Coulomb breakup of psd-shell neutron-rich nuclei

被引:2
|
作者
Pramanik, UD
Adrich, P
Aumann, T
Boretzky, K
Cortina, D
Elze, TW
Emling, H
Geissel, H
Hellström, M
Jones, KL
Khiem, LH
Kratz, JV
Kulessa, R
Leifels, Y
Münzenberg, G
Nocifor, C
Palit, R
Scheif, H
Simon, H
Sümmerer, K
Typel, S
Walus, W
Weick, H
机构
[1] Saha Inst Nucl Phys, Kolkata 700009, W Bengal, India
[2] Gesell Schwerionenforsch Inst Darmstadt, D-6100 Darmstadt, Germany
[3] Univ Santiago de Compostela, Santiago De Compostela, Spain
[4] Goethe Univ Frankfurt, Inst Kernphys, D-6000 Frankfurt, Germany
[5] Johannes Gutenberg Univ Mainz, Inst Kernchem, D-6500 Mainz, Germany
[6] Jagiellonian Univ, Inst Fiz, Krakow, Poland
[7] Inst Kernphys, Heidelberg, Germany
关键词
D O I
10.1088/0954-3899/31/10/037
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
Inelastic scattering of loosely bound nuclei by Coulomb interaction at intermediate energies (400-600 MeV/nucleon) has been utilized as a spectroscopic tool for exotic nuclei. The observed electromagnetic dipole (E1) strength above the one neutron threshold of neutron-rich C, Be, B and 0 isotopes can be explained by a non-resonant transition of a neutron into the continuum. The shape of these strength distributions reflects properties of the wavefunction of the released neutron in the nucleus and hence groundstate properties of these isotopes. Neutron capture cross-sections such as for the C-14(n,gamma)C-15 reaction which are of astrophysical relevance can be deduced indirectly.
引用
收藏
页码:S1583 / S1587
页数:5
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