Part 2 · Chapter 6

Electric Potential and Energy

A vector field at every point is a lot to track. Electrostatics offers a shortcut: a single scalar, the potential, whose hill-slope is the field itself. From it flow voltage, the conservative law behind every circuit, and the energy locked in the field.

Electromagnetic Field Theory Prof. Mithun Mondal Reading time ≈ 55 min
i What you'll learn
  • The work done moving a charge through a field, and how it defines potential difference.
  • The potential of a point charge and, by superposition, of any distribution.
  • The field–potential relation \(\vec{E} = -\nabla V\) — the gradient of Chapter 3 made physical.
  • Why the electrostatic field is conservative: \(\oint\vec{E}\cdot d\vec{l}=0\), Maxwell's curl equation for statics.
  • The electric dipole, its potential, and the \(1/r^2\) and \(1/r^3\) falloffs.
  • The energy stored in an electrostatic field and its energy density.
Section 6-1

Work & Potential Difference

To move a charge \(Q\) against an electric field, you must do work. The field pushes with force \(Q\vec{E}\); you push the other way. The work done by you in carrying \(Q\) from point \(A\) to point \(B\) is the line integral met in Chapter 3:

Work done moving a charge
\[ W = -Q\int_A^B \vec{E}\cdot d\vec{l} \]

The potential difference \(V_{AB}\) is this work per unit charge — the work to move one coulomb from \(B\) to \(A\). Its unit is the volt (J/C):

Potential difference
\[ V_{AB} = V_A - V_B = -\int_B^A \vec{E}\cdot d\vec{l} \quad (\text{V}) \]
The minus sign, explained. The field points "downhill", from high potential to low. Moving a positive charge uphill (against \(\vec{E}\)) costs work and raises its potential energy — hence the minus. It is the same convention as gravity: lifting a mass against \(\vec{g}\) stores energy.
Section 6-2

Potential of a Point Charge

Taking the reference point at infinity (where \(V=0\)) and integrating the point-charge field inward gives the absolute potential. Because \(\vec{E}\) is radial and falls as \(1/r^2\), its integral gives a clean \(1/r\):

Potential of a point charge
\[ V = \frac{Q}{4\pi\varepsilon_0 r} \quad (\text{relative to } \infty) \]
+Q V = const
Equipotentials (blue) are spheres; field lines (green) cross them at right angles

Surfaces of constant \(V\) are equipotentials — spheres for a point charge. Since no work is done moving along an equipotential, the field can have no component along it, so \(\vec{E}\) is always perpendicular to equipotential surfaces. Potential is a scalar, so unlike \(\vec{E}\) it adds by simple arithmetic, not vectors.

Section 6-3

Potential of Distributions

Because potential superposes as a scalar sum, the potential of many charges — or a continuous distribution — is just the sum or integral of point-charge potentials. No components, no angles to resolve:

Potential by superposition
\[ V = \frac{1}{4\pi\varepsilon_0}\sum_k \frac{Q_k}{r_k}, \qquad V = \frac{1}{4\pi\varepsilon_0}\int \frac{dQ}{r} \]
🔑
Scalar first, vector second
Find \(V\) by a scalar integral, then get \(\vec{E} = -\nabla V\)

It is almost always easier to compute the scalar \(V\) and then differentiate than to integrate the vector \(\vec{E}\) directly. This "potential-first" strategy is the workhorse of electrostatic problem-solving.

Section 6-4

The Relation E = −∇V

Potential difference is a line integral of \(\vec{E}\); reversing that relationship, the field is the negative gradient of the potential. This is the gradient of Chapter 3 given physical meaning: \(\vec{E}\) points in the direction of steepest decrease of \(V\), downhill on the potential landscape.

Field from potential
\[ \vec{E} = -\nabla V \]

This single equation explains the picture above: since \(\nabla V\) is perpendicular to equipotentials (Chapter 3), so is \(\vec{E}\). It also confirms the units — \(\nabla V\) has units of volts per metre, exactly the units of \(\vec{E}\).

