε0A,\Delta V=Ed=\frac{Qd}{\varepsilon_0 A},

so the capacitance is

C=QΔV=ε0Ad.C=\frac{Q}{\Delta V}=\frac{\varepsilon_0 A}{d}.

Near the edges, the field bulges outward, so the capacitance is slightly larger than ε0A/d\varepsilon_0A/d, but this is usually ignored.

Example. A parallel-plate capacitor has plate area A=2.0×10−3 m2A=2.0\times10^{-3}\ \text{m}^2 and separation d=1.0 mmd=1.0\ \text{mm}. It is connected to a 12 V12\ \text{V} battery. Find the capacitance, stored charge, and electric field between the plates.

The capacitance is

C=ε0Ad=(8.85×10−12)(2.0×10−3)1.0×10−3=1.77×10−11 F.C=\frac{\varepsilon_0A}{d} =\frac{(8.85\times10^{-12})(2.0\times10^{-3})}{1.0\times10^{-3}} =1.77\times10^{-11}\ \text{F}.

The charge is

Q=CV=(1.77×10−11)(12)=2.1×10−10 C.Q=CV=(1.77\times10^{-11})(12)=2.1\times10^{-10}\ \text{C}.

The field is

E=Vd=121.0×10−3=1.2×104 V/m.E=\frac{V}{d} =\frac{12}{1.0\times10^{-3}} =1.2\times10^4\ \text{V/m}.

The battery fixes ΔV\Delta V; the geometry then decides how much charge must move onto the plates.

For capacitors with symmetry, the standard procedure is:

  1. Use Gauss’s law to find E(r)E(r) between the conductors.
  2. Integrate ΔV=−∫E⃗⋅dℓ⃗\Delta V=-\int\vec E\cdot d\vec\ell.
  3. Use C=Q/ΔVC=Q/\Delta V.

For coaxial cylinders of length LL, inner radius aa, and outer radius bb,

E(r)=λ2πε0r,ΔV=λ2πε0ln⁡ba,C=2πε0Lln⁡(b/a).E(r)=\frac{\lambda}{2\pi\varepsilon_0r}, \qquad \Delta V=\frac{\lambda}{2\pi\varepsilon_0}\ln\frac{b}{a}, \qquad C=\frac{2\pi\varepsilon_0L}{\ln(b/a)}.

For concentric spherical conductors with inner radius aa and outer radius bb,

E(r)=kQr2,ΔV=kQ(1a−1b),C=4πε01/a−1/b.E(r)=\frac{kQ}{r^2}, \qquad \Delta V=kQ\left(\frac{1}{a}-\frac{1}{b}\right), \qquad C=\frac{4\pi\varepsilon_0}{1/a-1/b}.

Letting b→∞b\to\infty recovers the isolated sphere result C=4πε0aC=4\pi\varepsilon_0a.

Example. A coaxial cable has inner conductor radius aa, outer conductor inner radius bb, and length LL. It carries charge +λL+\lambda L on the inner conductor and −λL-\lambda L on the outer conductor. Find the capacitance per unit length.

Between the conductors, Gauss’s law with a coaxial cylindrical surface gives

E(2πrL)=λLε0⟹E(r)=λ2πε0r.E(2\pi rL)=\frac{\lambda L}{\varepsilon_0} \quad\Longrightarrow\quad E(r)=\frac{\lambda}{2\pi\varepsilon_0r}.

The potential difference from inner to outer conductor is

Va−Vb=∫abE(r) dr=λ2πε0ln⁡ba.V_a-V_b=\int_a^b E(r)\,dr =\frac{\lambda}{2\pi\varepsilon_0}\ln\frac{b}{a}.

Thus

CL=λVa−Vb=2πε0ln⁡(b/a).\frac{C}{L}=\frac{\lambda}{V_a-V_b} =\frac{2\pi\varepsilon_0}{\ln(b/a)}.

The logarithm is the signature of cylindrical symmetry; if you see coaxial conductors, expect ln⁡(b/a)\ln(b/a) to appear.

