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3.3 - Potential Energy

Definition and Basic Properties

Potential energy is energy stored in a system because of where its objects are or how they’re arranged.
You need a couple of things for potential energy: a system with two or more objects, and objects that interact only through conservative forces. It’s a scalar (magnitude, no direction), it’s tied to the positions of the objects, and it can be positive, negative, or zero depending on the reference point you choose.

Review: Common Potential Energy Equations

From algebra-based physics you’ve already met these.
Gravitational potential energy near Earth’s surface:
Ug=mghU_g = mgh
Elastic potential energy (springs):
Us=12kx2U_s = \frac{1}{2}kx^2
Universal gravitational potential energy:
UG=−Gm1m2rU_G = -G\frac{m_1 m_2}{r}
On the AP equation sheet these are written as Us=12k(Δx)2U_s = \frac{1}{2}k(\Delta x)^2, UG=−Gm1m2rU_G = -G\frac{m_1m_2}{r}, and ΔUg=mgΔy\Delta U_g = mg\Delta y. A few details matter:
Springs: Δx\Delta x is how far the spring is stretched or compressed from its natural (unstretched) length, not the block’s position on some other axis. Stretching or compressing by the same amount stores the same energy, since (Δx)2(\Delta x)^2 is positive either way.
Universal gravity: rr is the distance between the centers of the two objects (for planets, moons, and stars, center to center), and UG=0U_G = 0 when they’re infinitely far apart. That’s why UGU_G is always negative.
Near a planet’s surface: ΔUg=mgΔy\Delta U_g = mg\Delta y gives the change in potential energy when an object moves up or down by Δy\Delta y. It works because the gravitational field is nearly constant close to the surface. Far from the surface (satellites, rockets), use UGU_G instead (see below).

Choosing the Zero Point

Where potential energy equals zero is a choice you make to simplify the problem. You get to pick where U=0U = 0 (where h=0h = 0 or x=0x = 0), and you should pick whatever makes the problem easiest. If the problem gives you a zero point, use it; if not, you’re free to choose. Common picks: for gravity, ground level, the lowest point of the motion, or infinity (for universal gravitation); for springs, the natural unstretched length; and in general, setting zero at an initial or final position when it’s convenient.
Example: a 0.50 kg book on a shelf 2.0 m above the floor gets moved to a desk 0.80 m above the floor (g=10g = 10 m/s²).
Zero chosen at
UU on shelf
UU on desk
ΔU\Delta U
Floor
10 J
4.0 J
−6.0-6.0 J
Shelf
0 J
−6.0-6.0 J
−6.0-6.0 J
The values of UU depend on your choice, but ΔU\Delta U, which is what actually shows up in energy equations, doesn’t. A negative UU just means below the zero you picked.

Relationship Between Force and Potential Energy

This is the new calculus-based piece that goes beyond algebra-based physics.
Finding potential energy from force (integration). A conservative force and the potential energy are linked by:
ΔU=−∫F⃗(r⃗)⋅dr⃗\Delta U = -\int \vec{F}(\vec{r}) \cdot d\vec{r}
For one-dimensional motion:
ΔU=−∫xixfF(x) dx\Delta U = -\int_{x_i}^{x_f} F(x) \, dx
That negative sign is crucial: potential energy is the work done against the conservative force. To raise potential energy (like lifting something), you work against the conservative force (gravity pulling down), and the negative sign captures that opposition.

