Phys. Rev. C
74,
024309
(2006)
[15 pages]
The (t,3He) and (3He, t) reactions as probes of Gamow-Teller strength
R. G. T. Zegers et al.
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R. G. T. Zegers1,2,3, H. Akimune4, Sam M. Austin1,3, D. Bazin1, A. M.van den Berg5, G. P. A. Berg6,7, B. A. Brown1,2,3, J. Brown8, A. L. Cole1,3, I. Daito9, Y. Fujita10, M. Fujiwara11,12, S. Galès13, M. N. Harakeh5, H. Hashimoto12, R. Hayami14, G. W. Hitt1,2, M. E. Howard3,15, M. Itoh16, J. Jänecke17, T. Kawabata18, K. Kawase12, M. Kinoshita4, T. Nakamura19, K. Nakanishi12, S. Nakayama14, S. Okumura12, W. A. Richter20, D. A. Roberts17, B. M. Sherrill1,2,3, Y. Shimbara1,3, M. Steiner1, M. Uchida21, H. Ueno22, T. Yamagata19, and M. Yosoi12
1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321, USA 2Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA 3Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA 4Department of Physics, Konan University, Kobe, Hyogo 658-8501, Japan 5Kernfysisch Versneller Instituut, University of Groningen, Zernikelaan 25, 9747 AA Groningen, The Netherlands 6Department of Physics, University of Notre Dame, Indiana 46556-5670, USA 7Joint Institute for Nuclear Astrophysics, University of Notre Dame, Indiana 46556-5670, USA 8Department of Physics, Wabash College, Crawfordsville, Indiana 47933, USA 9Advanced Photon Research Center, Japan Atomic Research Institute, Kizu, Kyoto 619-0215, Japan 10Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan 11Kansai Photon Science Institute, Japan Atomic Energy Agency, Kizu, Kyoto 619-0215, Japan 12Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047, Japan 13Institut de Physique Nucléaire, IN2P3-CNRS, Orsay, France 14Department of Physics, University of Tokushima, Tokushima 770-8502, Japan 15Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA 16Cyclotron and Radioisotope Center, Tohoku University, Sendai, Miyagi 980-8578, Japan 17Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA 18Center for Nuclear Study, University of Tokyo, RIKEN Campus, Wako, Saitama 351-0198, Japan 19Tokyo Institute of Technology, Megro, Tokyo 152-8550, Japan 20Department of Physics, University of Western Cape, Bellville 7530, South Africa 21Tokyo Institute of Technology, 2-12-1 O-Okayama, Tokyo 152-8550, Japan 22Applied Nuclear Physics Laboratory, RIKEN, Wako, Saitama 351-0198, Japan
Received 29 September 2005; revised 21 December 2005; published 18 August 2006
It is shown via a study on a 26Mg target that the (t,3He) reaction at 115 MeV/nucleon reaction is an accurate probe for extracting Gamow-Teller transition strengths. To do so, the data are complemented by results from the 26Mg(3He, t) reaction at 140 MeV/nucleon that allows for a comparison of T=2 analog states excited via the mirror reactions. Extracted Gamow-Teller strengths from 26Mg(t,3He) and 26Mg(3He, t) are compared with those from 26Mg(d,2He) and 26Mg(p,n) studies, respectively. A good correspondence is found, indicating probe independence of the strength extraction. Furthermore, we test shell-model calculations using the new USD-05B interaction in the sd-model space and show that it reproduces the experimental Gamow-Teller strength distributions well. In anticipation of further (t,3He) experiments on medium-heavy nuclei aimed at determining weak-interaction rates of relevance for stellar evolution, a second goal of this work is to improve the understanding of the (t,3He) and (3He, t) reaction mechanisms at intermediate energies because detailed studies are scarce. The distorted-wave Born approximation is employed, taking into account the composite structures of the 3He and triton particles. The reaction model provides the means to explain systematic uncertainties at the 10%–20% level in the extraction of Gamow-Teller strengths as being because of interference between Gamow-Teller ΔL=0,ΔS=1 and ΔL=2,ΔS=1 amplitudes that both contribute to transitions from 0+ to 1+ states.
© 2006 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevC.74.024309
DOI:
10.1103/PhysRevC.74.024309
PACS:
25.40.Kv, 21.60.Cs, 25.55.Kr, 27.30.+t
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