摘要The rare-earth nuclei 174Hf and 174Yb are studied in the framework of the projected shell model. The calculations are carried out with an improved version of code which contains all types of four−quasiparticle basis in the configuration space. Both the yrast band and the multi-quasiparticle excited bands can be well reproduced. Compared with the experimental data, our calculations improve the previous results, especially for high spin states. This improvement suggests that the newly added configurations are important. In 174Yb, a new possible configuration is suggested for the observed Kπ=14+ band, and the decay of the Kπ=6+ isomeric state to the yrast band is discussed.
Abstract:The rare-earth nuclei 174Hf and 174Yb are studied in the framework of the projected shell model. The calculations are carried out with an improved version of code which contains all types of four−quasiparticle basis in the configuration space. Both the yrast band and the multi-quasiparticle excited bands can be well reproduced. Compared with the experimental data, our calculations improve the previous results, especially for high spin states. This improvement suggests that the newly added configurations are important. In 174Yb, a new possible configuration is suggested for the observed Kπ=14+ band, and the decay of the Kπ=6+ isomeric state to the yrast band is discussed.
CHEN Fang-Qi;ZHOU Xian-Rong**
. 174Hf and 174Yb by the Projected Shell Model with Improved 4-quasiparticle basis[J]. 中国物理快报, 2011, 28(4): 42101-042101.
CHEN Fang-Qi, ZHOU Xian-Rong**
. 174Hf and 174Yb by the Projected Shell Model with Improved 4-quasiparticle basis. Chin. Phys. Lett., 2011, 28(4): 42101-042101.
[1] Hara K and Sun Y 1995 Int. J. Mod. Phys. E 4 637
[2] Hara K and Sun Y 1991 Nucl. Phys. A 529 445
[3] Sun Y and Egido J L 1994 Nucl. Phys. A 580 1
[4] Sun Y and Egido J L 1994 Phys. Rev. C 50 1893
[5] Archer D E, Riley M A et al 1995 Phy. Rev. C 52 1326
[6] Wen S X and Zheng H 1996 Phys. Rev. C 54 1015
[7] Palit R, Sheikh J A et al 2001 Nucl. Phys. A 686 141
[8] Doring J, Johns G D et al 1998 Phys. Rev. C 57 3912
[9] Shen S F, Wang F G et al 2006 High Energy Phys. Nucl. Phys. 12 1234
[10] Al-Khudiar F, Long G L et al 2009 Phys. Rev. C 79 034320
[11] Sun Y 2008 Rev. Mexi. Fisica S 54 122
[12] Tu Y et al 2006 High Energy Phys. Nucl. Phys. 30 SII 109
[13] Sun Y, Zhou X R et al 2004 Phys. Lett. B 589 83
[14] Zhou X R, Sun Y 2002 Chin. Phys. Lett. 19 1274
[15] Sun Y et al 1997 Phys. Rev. Lett. 78 2321
[16] Sun Y and Guidry M 1995 Phys. Rev. C 52 2844
[17] Sun Y et al 1997 Comput. Phys. Commun. 104 245
[18] Shen S F et al, 2010 Nucl. Phys. A834 90c
[19] Dracoulis G D, Lane G J et al 2005 Phys. Rev. C 71 044326
[20] Cullen D M, Baktash C et al 1995 Phys. Rev. C 52 2415
[21] Gjørup N L, Walker P M et al 1995 Nucl. Phys. A 582 369
[22] Mullins S M et al 1997 Phys. Lett. B 393 279
[23] Mullins S M et al 1997 Phys. Lett. B 400 401
[24] Hayes A B, Cline D et al 2007 Phys. Rev. C 75 034308
[25] Basunia M S 2006 Nucl. Data Sheets 107 791
[26] Purrt C S, Walker P M et al 1998 Nucl. Phys. A 632 229
[27] Herzberg R D, Greenlees P T et al 2006 Nature 442 896
[28] Nilsson S G et al 1969 Nucl. Phys. A 131 1
[29] Browne E and Junde H 1999 Nucl. Data Tables 87 15
[30] Bengtsson R et al 1986 At. Data Nucl. Data Tables 35 15
[31] Zeng J Y, Cheng T S et al 1984 Nucl. Phys. A 253 414
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[15]
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