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Conservative Forces and Potential Energy

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Conservative Forces and Potential Energy

A force can transfer energy to or from a particle by doing work. For a special and very important class of forces, the work between two positions depends only on the endpoints and not on the path followed between them. Such a force is called conservative.

For a conservative force, the work done from point A to point B can be represented by a scalar function of position called the potential energy U:

|--------------------------------|
W  (A  → B ) = − [U (B) − U (A)].|
---c------------------------------
(1)

Equivalently,

|------------|
|ΔU  = − Wc. |
--------------
(2)

This relation is the central idea of the article. It turns certain force calculations into energy bookkeeping and prepares the way for conservation of mechanical energy.

PIC

Figure 1. For a conservative force, all paths joining the same two endpoints give the same work. Path independence allows the work to be represented by a scalar potential-energy difference.

1 What makes a force conservative?

A force is conservative if the work it does between two fixed positions is independent of the path.

If a particle moves from point A to point B along two different paths C1 and C2, then a conservative force satisfies

∫           ∫
   F ⋅ dr =    F  ⋅ dr.
 C1          C2
(3)

Therefore the work can depend only on the endpoints A and B.

This is a strong restriction. Many familiar forces are conservative in idealized mechanics, including

  • uniform gravity near Earth’s surface,
  • Newtonian inverse-square gravity,
  • the force of an ideal spring,
  • the electrostatic Coulomb force.

Common examples of nonconservative forces include kinetic friction and many forms of drag.

2 Closed-path test

Suppose a conservative force carries a particle from A to B along one path and the particle returns from B to A along another path.

Because the work between fixed endpoints is path independent,

W (A →  B ) = − W (B →  A ).
(4)

Therefore the total work around the closed path is zero:

|∮-------------|
|              |
| C F ⋅ dr = 0.|
---------------
(5)

For the class of force fields considered in elementary mechanics, the following statements are equivalent:

  1. the work between two points is path independent,
  2. the work around every closed path is zero,
  3. a potential-energy function can be defined,
  4. the force can be obtained from the spatial derivative of that potential energy.

The last statement will be developed carefully below.

3 Defining potential-energy difference

Let a conservative force do work

Wc (A  → B ).
(6)

Define the change in potential energy by

|--------------------------|
|UB − UA  = − Wc (A →  B ).|
---------------------------
(7)

Thus

|------------|
|ΔU  = − Wc. |
--------------
(8)

The minus sign is essential.

If the conservative force does positive work,

Wc >  0,
(9)

then

ΔU   < 0.
(10)

The potential energy decreases.

If the conservative force does negative work,

Wc <  0,
(11)

then

ΔU   > 0.
(12)

The potential energy increases.

PIC

Figure 2. Positive work by a conservative force corresponds to decreasing potential energy. Negative work by the force corresponds to increasing potential energy.

4 Potential energy is defined up to a constant

Only differences in potential energy are determined by force.

If U(r) is a valid potential-energy function, then

U ′(r) = U (r) + C
(13)

is equally valid for any constant C.

This is because

U′B − U′A = (UB + C) − (UA + C) (14)
= UB − UA. (15)

Therefore the physics is unchanged.

One is free to choose a convenient reference level at which

U  = 0.
(16)

For uniform gravity near Earth’s surface, the reference height can be chosen arbitrarily. For Newtonian gravity, a common and useful convention is

U (∞ ) = 0.
(17)

5 One-dimensional force from potential energy

In one-dimensional motion,

dU =  − F dx.
         x
(18)

Divide by dx:

|------------|
|       dU   |
|Fx = − --- .|
---------dx--
(19)

This equation contains a powerful geometric idea.

The force points in the direction in which potential energy decreases most rapidly.

If

dU-
dx  > 0,
(20)

then

Fx < 0.
(21)

If

dU- < 0,
dx
(22)

then

F  > 0.
 x
(23)

If

dU- = 0,
dx
(24)

then

F  = 0.
 x
(25)

PIC

Figure 3. In one dimension, force is minus the slope of the potential-energy curve. A positive slope produces force toward negative x, while a negative slope produces force toward positive x.

