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The slow neutron-capture process, or s-process, is a series of reactions in nuclear astrophysics that occur in stars, particularly asymptotic giant branch stars. The s-process is responsible for the creation (nucleosynthesis) of approximately half the atomic nuclei heavier than iron.
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Explore the main themes, entities and connections around S-process. Start with the topic map, then use the sections below for research and deeper semantic analysis.
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isotopes neutron stars iron elements neutrons nuclei occur mass decay r-process abundances series stable grains seed flux abundance heavier higher
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| thorium or uranium | instance of | this process does not have the ability to produce any of the heavy radioactive isotopes | 0.80 | text |
| S-process | related to history | The | 0.60 | section |
| S-process | related to history | Hans Suess | 0.60 | section |
| S-process | related to history | Harold Urey | 0.60 | section |
| S-process | related to history | Among | 0.60 | section |
| S-process | related to history | This | 0.60 | section |
| S-process | related to history | B2FH | 0.60 | section |
| S-process | related to history | There | 0.60 | section |
| S-process | related to history | In | 0.60 | section |
| S-process | related to history | S-type | 0.60 | section |
| S-process | related to history | Paul | 0.60 | section |
| S-process | related to history | Merrill | 0.60 | section |
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