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The flatness problem (also known as the oldness problem) is a cosmological fine-tuning problem within the Big Bang model of the universe. Measurements find the current universe close to perfectly flat and expansion of the universe increases flatness. Consequently the early universe must have been exceptionally close to flat. In standard cosmology based…
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universe density problem flatness value displaystyle matter one flat rho energy inflation curvature since would time anthropic theory different close
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| galaxies | instance of | In either case the universe would contain no complex structures | 0.80 | text |
| stars | instance of | In either case the universe would contain no complex structures | 0.80 | text |
| planets | instance of | In either case the universe would contain no complex structures | 0.80 | text |
| any form of life.This problem with the Big Bang model was first pointed out by Robert Dicke in 1969 | instance of | In either case the universe would contain no complex structures | 0.80 | text |
| and it motivated a search for some reason the density should take such a specific value | instance of | In either case the universe would contain no complex structures | 0.80 | text |
| humans | instance of | only those universes with exactly the correct density for forming galaxies and stars would give rise to intelligent observers | 0.80 | text |
| Flatness problem | related to Anthropic principle | One | 0.60 | section |
| Flatness problem | related to Anthropic principle | If | 0.60 | section |
| Flatness problem | related to Anthropic principle | The | 0.60 | section |
| Flatness problem | related to Anthropic principle | Collins | 0.60 | section |
| Flatness problem | related to Anthropic principle | Stephen Hawking | 0.60 | section |
| Flatness problem | related to Anthropic principle | In | 0.60 | section |
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