Bianchi type cosmologies
E446863
Bianchi type cosmologies are a class of spatially homogeneous but generally anisotropic cosmological models that classify possible three-dimensional Lie group symmetries of spacetime in general relativity.
All labels observed (12)
| Label | Occurrences |
|---|---|
| Bianchi cosmological models | 1 |
| Bianchi type I | 1 |
| Bianchi type II | 1 |
| Bianchi type III | 1 |
| Bianchi type IV | 1 |
| Bianchi type IX | 1 |
| Bianchi type V | 1 |
| Bianchi type VII | 1 |
| Bianchi type VIII | 1 |
| Bianchi type cosmologies canonical | 1 |
| Mixmaster universe | 1 |
| Mixmaster universe model | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T4493030 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Bianchi type cosmologies Context triple: [Gödel metric, relatedTo, Bianchi type cosmologies]
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A.
FLRW cosmological models
FLRW cosmological models are a family of solutions to Einstein’s field equations that describe a homogeneous and isotropic expanding or contracting universe, forming the standard framework for modern cosmology.
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B.
American school of relativistic cosmology
The American school of relativistic cosmology was a mid-20th-century research tradition in the United States that advanced the mathematical and physical foundations of general relativity and modern cosmology through the work of theorists such as Howard P. Robertson.
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C.
An Essay in Cosmology
An Essay in Cosmology is the subtitle of Alfred North Whitehead’s major philosophical work *Process and Reality*, which presents his influential process philosophy and metaphysical system.
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D.
Lemaître–Tolman metric
The Lemaître–Tolman metric is an exact spherically symmetric, inhomogeneous solution of Einstein’s field equations used in cosmology to model non-uniform distributions of matter without assuming spatial homogeneity.
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E.
Essai de cosmologie
Essai de cosmologie is an 18th-century philosophical and scientific treatise by Pierre-Louis Moreau de Maupertuis that explores the structure and origins of the universe within the framework of early Enlightenment cosmology.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Bianchi type cosmologies Target entity description: Bianchi type cosmologies are a class of spatially homogeneous but generally anisotropic cosmological models that classify possible three-dimensional Lie group symmetries of spacetime in general relativity.
-
A.
FLRW cosmological models
FLRW cosmological models are a family of solutions to Einstein’s field equations that describe a homogeneous and isotropic expanding or contracting universe, forming the standard framework for modern cosmology.
-
B.
American school of relativistic cosmology
The American school of relativistic cosmology was a mid-20th-century research tradition in the United States that advanced the mathematical and physical foundations of general relativity and modern cosmology through the work of theorists such as Howard P. Robertson.
-
C.
An Essay in Cosmology
An Essay in Cosmology is the subtitle of Alfred North Whitehead’s major philosophical work *Process and Reality*, which presents his influential process philosophy and metaphysical system.
-
D.
Lemaître–Tolman metric
The Lemaître–Tolman metric is an exact spherically symmetric, inhomogeneous solution of Einstein’s field equations used in cosmology to model non-uniform distributions of matter without assuming spatial homogeneity.
-
E.
Essai de cosmologie
Essai de cosmologie is an 18th-century philosophical and scientific treatise by Pierre-Louis Moreau de Maupertuis that explores the structure and origins of the universe within the framework of early Enlightenment cosmology.
- F. None of above. chosen
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
anisotropic cosmology
ⓘ
cosmological model ⓘ solution of Einstein field equations ⓘ spatially homogeneous cosmology ⓘ |
| appliesTo | general relativity NERFINISHED ⓘ |
| basedOn | three-dimensional Lie groups ⓘ |
| canInclude |
cosmological constant
ⓘ
perfect fluid matter content ⓘ scalar field matter content ⓘ |
| characterizedBy |
constant-time hypersurfaces with group symmetry
ⓘ
structure constants of a three-dimensional Lie algebra ⓘ |
| classifiedBy | Bianchi classification NERFINISHED ⓘ |
| describes | spacetimes with homogeneous spatial sections ⓘ |
| generalizes | Friedmann–Lemaître–Robertson–Walker cosmology NERFINISHED ⓘ |
| hasMathematicalFramework |
Hamiltonian formulation of cosmology
ⓘ
orthonormal frame formalism ⓘ |
| hasProperty |
group-invariant spatial hypersurfaces
ⓘ
possible anisotropy ⓘ spatial homogeneity ⓘ three-dimensional isometry group acting transitively on spatial slices ⓘ |
| hasSubset |
diagonal Bianchi models
ⓘ
locally rotationally symmetric Bianchi models ⓘ non-tilted Bianchi models ⓘ tilted Bianchi models ⓘ |
| includes |
Bianchi class A models
NERFINISHED
ⓘ
Bianchi class B models NERFINISHED ⓘ Bianchi type I cosmology NERFINISHED ⓘ Bianchi type II cosmology NERFINISHED ⓘ Bianchi type III cosmology NERFINISHED ⓘ Bianchi type IV cosmology NERFINISHED ⓘ Bianchi type IX cosmology ⓘ Bianchi type V cosmology NERFINISHED ⓘ Bianchi type VI cosmology ⓘ Bianchi type VII cosmology NERFINISHED ⓘ Bianchi type VIII cosmology NERFINISHED ⓘ |
| namedAfter | Luigi Bianchi NERFINISHED ⓘ |
| relatedTo |
Friedmann–Lemaître–Robertson–Walker cosmology
NERFINISHED
ⓘ
Kasner solution NERFINISHED ⓘ Mixmaster universe NERFINISHED ⓘ |
| studiedIn |
mathematical cosmology
ⓘ
relativistic cosmology ⓘ |
| usedIn |
dynamical systems approach to cosmology
ⓘ
study of cosmic microwave background anomalies ⓘ study of cosmological singularities ⓘ study of early universe anisotropies ⓘ |
| usedToTest |
cosmic no-hair conjecture
NERFINISHED
ⓘ
isotropy of the universe ⓘ |
| uses | Lie algebra of Killing vector fields ⓘ |
How these facts were elicited
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You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Subject: Bianchi type cosmologies Description of subject: Bianchi type cosmologies are a class of spatially homogeneous but generally anisotropic cosmological models that classify possible three-dimensional Lie group symmetries of spacetime in general relativity.
Referenced by (12)
Full triples — surface form annotated when it differs from this entity's canonical label.