{57}$Zn $\beta$-delayed proton emission establishes the $^{56}$Ni $rp$-process waiting point bypass

•In our letter, we address the dominant uncertainty regarding the extent of the rp-process flow bypass around Ni 56 waiting point for astrophysical conditions relevant to Type-1 X-ray bursts.•We removed the final significant uncertainty, the beta-delayed proton branching ratio for Zn 57 , definitive...

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Veröffentlicht in:	Physics letters. B 2022-06, Vol.829
Hauptverfasser:	Saxena, M., Ong, W.-J, Meisel, Z., Hoff, D.E.M., Smirnova, N., Bender, P.C., Burcher, S.P., Carpenter, M.P., Carroll, J.J., Chester, A., Chiara, C.J., Conaway, R., Copp, P.A., Crider, B.P., Derkin, J., Estradé, A., Hamad, G., Harke, J.T., Jain, R., Jayatissa, H., Liddick, S.N., Longfellow, B., Mogannam, M., Montes, F., Nepal, N., Ogunbeku, T.H., Richard, A.L., Schatz, H., Soltesz, D., Subedi, S.K., Sultana, I., Tamashiro, A.S., Tripathi, V., Xiao, Y., Zink, R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Nuclear Theory Physics
Online-Zugang:	Volltext
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