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Decay of the r-process nuclides 137,138,139Sb, and the A=130 solar r-process abundance peak

O. Arndt, K.-L. Kratz, W. B. Walters, K. Farouqi, U. Köster, V. Fedosseev, S. Hennrich, C. J. Jost, A. Wöhr, A. A. Hecht, B. Pfeiffer, J. Shergur, and N. Hoteling
Phys. Rev. C 84, 061307(R) – Published 28 December 2011

Abstract

Half-life (T1/2) and β-delayed neutron branching (Pn) values of 492(25) ms and 49(8)%, 350(15) ms and 72(8)%, and 93(13) ms and 90(10)% for the r-process nuclei 137,138,139Sb, respectively, have been measured at the CERN On-Line Isotope Mass Separator (ISOLDE) facility by counting β-delayed neutrons. More precise T1/2 and Pn values of 300(15) ms and 27(4)%, and 273(7) ms and 50(8)% for 136,137Sn, respectively, have also been measured. The sources were prepared by using the selective ionization of Sb or Sn with the Resonance Ionization Laser Ion Source and the high-resolution mass separator. The new data for Sb isotopes are compared with calculated T1/2 and Pn values for both spherical and nonspherical shapes. The data have been incorporated into parametrized nucleosynthesis calculations of the r process in high-entropy winds of core-collapse supernovae in order to study the properties of the A = 130 solar-system r-process abundance peak.

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  • Received 22 September 2011

DOI:https://doi.org/10.1103/PhysRevC.84.061307

©2011 American Physical Society

Authors & Affiliations

O. Arndt1, K.-L. Kratz1, W. B. Walters2, K. Farouqi1, U. Köster3, V. Fedosseev4, S. Hennrich1, C. J. Jost1, A. Wöhr2,5, A. A. Hecht2,5, B. Pfeiffer1, J. Shergur2,5, and N. Hoteling2,5

  • 1Max-Planck-Institut für Chemie, Otto-Hahn-Institut, Joh.-J. Becherweg 27, D-55128 Mainz, Germany
  • 2Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
  • 3Institut Laue-Langevin, F-38042 Grenoble, France
  • 4CERN, CH-1211 Geneva 23, Switzerland
  • 5Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA

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Issue

Vol. 84, Iss. 6 — December 2011

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