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Electric Potential & Energy

The electric potential $V$ is a scalar field whose negative gradient gives $\vec E$. Working with $V$ is usually easier than with $\vec E$ directly: it's a scalar sum rather than a vector sum. The energy stored in an electric field is $u=\varepsilon_0 E^2/2$ per unit volume.

Key Concepts

Electric Potential
V(r)=OrEdlV(\vec r)=-\int_{\mathcal{O}}^{\vec r}\vec E\cdot d\vec l (reference point O\mathcal{O} usually at infinity). For a point charge: V=kq/rV=kq/r. E=V\vec E=-\nabla V.
Superposition
VV is a scalar, so the potential of multiple charges is the algebraic sum: V=ikqi/riV=\sum_i kq_i/r_i. Much simpler than the vector sum for E\vec E.
Energy of a Charge Distribution
The energy stored in assembling a continuous charge distribution: W=ε02E2d3rW=\frac{\varepsilon_0}{2}\int E^2\,d^3r. Energy density: u=ε0E2/2u=\varepsilon_0 E^2/2.
Method of Images
A point charge +q+q at height dd above a grounded infinite conductor can be replaced by +q+q plus an image charge q-q at depth dd below the surface. The boundary condition V=0V=0 at the surface is automatically satisfied.

Key Equations

Potential of point charge
V=14πε0qrV = \frac{1}{4\pi\varepsilon_0}\frac{q}{r}
Scalar; superpose for multiple charges.
Energy density
u=ε02E2=12μ0B2u = \frac{\varepsilon_0}{2}E^2 = \frac{1}{2\mu_0}B^2
Energy stored per unit volume in EM fields.
Energy of point charges
W=12iqiV(ri)W = \frac{1}{2}\sum_i q_i V(\vec{r}_i)
Total electrostatic energy; factor ½ avoids double-counting.
Worked Example

Potential of Two Charges

Problem

Charge q1=+3.0q_1=+3.0 nC is at the origin and q2=1.0q_2=-1.0 nC is at x=0.40x=0.40 m. Find the potential at P=(0.40,0.30,0)P=(0.40,0.30,0) m.

Solution

Distance from q1q_1 to PP: r1=0.16+0.09=0.50r_1=\sqrt{0.16+0.09}=0.50 m.

Distance from q2q_2 to PP: r2=(0.400.40)2+0.09=0.30r_2=\sqrt{(0.40-0.40)^2+0.09}=0.30 m.

V=k(q1r1+q2r2)=8.99×109(3×1090.50+1090.30)V = k\left(\frac{q_1}{r_1}+\frac{q_2}{r_2}\right) = 8.99\times10^9\left(\frac{3\times10^{-9}}{0.50}+\frac{-10^{-9}}{0.30}\right)
V=8.99×109(6×1093.33×109)=8.99×109×2.67×109=24.0 VV = 8.99\times10^9(6\times10^{-9}-3.33\times10^{-9}) = 8.99\times10^9\times2.67\times10^{-9} = 24.0\text{ V}
Answer V=24.0V=24.0 V.
Practice

Exercises

7 problems
1 of 7

Drag the slider along the V = kQ/r curve and watch the equipotential rings change. For Q = 5.0 nC, find V at r = 0.30 m (in V).

electric potential
Explore radius r V(0.30 m) = 149.8 V

V = kQ/r falls off as 1/r — halving the distance doubles the potential. Equipotential surfaces are spheres.

V at r=0.3 m
V = V

V = kQ/r, k=8.99×10⁹, Q=5 nC, r=0.3 m

2 of 7

Watch the test charge move from r₁ to r₂ along the potential curve. The shaded area is ΔV. Find the work W (in nJ) to move q = 2.0 nC from r₁ = 0.50 m to r₂ = 0.20 m near Q = 4.0 nC.

work & potential

Work done = charge × potential difference. Moving toward a like-sign source takes positive work.

W = q·ΔV
W = nJ

q=2 nC, Q=4 nC, r₁=0.5 m → r₂=0.2 m

3 of 7

Energy stored assembling two charges q1=q2=1.0×109q_1=q_2=1.0\times10^{-9} C separated by d=0.10d=0.10 m (in J). W=kq1q2/dW=kq_1q_2/d.

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4 of 7

Energy density in a uniform E=1000E=1000 N/C field (in J/m³). u=ε0E2/2u=\varepsilon_0 E^2/2.

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5 of 7

A charge q=+1.0×109q=+1.0\times10^{-9} C is at distance d=0.10d=0.10 m above a grounded conductor. The image charge is 1.0×109-1.0\times10^{-9} C. Find the attractive force (in N) between the charge and its image (2d2d apart).

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6 of 7

A capacitor has Q=3.0×106Q=3.0\times10^{-6} C on plates with area A=0.010A=0.010 m² and separation d=0.001d=0.001 m (ε0=8.85×1012\varepsilon_0=8.85\times10^{-12}). Find the electric field E=σ/ε0E=\sigma/\varepsilon_0 (in N/C). σ=Q/A\sigma=Q/A.

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7 of 7

For the same capacitor, find the energy stored (in J). U=Q2/(2C)=ε0E2Ad/2U=Q^2/(2C)=\varepsilon_0 E^2 Ad/2. C=ε0A/d=8.85×1012×0.01/0.001=8.85×1011C=\varepsilon_0 A/d=8.85\times10^{-12}\times0.01/0.001=8.85\times10^{-11} F.

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Key Takeaways

  • VV is a scalar — superpose algebraically. Then E=V\vec E=-\nabla V gives the field.
  • Work done moving charge qq through potential difference ΔV\Delta V: W=qΔVW=q\Delta V.
  • Energy density u=ε0E2/2u=\varepsilon_0E^2/2 tells you where the electromagnetic energy is stored.
  • Method of images solves boundary value problems by replacing the conductor with image charges that maintain the boundary condition.