Mechanics of particles and systems Definition
Potential energy
Builds on Conservative vector fieldGradient
Definition
Let be open and let be a continuous force field. A potential energy for is a function of class such that where is the gradient of . For particles in , take , so that and the force on particle is .
Remarks
A potential energy exists exactly when is a conservative vector field, and then is a scalar potential of . On a connected set , the potential energy is unique up to an additive constant. Example: uniform gravity on has the potential energy , since . A spring force with has . Non-example: the field has no potential energy on , since its line integral around the unit circle in the plane is .
Reading path
To understand this page from the ground up, read these 18 pages in order. The foundations come first.
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- no evidence level
- Euclidean space object
- Function concept
- Fréchet derivative definition
- Function of several variables concept
- Vector-valued function concept
- Limit of a function of several variables concept
- Partial derivative concept
- Continuity in R^n definition
- Differentiable function of several variables definition
- Partial derivative definition
- Gradient definition
- Differentiable on an open set definition
- Higher partial derivatives definition
- Iterated derivative definition
- C^k function characterised by continuous derivatives statement
- Vector field definition
- Conservative vector field definition
- Potential energy definition
Where this leads
84 pages build on this one.
- Emden–Chandrasekhar equation
- Newton's law of universal gravitation
- Chandrasekhar's white dwarf equation
- Dedekind ellipsoid
- Hydrostatic equilibrium
- Tidal force
- Magnetic braking
- Virial theorem
- Tests of general relativity
- Milankovitch cycles
- Stellar structure
- Modified Newtonian dynamics
- Kelvin–Helmholtz mechanism
- Hohmann transfer orbit
- Central configuration
- Schwarzschild criterion for convection
- Virial mass
- von Zeipel theorem
- Jacobi integral
- Galaxy rotation curve
- Celestial mechanics
- Weak gravitational lensing
- Kepler's equation
- Bi-elliptic transfer
- Mass–luminosity relation
- Accretion disk
- Conservation of energy
- Einstein–Infeld–Hoffmann equations
- Lens equation
- Two-body problem
- Ledoux criterion
- Orbital mechanics
- Bonnor–Ebert mass
- Tolman–Oppenheimer–Volkoff limit
- Post-Newtonian expansion
- Adams–Williamson equation
- Tisserand's parameter
- Polytrope
- Gravitational microlensing
- Hayashi track
- Stellar pulsation
- Euler's three-body problem
- Conservation of angular momentum
- Parker solar wind model
- Escape velocity
- Chandrasekhar limit
- Tidal acceleration
- Gravitational deflection of light
- Maclaurin spheroid
- Jacobi integral
- Kepler's laws of planetary motion
- Dynamical friction
- Mixing length theory
- Kepler's equation
- Kepler orbit
- Hill sphere
- Spherical astronomy
- Roche limit
- Mechanical similarity
- Schönberg–Chandrasekhar limit
- Geopotential
- N-body simulation
- Celestial mechanics
- Vogt–Russell theorem
- Eddington luminosity
- Hill sphere
- Barnes–Hut simulation
- Vis-viva equation
- Stellar dynamics
- Parker instability
- Central force
- Einstein radius
- Sitnikov problem
- Free-fall time
- Jacobi ellipsoid
- Lagrange points
- Two-body relaxation time
- Parker spiral
- Newtonian limit
- Strong gravitational lensing
- Einstein ring
- Circular restricted three-body problem
- Bullen parameter
- Roche lobe
Further reading
About this page
| Tag | 5T5GAKQD3S |
|---|---|
| URI | m2://5T5GAKQD3S |
| Kind | definition |
| Writing | W0 stub |
| MSC | 70A05, 70F10 |
| Defines | Potential energy |
| Uses | Conservative vector field, Gradient |
| Changed | 3 November 2026 |
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