6 Recovering potential energy from force

If the force is known, potential energy can be found by integration.

From

dU  = − Fx(x )dx,
(26)

integrate from a reference point x0 to x:

                  ∫
                    x     ′   ′
U(x) − U (x0) = −     Fx(x )dx .
                   x0
(27)

Therefore

|----------------∫-------------|
|                  x     ′   ′ |
|U(x ) = U (x0) −    Fx(x )dx .|
------------------x0------------
(28)

The variable x′ is a dummy integration variable. It prevents confusion between the integration variable and the endpoint x.

7 Example 1: constant force

Suppose

Fx = F0
(29)

is constant.

Then

U(x) − U(x0) = −∫ x0xF 0 dx′ (30)
= −F0(x − x0). (31)

Thus

U(x) = − F0x + C,
(32)

where

C  = U (x0) + F0x0.
(33)

A constant force therefore corresponds to a linear potential-energy function.

8 Uniform gravity near Earth’s surface

Near Earth’s surface, take the y axis positive upward.

The gravitational force on a mass m is

Fg = − mg  ey.
(34)

In one dimension,

Fy =  − mg.
(35)

The potential-energy derivative satisfies

       dU
Fy = − ---g.
        dy
(36)

Therefore

          dUg-
− mg  = −  dy ,
(37)

so

dUg
---- = mg.
 dy
(38)

Integrating,

|------------------|
|Ug(y) = mgy  + C. |
-------------------
(39)

If the zero of potential energy is chosen at y = 0, then

|----------|
Ug  = mgy. |
------------
(40)

The difference between two heights is

|--------------------|
|ΔU   = mg (y  − y ).|
----g--------f----i--
(41)

The work done by gravity is

-----------------------------
|                            |
-Wg--=-−-ΔUg--=-mg-(yi −-yf).|
(42)

PIC

Figure 4. Near Earth’s surface, gravitational potential energy increases linearly with height. Gravity points downward, toward decreasing potential energy.

9 Example 2: lifting a mass

A 3.0 kg mass is raised vertically from yi = 1.0 m to yf = 6.0 m.

The change in gravitational potential energy is

ΔUg = mg(yf − yi) (43)
= (3.0)(9.81)(5.0) (44)
= 147 J. (45)

Therefore gravity does

W   = − 147 J.
  g
(46)

The result depends only on the change in height. It does not depend on whether the mass moved vertically, along a ramp, or along some other path, provided gravity is the same uniform conservative field.

10 Elastic potential energy of an ideal spring

For an ideal spring,

Fx  = − kx.
(47)

Use

       dUs-
Fx = −  dx .
(48)

Then

         dUs
− kx = − ----,
          dx
(49)

so

dUs-=  kx.
dx
(50)

Integrating,

         1   2
Us (x) = 2kx  +  C.
(51)

Choosing

Us(0) = 0
(52)

gives

|--------------|
|        1-  2 |
|Us(x) = 2 kx .|
----------------
(53)

This is the elastic potential energy stored by an ideal spring.

PIC

Figure 5. The ideal-spring potential Us = 1
2kx2 has a minimum at equilibrium. The force Fx = −dU∕dx = −kx always points back toward x = 0.

11 Work and spring potential energy

The spring work from xi to xf is

Ws  = − ΔUs.
(54)

Therefore

Ws = −(             )
  1-  2   1- 2
  2kx f − 2kxi (55)
= 1-
2kxi2 −1-
2kxf2 . (56)

This reproduces the result derived directly from the work integral in M03-03.

The energy viewpoint and the force-integral viewpoint are not separate physical laws. They are two descriptions of the same conservative interaction.

12 Newtonian gravitational potential energy

Consider two masses M and m separated by distance r.

