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57Zn β-delayed proton emission establishes the 56Ni rp-process waiting point bypass

Journal Article · · Physics Letters. B
 [1];  [2];  [3];  [4];  [5];  [6];  [2];  [7];  [8];  [9];  [8];  [3];  [7];  [10];  [3];  [11];  [3];  [2];  [9];  [7] more »;  [9];  [9];  [9];  [9];  [11];  [12];  [13];  [9];  [3];  [3];  [11];  [14];  [15];  [12];  [3] « less
  1. Ohio Univ., Athens, OH (United States); Michigan State University
  2. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  3. Ohio Univ., Athens, OH (United States)
  4. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States); Univ. of Massachusetts, Lowell, MA (United States)
  5. CNRS/IN2P3 and Univ. de Bordeaux, Gradignan Cedex (France)
  6. Univ. of Massachusetts, Lowell, MA (United States)
  7. Argonne National Lab. (ANL), Argonne, IL (United States)
  8. DEVCOM/Army Research Lab., Adelphi, MD (United States)
  9. Michigan State Univ., East Lansing, MI (United States)
  10. Mississippi State Univ., Starkville, MS (United States)
  11. Central Michigan Univ., Mount Pleasant, MI (United States)
  12. Michigan State Univ., East Lansing, MI (United States); Mississippi State Univ., Starkville, MS (United States)
  13. Michigan State Univ., East Lansing, MI (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  14. Oregon State Univ., Corvallis, OR (United States)
  15. Florida State Univ., Tallahassee, FL (United States)
We measured the 57Zn β-delayed proton (βp) and γemission at the National Superconducting Cyclotron Laboratory. We find a 57Zn half-life of 43.6 ± 0.2ms, βp branching ratio of (84.7 ±1.4)%, and identify four transitions corresponding to the exotic β-γ-pdecay mode, the second such identification in the fp-shell. The p/γratio was used to correct for isospin mixing while determining the 57Zn mass via the isobaric multiplet mass equation. Previously, it was uncertain as to whether the rp-process flow could bypass the textbook waiting point 56Ni for astrophysical conditions relevant to Type-I X-ray bursts. Our results definitively establish the existence of the 56Ni bypass, with 14-17% of the rp-process flow taking this route.
Research Organization:
Argonne National Laboratory (ANL), Argonne, IL (United States); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Michigan State Univ., East Lansing, MI (United States); Ohio Univ., Athens, OH (United States)
Sponsoring Organization:
National Science Foundation; USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC), Nuclear Physics (NP)
Grant/Contract Number:
AC02-06CH11357; AC52-07NA27344; FG02-88ER40387; NA0003906; NA0003909; SC0019042; SC0020451
OSTI ID:
1864489
Alternate ID(s):
OSTI ID: 1864684
OSTI ID: 1888121
OSTI ID: 1903748
Report Number(s):
LLNL-JRNL-839052
Journal Information:
Physics Letters. B, Journal Name: Physics Letters. B Vol. 829; ISSN 0370-2693
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English

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