Projected shell model description for high-spin states in neutron-rich Fe isotopes

2009 ◽  
Vol 80 (5) ◽  
Author(s):  
Yang Sun ◽  
Ying-Chun Yang ◽  
Hong-Liang Liu ◽  
Kazunari Kaneko ◽  
Munetake Hasegawa ◽  
...  
2004 ◽  
Vol 69 (6) ◽  
Author(s):  
D. Bucurescu ◽  
N. Mărginean ◽  
C. Rossi Alvarez ◽  
Y. Sun ◽  
C. A. Ur ◽  
...  

2005 ◽  
Vol 72 (6) ◽  
Author(s):  
Rani Devi ◽  
B. D. Sehgal ◽  
S. K. Khosa ◽  
J. A. Sheikh

1995 ◽  
Vol 04 (04) ◽  
pp. 637-785 ◽  
Author(s):  
KENJI HARA ◽  
YANG SUN

Most of the nuclei in the nuclear chart are deformed except for those in the vicinity of the magic numbers. It is difficult to treat such nuclei within the framework of the standard (spherical) shell model. On the other hand, the necessity for a proper quantum mechanical treatment of high-spin states has been steadily growing ever since modern experimental techniques made it possible to measure the fine details of the high-spin states of heavy nuclei. The present article reviews an approach based on the angular momentum projection technique which was initiated in the late seventies for the purpose of carrying out shell model configuration mixing calculations efficiently. A large number of examples is presented with an emphasis on the physical interpretation of the numerical results. Computing time for the whole spectrum up to spin ≈ 40 of an axially symmetric rare-earth nucleus takes only a few minutes on a Mainframe, showing the efficiency of the method. Most of the present calculations were carried out on a Workstation, but computation on a modern PC also presents no problem, so that one can enjoy a genuine quantum mechanical analysis of high-spin data using a facility available everywhere. Detailed technical information which may be useful for programming purposes is given in an Appendix.


2017 ◽  
Vol 95 (6) ◽  
Author(s):  
S. Biswas ◽  
R. Palit ◽  
J. Sethi ◽  
S. Saha ◽  
A. Raghav ◽  
...  

2019 ◽  
Vol 2019 (10) ◽  
Author(s):  
Praveen C Srivastava ◽  
Bharti Bhoy ◽  
M J Ermamatov

Abstract In the present work, available experimental data up to high-spin states of $^{119-126}$Sn isotopes with different seniority ($v$), including $v = 4$, 5, 6, and 7, are interpreted with the shell model, by performing shell-model calculations in the 50–82 valence shell composed of $1g_{7/2}$, $2d_{5/2}$, $1h_{11/2}$, $3s_{1/2}$, and $2d_{3/2}$ orbitals. The results are compared with the available experimental data. These states are described in terms of broken neutron pairs occupying the $h_{11/2}$ orbital. Possible configurations of seniority isomers in these nuclei are discussed. The breaking of three neutron pairs is responsible for generating high-spin states. The isomeric states $5^-$, $7^-$, $10^+$, and $15^-$ of even Sn isotopes, and isomeric states $19/2^+$, $23/2^+$, $27/2^-$, and $35/2^+$ of odd Sn isotopes, are described in terms of different seniority. For even Sn isotopes, the isomeric states $5^-$, $7^-$, and $10^+$ are due to seniority $v = 2$; the isomeric state $15^-$ is due to seniority $v = 4$, and, in the case of odd Sn isotopes, the isomeric states $19/2^+$, $23/2^+$, and $27/2^-$ are due to seniority $v = 3$, and the isomeric state $35/2^+$ in $^{123}$Sn is due to seniority $v = 5$. These are maximally aligned spins, which involve successive pair breakings in the $\nu (h_{11/2})$ orbital.


1994 ◽  
Vol 49 (4) ◽  
pp. 1896-1903 ◽  
Author(s):  
J. Heese ◽  
H. Grawe ◽  
K. H. Maier ◽  
R. Schubart ◽  
F. Cristancho ◽  
...  

2015 ◽  
Vol 91 (2) ◽  
Author(s):  
Tomoaki Togashi ◽  
Noritaka Shimizu ◽  
Yutaka Utsuno ◽  
Takaharu Otsuka ◽  
Michio Honma

1985 ◽  
Vol 321 (3) ◽  
pp. 485-498 ◽  
Author(s):  
K. Oxorn ◽  
S. K. Mark ◽  
J. E. Kitching ◽  
S. S. M. Wong

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