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The Friedmann equations, also known as the Friedmann–Lemaître (FL) equations, are a set of equations in physical cosmology that govern cosmic expansion in homogeneous and isotropic models of the universe within the context of general relativity. They were first derived by Alexander Friedmann in 1922 from Einstein's field equations of gravitation for the…
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Friedmann equations | related to Assumptions | The Friedmann | 0.60 | section |
| Friedmann equations | related to Assumptions | Friedmann | 0.60 | section |
| Friedmann equations | related to Assumptions | Lemaître | 0.60 | section |
| Friedmann equations | related to Assumptions | Robertson | 0.60 | section |
| Friedmann equations | related to Assumptions | Walker | 0.60 | section |
| Friedmann equations | related to Assumptions | Einstein's | 0.60 | section |
| Friedmann equations | related to Dimensionless scale factor | The Friedmann | 0.60 | section |
| Friedmann equations | related to Dust models | Setting | 0.60 | section |
| Friedmann equations | related to Dust models | Friedmann | 0.60 | section |
| Friedmann equations | related to Equations | There | 0.60 | section |
| Friedmann equations | related to Equations | Friedmann | 0.60 | section |
| Friedmann equations | related to Equations | The | 0.60 | section |
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