CONTRASTING HIGH-SPIN YRAST BANDS IN OS-172 AND OS-174 AND AN UNEXPECTED LOW-FREQUENCY ANOMALY IN OS-172

被引：46

作者：

DURELL, JL ^{[1
]}

DRACOULIS, GD ^{[1
]}

FAHLANDER, C ^{[1
]}

BYRNE, AP ^{[1
]}

机构：

[1] AUSTRALIAN NATL UNIV,RES SCH PHYS SCI,DEPT NUCL PHYS,CANBERRA,ACT 2600,AUSTRALIA

来源：

PHYSICS LETTERS B | 1982年 / 115卷 / 05期

关键词：

D O I：

10.1016/0370-2693(82)90519-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：367 / 371

页数：5

共 19 条

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[2] INTERPRETATION OF BACKBENDING IN TERMS OF THE CROSSING OF THE GROUND-STATE BAND WITH AN ALIGNED 2-QUASI-PARTICLE BAND [J].

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[3]

BENGTSSON R, 1980, J PHYS A, V10, P84

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[6] BACKBENDING IN W-178 [J].

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[7] CAUSE OF BACKBENDING IN OS REGION [J].

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[8] SYSTEMATICS OF THE 1/2+[660] QUASI-NEUTRON CONFIGURATION IN OS-176-OS-186 AS DETERMINED FROM BAND-CROSSING FREQUENCIES [J].

GARRETT, JD ;

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PHYSICS LETTERS B, 1982, 108 (02) :77-82

[9] ALPHA-DECAY OF NEUTRON-DEFICIENT MERCURY ISOTOPES AND THEIR DAUGHTERS [J].

HAGBERG, E ;

HANSEN, PG ;

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JONSON, B ;

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NUCLEAR PHYSICS A, 1979, 318 (1-2) :29-44

[10] SHELL STRUCTURE EFFECTS ON HIGH-SPIN ROTATIONAL STATES IN YTTERBIUM NUCLEI [J].

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