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Physics · General Physics and Classical Mechanics

Work and Potential Energy as a Gradient in Conservative Force Fields

Work is a line integral and the net work equals the change in kinetic energy; a conservative force does path-independent work, has zero curl, and equals minus the gradient of a potential energy, so mechanical energy is conserved and a 1D potential curve U(x) encodes equilibria, stability and oscillation frequencies.

Work and Potential Energy as a Gradient in Conservative Force Fields

Energy methods are the shortest route through most of mechanics, and they rest on one idea from Chapter 1: for a certain class of force fields, the work done is the difference of a scalar function between the endpoints, so the force is the (negative) gradient of that scalar. Such forces are called conservative, the scalar is the potential energy, and the statement F⃗=−∇U\vec{F} = -\nabla U is the bridge between the vector language of forces and the scalar language of energy.

This chapter makes that bridge rigorous. It defines work as a line integral, proves the work–energy theorem from Newton's second law, gives four equivalent characterisations of whether a force is conservative, and then shows how a one-dimensional potential-energy curve U(x)U(x) encodes the entire qualitative dynamics — equilibria, stability, turning points, oscillation frequencies — before a single equation of motion is solved. The reading is Morin and the early chapters of Goldstein.

Why "as a gradient" is in the title. The high-school picture of potential energy as "stored energy" is fine as far as it goes, but the operational definition you need is geometric: UU is a scalar field, its level surfaces are surfaces of constant energy, and F⃗=−∇U\vec{F} = -\nabla U points downhill on that field, perpendicular to the level surfaces, steepest where they are closest together.

1. Work as a Line Integral

The work done by a force F⃗\vec{F} on a particle moving along a path C\mathcal{C} from point AA to point BB is

WAB=∫CF⃗⋅dℓ⃗W_{AB} = \int_{\mathcal{C}} \vec{F}\cdot d\vec{\ell}

where dℓ⃗d\vec{\ell} is the infinitesimal tangent vector along the path. Only the component of F⃗\vec{F} along the motion contributes: a force perpendicular to the velocity (the normal force on a slope, the magnetic force, the tension in a whirling string) does zero work. In general this integral depends on the whole path C\mathcal{C}, not merely on AA and BB — friction is the standard example, doing more negative work along a longer route.

2. The Work–Energy Theorem

Take the total force on a particle of mass mm and dot Newton's second law with the velocity:

F⃗net⋅v⃗=mdv⃗dt⋅v⃗=ddt(12m v⃗⋅v⃗)=ddt(12mv2)\vec{F}_{\text{net}}\cdot\vec{v} = m\frac{d\vec{v}}{dt}\cdot\vec{v} = \frac{d}{dt}\left(\tfrac{1}{2}m\,\vec{v}\cdot\vec{v}\right) = \frac{d}{dt}\left(\tfrac{1}{2}mv^2\right)

Integrating over time from AA to BB, and using v⃗ dt=dℓ⃗\vec{v}\,dt = d\vec{\ell} on the left,

 Wnet=∫ABF⃗net⋅dℓ⃗=12mvB2−12mvA2=ΔK \boxed{\,W_{\text{net}} = \int_A^B \vec{F}_{\text{net}}\cdot d\vec{\ell} = \tfrac{1}{2}mv_B^2 - \tfrac{1}{2}mv_A^2 = \Delta K\,}

The net work done by all forces equals the change in kinetic energy. This holds for any force whatsoever — conservative or not, constant or not — because it is just Newton's second law integrated. It is the workhorse for speed-at-a-point problems.

3. Path Independence and Conservative Forces

A force field F⃗(r⃗)\vec{F}(\vec{r}) is conservative if the work it does between any two points is independent of the path taken. Equivalently, the work around every closed loop is zero:

∮CF⃗⋅dℓ⃗=0for every closed C\oint_{\mathcal{C}} \vec{F}\cdot d\vec{\ell} = 0 \qquad\text{for every closed } \mathcal{C}

The physical content: a conservative force cannot be used to extract energy by running a particle around a cycle. Gravity, the electrostatic force and ideal spring forces are conservative; friction, air drag and the force from a person's muscles are not (they are dissipative or non-conservative).

4. Four Equivalent Statements

On a simply connected region, the following four statements about a force field F⃗\vec{F} are all equivalent — any one implies the other three:

  1. F⃗\vec{F} is conservative (work is path-independent).
  2. ∮F⃗⋅dℓ⃗=0\displaystyle\oint \vec{F}\cdot d\vec{\ell} = 0 around every closed loop.
  3. ∇×F⃗=0⃗\nabla\times\vec{F} = \vec{0} everywhere (the field is irrotational).
  4. F⃗=−∇U\vec{F} = -\nabla U for some single-valued scalar field UU (a potential energy exists).

The chain of implications: 2⇔12 \Leftrightarrow 1 by definition; 2⇒32 \Rightarrow 3 by shrinking the loop and invoking the curl-as-circulation-density interpretation, and 3⇒23 \Rightarrow 2 by Stokes' theorem; 1⇒41 \Rightarrow 4 by defining U(r⃗)=−∫r⃗0r⃗F⃗⋅dℓ⃗U(\vec{r}) = -\int_{\vec{r}_0}^{\vec{r}} \vec{F}\cdot d\vec{\ell} (well-defined precisely because the integral is path-independent), and 4⇒34 \Rightarrow 3 because the curl of a gradient is identically zero.

