Gamow-Teller Transition Strengths from 56Ni
Creators
- Sasano, M.1, 2
- Perdikakis, G.1, 2
- Austin, Sam M.1, 2
- Montes, F.1, 2
- Zegers, R. G. T.3, 1, 2
- Brown, B. A.3, 1, 2
- Deaven, J. M.3, 1, 2
- Meharchand, R.3, 1, 2
- Prinke, A.3, 1, 2
- Scott, M.3, 1, 2
- Valdez, L.3, 1, 2
- Bazin, D.2
- Stolz, A.2
- Caesar, C.4
- Cole, A. L.5
- Ferrante, N.6
- Palardy, J.6
- Riley, L. A.6
- Guess, C. J.1, 7
- Hitt, G. W.8
- and others
- 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
Identifiers
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
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43083866
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- CHARGE-EXCHANGE REACTIONS; COPPER 56; ELECTRON CAPTURE; GAMOW-TELLER RULES; IRON; MEV RANGE 100-1000; NEUTRONS; NICKEL 56; NICKEL 56 TARGET; PROTON REACTIONS; SHELL MODELS; SIMULATION; SPIN; SUPERNOVAE
- Descriptors DEC
- ANGULAR MOMENTUM; BARYON REACTIONS; BARYONS; BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; BINARY STARS; CAPTURE; CHARGED-PARTICLE REACTIONS; COPPER ISOTOPES; DAYS LIVING RADIOISOTOPES; ELECTRON CAPTURE RADIOISOTOPES; ELEMENTARY PARTICLES; ELEMENTS; ENERGY RANGE; ERUPTIVE VARIABLE STARS; EVEN-EVEN NUCLEI; FERMIONS; HADRON REACTIONS; HADRONS; INTERMEDIATE MASS NUCLEI; ISOTOPES; MATHEMATICAL MODELS; METALS; MEV RANGE; MILLISECONDS LIVING RADIOISOTOPES; NICKEL ISOTOPES; NUCLEAR MODELS; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; NUCLEONS; ODD-ODD NUCLEI; PARTICLE PROPERTIES; RADIOISOTOPES; STARS; TARGETS; TRANSITION ELEMENTS; VARIABLE STARS
Optional Information
- Notes
- (c) 2011 American Institute of Physics