Deriving Common Potential Energy Formulas

Example 1: Gravitational potential energy. The conservative force is the weight Fg=mgF_g = mg (downward), which is −mg-mg if up is positive:
ΔU=−∫0h(−mg) dy=mg∫0hdy=mg[y]0h=mgh\Delta U = -\int_0^h (-mg) \, dy = mg\int_0^h dy = mg[y]_0^h = mgh
That recovers the familiar mghmgh.
Example 2: Elastic potential energy. The spring force is Fs=−kxF_s = -kx:
ΔU=−∫0x(−kx′) dx′=∫0xkx′ dx′=k[x′22]0x=12kx2\Delta U = -\int_0^x (-kx') \, dx' = \int_0^x kx' \, dx' = k\left[\frac{x'^2}{2}\right]_0^x = \frac{1}{2}kx^2
That recovers the spring formula.
Example 3: Universal gravitational potential energy. The force is FG=−Gm1m2r2F_G = -G\frac{m_1 m_2}{r^2} (negative because it’s attractive), and integrating from infinity to distance rr:
ΔU=−∫∞r(−Gm1m2r′2)dr′=Gm1m2∫∞rdr′r′2=Gm1m2[−1r′]∞r=Gm1m2(−1r+0)=−Gm1m2r\Delta U = -\int_{\infty}^r \left(-G\frac{m_1 m_2}{r'^2}\right) dr' = G m_1 m_2 \int_{\infty}^r \frac{dr'}{r'^2} = G m_1 m_2 \left[-\frac{1}{r'}\right]_{\infty}^r = G m_1 m_2 \left(-\frac{1}{r} + 0\right) = -G\frac{m_1 m_2}{r}
That’s why universal gravitational potential energy is negative (with zero set at infinity).
Where mgΔymg\Delta y comes from. Move an object of mass mm from a planet’s surface (radius RR, mass MM) up to a height hh. Using UGU_G:
ΔU=(−GMmR+h)−(−GMmR)=GMmhR(R+h)\Delta U = \left(-\frac{GMm}{R+h}\right) - \left(-\frac{GMm}{R}\right) = \frac{GMmh}{R(R+h)}
When hh is much smaller than RR, R+h≈RR + h \approx R, so ΔU≈GMR2mh\Delta U \approx \frac{GM}{R^2}mh. And GMR2\frac{GM}{R^2} is just gg at the surface, so ΔU≈mgh\Delta U \approx mgh. The approximation is off by a factor of RR+h\frac{R}{R+h}. For a 100 m tower on Earth that’s an error of about 0.002%, but it gets big fast for satellites.
Example: how much does the potential energy of the Earth-satellite system increase when a 500 kg satellite is lifted from Earth’s surface to an altitude equal to Earth’s radius? Use ME=5.97×1024M_E = 5.97 \times 10^{24} kg and RE=6.37×106R_E = 6.37 \times 10^6 m (problems give these; they aren’t on the equation sheet). At the surface r=REr = R_E, and at the final altitude r=2REr = 2R_E:
ΔUG=−GMEm2RE−(−GMEmRE)=GMEm2RE=(6.67×10−11)(5.97×1024)(500)2(6.37×106)≈1.6×1010 J\Delta U_G = -\frac{GM_Em}{2R_E} - \left(-\frac{GM_Em}{R_E}\right) = \frac{GM_Em}{2R_E} = \frac{(6.67 \times 10^{-11})(5.97 \times 10^{24})(500)}{2(6.37 \times 10^6)} \approx 1.6 \times 10^{10} \text{ J}
Using mgΔymg\Delta y instead gives (500)(10)(6.37×106)≈3.2×1010(500)(10)(6.37 \times 10^6) \approx 3.2 \times 10^{10} J, about twice the real answer, because gravity gets weaker as the satellite climbs. Use mgΔymg\Delta y near the surface, and UG=−Gm1m2rU_G = -G\frac{m_1m_2}{r} whenever the distance from the planet’s center changes by a noticeable fraction.

Finding Force from Potential Energy (Differentiation)

If you know the potential energy function, you get the conservative force by differentiating:
F(x)=−dUdxF(x) = -\frac{dU}{dx}
So the force is the negative of the slope of the potential energy graph. In three dimensions:
F⃗=−∇U=−(∂U∂xi^+∂U∂yj^+∂U∂zk^)\vec{F} = -\nabla U = -\left(\frac{\partial U}{\partial x}\hat{i} + \frac{\partial U}{\partial y}\hat{j} + \frac{\partial U}{\partial z}\hat{k}\right)
but for AP Physics C Mechanics you usually stay in one dimension.
3.3 - Potential Energy
Key observations: where UU has a negative slope the force is positive (points right/up), where UU has a positive slope the force is negative (points left/down), where UU is at a minimum the force is zero (stable equilibrium), and where UU is at a maximum the force is also zero (unstable equilibrium).

