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In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the very early universe. This enormous expansion supercooled the universe and ended when the energy content of the field driving inflation condensed into hot, dense particles, a process called reheating. Following the…
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universe inflation energy field density theory model models early inflationary expansion cosmology problem time quantum initial cosmological inflaton would cosmic
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| vortices in liquid helium | instance of | dense state it triggered a series of phase transitions much like what happens in condensed-matter systems | 0.80 | text |
| Cosmic inflation | related to Concept | Cosmic | 0.60 | section |
| Cosmic inflation | related to Concept | Distances | 0.60 | section |
| Cosmic inflation | related to Concept | All | 0.60 | section |
| Cosmic inflation | related to Concept | At | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | Once | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | CMB | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | One | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | Guth's | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | The | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | Topological | 0.60 | section |
| Cosmic inflation | related to Demise of topological defects rival | Magnetic | 0.60 | section |
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