Section 6-5

The Conservative Field

Because \(\vec{E}\) is a gradient, the work to move a charge between two points depends only on the endpoints, never on the path. Equivalently, the work around any closed loop is zero. This makes the electrostatic field conservative:

Conservative field — integral and point form
\[ \oint_L \vec{E}\cdot d\vec{l} = 0, \qquad \nabla\times\vec{E} = 0 \]

The point form follows from Stokes' theorem (Chapter 3) and the identity that the curl of a gradient is always zero. This is Maxwell's curl equation for statics — and it is precisely Kirchhoff's voltage law: the sum of potential rises and drops around any circuit loop is zero. The circuit law you already know is electrostatics in disguise.

Section 6-6

The Electric Dipole

An electric dipole is two equal and opposite charges \(\pm Q\) separated by a small distance \(d\). Its dipole moment is \(\vec{p} = Q\vec{d}\), pointing from the negative to the positive charge. Far from the dipole (\(r\gg d\)), the two potentials nearly cancel, leaving a field that fades faster than a single charge's:

Dipole potential and field
\[ V = \frac{Q d\cos\theta}{4\pi\varepsilon_0 r^2} = \frac{\vec{p}\cdot\hat{a}_r}{4\pi\varepsilon_0 r^2}, \qquad E \propto \frac{1}{r^3} \]
−Q +Q d p = Qd
A dipole: moment p points from −Q to +Q; its potential falls as 1/r²
Section 6-7

Electrostatic Energy

Assembling a set of charges takes work, and that work is stored as electrostatic energy. Bringing in each charge against the potential of those already placed gives:

Energy of a charge assembly
\[ W_E = \frac{1}{2}\sum_{k=1}^{N} Q_k V_k \]

The factor of \(\tfrac{1}{2}\) avoids double-counting each pair. Remarkably, this energy can be re-expressed as living in the field itself, spread through all of space with an energy density:

Field energy and energy density
\[ W_E = \frac{1}{2}\int_v \vec{D}\cdot\vec{E}\,dv, \qquad w_E = \frac{1}{2}\varepsilon_0 E^2 \quad (\text{J/m}^3) \]
Where does the energy live? The two formulas give the same number, but the second tells a deeper story: energy is not "in the charges", it is stored in the field everywhere \(\vec{E}\) is non-zero. This field-energy view becomes essential in Part 5, where a travelling electromagnetic wave carries its energy through empty space with no charges in sight.
Section 6-8

Worked Examples

1 Potential of a point charge

Problem. Find \(V\) at \(0.3\ \text{m}\) from a \(+6\ \text{nC}\) charge.

Solution. Apply \(V = Q/4\pi\varepsilon_0 r\):

Working
\[ V = \frac{9\times10^9\,(6\times10^{-9})}{0.3} = 180\ \text{V} \]
2 Work to move a charge

Problem. How much work moves \(+2\ \text{nC}\) from a point at \(50\ \text{V}\) to one at \(120\ \text{V}\)?

Solution. Work equals charge times potential rise, \(W = Q(V_B - V_A)\):

Working
\[ W = 2\times10^{-9}\,(120 - 50) = 140\ \text{nJ} \]
3 E from V

Problem. Given \(V = x^2 y + 2z\ \text{V}\), find \(\vec{E}\).

Solution. Take the negative gradient:

Working
\[ \vec{E} = -\nabla V = -2xy\,\hat{a}_x - x^2\,\hat{a}_y - 2\,\hat{a}_z\ \text{V/m} \]
4 Potential of two charges

Problem. Charges \(+4\ \text{nC}\) and \(-4\ \text{nC}\) sit \(0.2\ \text{m}\) apart. Find \(V\) at the point \(0.1\ \text{m}\) from each.

