Halo structure of the island of inversion nucleus 31Ne.

Halo structure of the island of inversion nucleus 31Ne.
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DOI:
10.1103/physrevlett.103.262501
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发表时间:
2009-12
影响因子:
8.6
通讯作者:
Takashi Nakamura;N. Kobayashi;Y. Kondo;Y. Satou;N. Aoi;H. Baba;S. Deguchi;N. Fukuda;J. Gibelin;N. Inabe;M. Ishihara;D. Kameda;Y. Kawada;T. Kubo;K. Kusaka;A. Mengoni;T. Motobayashi;T. Ohnishi;M. Ohtake;N. Orr;H. Otsu;T. Otsuka;A. Saito;H. Sakurai;S. Shimoura;T. Sumikama;H. Takeda;E. Takeshita;M. Takechi;Shotaro Takeuchi;Kazuhiro Tanaka;K. Tanaka;N. Tanaka;Y. Togano;Y. Utsuno;K. Yoneda;A. Yoshida;K. Yoshida
Takashi Nakamura;N. Kobayashi;Y. Kondo;Y. Satou;N. Aoi;H. Baba;S. Deguchi;N. Fukuda;J. Gibelin;N. Inabe;M. Ishihara;D. Kameda;Y. Kawada;T. Kubo;K. Kusaka;A. Mengoni;T. Motobayashi;T. Ohnishi;M. Ohtake;N. Orr;H. Otsu;T. Otsuka;A. Saito;H. Sakurai;S. Shimoura;T. Sumikama;H. Takeda;E. Takeshita;M. Takechi;Shotaro Takeuchi;Kazuhiro Tanaka;K. Tanaka;N. Tanaka;Y. Togano;Y. Utsuno;K. Yoneda;A. Yoshida;K. Yoshida
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
Takashi Nakamura;N. Kobayashi;Y. Kondo;Y. Satou;N. Aoi;H. Baba;S. Deguchi;N. Fukuda;J. Gibelin;N. Inabe;M. Ishihara;D. Kameda;Y. Kawada;T. Kubo;K. Kusaka;A. Mengoni;T. Motobayashi;T. Ohnishi;M. Ohtake;N. Orr;H. Otsu;T. Otsuka;A. Saito;H. Sakurai;S. Shimoura;T. Sumikama;H. Takeda;E. Takeshita;M. Takechi;Shotaro Takeuchi;Kazuhiro Tanaka;K. Tanaka;N. Tanaka;Y. Togano;Y. Utsuno;K. Yoneda;A. Yoshida;K. Yoshida

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利用日本理化学研究所的RIBF装置,在230 MeV/核子的能量下,测量了丰中子核~(31)Ne在Pb和C靶上的单中子去除截面。推导出的540(70)mb的大库仑破裂截面是软E1激发的指示。与直接破裂模型计算结果的比较表明,31 Ne的价中子占据低l轨道(最可能是2 p(3/2)),分离能小(S(n)约< 0.8 MeV),而不是像传统壳层有序理论所预期的那样主要在1f(7/2)轨道。这些发现表明,31 Ne是已知最重的晕系统。
The cross sections for single-neutron removal from the very neutron-rich nucleus 31Ne on Pb and C targets have been measured at 230 MeV/nucleon using the RIBF facility at RIKEN. The deduced large Coulomb breakup cross section of 540(70) mb is indicative of a soft E1 excitation. Comparison with direct-breakup model calculations suggests that the valence neutron of 31Ne occupies a low-l orbital (most probably 2p(3/2)) with a small separation energy (S(n) approximately < 0.8 MeV), instead of being predominantly in the 1f(7/2) orbital as expected from the conventional shell ordering. These findings suggest that 31Ne is the heaviest halo system known.