Suppressed electric quadrupole collectivity in 32Si

被引:0
|
作者
Heery, J. [1 ]
Henderson, J. [1 ]
Hoffman, C. R. [2 ]
Hill, A. M. [3 ,4 ]
Beck, T. [4 ]
Cousins, C. [1 ]
Farris, P. [3 ,4 ]
Gade, A. [3 ,4 ]
Gillespie, S. A. [4 ]
Holt, J. D. [5 ,6 ]
Hu, B. [5 ]
Iwasaki, H. [3 ,4 ]
Kisyov, S. [7 ,11 ]
Kuchera, A. N. [8 ]
Longfellow, B. [7 ]
Mueller-Gatermann, C. [2 ]
Poves, A. [9 ,10 ]
Rubino, E. [4 ,12 ]
Russell, R. [1 ]
Salinas, R. [3 ,4 ]
Sanchez, A. [3 ,4 ]
Weisshaar, D. [4 ]
Wu, C. Y. [7 ]
Wu, J. [4 ,13 ]
机构
[1] Univ Surrey, Sch Phys & Maths, Guildford GU2 7XH, England
[2] Argonne Natl Lab, Phys Div, Lemont, IL 60439 USA
[3] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[4] Michigan State Univ, Facil Rare Isotope Beams, E Lansing, MI 48824 USA
[5] TRIUMF, Vancouver, BC V6T 2A3, Canada
[6] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[7] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[8] Davidson Coll, Dept Phys, Davidson, NC 28035 USA
[9] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
[10] Univ Autonoma Madrid, IFT, UAM CSIC, E-28049 Madrid, Spain
[11] Lawrence Berkeley Natl Lab, Accelerator Technol & Appl Phys Div, Berkeley, CA 94720 USA
[12] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[13] Brookhaven Natl Lab, Natl Nucl Data Ctr, Upton, NY 11973 USA
基金
加拿大自然科学与工程研究理事会;
关键词
SHELL-MODEL; COULOMB-EXCITATION; NEUTRON; NUCLEUS; SI-32; GERMANIUM; MOMENTS; SHAPES; STATES;
D O I
10.1103/PhysRevC.109.014327
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Lying between 16O and 40Ca, the sd shell is well described by robust phenomenological and ab initio nuclear theories. In this work, however, we highlight an unexplained reduction in electric-quadrupole strength in the rare isotope 32Si, studied through sub-barrier Coulomb excitation. It is found that the oblate nature of the deformation is well reproduced, while the absolute scale of quadrupole deformation, however, is inhibited by approximately a factor of 2 compared to theoretical predictions. Through comparison with shell-model and ab initio calculations, we present a number of possible explanations for this inhibited E2 strength. By comparing the results of these calculations to multiple observables, we conclude that there is a reduced role for out-of-space excitations in 32Si, resulting in a reduction in the corrections normally applied to both models.
引用
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页数:8
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