Solution. Add the scalar potentials — equal magnitudes, opposite signs:

Working
\[ V = \frac{9\times10^9(4\times10^{-9})}{0.1} + \frac{9\times10^9(-4\times10^{-9})}{0.1} = 0\ \text{V} \]
5 Path independence

Problem. Show the work moving a charge around a closed triangle in a uniform field \(\vec{E}=E_0\,\hat{a}_x\) is zero.

Solution. A conservative field gives zero circulation:

Working
\[ W = -Q\oint_L \vec{E}\cdot d\vec{l} = 0 \quad(\text{since } \nabla\times\vec{E}=0) \]
6 Energy density

Problem. Find the energy density where \(E = 2\times10^{5}\ \text{V/m}\) in free space.

Solution. Apply \(w_E = \tfrac{1}{2}\varepsilon_0 E^2\):

Working
\[ w_E = \tfrac{1}{2}(8.854\times10^{-12})(2\times10^{5})^2 = 0.177\ \text{J/m}^3 \]
Review

Chapter Summary

Potential difference

\(V_{AB}=-\int_B^A\vec{E}\cdot d\vec{l}\); work per unit charge; unit volt.

Point-charge V

\(V=\dfrac{Q}{4\pi\varepsilon_0 r}\); a scalar, so it superposes by simple addition.

E = −∇V

Field is steepest descent of potential; always perpendicular to equipotentials.

Conservative

\(\oint\vec{E}\cdot d\vec{l}=0\), \(\nabla\times\vec{E}=0\); this is Kirchhoff's voltage law.

Dipole

\(\vec{p}=Q\vec{d}\); \(V\propto 1/r^2\), \(E\propto 1/r^3\) — faster falloff than a point charge.

Energy

\(W_E=\tfrac12\int\vec{D}\cdot\vec{E}\,dv\); density \(w_E=\tfrac12\varepsilon_0 E^2\); energy lives in the field.

Practice

Problems

For each item, decide whether to work with the scalar \(V\) or the vector \(\vec{E}\) first — usually \(V\) — then convert if needed. Difficulty rises down the list.

  1. Find the potential \(3\ \text{m}\) from a \(-12\ \text{nC}\) point charge.
  2. Compute the work to move \(+5\ \text{nC}\) from \(20\ \text{V}\) to \(95\ \text{V}\).
  3. For \(V = 4xy - z^2\ \text{V}\), find \(\vec{E}\) at \((1,1,1)\).
  4. Two charges \(+Q\) sit at \((\pm a,0,0)\). Find \(V\) on the \(y\)-axis and then \(\vec{E}\) there.
  5. A charge \(+8\ \text{nC}\) at the origin and \(-8\ \text{nC}\) at \((0.1,0,0)\) form a dipole. Find \(V\) at \((0,0,0.2)\).
  6. Show that the work to move a charge between two points is independent of path for \(\vec{E}=k\,\hat{a}_x\).
  7. A uniformly charged ring of radius \(a\) carries total charge \(Q\). Find \(V\) on its axis, then \(\vec{E}\) by differentiation.
  8. Compute the total energy stored by assembling three \(+Q\) charges at the corners of an equilateral triangle of side \(a\).
  9. The potential in a region is \(V = 50/r\ \text{V}\) (spherical). Find \(\vec{E}\) and the charge producing it.
  10. Find the energy density at the surface of a \(1\ \text{cm}\)-radius sphere carrying \(10\ \text{nC}\).
  11. Derive \(\vec{E}=-\nabla V\) for the point-charge potential and confirm it matches Coulomb's field.
  12. Explain, using \(\nabla\times\vec{E}=0\), why a static electric field can never form closed loops, and contrast this with the magnetic field of Part 3.
Tip: when a problem gives charges and asks for the field, resist integrating \(\vec{E}\) directly. Sum the scalar potential \(V\) first — no angles, no components — then take \(-\nabla V\). The detour through a scalar is almost always the shortest road to the vector. And whenever you see "work around a loop" or "independent of path", the answer is built into \(\nabla\times\vec{E}=0\) before you compute anything.