Test 3 is the practical one. Given a force field, compute its curl. If it vanishes identically, the force is conservative and a potential exists; if any component is non-zero anywhere, it is not.

5. Potential Energy and F⃗=−∇U\vec{F} = -\nabla U

When a potential energy exists, the work done by the conservative force is

WAB=∫ABF⃗⋅dℓ⃗=−∫AB∇U⋅dℓ⃗=−[U(B)−U(A)]=U(A)−U(B)W_{AB} = \int_A^B \vec{F}\cdot d\vec{\ell} = -\int_A^B \nabla U\cdot d\vec{\ell} = -\big[U(B) - U(A)\big] = U(A) - U(B)

by the gradient theorem. Combining with the work–energy theorem WAB=KB−KAW_{AB} = K_B - K_A (when only conservative forces act):

KA+U(A)=KB+U(B)⟹E=K+U=constantK_A + U(A) = K_B + U(B) \qquad\Longrightarrow\qquad E = K + U = \text{constant}

— conservation of mechanical energy. The relation F⃗=−∇U\vec{F} = -\nabla U inverts as U(r⃗)=−∫r⃗0r⃗F⃗⋅dℓ⃗U(\vec{r}) = -\displaystyle\int_{\vec{r}_0}^{\vec{r}} \vec{F}\cdot d\vec{\ell}, defined up to the arbitrary additive constant set by the choice of reference point r⃗0\vec{r}_0.

Worked example — three standard potentials.

  • Uniform gravity: F⃗=−mg z^\vec{F} = -mg\,\hat{z}. Then ∇×F⃗=0⃗\nabla\times\vec{F} = \vec{0}, and U=mgzU = mgz (taking U=0U = 0 at z=0z = 0), since −∂U/∂z=−mg-\partial U/\partial z = -mg.
  • Ideal spring: F=−kxF = -kx in 1D. Then U=12kx2U = \tfrac{1}{2}kx^2, since −dU/dx=−kx-dU/dx = -kx.
  • Inverse-square (gravitational/Coulomb): F⃗=−GMmr2 r^\vec{F} = -\dfrac{GMm}{r^2}\,\hat{r}. Using ∇g(r)=g′(r)r^\nabla g(r) = g'(r)\hat{r} backwards, U(r)=−GMmrU(r) = -\dfrac{GMm}{r} (with U→0U \to 0 as r→∞r \to \infty), since −dUdr=−GMmr2-\dfrac{dU}{dr} = -\dfrac{GMm}{r^2}. Its curl is zero everywhere it is defined, so it is conservative.

6. Worked Example: Testing a Field and Building Its Potential

Consider F⃗=(2xy+z3) x^+x2 y^+3xz2 z^\vec{F} = (2xy + z^3)\,\hat{x} + x^2\,\hat{y} + 3xz^2\,\hat{z} (units: newtons, with coordinates in metres). Is it conservative, and if so what is UU?

Curl test.

(∇×F⃗)z=∂(x2)∂x−∂(2xy+z3)∂y=2x−2x=0(\nabla\times\vec{F})_z = \frac{\partial(x^2)}{\partial x} - \frac{\partial(2xy + z^3)}{\partial y} = 2x - 2x = 0 (∇×F⃗)y=∂(2xy+z3)∂z−∂(3xz2)∂x=3z2−3z2=0(\nabla\times\vec{F})_y = \frac{\partial(2xy + z^3)}{\partial z} - \frac{\partial(3xz^2)}{\partial x} = 3z^2 - 3z^2 = 0 (∇×F⃗)x=∂(3xz2)∂y−∂(x2)∂z=0−0=0(\nabla\times\vec{F})_x = \frac{\partial(3xz^2)}{\partial y} - \frac{\partial(x^2)}{\partial z} = 0 - 0 = 0

The curl vanishes identically, so the force is conservative.

Constructing UU. From Fx=−∂U/∂xF_x = -\partial U/\partial x, integrate: U=−∫(2xy+z3) dx=−x2y−xz3+g(y,z)U = -\int(2xy + z^3)\,dx = -x^2 y - x z^3 + g(y,z). Then −∂U/∂y=x2−∂g/∂y-\partial U/\partial y = x^2 - \partial g/\partial y must equal Fy=x2F_y = x^2, so ∂g/∂y=0\partial g/\partial y = 0. And −∂U/∂z=3xz2−∂g/∂z-\partial U/\partial z = 3xz^2 - \partial g/\partial z must equal Fz=3xz2F_z = 3xz^2, so ∂g/∂z=0\partial g/\partial z = 0. Hence gg is a constant and

U(x,y,z)=−x2y−xz3+CU(x,y,z) = -x^2 y - x z^3 + C

7. Energy Diagrams and Equilibrium

For one-dimensional motion, plotting U(x)U(x) against xx gives the qualitative dynamics at a glance, because E=12mx˙2+U(x)E = \tfrac{1}{2}m\dot{x}^2 + U(x) is constant and 12mx˙2≥0\tfrac{1}{2}m\dot{x}^2 \ge 0:

  • Allowed region: motion is confined to xx where U(x)≤EU(x) \le E. Boundaries where U(x)=EU(x) = E are turning points (x˙=0\dot{x} = 0, then reverses).
  • Equilibrium: points where F=−dU/dx=0F = -dU/dx = 0, i.e. extrema of UU. A minimum of UU is stable (a displacement produces a restoring force); a maximum is unstable; a flat region is neutral.
  • Small oscillations: near a stable equilibrium x0x_0, Taylor-expand U(x)≈U(x0)+12U′′(x0)(x−x0)2U(x) \approx U(x_0) + \tfrac{1}{2}U''(x_0)(x - x_0)^2. The force is then F≈−U′′(x0)(x−x0)F \approx -U''(x_0)(x - x_0), simple harmonic motion with
ω=U′′(x0)m\omega = \sqrt{\frac{U''(x_0)}{m}}

Worked example. A particle of mass mm moves in U(x)=U0[(ax)12−2(ax)6]U(x) = U_0\left[\left(\dfrac{a}{x}\right)^{12} - 2\left(\dfrac{a}{x}\right)^{6}\right] (the Lennard-Jones form). Setting dU/dx=0dU/dx = 0: −12a12x13+12a6x7=0-12\dfrac{a^{12}}{x^{13}} + 12\dfrac{a^6}{x^7} = 0, giving x0=ax_0 = a. There U(a)=U0[1−2]=−U0U(a) = U_0[1 - 2] = -U_0 (the well depth). Differentiating again and evaluating at x0=ax_0 = a gives U′′(a)=72 U0a2U''(a) = \dfrac{72\,U_0}{a^2}, so small vibrations about the bottom of the well have angular frequency ω=72 U0ma2\omega = \sqrt{\dfrac{72\,U_0}{m a^2}}. A particle with energy −U0<E<0-U_0 < E < 0 is bound and oscillates between two turning points; a particle with E≥0E \ge 0 is unbound and escapes to x→∞x \to \infty.

8. Common Pitfalls

  • Applying energy conservation when a non-conservative force acts. If friction or drag is present, use Wnet=ΔKW_{\text{net}} = \Delta K with all forces, or ΔEmech=Wnon-cons\Delta E_{\text{mech}} = W_{\text{non-cons}}.
  • Forgetting the minus sign in F⃗=−∇U\vec{F} = -\nabla U. The force points toward decreasing potential energy — downhill on the UU landscape.
  • Assuming zero curl guarantees a potential on any domain. It does so only where the region is simply connected; a field like −y x^+x y^x2+y2\dfrac{-y\,\hat{x} + x\,\hat{y}}{x^2 + y^2} is irrotational but has no single-valued UU on a loop around the zz-axis.
  • Confusing a turning point with an equilibrium. At a turning point x˙=0\dot{x} = 0 but F≠0F \ne 0 (the particle accelerates away); at an equilibrium F=0F = 0.
  • Reading stability off the value of UU rather than its curvature. Stability depends on the sign of U′′U'', not on whether UU is positive or negative.
  • Dropping the arbitrary constant carelessly. UU is defined only up to an additive constant; differences U(A)−U(B)U(A) - U(B) and the equilibrium/oscillation analysis are what carry physical meaning.

Summary

  • Work is the line integral W=∫CF⃗⋅dℓ⃗W = \int_{\mathcal{C}} \vec{F}\cdot d\vec{\ell}; only the tangential component of F⃗\vec{F} contributes, and in general the value depends on the path.
  • Work–energy theorem: Wnet=ΔKW_{\text{net}} = \Delta K, true for every force, being Newton's second law dotted with v⃗\vec{v} and integrated.
  • A conservative force does path-independent work, equivalently zero work around every closed loop.
  • Four equivalent tests (simply connected domain): path-independence ⇔\Leftrightarrow ∮F⃗⋅dℓ⃗=0\oint\vec{F}\cdot d\vec{\ell} = 0 ⇔\Leftrightarrow ∇×F⃗=0⃗\nabla\times\vec{F} = \vec{0} ⇔\Leftrightarrow F⃗=−∇U\vec{F} = -\nabla U. The curl test is the practical one.
  • F⃗=−∇U\vec{F} = -\nabla U gives WAB=U(A)−U(B)W_{AB} = U(A) - U(B) and hence E=K+U=constE = K + U = \text{const} when only conservative forces act. U=−∫F⃗⋅dℓ⃗U = -\int \vec{F}\cdot d\vec{\ell}, up to a constant.
  • Standard potentials: U=mgzU = mgz (uniform gravity), U=12kx2U = \tfrac{1}{2}kx^2 (spring), U=−GMm/rU = -GMm/r (inverse square).
  • Energy diagrams: motion confined to U(x)≤EU(x) \le E; turning points where U=EU = E; equilibria at extrema of UU (minimum stable, maximum unstable); small oscillations at ω=U′′(x0)/m\omega = \sqrt{U''(x_0)/m}.