To charge a capacitor slowly, each extra bit of charge dqdq must be moved across the current potential difference V=q/CV=q/C. Therefore

U=∫0QV dq=∫0QqC dq=Q22C.U=\int_0^Q V\,dq =\int_0^Q\frac{q}{C}\,dq =\frac{Q^2}{2C}.

The usual equivalent forms are

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

For a parallel-plate capacitor, this energy can also be viewed as living in the electric field. Since C=ε0A/dC=\varepsilon_0A/d and E=V/dE=V/d,

U=12CV2=12ε0E2(Ad).U=\frac{1}{2}CV^2 =\frac{1}{2}\varepsilon_0E^2(Ad).

So the energy density of an electric field is

uE=12ε0E2.u_E=\frac{1}{2}\varepsilon_0E^2.

This field-energy formula is much more general than the parallel-plate derivation suggests.

For capacitors in parallel, the plates share the same potential difference. Charges add:

Qtot=Q1+Q2+⋯⟹Ceq=C1+C2+⋯ .Q_{\text{tot}}=Q_1+Q_2+\cdots \quad\Longrightarrow\quad C_{\text{eq}}=C_1+C_2+\cdots.

For capacitors in series, there is one path and the same charge magnitude appears on each capacitor. Potential differences add:

Vtot=V1+V2+⋯=Q(1C1+1C2+⋯ ),V_{\text{tot}}=V_1+V_2+\cdots =Q\left(\frac{1}{C_1}+\frac{1}{C_2}+\cdots\right),

so

1Ceq=1C1+1C2+⋯ .\frac{1}{C_{\text{eq}}} =\frac{1}{C_1}+\frac{1}{C_2}+\cdots.

A quick way to tell parallel from series is that in parallel, the capacitors have the same voltage passed through them, while in series, the voltages add.

Two circuit facts are especially useful in electrostatics problems:

  • Points connected by ideal wire are at the same potential.
  • The total charge on an isolated connected conductor network is conserved.

Example. Capacitors C1=2.0 μFC_1=2.0\ \mu\text{F} and C2=6.0 μFC_2=6.0\ \mu\text{F} are connected in series across a 12 V12\ \text{V} battery. Find the equivalent capacitance, charge on each capacitor, and voltage across each capacitor.

For series capacitors,

1Ceq=12.0+16.0=23(μF)−1,\frac{1}{C_{\text{eq}}} =\frac{1}{2.0}+\frac{1}{6.0} =\frac{2}{3} \quad(\mu\text{F})^{-1},

so

Ceq=1.5 μF.C_{\text{eq}}=1.5\ \mu\text{F}.

The same charge magnitude appears on both capacitors:

Q=CeqV=(1.5 μF)(12 V)=18 μC.Q=C_{\text{eq}}V=(1.5\ \mu\text{F})(12\ \text{V})=18\ \mu\text{C}.

The voltage drops are

V1=QC1=182.0=9.0 V,V2=QC2=186.0=3.0 V.V_1=\frac{Q}{C_1}=\frac{18}{2.0}=9.0\ \text{V}, \qquad V_2=\frac{Q}{C_2}=\frac{18}{6.0}=3.0\ \text{V}.

The smaller capacitor gets the larger voltage drop. That is the capacitor version of “same charge, different capacitance.”

The plates of a charged capacitor attract. For a parallel-plate capacitor with fixed charge QQ and area AA, one plate feels the field from the other plate, not its own field:

Eother=σ2ε0.E_{\text{other}}=\frac{\sigma}{2\varepsilon_0}.

Thus

F=QEother=σ2A2ε0=Q22ε0A.F=QE_{\text{other}} =\frac{\sigma^2A}{2\varepsilon_0} =\frac{Q^2}{2\varepsilon_0A}.

Equivalently, the field pressure is

P=FA=12ε0E2=σ22ε0.P=\frac{F}{A}=\frac{1}{2}\varepsilon_0E^2=\frac{\sigma^2}{2\varepsilon_0}.

This is the same pressure formula from charged conductor surfaces, now showing up as a plate force.