The gravitational force on m is radial and inward:

        GM--m--
Fg =  −   r2  er.
(57)

For radial motion,

        GM  m
Fr =  − ---2--.
          r
(58)

The potential satisfies

Fr = − dU- .
        dr
(59)

Thus

  GM--m--    dU-
−   r2   = −  dr ,
(60)

so

dU- = GM---m-.
dr       r2
(61)

Integrating,

          GM  m
U (r) = − -------+ C.
            r
(62)

With the standard reference

U (∞ ) = 0,
(63)

we obtain

-------------------
|          GM  m   |
|Ug(r) = − -------.|
--------------r----|
(64)

The negative sign reflects the chosen zero at infinite separation. At any finite separation, the gravitational potential energy is lower than at infinity.

13 Why near-Earth gravity gives mgy

The inverse-square potential is

U (r) = − GM--m-.
            r
(65)

Near Earth’s surface, write

r = RE +  y,
(66)

where

|y | ≪ RE.
(67)

A first-order expansion gives

---1----   -1--  -y--
RE  + y ≈  RE  − R2E.
(68)

Therefore

U(RE + y) ≈−GM--m--
  RE + GM--m--
 R2Ey. (69)

Since

    GM
g = ---2-,
     R E
(70)

this becomes

               GM   m
U (RE  + y) ≈ − -------+ mgy.
                 RE
(71)

The first term is a constant reference offset, so locally

|--------------|
|ΔU  ≈  mg Δy. |
---------------
(72)

Thus the familiar near-Earth formula is the local approximation to the inverse-square gravitational potential.

14 Potential energy in several dimensions

In three-dimensional Cartesian coordinates,

F  = Fxex + Fyey +  Fzez.
(73)

For a conservative force,

dU =  − F ⋅ dr.
(74)

Since

dr = dx e +  dye  + dz e ,
         x      y       z
(75)

we have

dU =  − Fxdx −  Fy dy − Fz dz.
(76)

But the total differential of U(x,y,z) is

      ∂U--     ∂U--    ∂U--
dU =  ∂x dx +  ∂y dy +  ∂z dz.
(77)

Comparing coefficients,

Fx = −∂U
----
∂x, (78)
Fy = −∂U--
∂y, (79)
Fz = −∂U
----
∂z. (80)

Therefore

|----------|
F  = − ∇U. |
------------
(81)

The gradient is

       ∂U      ∂U      ∂U
∇U  =  ---ex + ---ey + ----ez.
       ∂x      ∂y       ∂z
(82)

The force points toward decreasing potential energy.

15 Equipotential surfaces

A surface on which

U =  constant
(83)

is called an equipotential surface.

For a displacement tangent to an equipotential surface,

dU =  0.
(84)

Since

dU =  − F ⋅ dr,
(85)

we obtain

F  ⋅ dr = 0.
(86)

Thus the conservative force is perpendicular to an equipotential surface.

For Newtonian gravity around a spherical mass, the equipotential surfaces are spheres centered on the mass.

16 Potential-energy curves

In one-dimensional problems, a graph of U(x) reveals important dynamical information.

Because

       dU
Fx = − -dx ,
(87)

the slope tells us the force direction.

A local minimum of U satisfies

dU- = 0
dx
(88)

and typically corresponds to stable equilibrium.

A local maximum also satisfies

dU-
dx  = 0,
(89)

but it typically corresponds to unstable equilibrium.

PIC

Figure 6. Equilibrium occurs where dU∕dx = 0. A local minimum corresponds to stable equilibrium, while a local maximum corresponds to unstable equilibrium.

17 Stable equilibrium

Suppose x = x0 is a local minimum of the potential energy.

Then

   |
dU-||
dx |  = 0,
    x0
(90)

so

F (x0) = 0.
(91)

For a small displacement to the right of x0, the potential rises:

dU-
dx  > 0.
(92)

Therefore

Fx < 0,
(93)

which points back toward equilibrium.