Potential Energy Graphs

In calculus-based physics, potential energy graphs get more interesting because they’re real functions, not just straight lines. A few features to spot:
  1. Equilibrium points, where dUdx=0\frac{dU}{dx} = 0 (the force is zero). A local minimum of UU is stable equilibrium (like a valley), and a local maximum is unstable equilibrium (like a hilltop).
  1. Turning points, where the total energy line E=K+UE = K + U crosses U(x)U(x). There the object has K=0K = 0 (momentarily at rest) and reverses direction.
  1. Forbidden regions, where U(x)>EtotalU(x) > E_{total}. Reaching them would need K<0K < 0, which is impossible, so the object can’t go there.
Stable equilibrium is a position where a small displacement produces a force pointing back toward equilibrium, so the object accelerates back. On a U(x)U(x) graph that’s a local minimum: nudge the object right and the slope is positive, so F=−dUdxF = -\frac{dU}{dx} points left; nudge it left and the slope is negative, so FF points right.
Unstable equilibrium is a position where a small displacement produces a force in the same direction as the displacement, so the object accelerates away. On a U(x)U(x) graph that’s a local maximum.
A quick calculus check: at an equilibrium point (dUdx=0\frac{dU}{dx} = 0), if d2Udx2>0\frac{d^2U}{dx^2} > 0 the curve is concave up (a minimum, stable), and if d2Udx2<0\frac{d^2U}{dx^2} < 0 it’s concave down (a maximum, unstable).

Example Problem: Reading a Potential Energy Curve

A 0.25 kg particle moves along the xx-axis, and the only force on it is conservative, with potential energy
U(x)=3.0x2−1.0x3U(x) = 3.0x^2 - 1.0x^3
where UU is in joules and xx is in meters. The particle is released from rest at x=1.0x = 1.0 m.
  1. Find the force on the particle at x=1.0x = 1.0 m.
  1. Find the equilibrium positions and classify each one as stable or unstable.
  1. Find the turning points of the motion and the particle’s maximum speed.
3.3 - Potential Energy
Part (a): Force. Differentiate and take the negative:
F(x)=−dUdx=−(6.0x−3.0x2)=−6.0x+3.0x2F(x) = -\frac{dU}{dx} = -(6.0x - 3.0x^2) = -6.0x + 3.0x^2
At x=1.0x = 1.0 m, F=−6.0+3.0=−3.0F = -6.0 + 3.0 = -3.0 N. The force points in the −x-x direction, which is downhill on the graph (toward lower UU), so the particle starts moving left.
Part (b): Equilibrium positions. Set dUdx=0\frac{dU}{dx} = 0: 6.0x−3.0x2=3.0x(2.0−x)=06.0x - 3.0x^2 = 3.0x(2.0 - x) = 0, so x=0x = 0 and x=2.0x = 2.0 m. The second derivative is d2Udx2=6.0−6.0x\frac{d^2U}{dx^2} = 6.0 - 6.0x. At x=0x = 0 it’s +6.0+6.0 (a minimum, stable), and at x=2.0x = 2.0 m it’s −6.0-6.0 (a maximum, unstable).
Check with forces: at x=0.10x = 0.10 m, F=−0.57F = -0.57 N, which pushes back toward x=0x = 0 (stable). At x=2.1x = 2.1 m, F=+0.63F = +0.63 N, which pushes farther right, away from x=2.0x = 2.0 m (unstable).
Part (c): Turning points and maximum speed. Released from rest, the total energy is E=K+U=0+U(1.0)=3.0−1.0=2.0E = K + U = 0 + U(1.0) = 3.0 - 1.0 = 2.0 J, the red line on the graph. Turning points are where U(x)=EU(x) = E:
3x2−x3=2  ⟹  (x−1)(x2−2x−2)=03x^2 - x^3 = 2 \implies (x - 1)(x^2 - 2x - 2) = 0
so x=1.0x = 1.0 m or x=1±3x = 1 \pm \sqrt{3} m. The particle starts at x=1.0x = 1.0 m and moves left, so it swings back and forth between x=1.0x = 1.0 m and x=1−3≈−0.73x = 1 - \sqrt{3} \approx -0.73 m. The third crossing, x=1+3≈2.7x = 1 + \sqrt{3} \approx 2.7 m, can’t be reached: getting there means climbing over the hill at x=2.0x = 2.0 m, where U=4.0U = 4.0 J is more than EE (a forbidden region).
The speed is greatest where UU is smallest, at the bottom of the well (x=0x = 0, U=0U = 0):
Kmax=E−U(0)=2.0−0=2.0 J  ⟹  vmax=2Kmaxm=2(2.0)0.25=4.0 m/sK_{max} = E - U(0) = 2.0 - 0 = 2.0 \text{ J} \implies v_{max} = \sqrt{\frac{2K_{max}}{m}} = \sqrt{\frac{2(2.0)}{0.25}} = 4.0 \text{ m/s}
If the particle had more than 4.0 J of total energy, it could pass over the hill at x=2.0x = 2.0 m and keep going to the right, speeding up as UU drops.

