Mechanics of particles and systems Definition
Classical mechanics
Builds on Euclidean spaceOrdinary differential equationPicard–Lindelöf theorem
Definition
A Newtonian system of point particles consists of the following data.
- Masses .
- For each , a position at time , where is three-dimensional Euclidean space.
- For each , a force law , a function of the time , of all positions and of all velocities .
A motion of the system is a twice differentiable map on an interval that solves the ordinary differential equations Classical mechanics, in its Newtonian form, is the study of such systems and their motions.
Remarks
Example: one particle of mass under the constant force with . The map is a motion, since . Non-example: the map is not a motion of this system, since . If the force laws are locally Lipschitz, the Picard–Lindelöf theorem shows that the initial positions and velocities determine the motion on some interval. A dot over a symbol denotes the derivative with respect to time.
Reading path
To understand this page from the ground up, read these 15 pages in order. The foundations come first.
Show the path as a graph
- no evidence level
- Differential equation concept
- Euclidean space object
- Function concept
- Interval concept
- Ordinary differential equation concept
- Ordinary differential equation definition
- Lipschitz condition definition
- Solution of an ordinary differential equation definition
- Initial value problem definition
- Picard–Lindelöf hypotheses definition
- Picard operator definition
- Integral equation form of an initial value problem statement
- An iterate of the Picard operator is a contraction statement
- Picard–Lindelöf theorem statement
- Classical mechanics definition
Where this leads
96 pages build on this one.
- Emden–Chandrasekhar equation
- Newton's law of universal gravitation
- Chandrasekhar's white dwarf equation
- Dedekind ellipsoid
- Hydrostatic equilibrium
- Kinetic energy
- Tidal force
- Friction
- 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
- Galilean invariance
- Mass–luminosity relation
- Accretion disk
- Conservation of energy
- Einstein–Infeld–Hoffmann equations
- Lens equation
- Inelastic collision
- Two-body problem
- Ledoux criterion
- Orbital mechanics
- Bonnor–Ebert mass
- Tolman–Oppenheimer–Volkoff limit
- Post-Newtonian expansion
- Adams–Williamson equation
- Tisserand's parameter
- Polytrope
- Angular momentum
- Gravitational microlensing
- Tsiolkovsky rocket equation
- Hayashi track
- Stellar pulsation
- Euler's three-body problem
- Conservation of angular momentum
- Parker solar wind model
- Impulse
- Momentum
- Escape velocity
- Chandrasekhar limit
- Tidal acceleration
- Gravitational deflection of light
- Maclaurin spheroid
- Coefficient of restitution
- Jacobi integral
- Kepler's laws of planetary motion
- Dynamical friction
- Mixing length theory
- Kepler's equation
- Kepler orbit
- Hill sphere
- Spherical astronomy
- Roche limit
- Schönberg–Chandrasekhar limit
- Geopotential
- N-body simulation
- Celestial mechanics
- Vogt–Russell theorem
- Eddington luminosity
- Hill sphere
- Elastic collision
- Barnes–Hut simulation
- Vis-viva equation
- Work–energy theorem
- Stellar dynamics
- Conservation of momentum
- Variable-mass system
- 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 | SH7J0X3NCC |
|---|---|
| URI | m2://SH7J0X3NCC |
| Kind | definition |
| Writing | W0 stub |
| MSC | 70A05, 70F10 |
| Defines | Classical mechanics |
| Uses | Euclidean space, Ordinary differential equation, Picard–Lindelöf theorem |
| Changed | 3 November 2026 |
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