For a small displacement to the left,

dU
--- < 0,
dx
(94)

so

Fx > 0,
(95)

again pointing back toward equilibrium.

This is why a potential-energy minimum is stable.

A mathematical test is

|----------------------------|
-U-′(x0)-=-0,-----U-′′(x0-) >-0.|
(96)

18 Unstable equilibrium

At a local maximum,

  ′
U (x0) = 0,
(97)

but

U ′′(x0) < 0.
(98)

A small displacement produces a force that pushes the particle farther away from the equilibrium point.

Thus a local maximum corresponds to unstable equilibrium.

19 Example 3: equilibrium from a potential

Let

U (x ) = ax4 − bx2,
(99)

where

a >  0,    b > 0.
(100)

Equilibrium occurs where

dU-
dx  = 0.
(101)

Differentiate:

dU        3
--- = 4ax  − 2bx.
dx
(102)

Factor:

dU- = 2x (2ax2 − b).
dx
(103)

Thus the equilibria are

x = 0
(104)

and

      ∘ ---
        -b-
x = ±   2a .
(105)

The second derivative is

U′′(x ) = 12ax2 − 2b.
(106)

At

x = 0,
(107)

we have

U ′′(0) = − 2b < 0,
(108)

so the origin is unstable.

At

      ∘ ---
         b
x = ±   ---,
        2a
(109)

we obtain

U′′ = 12a(   )
   b
  2a-− 2b (110)
= 4b > 0. (111)

These two equilibria are stable.

20 Conservative and nonconservative forces

A conservative force stores and releases mechanical energy through a potential-energy function.

A nonconservative force generally cannot be represented globally by a single-valued position-only potential energy.

For example, kinetic friction usually does

Wf  < 0
(112)

over a path of nonzero length.

If the particle returns to its starting position after traveling around a loop, friction has generally done net negative work:

∮
  F  ⋅ dr < 0.
    f
(113)

Therefore friction fails the closed-path test for a conservative force.

The energy removed from mechanical motion is not destroyed. It is transferred into thermal energy, deformation, sound, and microscopic degrees of freedom.

21 Path independence versus path length

A common source of confusion is to think that conservative work depends on path length.

It does not.

Consider uniform gravity. A particle may descend from height yi to height yf by

  • falling vertically,
  • sliding along a straight incline,
  • moving along a curved track.

If only the gravitational work is being calculated, all three paths give

Wg =  mg (yi − yf).
(114)

The actual distances traveled can be different, but the gravitational work depends only on the endpoint heights.

22 Dimensional checks

Potential energy has the same dimensions as work:

[U] = M L2T − 2.
(115)

For uniform gravity,

U =  mgy,
(116)

so

         ( L )
[U] = M    -2- L  = M L2T − 2.
           T
(117)

For a spring,

     1
U  = --kx2.
     2
(118)

Since

[k ] = F-=  M T −2,
      x
(119)

we obtain

[kx2] = M L2T − 2.
(120)

For inverse-square gravity,

       GM--m--
U =  −   r   ,
(121)

which also has units of joules.

23 Common mistakes

  1. Forgetting the minus sign in ΔU = −Wc.
  2. Assuming every force has a potential-energy function.
  3. Treating the absolute value of potential energy as physically unique.
  4. Forgetting that only potential-energy differences affect mechanics.
  5. Writing F = dU∕dx instead of F = −dU∕dx.
  6. Confusing stable equilibrium with any point where U′(x) = 0.
  7. Assuming a local maximum of U is stable.
  8. Using mgy over altitude ranges where constant g is no longer a good approximation.
  9. Forgetting that U = −GMm∕r uses the reference U(∞) = 0.
  10. Assuming path-independent gravitational work means the particle travels the same distance along every path.
  11. Treating frictional work as if it could be represented by a position-only potential energy.