Example Problem: Non-Linear Spring

A spring stretched by xx produces a restoring force of:
F(x)=−ax−bx2F(x) = -ax - bx^2
where aa and bb are positive constants. How much work does an external force do in stretching the spring by an amount DD from equilibrium?
Key idea: potential energy is the work done against the restoring force. The spring’s restoring force is Fspring(x)=−ax−bx2F_{spring}(x) = -ax - bx^2, so an external force pulls the other way, Fext(x)=ax+bx2F_{ext}(x) = ax + bx^2.
Set up the work integral (external work equals the change in potential energy):
W=ΔU=−∫0DFspring(x) dx=−∫0D(−ax−bx2) dx=∫0D(ax+bx2) dxW = \Delta U = -\int_0^D F_{spring}(x) \, dx = -\int_0^D (-ax - bx^2) \, dx = \int_0^D (ax + bx^2) \, dx
Integrate with the power rule:
W=[ax22+bx33]0D=aD22+bD33W = \left[\frac{ax^2}{2} + \frac{bx^3}{3}\right]_0^D = \frac{aD^2}{2} + \frac{bD^3}{3}
So the external force does aD22+bD33\frac{aD^2}{2} + \frac{bD^3}{3} (equivalently 12aD2+13bD3\frac{1}{2}aD^2 + \frac{1}{3}bD^3) of work. Unlike an ideal spring where U=12kx2U = \frac{1}{2}kx^2, this one has both quadratic and cubic terms because of the non-linear restoring force: the bx2bx^2 term in the force turns into a 13bx3\frac{1}{3}bx^3 term in the potential energy.

Systems With More Than Two Objects

Potential energy belongs to a pair of interacting objects. With three or more objects, add up the potential energy of every pair: Utotal=U12+U13+U23+…U_{total} = U_{12} + U_{13} + U_{23} + \ldots For NN objects there are N(N−1)2\frac{N(N-1)}{2} pairs (3 pairs for 3 objects, 6 pairs for 4).
Example: three small spheres sit at the corners of a right triangle: A (2.0 kg) at the right angle, B (3.0 kg) 3.0 m from A, and C (4.0 kg) 4.0 m from A, so B and C are 5.0 m apart. The gravitational potential energy of the system is:
U=−G(mAmBrAB+mAmCrAC+mBmCrBC)=−(6.67×10−11)((2.0)(3.0)3.0+(2.0)(4.0)4.0+(3.0)(4.0)5.0)U = -G\left(\frac{m_Am_B}{r_{AB}} + \frac{m_Am_C}{r_{AC}} + \frac{m_Bm_C}{r_{BC}}\right) = -(6.67 \times 10^{-11})\left(\frac{(2.0)(3.0)}{3.0} + \frac{(2.0)(4.0)}{4.0} + \frac{(3.0)(4.0)}{5.0}\right)U=−(6.67×10−11)(6.4)≈−4.3×10−10 JU = -(6.67 \times 10^{-11})(6.4) \approx -4.3 \times 10^{-10} \text{ J}
Each pair counts once (don’t add both UABU_{AB} and UBAU_{BA}). The negative total means you’d have to do 4.3×10−104.3 \times 10^{-10} J of work to pull all three apart to infinite separation.
The same idea works with different kinds of potential energy. For a block hanging on a vertical spring near Earth, the system (block, spring, and Earth) has Utotal=Ug+UsU_{total} = U_g + U_s: gravitational energy from the block-Earth pair plus elastic energy in the spring.

