Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110

A. Ekstrom; J. Cederkaell; C. Fahlander; A. Hjorth-Jensen; F. Ames; P. A. Butler; T. Davinson; J. Eberth; G. Georgiev; A. Gorgen; M. Gorska; D. Habs; M. Huyse; O. Ivanov; J. Iwanicki; O. Kester; U. Koester; B. A. Marsh; P. Reiter; H. Scheit; D. Schwalm; S. Siem; I. Stefanescu; G. M. Tveten; J. Van de Walle; P. Van Duppen; D. Voulot; N. Warr; D. Weisshaar; E. Wenander; M. Zielinska

Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110

A. Ekstrom
, J. Cederkaell
, C. Fahlander
, A. Hjorth-Jensen
, F. Ames
, P. A. Butler
, T. Davinson
, J. Eberth
, G. Georgiev
, A. Gorgen
, M. Gorska
, D. Habs
, M. Huyse
, O. Ivanov
, J. Iwanicki
, O. Kester
, U. Koester
, B. A. Marsh
, P. Reiter
, H. Scheit

D. Schwalm, S. Siem, I. Stefanescu, G. M. Tveten, J. Van de Walle, P. Van Duppen, D. Voulot, N. Warr, D. Weisshaar, E. Wenander, M. Zielinska

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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.

Original language	Undefined/Unknown
Title of host publication	FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2
Editors	P Demetriuo, SV Harissopulos
Pages	296-299
Number of pages	4
Volume	1012
Publication status	Published - 2008

Publication series

Name	AIP CONFERENCE PROCEEDINGS

Cite this

Ekstrom, A., Cederkaell, J., Fahlander, C., Hjorth-Jensen, A., Ames, F., Butler, P. A., Davinson, T., Eberth, J., Georgiev, G., Gorgen, A., Gorska, M., Habs, D., Huyse, M., Ivanov, O., Iwanicki, J., Kester, O., Koester, U., Marsh, B. A., Reiter, P., ... Zielinska, M. (2008). Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110. In P. Demetriuo, & SV. Harissopulos (Eds.), FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2 (Vol. 1012, pp. 296-299). (AIP CONFERENCE PROCEEDINGS).

@inproceedings{7ee2ffc30b524c8a9ee8070c6a724baf,

title = "Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110",

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 = "A. Ekstrom and J. Cederkaell and C. Fahlander and A. Hjorth-Jensen and F. Ames and Butler, \{P. A.\} and T. Davinson and J. Eberth and G. Georgiev and A. Gorgen and M. Gorska and D. Habs and M. Huyse and O. Ivanov and J. Iwanicki and O. Kester and U. Koester and Marsh, \{B. A.\} and P. Reiter and H. Scheit and D. Schwalm and S. Siem and I. Stefanescu and Tveten, \{G. M.\} and \{Van de Walle\}, J. and \{Van Duppen\}, P. and D. Voulot and N. Warr and D. Weisshaar and E. Wenander and M. Zielinska",

note = "Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, Crete, GREECE, SEP 10-14, 2007",

year = "2008",

language = "Undefined/Unknown",

volume = "1012",

series = "AIP CONFERENCE PROCEEDINGS",

pages = "296--299",

editor = "P Demetriuo and SV Harissopulos",

booktitle = "FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2",

}

Ekstrom, A, Cederkaell, J, Fahlander, C, Hjorth-Jensen, A, Ames, F, Butler, PA, Davinson, T, Eberth, J, Georgiev, G, Gorgen, A, Gorska, M, Habs, D, Huyse, M, Ivanov, O, Iwanicki, J, Kester, O, Koester, U, Marsh, BA, Reiter, P, Scheit, H, Schwalm, D, Siem, S, Stefanescu, I, Tveten, GM, Van de Walle, J, Van Duppen, P, Voulot, D, Warr, N, Weisshaar, D, Wenander, E & Zielinska, M 2008, Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110. in P Demetriuo & SV Harissopulos (eds), FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. vol. 1012, AIP CONFERENCE PROCEEDINGS, pp. 296-299.

TY - GEN

T1 - Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110

AU - Ekstrom, A.

AU - Cederkaell, J.

AU - Fahlander, C.

AU - Hjorth-Jensen, A.

AU - Ames, F.

AU - Butler, P. A.

AU - Davinson, T.

AU - Eberth, J.

AU - Georgiev, G.

AU - Gorgen, A.

AU - Gorska, M.

AU - Habs, D.

AU - Huyse, M.

AU - Ivanov, O.

AU - Iwanicki, J.

AU - Kester, O.

AU - Koester, U.

AU - Marsh, B. A.

AU - Reiter, P.

AU - Scheit, H.

AU - Schwalm, D.

AU - Siem, S.

AU - Stefanescu, I.

AU - Tveten, G. M.

AU - Van de Walle, J.

AU - Van Duppen, P.

AU - Voulot, D.

AU - Warr, N.

AU - Weisshaar, D.

AU - Wenander, E.

AU - Zielinska, M.

N1 - Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, Crete, GREECE, SEP 10-14, 2007

PY - 2008

Y1 - 2008

N2 - 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.

AB - 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.

M3 - Conference contribution

VL - 1012

T3 - AIP CONFERENCE PROCEEDINGS

SP - 296

EP - 299

BT - FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2

A2 - Demetriuo, P

A2 - Harissopulos, SV

ER -