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Structures and decay of deep-hole states in light nuclei populated by the (p, 2p 2p) reactions
Authors:M Yosoi  H Akimune  I Daito  H Ejiri  H Fujimura  M Fujiwara  K Hara  K Y Hara  T Ishikawa  M Itoh  Y Itow  T Kawabata  K Kobayashi  M Nakamura  T Noro  E Obayashi  H Sakaguchi  Y Sakemi  M Shiozawa  H Takeda  T Taki  A Tamii  H Toyokawa  N Tsukahara  M Uchida  T Yamada  Y Yasuda  H P Yoshida  R G T Zegers
Institution:(1) Department of Physics, Kyoto University, Kyoto, Japan;(2) Department of Physics, Konan University, Kobe, Japan;(3) Research Center for Nuclear Physics, Osaka University, Osaka, Japan;(4) Japan Synchrotron Radiation Research Institute, Sayo, Hyogo, Japan;(5) Laboratory of Nuclear Science, Tohoku University, Sendai, Japan;(6) Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan;(7) Center for Nuclear Study, University of Tokyo, Hongo, Tokyo, Japan;(8) Department of Physics, Kyushu University, Fukuoka, Japan;(9) RI Beam Science Laboratory, RIKEN, Wako, Japan;(10) Laboratory of Physics, Kanto Gakuin University, Yokohama, Japan;(11) NSCL/MSU, East Lansing, USA
Abstract:Decay particles from the s-hole states in 11B and 15N have been measured in coincidence with the quasifree 12C(p, 2p) and 16O(p, 2p) reactions at E p =392 MeV. Triton decay is found to be dominant for the 11B(s-hole) state and also found to be larger than α decay for the 15N(s-hole) state despite its smaller Q value compared to α decay. Measured decay branching ratios are discussed in comparison with the results of statistical-model, SU(3)-model, and shell-model calculations. The energy spectra around the s-hole states in both 11B and 15N exhibit some bumplike structures, which can be qualitatively explained by recent shell-model calculations for both nuclei.
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