β-decay half-lives and β-delayed neutron emission probabilities for neutron rich nuclei close to the N=82r-process path

F. Montes, A. Estrade, P. T. Hosmer, S. N. Liddick, P. F. Mantica, A. C. Morton, W. F. Mueller, M. Ouellette, E. Pellegrini, P. Santi, H. Schatz, A. Stolz, B. E. Tomlin, O. Arndt, K.-L. Kratz, B. Pfeiffer, P. Reeder, W. B. Walters, A. Aprahamian, and A. Wöhr
Phys. Rev. C 73, 035801 – Published 10 March 2006

Abstract

β-delayed neutron emission branchings (or upper limits) for neutron rich Rh116120, Pd120122, and Ag124 have been measured. These branching ratios serve as direct inputs to astrophysical rapid neutron capture process models and affect the final abundances calculated in these models. In addition, half-lives for neutron rich Tc114115, Ru114118, Rh116121, and Pd119124 near the proposed path of the r-process have also been measured. The results agree with theoretical quasiparticle random-phase approximation calculations within model uncertainties; the only exception is the delayed neutron branching in the decay of Rh120, which is found to be much smaller than predicted.

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  • Received 21 November 2005

DOI:https://doi.org/10.1103/PhysRevC.73.035801

©2006 American Physical Society

Authors & Affiliations

F. Montes1,2,4, A. Estrade1,2,4, P. T. Hosmer1,2,4, S. N. Liddick3,4,*, P. F. Mantica3,4, A. C. Morton4,†, W. F. Mueller4, M. Ouellette1,2,4, E. Pellegrini2,4, P. Santi4,‡, H. Schatz1,2,4, A. Stolz4, B. E. Tomlin3,4, O. Arndt5,6, K.-L. Kratz5,6, B. Pfeiffer5,6, P. Reeder7, W. B. Walters8, A. Aprahamian9, and A. Wöhr9

  • 1Joint Institute for Nuclear Astrophysics, USA§
  • 2Dept. of Physics and Astronomy, Michigan State University, E. Lansing, Michigan 48824, USA
  • 3Dept. of Chemistry, Michigan State University, E. Lansing, Michigan 48824, USA
  • 4National Superconducting Cyclotron Laboratory, Michigan State University, E. Lansing, Michigan 48824, USA
  • 5Institut für Kernchemie, Universität Mainz, Fritz-Strassmann Weg 2, D-55128 Mainz, Germany
  • 6VISTARS–Virtuelles Institut der Struktur der Kerne und nuklearer Astrophysik, Mainz, Germany∥
  • 7Richland, Washington 99352, USA
  • 8Dept. of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
  • 9Joint Institute for Nuclear Astrophysics, and Institute for Structure and Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46616, USA

  • *Current address: UNIRIB, Oak Ridge, TN, USA.
  • Current address: TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 1R9 Canada.
  • Current address: Los Alamos National Laboratory, Safeguards Science and Technology Group (N-1), E540, Los Alamos, NM 87544, USA.
  • §http://www.vistars.de
  • http://www.jinaweb.org

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Vol. 73, Iss. 3 — March 2006

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