Summary of Force and Potential Energy Relationships

Given
Find
Operation
Formula
Force F(x)F(x)
Potential energy U(x)U(x)
Integrate
ΔU=−∫F(x)dx\Delta U = -\int F(x) dx
Potential energy U(x)U(x)
Force F(x)F(x)
Differentiate
F(x)=−dUdxF(x) = -\frac{dU}{dx}
A quick memory aid: going from force to potential energy you integrate (accumulate work), and going from potential energy to force you differentiate (find the slope).

Common Mistakes

  1. Dropping the negative sign. Both formulas have one: ΔU=−∫F dx\Delta U = -\int F \, dx and F=−dUdxF = -\frac{dU}{dx}.
  1. Confusing force direction with potential energy change. Lifting an object (raising its potential energy) means working against gravity, which is what the negative sign accounts for.
  1. Wrong integration limits. Integrate from the initial to the final position. Stretching a spring from natural length means going from 0 to xx.
  1. Thinking potential energy is always positive. It can be negative (like gravitational PE with zero at infinity). Only kinetic energy must be non-negative.
  1. Missing equilibrium points on U(x)U(x) graphs. Where the slope is zero (dUdx=0\frac{dU}{dx} = 0), the force is zero and you’re at equilibrium.
  1. Confusing stable and unstable equilibrium. Stable is a minimum of UU (ball in a valley), unstable is a maximum (ball on a hilltop).
  1. Wrong derivative of UU. If U(x)=12kx2U(x) = \frac{1}{2}kx^2, then dUdx=kx\frac{dU}{dx} = kx, so F=−kxF = -kx (not +kx+kx). The negative sign in the formula is separate from any sign in the function.
  1. Not evaluating both limits. ∫abf(x)dx=F(b)−F(a)\int_a^b f(x)dx = F(b) - F(a). Subtract the lower-limit value.
  1. Picking an awkward zero point. You can choose any zero, but bad choices make problems harder. Put zero at a point that’s actually involved.
  1. Mixing up work by vs. against a conservative force. Work done by a conservative force is −ΔU-\Delta U. Work done against it is +ΔU+\Delta U.
  1. Not noticing whether you’re given force or potential. Given F(x)F(x), integrate for UU. Given U(x)U(x), differentiate for FF.
  1. Integrating polynomials wrong. ∫xndx=xn+1n+1+C\int x^n dx = \frac{x^{n+1}}{n+1} + C. For x2x^2 you get x33\frac{x^3}{3}, not x32\frac{x^3}{2}.
  1. Assuming every spring follows Hooke’s law. In calculus-based physics, springs can be non-linear like F=−ax−bx2F = -ax - bx^2. Use the given function, not automatically F=−kxF = -kx.
  1. Chain rule slips. If U=12k(x−x0)2U = \frac{1}{2}k(x-x_0)^2, then dUdx=k(x−x0)\frac{dU}{dx} = k(x-x_0), so F=−k(x−x0)F = -k(x-x_0).
  1. Confusing total energy with potential energy on graphs. A horizontal line on a UU vs. xx graph is usually the total energy EE, and E−UE - U is the kinetic energy at that position.

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