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Magnetic moments of the first excited 2(+) states in the semi-magic Sn-112,Sn-114,Sn-116,Sn-122,Sn-124 isotopes

Walker, J. ; Jungclaus, A. ; Leske, J. ; Speidel, K. -H. ; Ekström, Andreas LU ; Boutachkov, P. ; Cederkäll, Joakim LU ; Doornenbal, P. ; Gerl, J. and Gernhaeuser, R. , et al. (2011) In Physical Review C (Nuclear Physics) 84(1).
Abstract
The g factors of the first excited 2(+) states in the Sn-112,Sn-114,Sn-116,Sn-122,Sn-124 isotopes have been measured with high accuracy using the transient field technique in combination with Coulomb excitation in inverse kinematics. The experimental results are discussed in a qualitative way on the basis of empirical single-particle g factors of the relevant proton and neutron orbitals and are compared to a number of different theoretical calculations. The results are found to be best described by shell-model calculations in an extended configuration space. Clear evidence for the contribution of neutron pair excitations from the 1d(3/2) to the 0h(11/2) orbital to the wave function of the 2(1)(+) state in Sn-122,Sn-124 has been obtained.
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organization
publishing date
type
Contribution to journal
publication status
published
subject
in
Physical Review C (Nuclear Physics)
volume
84
issue
1
article number
014319
publisher
American Physical Society
external identifiers
  • wos:000292875300001
  • scopus:79961125002
ISSN
0556-2813
DOI
10.1103/PhysRevC.84.014319
language
English
LU publication?
yes
id
8aadc114-aa93-43a0-a0fd-4adf7269ecd0 (old id 2093899)
date added to LUP
2016-04-01 14:20:29
date last changed
2022-01-28 00:02:11
@article{8aadc114-aa93-43a0-a0fd-4adf7269ecd0,
  abstract     = {{The g factors of the first excited 2(+) states in the Sn-112,Sn-114,Sn-116,Sn-122,Sn-124 isotopes have been measured with high accuracy using the transient field technique in combination with Coulomb excitation in inverse kinematics. The experimental results are discussed in a qualitative way on the basis of empirical single-particle g factors of the relevant proton and neutron orbitals and are compared to a number of different theoretical calculations. The results are found to be best described by shell-model calculations in an extended configuration space. Clear evidence for the contribution of neutron pair excitations from the 1d(3/2) to the 0h(11/2) orbital to the wave function of the 2(1)(+) state in Sn-122,Sn-124 has been obtained.}},
  author       = {{Walker, J. and Jungclaus, A. and Leske, J. and Speidel, K. -H. and Ekström, Andreas and Boutachkov, P. and Cederkäll, Joakim and Doornenbal, P. and Gerl, J. and Gernhaeuser, R. and Goel, N. and Gorska, M. and Kojouharov, I. and Maier-Komor, P. and Modamio, V. and Naqvi, F. and Pietralla, N. and Pietri, S. and Prokopowicz, W. and Schaffner, H. and Schwengner, R. and Wollersheim, H. -J.}},
  issn         = {{0556-2813}},
  language     = {{eng}},
  number       = {{1}},
  publisher    = {{American Physical Society}},
  series       = {{Physical Review C (Nuclear Physics)}},
  title        = {{Magnetic moments of the first excited 2(+) states in the semi-magic Sn-112,Sn-114,Sn-116,Sn-122,Sn-124 isotopes}},
  url          = {{http://dx.doi.org/10.1103/PhysRevC.84.014319}},
  doi          = {{10.1103/PhysRevC.84.014319}},
  volume       = {{84}},
  year         = {{2011}},
}