A new method to prove the closed shell of N=184 for the neutron-rich superheavy elements

DING Bin-Gang; ZHANG Da-Li; LU Ding-Hui

Chinese Physics C> 2006, Vol. 30> Issue(4) : 310-313

A new method to prove the closed shell of N=184 for the neutron-rich superheavy elements

College of Science, Huzhou Tearcher's College, Zhejiang Huzhou 313000, China2 Institute of Modern Physics, Zhejiang University, Hangzhou 310027, China

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Abstract：
The clear shell effect of the pairing strength is proved based on the frame of the relativistic mean filed theory. With the same theory, the closed shell problem of the superheavy isotope chain around Z=96—102 is studied. The results show that N=184 for neutron is a closed shell. According to the study, a new method to check the shell closure is given.

References

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DING Bin-Gang, ZHANG Da-Li and LU Ding-Hui. A new method to prove the closed shell of N=184 for the neutron-rich superheavy elements[J]. Chinese Physics C, 2006, 30(4): 310-313.

DING Bin-Gang, ZHANG Da-Li and LU Ding-Hui. A new method to prove the closed shell of N=184 for the neutron-rich superheavy elements[J]. Chinese Physics C, 2006, 30(4): 310-313. shu

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Received: 2005-11-04
Revised: 2005-12-12

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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

A new method to prove the closed shell of N=184 for the neutron-rich superheavy elements

Corresponding author: DING Bin-Gang,

College of Science, Huzhou Tearcher's College, Zhejiang Huzhou 313000, China2 Institute of Modern Physics, Zhejiang University, Hangzhou 310027, China

Received Date: 2005-11-04

Accepted Date: 2005-12-12

Available Online: 2006-04-05

Abstract: The clear shell effect of the pairing strength is proved based on the frame of the relativistic mean filed theory. With the same theory, the closed shell problem of the superheavy isotope chain around Z=96—102 is studied. The results show that N=184 for neutron is a closed shell. According to the study, a new method to check the shell closure is given.

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A new method to prove the closed shell of N=184 for the neutron-rich superheavy elements

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