Potential Energy
The Physics Hypertextbook™
© 1998-2008 by Glenn Elert -- A Work in Progress
All Rights Reserved -- Fair Use Encouraged
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Discussion
W J M Rankine coined the term potential energy 150 years ago.
gravitational potential energy
ΔU = mgΔh
- acceleration due to gravity is nearly constant
- height change is small compared to the separation between centers
the more general form will be dealt with later
work-energy theorem, two possibilities
- conservative forces
- work done is independent of path
- W = ∮ F·dr = 0
- can be associated with a potential energy function
- nonconservative forces
- work done depends on path
- W = ∮ F·dr > 0
- cannot be associated with a potential energy function
force and potential energy
| one-dimensional |
|
three-dimensional |
|
compact notation |
| F(r) = − |
dU |
|
|
F(r) = − |
∂U |
ˆi − |
∂U |
ˆj − |
∂U |
ˆk |
F(r) = − ∇U |
| dr |
∂x |
∂y |
∂z |
constant total energy, horizontal line above curve, kinetic energy is difference between line and curve
bounded and unbounded states, binding energy
stability of equilibrium
| stable equilibrium |
unstable equilibrium |
neutral equilibrium |
| [diagram] |
[diagram] |
[diagram] |
| local maximum |
local minimum |
constant potential energy |
Summary
- Potential energy …
- is energy associated with position in a field (a force that exists at many locations)
- comes in four fundamental types, one for each of the fundamental forces, and several subtypes
- gravitational
- electromagnetic
- electrostatic
- chemical
- elastic
- strong
- primary: between quarks, within nucleons (and other hadrons)
- residual: between nucleons, within the nucleus
- weak
- Gravitational potential energy
- can be computed through one of two formulas
| |
|
| the simplified formula |
the more general formula |
| ΔU = mgΔh |
|
| assumes that |
is dealt with in a later section of this book |
- acceleration due to gravity is nearly constant
- height change is small compared to the separation between
centers
|
| |
- Forces and Potential Energy
- nonconservative forces
- work done depends on path
- W = ∮ F·dr > 0
- cannot be associated with a potential energy function
- conservative forces
- work done is independent of path
- W = ∮ F·dr = 0
- can be associated with a potential energy function
- Forces and Potential Energy
- work is the force-displacement integral
- this is the work energy theorem
- a conservative force is the gradient of potential energy
| |
|
|
|
|
| one-dimensional |
|
three-dimensional |
|
compact notation |
| F(r) = − |
dU |
|
|
F(r) = − |
∂U |
ˆi − |
∂U |
ˆj − |
∂U |
|
F(r) = − ∇U |
| dr |
∂x |
∂y |
∂z |
| |
|
|
|
|
- Potential energy curves (or surfaces, or their higher order equivalents) are useful problem solving tools
- motion of a particle in a field
- constant total energy, horizontal line above curve
- kinetic energy is difference between line and curve
- bound and unbound states, binding energy
- stability of equilibrium
| |
|
|
| stable equilibrium |
unstable equilibrium |
neutral equilibrium |
| [diagram] |
[diagram] |
[diagram] |
| local maximum |
local minimum |
constant potential energy |
| |
|
|
Problems
practice
- Write something.
- Write something else.
- Calculate the gravitational potential energy released by the collapse of the World
Trade Center in New York City on 11 September 2001. Each 110 story
tower had a mass of about 550,000,000 kg and a height of 415 m (not
including the broadcast tower). Compare this to the energy released on 8 March 1993
when a truck carrying a fertilizer bomb exploded in the underground parking garage
of this same complex. Assume an explosive yield equivalent to a half ton of TNT.
(One ton of TNT has 4.184 × 109 J of chemical potential
energy.)
Solution …
Since the mass of the towers is distributed throughout their volume and
is not concentrated at a point, this problem is best solved using calculus.
Assume a uniform linear mass density and integrate the potential energy
formula over the height of the towers. Not surprisingly, the results show
that the center of mass of a tower lies at its geometric center, halfway
up.
| h = |
415 m |
| m = |
2(550,000,000 kg) = 1.1 × 109 kg |
| |
h |
|
h |
|
| Ug = |
⌠ ⌡ |
ρgy dy = |
mg |
⌠ ⌡ |
y dy = |
mg |
|
h2 |
= |
mgh |
|
| h |
h |
2 |
2 |
| |
0 |
|
0 |
|
| Ug = |
(1.1. × 109 kg)(9.8 m/s2)(415 m) |
|
| 2 |
|
| Ug = |
2.2 × 1012 J |
1 ton TNT |
= 530 ton TNT |
| 4.184 × 109 J |
The gravitational energy released when the towers collapsed was thus about
a thousand times greater than the chemical energy released when the truck
bomb exploded.
- Write something completely different.
numerical
- Determine the gravitational potential energy of a guillotine if the mouton
(the weighted blade) has a mass of 40 kg and is raised 2.5 m above
the neck of the condemned.
algebraic
- It's possible, but quite difficult, to balance an egg on it's end. It's
also possible, but even more difficult, to balance an egg on an egg. Say
you
had the talent and patience to balance a dozen eggs of mass m and
height h, one on top of the other. What potential energy would this
column of eggs have?
calculus
- The Great Pyramid of Cheops was built on the Ghiza Plateau just outside
of what is now Cairo, Egypt some time between 2589 and 2566 BCE. It serves
as the final resting place of the Pharaoh Cheops (also known as Khufu). As
its name suggests, the Great Pyramid is the largest structure of its kind
in the world. Determine the gravitational potential energy of the Great Pyramid
with respect to its base given the following dimensions:
- height: 136 m
- base: square, 230 m on a side
- top: square, 10 m on a side
- number of blocks: 2.3 million
- mass per block: 2.5 tons (average)
- Fun Functions!
|
| a. |
|
|
|
r > 0 |
|
b > a > 0 |
|
a combination of gravitational and centrifugal forces, used for satellite orbits |
|
| b. |
|
|
|
r > 0 |
|
a, b > 0 |
|
partly inverse and partly linear, not used for anything, just for practice |
|
| c. |
|
| U(r) = 4a |
⎡ ⎣ |
⎛ ⎝ |
b |
⎞12 ⎠ |
− |
⎛ ⎝ |
b |
⎞6 ⎠ |
⎤ ⎦ |
| r |
r |
|
|
r > 0 |
|
a, b > 0 |
|
the lennard-jones potential, a simplified model of interatomic forces |
|
| d. |
|
|
|
r > 0 |
|
|
|
partly inverse and partly quadratic, not used for anything, just for practice |
|
| e. |
|
| U(r) = |
1 |
+ |
20 |
| r |
(r − 3)2 + 2 |
|
|
r > 0 |
|
|
|
something like a dissociation reaction |
|
| f. |
|
U(x) = x3 − 3x2 − 6x + 8 |
|
− ∞ < x < + ∞ |
|
a cubic function, not used for anything, just for practice |
|
| g. |
|
| U(x) = |
4 |
− |
6 |
| x2 + 1 |
(4x)2 + 1 |
|
|
− ∞ < x < + ∞ |
|
attractive for short distances, repulsive for long distances |
|
| h. |
|
| U(x) = − |
1 |
− |
1 |
− |
1 |
| (x + 2)2 |
(x + 0)2 |
(x − 2)2 |
|
|
− ∞ < x < + ∞ |
|
three atoms in a row |
|
Resources
- general
- The Mechanical Universe and Beyond (video on demand, login required)
- Potential Energy, Potential energy provides a powerful model for understanding why the world has worked the same way since the beginning of time.
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