Published November 11, 2011 | Version v1
Journal article

Gamow-Teller Transition Strengths from 56Ni

  • 1. Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824 (United States)
  • 2. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321 (United States)
  • 3. Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States)
  • 4. GSI Darmstadt, Helmholtz-Zentrum fuer Schwerionenforschung, D-64291, Darmstadt (Germany)
  • 5. Physics Department, Kalamazoo College, Kalamazoo, Michigan 49006 (United States)
  • 6. Department of Physics and Astronomy, Ursinus College, Collegeville, Pennsylvania 19426 (United States)
  • 7. Department of Physics, University of Massachusetts Lowell, Lowell, Massachusetts 01854 (United States)
  • 8. Khalifa University of Science, Technology and Research, 127788 Abu Dhabi (United Arab Emirates)

Description

A new technique to measure (p,n) charge-exchange reactions in inverse kinematics at intermediate energies on unstable isotopes was successfully developed and used to study the 56Ni(p,n) reaction at 110 MeV/u. Gamow-Teller transition strengths from 56Ni leading to 56Cu were obtained and compared with shell-model predictions in the pf shell using the KB3G and GXPF1A interactions. The calculations with the GXPF1A interaction reproduce the experimental strength distribution much better than the calculations that employed the KB3G interaction, indicating deficiencies in the spin-orbit and proton-neutron residual potentials for the latter. The results are important for improving the description of electron-capture rates on nuclei in the iron region, which are important for modeling the late evolution of core-collapse and thermonuclear supernovae.

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
107
Journal Issue
20
Journal Page Range
p. 202501-202501.5
ISSN
0031-9007
CODEN
PRLTAO

Optional Information

Notes
(c) 2011 American Institute of Physics