An electric dipole is a pair of equal and opposite charges separated by a small displacement. Its dipole moment is

p⃗=qd⃗,\vec p=q\vec d,

where d⃗\vec d points from the negative charge to the positive charge. For a continuous charge distribution,

p⃗=∫r⃗ dq,\vec p=\int \vec r\,dq,

with dq=ρ dVdq=\rho\,dV, σ dA\sigma\,dA, or λ dℓ\lambda\,d\ell depending on the distribution. This definition assumes the total charge is zero; otherwise the dipole moment depends on the coordinate origin.

The point-dipole description is an approximation. If the observation distance rr is much larger than the charge separation dd, the separate charges cannot be resolved and their leading nonzero effect is controlled by p⃗\vec p. More generally, a localized charge distribution can be described by a multipole expansion:

  • its total charge is the monopole term, whose potential decays like 1/r1/r;
  • its dipole moment is the next term, whose potential decays like 1/r21/r^2;
  • higher moments such as the quadrupole decay still faster.

For a neutral distribution, the monopole term vanishes, so the dipole term usually controls the far field. The dipole moment is then independent of the choice of origin. To see why, shift the origin by a constant vector a⃗\vec a:

p⃗′=∫(r⃗−a⃗) dq=p⃗−a⃗∫dq=p⃗−a⃗Q.\vec p'=\int(\vec r-\vec a)\,dq =\vec p-\vec a\int dq =\vec p-\vec aQ.

When Q=0Q=0, this gives p⃗′=p⃗\vec p'=\vec p.

In a uniform electric field, the two forces on the charges cancel, so the net force is zero. But the forces usually form a torque:

τ⃗=p⃗×E⃗.\vec\tau=\vec p\times\vec E.

The potential energy is

U=−p⃗⋅E⃗=−pEcos⁡θ.U=-\vec p\cdot\vec E=-pE\cos\theta.

The lowest-energy orientation has p⃗\vec p parallel to E⃗\vec E; the highest-energy orientation has it antiparallel. If the field is nonuniform, the forces on the two ends no longer cancel exactly, so the dipole can feel a net force. In one dimension, when p⃗\vec p and E⃗\vec E both point along xx,

Fx=pdEdx.F_x=p\frac{dE}{dx}.

For a small permanent dipole whose moment does not change appreciably across the field,

F⃗=∇(p⃗⋅E⃗).\vec F=\nabla(\vec p\cdot\vec E).

In electrostatics, ∇×E⃗=0\nabla\times\vec E=0, so this is also commonly written as (p⃗⋅∇)E⃗(\vec p\cdot\nabla)\vec E. The gradient matters: a uniform field can rotate a dipole but cannot translate it, while a nonuniform field can pull an aligned dipole toward the stronger-field region.

Put charges +q+q and −q-q on the zz-axis, separated by distance dd, and look far away where r≫dr\gg d. The potential is approximately

V(r,θ)=kpcos⁡θr2=kp⃗⋅r^r2.V(r,\theta)=k\frac{p\cos\theta}{r^2} =k\frac{\vec p\cdot\hat r}{r^2}.

The important fact is the decay rate: a dipole potential falls like 1/r21/r^2, and its field falls like 1/r31/r^3, faster than a point charge because the total charge cancels at large distances.

Two special field values are worth knowing:

Eaxis=14πε02pr3along p⃗,E_{\text{axis}}=\frac{1}{4\pi\varepsilon_0}\frac{2p}{r^3} \quad\text{along } \vec p,

and

Eequator=14πε0pr3opposite p⃗.E_{\text{equator}}=\frac{1}{4\pi\varepsilon_0}\frac{p}{r^3} \quad\text{opposite } \vec p.

The middle plane perpendicular to p⃗\vec p has V=0V=0, but the electric field there is not zero.

Example. A dipole with moment pp is placed in a uniform electric field EE at angle θ\theta from the field direction. Find the torque magnitude and the work an external agent must do to rotate it slowly from parallel to perpendicular.

The torque magnitude is

τ=pEsin⁡θ.\tau=pE\sin\theta.

The potential energy is U=−pEcos⁡θU=-pE\cos\theta. Parallel means θ=0\theta=0, so Ui=−pEU_i=-pE. Perpendicular means θ=π/2\theta=\pi/2, so Uf=0U_f=0. If the rotation is slow, the external work equals the change in potential energy:

Wext=ΔU=0−(−pE)=pE.W_{\text{ext}}=\Delta U=0-(-pE)=pE.

