The (6Li,6Li*[3.56 MeV]) reaction at 100 MeV/u as a probe of Gamow-Teller transition strengths in the inelastic scattering channel

ORAL

Abstract

The (6Li,6Li[T = 1, Tz= 0, 0+, 3.56 MeV]) reaction at 100 MeV/u was developed as a probe for isolating the isovector spin-transfer response in the inelastic channel from which the Gamow-Teller transition strengths from nuclei of relevance for inelastic neutrino-nucleus scattering cross sections can be extracted. By measuring the 6Li ejectile in the Grand Raiden magnetic spectrometer and selecting events in which the 3.56 MeV γ ray from the decay of the 6Li*[3.56 MeV] state is detected, the isovector spin-transfer selectivity is obtained. HPGe clover detectors in the CAGRA array served to detect the γ rays. In the study of the 12C(6Li,6Li[3.56 MeV]) reaction, the isovector spin-transfer excitation-energy spectrum in the inelastic channel was successfully measured. For heavier target nuclei, the extraction of the isovector spin-transfer response was hampered by the background in the γ-spectra from isoscalar excitations.

Presenters

  • R. G.T. G.T. Zegers

    National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA, Department of Physics and Astronomy, Michigan State University, E, National Superconducting Cyclotron Laboratory, Michigan State University, Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements, Michigan State, National Superconducting Cyclotron Laboratory, Michigan State University, Department of Physics and Astronomy, Michigan State University, Michigan State Univ, NSCL/MSU, for the RCNP E441 Collaboration

Authors

  • R. G.T. G.T. Zegers

    National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA, Department of Physics and Astronomy, Michigan State University, E, National Superconducting Cyclotron Laboratory, Michigan State University, Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements, Michigan State, National Superconducting Cyclotron Laboratory, Michigan State University, Department of Physics and Astronomy, Michigan State University, Michigan State Univ, NSCL/MSU, for the RCNP E441 Collaboration