PROLATE OBLATE BAND MIXING AND NEW BANDS IN HG-182

被引：23

作者：

BINDRA, KS

HUA, PF

BABU, BRS

BAKTASH, C

BARRETO, J

CULLEN, DM

DAVIDS, CN

DENG, JK

GARRETT, JD

HALBERT, ML

HAMILTON, JH

JOHNSON, NR

KIROV, A

KORMICKI, J

LEE, IY

MA, WC

MCGOWAN, FK

RAMAYYA, AV

SARANTITES, DG

SORAMEL, F

WINCHELL, D

机构：

[1] ARGONNE NATL LAB, DIV PHYS, ARGONNE, IL 60439 USA

[2] WASHINGTON UNIV, DEPT CHEM, ST LOUIS, MO 63130 USA

[3] OAK RIDGE NATL LAB, OAK RIDGE, TN 37831 USA

[4] UNISOR, OAK RIDGE, TN 37831 USA

来源：

PHYSICAL REVIEW C | 1995年 / 51卷 / 01期

关键词：

D O I：

10.1103/PhysRevC.51.401

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

In-beam γ-ray spectroscopic studies of Hg182 have revealed five new bands. The 2+ state of the prolate band has been identified at an energy of 548.6 keV and is higher than in Hg184. A two parameter band mixing calculation results in an interaction energy of 83 keV between the prolate 2+ and the oblate 2+ states. Several additional new bands are seen including some which are interpreted as quadrupole vibrational bands built on the excited prolate minimum. © 1995 The American Physical Society.

引用

页码：401 / 404

页数：4

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