The field wants to align the dipole; an external agent must add energy to turn it away from alignment.

A dielectric is an insulating material whose charges are bound to atoms or molecules. It does not let charge travel macroscopically through the material the way a conductor does, but its positive and negative charges can shift slightly relative to one another. An external field can therefore create or align microscopic electric dipoles.

There are two main microscopic mechanisms:

  • Induced polarization: the electron cloud shifts slightly relative to the nucleus, creating an induced dipole moment. This occurs even in atoms and nonpolar molecules with no permanent dipole.
  • Orientational polarization: molecules with permanent dipole moments partially align with the applied field. Thermal motion prevents perfect alignment, so this effect generally depends on temperature.

The field acting on each molecule is not always exactly the macroscopic field E⃗\vec E because nearby dipoles also contribute a local field. For the usual continuum treatment, all of that microscopic behavior is summarized by the polarization vector P⃗\vec P, defined as dipole moment per unit volume:

P⃗(r⃗)=1ΔV∑i∈ΔVp⃗i.\vec P(\vec r)=\frac{1}{\Delta V}\sum_{i\in\Delta V}\vec p_i.

Here the averaging volume ΔV\Delta V is small compared with the object but large enough to contain many atoms. Its units are dipole moment per volume, C⋅m/m3=C/m2\text{C}\cdot\text{m}/\text{m}^3=\text{C}/\text{m}^2. A material is uniformly polarized when P⃗\vec P is constant.

For a simple homogeneous, isotropic, linear dielectric, the response is parallel and proportional to the macroscopic field:

P⃗=ε0χeE⃗.\vec P=\varepsilon_0\chi_e\vec E.

Here χe\chi_e is the electric susceptibility. This relation is a constitutive model, not a new fundamental law. In anisotropic materials P⃗\vec P need not be parallel to E⃗\vec E, and in nonlinear materials it need not be proportional to E⃗\vec E.

It is useful to separate charge into two bookkeeping categories:

  • Free charge ρf\rho_f is charge whose location is controlled externally, such as charge deposited on capacitor plates or supplied by a battery.
  • Bound charge ρb\rho_b is the net charge that appears when the positive and negative parts of a dielectric shift or orient. It remains tied to the polarized material.

“Free” does not mean that a charge experiences no force, and “bound” does not mean immobile at the atomic scale. The distinction describes the charge’s role in the macroscopic material model. The electric field responds to both:

∇⋅E⃗=ρtotalε0=ρf+ρbε0.\nabla\cdot\vec E =\frac{\rho_{\text{total}}}{\varepsilon_0} =\frac{\rho_f+\rho_b}{\varepsilon_0}.

To find the bound charge produced by a known polarization, imagine a small volume. Dipoles wholly inside it contribute equal positive and negative charge, so they cancel. A net charge appears only when dipoles terminate at a surface or when the polarization varies from place to place. The resulting densities are

ρb=−∇⋅P⃗\rho_b=-\nabla\cdot\vec P

in the volume and

σb=P⃗⋅n^\sigma_b=\vec P\cdot\hat n

on the surface of the dielectric, where n^\hat n points outward from the material.

The minus sign in ρb=−∇⋅P⃗\rho_b=-\nabla\cdot\vec P has a useful interpretation. If polarization vectors spread outward from a region, their negative ends are left behind there, producing negative bound volume charge. If P⃗\vec P is uniform, ∇⋅P⃗=0\nabla\cdot\vec P=0, so there is no bound charge in the bulk; opposite surface charges remain where the dipoles end.

Example. A long dielectric cylinder of radius RR is uniformly polarized with P⃗=Pz^\vec P=P\hat z. Find its bound volume and surface charge.

Because P⃗\vec P is constant,

ρb=−∇⋅P⃗=0.\rho_b=-\nabla\cdot\vec P=0.

