First evidence for a virtual 18B ground state

被引:38
|
作者
Spyrou, A. [1 ,2 ]
Baumann, T. [1 ]
Bazin, D. [1 ]
Blanchon, G. [3 ]
Bonaccorso, A. [4 ]
Breitbach, E. [5 ]
Brown, J. [6 ]
Christian, G. [1 ,2 ]
DeLine, A. [7 ]
DeYoung, P. A. [8 ]
Finck, J. E. [7 ]
Frank, N. [9 ]
Mosby, S. [1 ,2 ]
Peters, W. A. [10 ]
Russel, A. [7 ]
Schiller, A. [11 ]
Strongman, M. J. [1 ,2 ]
Thoennessen, M. [1 ,2 ]
机构
[1] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[2] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[3] DIF, DAM, CEA, F-91297 Arpajon, France
[4] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[5] Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA
[6] Wabash Coll, Dept Phys, Crawfordsville, IN 47933 USA
[7] Cent Michigan Univ, Dept Phys, Mt Pleasant, MI 48859 USA
[8] Hope Coll, Dept Phys, Holland, MI 49423 USA
[9] Augustana Coll, Dept Phys & Astron, Rock Isl, IL 61201 USA
[10] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA
[11] Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA
基金
美国国家科学基金会;
关键词
Neutron Spectroscopy; Neutron Drip Line; Virtual State; Exotic Nuclei; ATOMIC MASS EVALUATION; EXCITED-STATES; MULTINUCLEON TRANSFER; EXOTIC NUCLEI; LIGHT-NUCLEI; FRAGMENTATION; C-17; C-19; HALO; PROJECTILES; ISOTOPES;
D O I
10.1016/j.physletb.2009.12.016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The decay of the neutron unbound ground state of B-18 was studied for the first time through a single-proton knockout reaction from a 62 MeV/u C-19 beam. The decay energy spectrum was reconstructed from coincidence measurements between the emitted neutron and the B-17 fragment using the MoNA/Sweeper setup. An s-wave line shape was used to describe the experimental spectrum resulting in an upper limit for the scattering length of -50 fm which corresponds to a decay energy <10 keV. Observing an s-wave decay of B-18 provides an experimental verification that the ground state of C-19 includes a large s-wave component. The presence of this s-wave component shows that s-d mixing is still present in B-18 and that the s(1/2) orbital has not moved significantly below the d(5/2) orbital. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码:129 / 133
页数:5
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