Newtonian gravitational cosmology
E453397
Newtonian gravitational cosmology is a classical framework that applies Newton’s law of universal gravitation to model the large-scale structure, dynamics, and evolution of the universe before the advent of general relativity.
Observed surface forms (2)
| Surface form | Occurrences |
|---|---|
| Newtonian cosmology | 1 |
| Newtonian gravity by incorporating special relativity | 1 |
Statements (50)
| Predicate | Object |
|---|---|
| instanceOf |
classical theory
ⓘ
cosmological model ⓘ physical framework ⓘ |
| appliesTo |
dynamics of the universe
ⓘ
evolution of the universe ⓘ large-scale structure of the universe ⓘ |
| approximates |
general relativistic cosmology at low redshift
ⓘ
general relativistic cosmology on small scales ⓘ |
| assumes |
Euclidean space
ⓘ
absolute space ⓘ absolute time ⓘ action-at-a-distance gravitational interaction ⓘ |
| basedOn |
Newtonian gravity
NERFINISHED
ⓘ
Newtonian mechanics NERFINISHED ⓘ Newton’s law of universal gravitation NERFINISHED ⓘ |
| canApproximate | Friedmann–Lemaître–Robertson–Walker cosmology at low speeds ⓘ |
| canDerive | Friedmann-like expansion equations ⓘ |
| cannotDescribe |
cosmological horizons
ⓘ
gravitational waves ⓘ relativistic effects ⓘ |
| contrastsWith | relativistic cosmology ⓘ |
| facesProblem |
divergent gravitational potential in infinite homogeneous matter distribution
ⓘ
lack of consistent treatment of global spatial curvature ⓘ |
| hasLimitation |
incompatibility with finite propagation speed of gravity
ⓘ
no natural inclusion of a cosmological constant ⓘ |
| historicallyUsedFor |
Jeans instability analysis
ⓘ
early models of an expanding universe ⓘ studies of gravitational instability ⓘ |
| inspiredBy | Isaac Newton’s gravitational theory NERFINISHED ⓘ |
| involves |
gravitational potential field
ⓘ
mass density field ⓘ pressureless matter approximation ⓘ |
| models |
dust-filled universe
ⓘ
homogeneous universe ⓘ isotropic universe ⓘ self-gravitating fluid ⓘ |
| precedes | general relativity NERFINISHED ⓘ |
| relatedTo | Jeans swindle NERFINISHED ⓘ |
| studiedIn |
history of cosmology
ⓘ
theoretical astrophysics ⓘ |
| usedIn |
N-body simulations of large-scale structure (in Newtonian limit)
ⓘ
structure formation theory in the linear regime ⓘ |
| uses |
Euler equation for fluid motion
ⓘ
Poisson equation for gravitational potential ⓘ continuity equation for matter density ⓘ |
| usesConcept |
comoving coordinates (in Newtonian limit)
ⓘ
cosmological principle ⓘ scale factor (in Newtonian derivations) ⓘ |
| validInRegime |
non-relativistic velocities
ⓘ
weak gravitational fields ⓘ |
Referenced by (3)
Full triples — surface form annotated when it differs from this entity's canonical label.
subject surface form:
Physical cosmology
this entity surface form:
Newtonian cosmology
this entity surface form:
Newtonian gravity by incorporating special relativity