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A pair-instability supernova is a type of supernova predicted to occur when pair production — the production of free electrons and positrons in the collision between atomic nuclei and energetic gamma rays — temporarily reduces the internal radiation pressure supporting a supermassive star's core against gravitational collapse. This pressure drop leads to…
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gamma core star stars pair-instability pressure rays energy masses supernova mass collapse supernovae solar production stellar runaway pairs type pair
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Pair-instability supernova | is a | type of supernova predicted to occur when pair production | 0.90 | text |
| Pair-instability supernova | related to 130 to 250 solar masses | For | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | In | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | The | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | With | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | This | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | Cobalt-56 | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | Supernova | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | SN | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | Ni | 0.60 | section |
| Pair-instability supernova | related to 130 to 250 solar masses | Collision | 0.60 | section |
| Pair-instability supernova | related to Luminosity | Pair-instability | 0.60 | section |
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