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In physical cosmology, baryogenesis (also known as baryosynthesis) is the physical process that is hypothesized to have taken place during the early universe to produce baryonic asymmetry, the observation that only matter (baryons) and not antimatter (antibaryons) is detected in the universe (other than in cosmic ray collisions).: 22.3.6 Since it is…
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matter antimatter universe baryon number asymmetry phase particles baryons model would electroweak interactions physics imbalance theories also conditions big bang
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Baryogenesis | is a | decay reaction of B-mesogenesis | 0.90 | text |
| the B-meson decay into a visible Standard Model baryon as well as a dark antibaryon that is invisible to current observation techniques.Asymmetric dark matterThe asymmetric dark matter proposal investigates mechanisms that would explain the abundance of dark matter but lack of dark antimatter as the consequence of the same effect as would explain baryogenesis | instance of | particles | 0.80 | text |
| the B-meson decay into a visible Standard Model baryon as well as a dark antibaryon that is invisible to current observation techniques | instance of | particles | 0.80 | text |
| Baryogenesis | related to Asymmetric dark matter | The | 0.60 | section |
| Baryogenesis | related to B-meson decay | Another | 0.60 | section |
| Baryogenesis | related to B-meson decay | B-mesogenesis | 0.60 | section |
| Baryogenesis | related to B-meson decay | This | 0.60 | section |
| Baryogenesis | related to B-meson decay | B-meson | 0.60 | section |
| Baryogenesis | related to B-meson decay | Standard Model | 0.60 | section |
| Baryogenesis | related to In the Standard Model | The Standard Model | 0.60 | section |
| Baryogenesis | related to In the Standard Model | There | 0.60 | section |
| Baryogenesis | related to In the Standard Model | This | 0.60 | section |
These clusters group vocabulary that occurs around closely connected concepts in the source material.
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