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Reading Time: 6 min
Last Updated: March 13, 2026
Main Ideas: 5
Reading Time: 6 min
Last Updated: March 13, 2026
Main Ideas: 5

Topic 3.3 Notes – Potential Energy

Verified for 2027 AP® Physics C: Mechanics Exam
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You’ll connect conservative forces to energy through calculus, interpret potential energy graphs, and use common formulas for springs and gravity. This topic sets up energy conservation and equilibrium analysis.

1. What Potential Energy Is

Potential energy UU belongs to a system, not a single object. A system has potential energy when its objects interact only through conservative forces like gravity or ideal springs.

  • It depends on relative position (separation distance, height, stretch).
  • It is a scalar. No direction.
  • Only changes in potential energy ΔU\Delta U matter physically.

If only conservative forces act, the system’s mechanical energy E=K+UE = K + U stays constant.

Conservative forces refresher

A force is conservative if:

  • Work is path-independent.
  • Work over any closed loop = 0.
  • You can define a potential energy function for it.

Gravity and ideal springs qualify. Kinetic friction does not.

Choosing the zero of UU

You are free to define where U=0U = 0. That choice:

  • Shifts all values by a constant.
  • Does not change forces or motion.

Common choices:

  • Ground level for near-Earth problems.
  • Spring equilibrium length.
  • r→∞r \to \infty for gravitational interactions between planets.

On FRQs, graders don’t care where you set zero as long as you stay consistent.

2. The Link Between Force and Potential Energy

The deep connection is through work.

ΔU=−∫abF⋅dr \Delta U = - \int_{a}^{b} \mathbf{F} \cdot d\mathbf{r}

So if a conservative force does positive work, UU decreases. If it does negative work, UU increases.

In one dimension, this becomes incredibly useful:

F(x)=−dUdx F(x) = -\frac{dU}{dx}

This means:

  • Force points toward decreasing UU.
  • Steeper slope → larger magnitude of force.
  • Flat region (dUdx=0)\left(\frac{dU}{dx}=0\right) → zero force → possible equilibrium.

If you’re given U(x)U(x) on a test, you should immediately think “take the derivative and add a minus sign.”

3. Reading and Using Potential Energy Graphs

Here’s a typical potential energy curve.

Study guide illustration

Potential energy U(x)U(x) with equilibrium and turning points

Slope tells you the force

Use the slope of the U(x)U(x) curve at any point.

  • Positive slope → F<0F < 0 (force left).
  • Negative slope → F>0F > 0 (force right).
  • Zero slope → equilibrium candidate.

Types of equilibrium

At any equilibrium, F=0F = 0 so dUdx=0\frac{dU}{dx} = 0. In the graph above, the bottom of the well is a stable equilibrium.

  • Stable equilibrium
    • Local minimum.
    • Small displacement → force pulls it back.
    • Mathematically d2Udx2>0 \frac{d^2U}{dx^{2}} > 0 .
  • Unstable equilibrium
    • Local maximum.
    • Small displacement → force pushes it away.
    • d2Udx2<0 \frac{d^2U}{dx^{2}} < 0 .
  • Neutral equilibrium
    • Flat region.
    • Small displacement → no restoring force.

On multiple-choice questions, they love asking which point is stable just from the graph. Always think “valley = stable.”

Total energy on the graph

Now add a horizontal line for total energy EE, like the one labeled ETotalE_{\text{Total}} in the figure.

  • Where E>UE > U, kinetic energy K=E−U>0K = E - U > 0. Motion allowed.
  • Where E=UE = U, K=0K = 0. These are turning points.
  • Where E<UE < U, motion is impossible.

If you see two turning points, that’s oscillatory motion trapped in a “well.”

4. Common Potential Energy Functions

Elastic spring

U=12k(Δx)2 U = \tfrac{1}{2}k(\Delta x)^{2}

  • Δx\Delta x is displacement from equilibrium.
  • Parabolic curve.
  • Minimum at Δx=0\Delta x = 0 → stable equilibrium.
  • Taking derivative gives F=−kxF = -kx.

Notice energy depends on x2x^{2}, so compression and stretch both store positive energy.

Gravitational potential energy (two-body)

U=−Gm1m2r U = -\frac{G m_{1} m_{2}}{r}

  • rr is center-to-center distance.
  • Negative because gravity is attractive.
  • Standard reference is U=0U = 0 at r→∞r \to \infty.

If total mechanical energy is negative, the system is bound. That shows up in orbit questions.

Near Earth’s surface

ΔU=mgΔy \Delta U = mg \Delta y

Valid when height is small compared to Earth’s radius so gg is constant. This is just a linear approximation of the full −Gm1m2/r-Gm_1m_{2}/r.

5. Systems with More Than Two Objects

For multiple objects, total potential energy is the sum of all pairwise interactions.

With nn objects, number of pairs is:

n(n−1)2 \frac{n(n-1)}{2}

Each pair contributes its own UU term.

So for three masses interacting gravitationally, you add:

  • U12U_{12}
  • U13U_{13}
  • U23U_{23}

Students often forget one pair on exams and lose easy points.

Lower total potential energy generally means a more stable configuration. Systems tend to move toward lower UU when possible.

Key Takeaways

Potential energy belongs to the system of interacting objects, not an individual object.
Only changes in UU matter; the zero level is arbitrary.
ΔU=−Wconservative \Delta U = -W_{\text{conservative}} .
In 1D, F(x)=−dU/dx F(x) = -dU/dx ; force always points downhill on the UU graph.
Local minima of U(x)U(x) are stable equilibrium; local maxima are unstable.
Turning points occur where total energy equals potential energy.
Memorize U=frac12kx2U= frac12 kx^{2}, U=−Gm1m2/rU=-Gm_1m_{2}/r, and ΔU=mgΔy\Delta U=mg\Delta y.
For multiple objects, add every pairwise interaction.

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Notes

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