57Zn β-delayed proton emission establishes the 56Ni rp-process waiting point bypass
/ Authors
M. Saxena, W. -J Ong, Z. Meisel, D. Hoff, N. Smirnova, P. Bender, S. Burcher, M. Carpenter, J. J. Carroll, A. Chester
and 25 more authors
C. Chiara, R. Conaway, P. Copp, B. Crider, J. Derkin, A. Estrade, G. Hamad, J. T. Harke, R. Jain, H. Jayatissa, S. Liddick, B. Longfellow, M. Mogannam, F. Montes, N. Nepal, T. Ogunbeku, A. Richard, H. Schatz, D. Soltesz, S. Subedi, I. Sultana, A. Tamashiro, V. Tripathi, Y. Xiao, R. Zink
/ Abstract
We measured the 57 Zn β -delayed proton ( β p ) and γ emission at the National Superconducting Cyclotron Laboratory. We find a 57 Zn half-life of 43 . 6 ± 0 . 2 ms, β p branching ratio of (84 . 7 ± 1 . 4)%, and identify four transitions corresponding to the exotic β - γ - p decay mode, the second such identification in the f p -shell. The p / γ ratio was used to correct for isospin mixing while determining the 57 Zn mass via the isobaric multiplet mass equation. Previously, it was uncertain as to whether the rp -process flow could bypass the textbook waiting point 56 Ni for astrophysical conditions relevant to Type-I X-ray bursts. Our results definitively establish the existence of the 56 Ni bypass, with 14-17% of the rp -process flow taking this route.
Journal: Physics Letters B