Session EH: Mini-symposium on Nuclear Physics in Extreme Astrophysical Conditions I
9:00 AM–12:00 PM, Wednesday, September 21, 2005
Ritz-Carlton Hotel Room: Plantation 1
Sponsoring Units:
DNP JPS
Chair: Shigeru Kubono, University of Tokyo
Abstract ID: BAPS.2005.HAW.EH.6
Abstract: EH.00006 : Investigation of proton resonant states in $^{23}$Al and $^{22}$Mg using radioactive beams at CNS
10:30 AM–10:45 AM
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Abstract
Authors:
Jianjun He
Shigeru Kubono
Takashi Teranishi
Masahiro Notani
Hidetada Baba
Shin'ichiro Michimasa
(Center for Nuclear Study, University of Tokyo (CNS), Japan)
Shunji Nishimura
Mizuki Nishimura
Yoshiyuki Yanagisawa
(RIKEN (The Institute of Physical and Chemical Research), Japan)
Hironori Iwasaki
(Department of Physics, University of Tokyo, Japan)
Naho Hokoiwa
Michiya Kibe
Yasuyuk Gono
(Department of Physics, Kyushu University, Japan)
Jun-Yung Moon
Ju-Hahn Lee
Chun-Sik Lee
(Department of Physics, Chung-Ang University, South Korea)
Seigo Kato
(Department of Physics, Yamagata University, Japan)
We have studied the proton resonances in $^{23}$Al and $^{22}$Mg via the resonant scattering of radioactive beams on a thick CH$_{2}$ target. The $^{22}$Mg and $^{21}$Na beams were separated by the {\textbf C}NS {\textbf R}adioactive {\textbf I}on {\textbf B}eam separator (CRIB) with energies of 4.4 AMeV and 4.0 AMeV, respectively. At scattering angles of $\theta _{lab}$= 4\r{ }, 17\r{ } and 23\r{ }, the recoiled particles were measured by three sets of $\Delta $E-E Si telescopes. As for nucleus $^{23}$Al (via $^{22}$Mg+p), several new resonant states were observed. As for nucleus $^{22}$Mg (via $^{21}$Na+p), the previously observed resonant states were confirmed. The states above the alpha threshold were observed, which are related to the $^{18}$Ne($\alpha $, p)$^{21}$Na reaction. The resonant parameters were deduced from an R-matrix code. The nuclear structures and the astrophysical implications are discussed.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2005.HAW.EH.6
