Cross-shell excited states in 32Si and 29Al populated using fusion-evaporation

被引:0
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作者
Williamsa, J. [1 ]
Hackmana, G. [1 ]
Starosta, K. [2 ]
Lubna, R. S. [4 ]
Choudhary, Priyanka [5 ,12 ]
Sahoo, S. [5 ]
Srivastava, P. C. [5 ]
Andreoiu, C. [2 ]
Annen, D. [2 ]
Asch, H. [3 ]
Badanage, M. D. H. K. G. [2 ]
Ball, G. C. [1 ]
Beuschlein, M. [6 ]
Bidaman, H. [7 ]
Bildstein, V. [7 ]
Coleman, R. [7 ]
Garnsworthy, A. B. [1 ]
Greaves, B. [7 ]
Leckenby, G. [1 ,8 ]
Karayonchev, V. [1 ,13 ]
Martin, M. S. [3 ,13 ]
Natzke, C. [1 ]
Petrache, C. M. [9 ]
Radich, A. [7 ]
Raleigh-Smitha, E. [1 ]
Rhodes, D. [1 ,14 ]
Russellj, R. [10 ]
Satrazani, M. [11 ]
Spagnoletti, P. [2 ]
Svensson, C. E. [1 ]
Tam, D. [3 ]
Wu, F. [2 ]
Yates, D. [1 ,8 ]
Yu, Z. [2 ]
机构
[1] TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada
[2] Simon Fraser Univ, Dept Chem, 8888 Univ Dr, Burnaby, BC V5A 1S6, Canada
[3] Simon Fraser Univ, Dept Phys, 8888 Univ Dr, Burnaby, BC V5A 1S6, Canada
[4] Michigan State Univ, Facil Rare Isotope Beams, 640 South Shaw Lane, E Lansing, MI 48824 USA
[5] Indian Inst Technol Roorkee, Dept Phys, Roorkee 247667, India
[6] Tech Univ Darmstadt, Inst Nucl Phys, Dept Phys, Schlossgartenstr 9, D-64289 Darmstadt, Germany
[7] Univ Guelph, Dept Phys, 50 Stone Rd, Guelph, ON N1G 2W1, Canada
[8] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[9] Univ Paris Saclay, CNRS, IN2P3, IJCLab, F-91405 Orsay, France
[10] Univ Surrey, Guildford GU2 7XH, England
[11] UNIV LIVERPOOL, LIVERPOOL L69 3BX, England
[12] KTH Royal Inst Technol, Dept Phys, SE-10691 Stockholm, Sweden
[13] Argonne Natl Lab, 9700 S Cass Ave, Lemont, IL 60439 USA
[14] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA
基金
加拿大自然科学与工程研究理事会;
关键词
Fusion-evaporation; Gamma-ray spectroscopy; Cross-shell excitation; Shell evolution;
D O I
10.1016/j.nuclphysa.2025.123042
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
In the neutron-rich sd shell near the N = 20 'island of inversion', the evolution of the N = 20 shell gap is indicated by the energies of negative-parity states which primarily arise due to single neutron excitation to higher lying orbitals across the shell gap. These negative-parity states often have high spin (due to the participation of the 0f7/2 orbital) and are therefore preferentially populated using fusion-evaporation reactions. We have studied the intermediate energy levels of 32Si and 29Al using 12C(22Ne,2p) and 12C(22Ne,alpha p) reactions, identifying several negative-parity states in both nuclides.
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页数:4
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