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Physics 2 · Electric Force, Field, and Potential · 14 min read · Updated 2026-05-11

Potential and Electric Potential Energy — AP Physics 2

AP Physics 2 · Electric Force, Field, and Potential · 14 min read

1. Core Definitions: Electric Potential Energy ★★☆☆☆ ⏱ 4 min

When a charge moves through an electric field, the change in electric potential energy equals the negative of the work done by the electric force on the charge: $ Delta U = -W_E$. If the charge moves at constant kinetic energy, this change equals the work done by an external force to move the charge: $ Delta U = W_{\text{ext}}$.

For any charge $q$ moving through a potential difference $ Delta V$, the change in potential energy simplifies to the core formula:

\Delta U = q \Delta V

For a system of two point charges $q_1$ and $q_2$ separated by distance $r$, with zero potential energy set at infinite separation, the absolute potential energy of the system is:

U = \frac{k q_1 q_2}{r} = \frac{1}{4 \pi \epsilon_0} \frac{q_1 q_2}{r}

If charges have the same sign, $U$ is positive: work must be done to bring repelling charges together from infinity. If charges have opposite signs, $U$ is negative: the system has less energy than when separated, so work must be done to pull them apart.

2. Electric Potential and Potential of Point Charge Systems ★★★☆☆ ⏱ 4 min

Potential difference (or voltage) $ Delta V = V_f - V_i$ is the difference in potential between two points, the measurable quantity used in circuits and experiments. For a single point charge $Q$, with $V=0$ at infinity, potential at distance $r$ is:

V = \frac{kQ}{r}

A key advantage of potential over electric field is that potential is a scalar quantity. For a system of multiple point charges, the total potential at any point is just the algebraic sum of potentials from each individual charge: $V_{\text{total}} = \sum \frac{k q_i}{r_i}$. No vector components are needed—just add signed values based on the sign of each charge.

3. Electric Field, Potential, and Equipotential Surfaces ★★★☆☆ ⏱ 4 min

Electric field and potential are closely related: the electric field points in the direction of maximum decreasing potential, and its magnitude equals the negative rate of change of potential with distance. For a uniform electric field aligned with the x-axis, this simplifies to:

E = - \frac{\Delta V}{\Delta x}

The magnitude of the field is $|E| = |\Delta V / d|$, where $d$ is the distance along the direction of the electric field between the two points.

No work is done to move a charge along an equipotential, so electric field lines are always perpendicular to equipotential surfaces. For point charges, equipotentials are concentric spheres; for uniform fields between parallel plates, they are parallel planes perpendicular to field lines.

4. Applications: Energy Conservation for Charged Particles ★★★★☆ ⏱ 3 min

Conservation of energy applies to conservative electric fields, allowing us to calculate the kinetic energy and speed of accelerated charged particles, a common AP Physics 2 problem type.

Common Pitfalls

Why: Similar names lead students to forget the definition of potential as "per unit charge".

Why: Students know E points to lower potential and reverse subtraction to get a "reasonable" sign, leading to wrong energy changes.

Why: Students just learned electric field is a vector, so they default to vector addition for potential.

Why: The point charge formula is only defined with zero potential at infinity.

Why: Students rush and confuse the orientation of the two line types.

Quick Reference Cheatsheet

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