Review Paper: Figure 15
Important nuclei from the delayed neutron emission sensitivity studies of Fig. 15 given criterion $F_{max} \ge 0.1$ for at least one astrophysical condition: (a) low entropy hot wind, (b) high entropy hot wind, (c) cold wind and (d) neutron star merger. Asterisk denotes $F_{max}$ below threshold of $0.01$. Data associated with the 2016 $r$-process review paper.
| Nucleus | Data | |||||
|---|---|---|---|---|---|---|
| Z | N | A | $F^a_{max}$ | $F^b_{max}$ | $F^c_{max}$ | $F^d_{max}$ |
Related Publications
| Year | Authors | Title (Click for more details) | Journal (PDF) |
|---|---|---|---|
| 2016 | M. Mumpower, R. Surman, G. C. McLaughlin, A. Aprahamian | The impact of individual nuclear properties on $r$-process nucleosynthesis | PPNP 86 86-126 |