Magnetic moments of the first excited 2(+) states in the semi-magic Sn-112,Sn-114,Sn-116,Sn-122,Sn-124 isotopes
(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.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/2093899
- author
- organization
- publishing date
- 2011
- 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}}, }