Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110
(2008) Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions 1012. p.296-299- Abstract
- The reduced transition probabilities between the first excited 2(+) state and the 0(+) ground state, B(E2; 0(+) -> 2(+)), have been measured in Sn-106,Sn-108,Sn-110 using sub-barrier Coulomb excitation in inverse kinematics at REX-ISOLDE. The results are, B(E2;0(+) -> 2(+)) = 0.220(22),0.226(17), and 0.228(32) e(2)b(2), for Sn-110, Sn-108, and Sn-106, respectively. The results for Sn-106,Sn-108 are preliminary. De-excitation gamma-rays were detected by the MINIBALL Ge-array. The B(E2) reveals detailed information about the nuclear wave function. A shell model prediction based on an effective CD-Bonn interaction in the nu(0g(7/2),2s, 1d, 0h(11/2)) model space using e(eff)(nu) =1.0 e follows the experimental values for the neutron rich... (More)
- The reduced transition probabilities between the first excited 2(+) state and the 0(+) ground state, B(E2; 0(+) -> 2(+)), have been measured in Sn-106,Sn-108,Sn-110 using sub-barrier Coulomb excitation in inverse kinematics at REX-ISOLDE. The results are, B(E2;0(+) -> 2(+)) = 0.220(22),0.226(17), and 0.228(32) e(2)b(2), for Sn-110, Sn-108, and Sn-106, respectively. The results for Sn-106,Sn-108 are preliminary. De-excitation gamma-rays were detected by the MINIBALL Ge-array. The B(E2) reveals detailed information about the nuclear wave function. A shell model prediction based on an effective CD-Bonn interaction in the nu(0g(7/2),2s, 1d, 0h(11/2)) model space using e(eff)(nu) =1.0 e follows the experimental values for the neutron rich Sn isotopes, but fails to reproduce the results presented here. (Less)
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/1407134
- author
- organization
- publishing date
- 2008
- type
- Chapter in Book/Report/Conference proceeding
- publication status
- published
- subject
- keywords
- mass number 90 to 149, nuclei with, Coulomb excitation, multipole matrix elements, shell model
- host publication
- Frontiers in Nuclear structure, Astrophysics and Reactions - Finustar 2, AIP Conference Proceedings
- volume
- 1012
- pages
- 296 - 299
- publisher
- American Institute of Physics (AIP)
- conference name
- Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions
- conference location
- Crete, Greece
- conference dates
- 2007-09-10 - 2007-09-14
- external identifiers
-
- wos:000256223700051
- scopus:85037701615
- ISSN
- 0094-243X
- 1551-7616
- DOI
- 10.1063/1.2939314
- language
- English
- LU publication?
- yes
- id
- 7cf174ff-212c-4e64-a1cb-ccfe96b0ebb3 (old id 1407134)
- date added to LUP
- 2016-04-01 12:21:11
- date last changed
- 2024-01-08 17:34:12
@inproceedings{7cf174ff-212c-4e64-a1cb-ccfe96b0ebb3, abstract = {{The reduced transition probabilities between the first excited 2(+) state and the 0(+) ground state, B(E2; 0(+) -> 2(+)), have been measured in Sn-106,Sn-108,Sn-110 using sub-barrier Coulomb excitation in inverse kinematics at REX-ISOLDE. The results are, B(E2;0(+) -> 2(+)) = 0.220(22),0.226(17), and 0.228(32) e(2)b(2), for Sn-110, Sn-108, and Sn-106, respectively. The results for Sn-106,Sn-108 are preliminary. De-excitation gamma-rays were detected by the MINIBALL Ge-array. The B(E2) reveals detailed information about the nuclear wave function. A shell model prediction based on an effective CD-Bonn interaction in the nu(0g(7/2),2s, 1d, 0h(11/2)) model space using e(eff)(nu) =1.0 e follows the experimental values for the neutron rich Sn isotopes, but fails to reproduce the results presented here.}}, author = {{Ekström, Andreas and Cederkäll, Joakim and Fahlander, Claes and Hjorth-Jensen, A. and Ames, F. and Butler, P. A. and Davinson, T. and Eberth, J. and Georgiev, G. and Gorgen, A. and Gorska, M. and Habs, D. and Huyse, M. and Ivanov, O. and Iwanicki, J. and Kester, O. and Koester, U. and Marsh, B. A. and Reiter, P. and Scheit, H. and Schwalm, D. and Siem, S. and Stefanescu, I. and Tveten, G. M. and Van de Walle, J. and Van Duppen, P. and Voulot, D. and Warr, N. and Weisshaar, D. and Wenander, E. and Zielinska, M.}}, booktitle = {{Frontiers in Nuclear structure, Astrophysics and Reactions - Finustar 2, AIP Conference Proceedings}}, issn = {{0094-243X}}, keywords = {{mass number 90 to 149; nuclei with; Coulomb excitation; multipole matrix elements; shell model}}, language = {{eng}}, pages = {{296--299}}, publisher = {{American Institute of Physics (AIP)}}, title = {{Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110}}, url = {{http://dx.doi.org/10.1063/1.2939314}}, doi = {{10.1063/1.2939314}}, volume = {{1012}}, year = {{2008}}, }