Program - Brookhaven National Laboratory
Program - Brookhaven National Laboratory
Program - Brookhaven National Laboratory
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PR 94<br />
Analysis of Three Body Resonances in the Complex Scaled Orthogonal Condition Model<br />
M. Odsuren, Meme Media <strong>Laboratory</strong>, Hokkaido University Sapporo 060-8628, Japan. M. Odsuren,<br />
Nuclear Research Center, <strong>National</strong> University of Mongolia, Mongolia. K. Kato, Faculty of Science,<br />
Hokkaido University, Sapporo 060-0810, Japan. M. Aikawa, Faculty of Science, Hokkaido University,<br />
Sapporo 060-0810, Japan.<br />
During the last four decades a resonance problem has emerged as a crucial and useful research area in<br />
nuclear structure. Several extensions of the basic problem have been studied, where, for instance, a unified<br />
treatment of nuclear scattering and structure has been developed. Furthermore, the interactions between<br />
composite particles have extensively been studied, and the role of the Pauli exclusion principle in scattering<br />
and reaction processes has been understood considerably. The complex scaling method (CSM) [1-2] and<br />
the orthogonal condition model (OCM) [3] have been successfully utilized to describe the resonance states<br />
of light and middle mass nuclei. Although many problems have been solved so far, but further researches<br />
are required still. In this study, the complex scaled orthogonal condition model (CSOCM) [4] is applied to<br />
the light nuclei for 9 Be and three-body resonances of α+α+n is investigated. The data on resonance states<br />
of nuclei are of interest to basic and applied research. Although resonance structures of α+α+n have been<br />
studied, experimentally [5-6] and theoretically [7-9], there are still need more accurate and comprehensive<br />
calculations in the structure and decay of the low-lying excited states. The nucleus 9 Be is created in the<br />
universe when cosmic rays induced fission in heavier elements found in interstellar gas and dust. According<br />
to this idea, 9 Be is one of the especial interest system in astrophysics, where formation of 9 Be can proceed<br />
through the reaction 4 He(αn,γ) 9 Be. In addition, the beryllium can be used as a moderator and reflector<br />
for the nuclear facilities, but also it is applicable to isotopic neutron sources, such as plutonium-beryllium<br />
and americium-beryllium source. Due to this interest, the investigation of beryllium isotopic structure is<br />
still important. The main objective of our study is to investigate the resonance states of 9 Be by using<br />
CSOCM for a three-cluster system. Therefore, certainly understanding of α+α and α+n subsystems is<br />
needed in order to perform calculations of an α+α+n system.<br />
[1] Y.K.Ho, Phys. Rep.99, 1(1983) [2] S.Aoyama, T.Myo, K.Kato; and K.Ikeda, Prog. Theor. Phys.116,<br />
1(2006) [3] S.Saito, Prog. Theor. Phys. 40, 893(1968); 41, 705 (1969); Prog. Theor. Phys. Suppl.<br />
62, 11(1977) [4] A.T.Kruppa and K.Kato;, Prog. Theor. Phys. 84, 1145(1990) [5] F.Ajzenberg-Selove,<br />
Nucl. Phys. A490 (1988) [6] T. A. D. Brown et al., Phys. Rev. C76, 054605 (2007). [7] J. Hiura and<br />
I. Shimodaya, Prog. Theor. Phys. 30, 585(1963) [8] H. Furutani, H. Kanada, T. Kaneko, S. Nagata, H.<br />
Nishioka, S. Okabe, S. Saito, T. Sakuda, and M. Seya, Prog. Theor. Phys.Suppl. 68, 193 (1980). [9] K.<br />
Arai, P. Descouvemont, D. Baye, and W. N. Catford, Phys. Rev. C 68, 014310 (2003).<br />
PR 95<br />
B(E2) Evaluation for 0 + 1 → 2+ 1 Transitions in Even-Even Nuclei for Z=2-56<br />
B. Pritychenko, <strong>National</strong> Nuclear Data Center, <strong>Brookhaven</strong> <strong>National</strong> <strong>Laboratory</strong>, Upton, NY 11973-5000,<br />
USA. M. Birch, Department of Physics & Astronomy, McMaster University, Hamilton, Ontario L8S<br />
4M1, Canada. M. Horoi, Department of Physics, Central Michigan University, Mount Pleasant, MI<br />
48859, USA. B. Singh, Department of Physics & Astronomy, McMaster University, Hamilton, Ontario<br />
L8S 4M1, Canada.<br />
The results of B(E2)↑ evaluation for even-even Z=2-56 nuclei will be presented. This work is a continuation<br />
of S. Raman work [1] on B(E2) values and was motivated by a large number of recent measurements. It<br />
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