LTB metric

E458534

The LTB metric is an exact solution of Einstein’s field equations describing a spherically symmetric, inhomogeneous dust-filled universe used in cosmology and gravitational collapse studies.

All labels observed (1)

Label Occurrences
LTB metric canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf cosmological model ⓘ
exact solution of Einstein's field equations ⓘ
gravitational collapse model ⓘ
inhomogeneous dust solution ⓘ
spherically symmetric spacetime metric ⓘ
allows radial dependence of density ⓘ
radial dependence of expansion rate ⓘ
assumes comoving coordinates for dust particles ⓘ
dust matter with zero pressure ⓘ
spherical symmetry ⓘ
basedOn Einstein's field equations ⓘ
belongsTo general relativity ⓘ
describes pressureless matter (dust) distribution ⓘ
radially inhomogeneous cosmological models ⓘ
spherically symmetric inhomogeneous dust-filled universe ⓘ
fullName Lemaître–Tolman–Bondi metric ⓘ
generalizes Friedmann–Lemaître–Robertson–Walker metric ⓘ
hasApplication relativistic astrophysics ⓘ
theoretical cosmology ⓘ
hasCoordinateSystem comoving synchronous coordinates ⓘ
hasSymmetry spherical symmetry ⓘ
includes bang time function ⓘ
energy (curvature) function ⓘ
radial mass function ⓘ
is radially inhomogeneous generalization of FLRW models ⓘ
matterContent pressureless dust ⓘ
metricSignature Lorentzian ⓘ
namedAfter Georges Lemaître ⓘ
Hermann Bondi ⓘ
Richard C. Tolman ⓘ
reducesTo FLRW metric for homogeneous density and curvature ⓘ
solves Einstein equations with dust stress–energy tensor ⓘ
spacetimeDimension 4 ⓘ
timeCoordinate proper time of comoving dust observers ⓘ
usedFor gravitational lensing in inhomogeneous backgrounds ⓘ
modeling Oppenheimer–Snyder-like collapse generalizations ⓘ
modeling cosmic voids ⓘ
modeling inhomogeneous Big Bang times ⓘ
studying apparent cosmic acceleration without dark energy ⓘ
studying light propagation in inhomogeneous universes ⓘ
testing Copernican principle ⓘ
usedIn cosmology ⓘ
gravitational collapse studies ⓘ
inhomogeneous cosmological models ⓘ
relativistic stellar collapse modeling ⓘ
studies of structure formation ⓘ
void models of cosmic acceleration ⓘ

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.