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

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