On the curved side, the outward normal is radial and perpendicular to P⃗\vec P, so σb=0\sigma_b=0. On the top face, n^=+z^\hat n=+\hat z and σb=+P\sigma_b=+P. On the bottom face, n^=−z^\hat n=-\hat z and σb=−P\sigma_b=-P. The cylinder therefore behaves like two oppositely charged end faces even though every molecule and the cylinder as a whole remain neutral.

The electric displacement field packages the effect of polarization into an auxiliary field:

D⃗=ε0E⃗+P⃗.\vec D=\varepsilon_0\vec E+\vec P.

Take the divergence and use ∇⋅E⃗=(ρf+ρb)/ε0\nabla\cdot\vec E=(\rho_f+\rho_b)/\varepsilon_0 together with ρb=−∇⋅P⃗\rho_b=-\nabla\cdot\vec P:

∇⋅D⃗=ε0∇⋅E⃗+∇⋅P⃗=ρf.\nabla\cdot\vec D =\varepsilon_0\nabla\cdot\vec E+\nabla\cdot\vec P =\rho_f.

Thus Gauss’s law for D⃗\vec D counts only enclosed free charge:

∮D⃗⋅dA⃗=Qfree, enc.\oint \vec D\cdot d\vec A=Q_{\text{free, enc}}.

This does not mean bound charge has stopped producing an electric field. Its contribution is already hidden inside P⃗\vec P in the definition of D⃗\vec D. The physical force on a point charge is still qE⃗q\vec E, not qD⃗q\vec D.

Across an interface carrying free surface charge σf\sigma_f, a thin Gaussian pillbox gives the normal-component boundary condition

(D⃗2−D⃗1)⋅n^=σf,(\vec D_2-\vec D_1)\cdot\hat n=\sigma_f,

where n^\hat n points from medium 1 into medium 2. When there is no free charge at the interface, the normal component of D⃗\vec D is continuous even though the normal component of E⃗\vec E may change.

For a homogeneous, isotropic, linear dielectric,

D⃗=ε0E⃗+P⃗=ε0(1+χe)E⃗=εE⃗=κε0E⃗,\vec D=\varepsilon_0\vec E+\vec P =\varepsilon_0(1+\chi_e)\vec E =\varepsilon\vec E =\kappa\varepsilon_0\vec E,

where κ=1+χe\kappa=1+\chi_e is the relative permittivity and ε=κε0\varepsilon=\kappa\varepsilon_0 is the permittivity. In this special case, symmetric Gauss-law problems often amount to replacing ε0\varepsilon_0 by ε\varepsilon. The shortcut is not reliable when the dielectric only partly fills the field region, κ\kappa varies with position, or the material is nonlinear or anisotropic.

If a parallel-plate capacitor is completely filled with a linear dielectric of constant κ\kappa,

C=κε0Ad.C=\kappa\frac{\varepsilon_0A}{d}.

The dielectric increases capacitance because polarization reduces the electric field for a given free charge:

E=σfreeκε0.E=\frac{\sigma_{\text{free}}}{\kappa\varepsilon_0}.

For fixed free charge QQ, inserting the dielectric lowers VV and lowers the stored energy U=Q2/(2C)U=Q^2/(2C). For fixed voltage VV, a connected battery supplies extra charge, so Q=CVQ=CV and U=12CV2U=\tfrac12CV^2 increase.

Example. A parallel-plate capacitor of capacitance C0C_0 is charged to voltage V0V_0 and then disconnected from the battery. A dielectric with constant κ\kappa is inserted so it fills the gap. Find the new capacitance, charge, voltage, and stored energy.

The capacitance becomes

C=κC0.C=\kappa C_0.

Because the capacitor is disconnected, no charge can enter or leave:

Q=Q0=C0V0.Q=Q_0=C_0V_0.

The new voltage is

V=QC=C0V0κC0=V0κ.V=\frac{Q}{C} =\frac{C_0V_0}{\kappa C_0} =\frac{V_0}{\kappa}.

The new energy is

U=Q22C=Q022κC0=1κU0.U=\frac{Q^2}{2C} =\frac{Q_0^2}{2\kappa C_0} =\frac{1}{\kappa}U_0.

The energy decreases. The missing energy goes into mechanical work as the dielectric is pulled into the capacitor (and eventually heat if the motion is damped).