24 Practice exercises

  1. A conservative force does +25 J of work on a particle. Find the change in potential energy.
  2. A conservative force does −18 J of work. Does the potential energy increase or decrease, and by how much?
  3. A force has potential energy U(x) = 4x2 in SI units. Find F x(x).
  4. A force is Fx = −6x2. Find a corresponding potential-energy function U(x).
  5. A 2.0 kg mass moves upward by 3.0 m near Earth’s surface. Find ΔUg.
  6. A spring with k = 250 N∕m is compressed by 0.12 m. Find its elastic potential energy relative to equilibrium.
  7. Starting from Fx = −kx, derive Us = 1
2kx2 + C.
  8. Starting from Fr = −GMm∕r2, derive U g = −GMm∕r + C.
  9. Show that adding a constant C to a potential-energy function does not change the force.
  10. For U(x) = ax4 − bx2 with a,b > 0, classify all equilibrium points.
  11. Explain why the gravitational work between two fixed heights is the same on a straight ramp and a curved track.
  12. A particle moves around a closed loop under a force field. The measured net work is 12 J. Can the force be conservative? Explain.
  13. A potential-energy curve has negative slope at some point. What is the sign of the force there?
  14. For U(x) = U0 cos(kx), derive Fx(x) and identify equilibrium positions.
  15. Explain physically why a local minimum of potential energy corresponds to stable equilibrium.

25 Summary

A conservative force does path-independent work:

|--------------------|
Wc-(A-→--B-)-=-−-ΔU.--
(122)

Equivalently,

|------------|
-ΔU--=-−-Wc.--
(123)

For a conservative force around a closed path,

|∮-------------|
|              |
|   F ⋅ dr = 0.|
--C------------
(124)

In one dimension,

|------------|
|F  = − dU- .|
--x------dx--|
(125)

In three dimensions,

|----------|
F  = − ∇U. |
------------
(126)

Important examples are

|----------|
|Ug = mgy  |
------------
(127)

near Earth’s surface,

|----------|
|     1-  2|
Us =  2kx  |
------------
(128)

for an ideal spring, and

|----------------|
Ug (r) = − GM--m-|
-------------r----
(129)

for Newtonian gravity with U(∞) = 0.

Potential-energy curves also reveal force direction and equilibrium:

|----------|
U ′(x0) = 0|
------------
(130)

at equilibrium, with

|-----------|
U ′′(x ) > 0 |
-----0-------
(131)

for stable equilibrium.

The next article, M03-06, combines kinetic and potential energy into the conservation of mechanical energy.

References

References

[1]   J. R. Taylor, Classical Mechanics, University Science Books, 2005.

[2]   D. Kleppner and R. Kolenkow, An Introduction to Mechanics, 2nd ed., Cambridge University Press, 2014.

[3]   H. Goldstein, C. Poole, and J. Safko, Classical Mechanics, 3rd ed., Addison-Wesley, 2002.

[4]   H. D. Young and R. A. Freedman, University Physics with Modern Physics, 15th ed., Pearson, 2020.

[5]   OpenStax, University Physics, Volume 1, Rice University, 2016.


"Conservative Forces and Potential Energy" is owned by bloftin.
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Also defines:  conservative force, potential energy, potential-energy difference, path independence, conservative field
Keywords:  conservative force, potential energy, path independence, closed path, work, gravitational potential energy, elastic potential energy, spring, potential-energy curve, force from potential, gradient

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GRE Physics Companion: Conservative Forces and Potential Energy (Example) by bloftin

Cross-references: net work, units, degrees of freedom, deformation, friction, graph, displacement, gradient, Cartesian coordinates, formula, physical laws, M03-03, work integral, equilibrium, mass, dimension, motion, fields, drag, kinetic friction, mechanics, relation, function, scalar, positions, work, particle, energy, force
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Physics Classification: 45.20.Dd (Newtonian mechanics)
 45.50.-j (Dynamics and kinematics of a particle and a system of particles)
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