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Evolution of the N=82 Shell Gap below 132Sn Inferred from Core Excited States in 131In

Gorska, M. ; Caceres, L. ; Grawe, H. ; Pfuetzner, M. ; Jungclaus, A. ; Pietri, S. ; Werner-Malento, E. ; Podolyak, Z. ; Regan, P. H. and Rudolph, Dirk LU orcid , et al. (2009) In Physics Letters. Section B: Nuclear, Elementary Particle and High-Energy Physics 672(4-5). p.313-316
Abstract
The gamma-ray decay of ail excited state in In-131, the one proton hole neighbor of the doubly magic (132)sn has been measured. A high-spin, core-excited isomer with T-1/2 = 630(60) us was identified following production by both relativistic fragmentation of a Xe-136 beam and fission Of a U-238 beam. This state deexcites by a single gamma-ray branch of 3782(2) keV from which direct evidence for the size of the N = 82 shell gal) is inferred. The results are discussed in comparison to a shell-model Calculation including configurations across the closed shells at N = 82 and Z = 50. (C) 2009 Elsevier B.V. All rights reserved.
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organization
publishing date
type
Contribution to journal
publication status
published
subject
in
Physics Letters. Section B: Nuclear, Elementary Particle and High-Energy Physics
volume
672
issue
4-5
pages
313 - 316
publisher
Elsevier
external identifiers
  • wos:000264371400001
  • scopus:60449087467
ISSN
0370-2693
DOI
10.1016/j.physletb.2009.01.027
language
English
LU publication?
yes
id
6d852ab1-1dd2-4d9d-83df-675e9e23a346 (old id 1401714)
date added to LUP
2016-04-01 13:22:42
date last changed
2022-04-06 04:48:05
@article{6d852ab1-1dd2-4d9d-83df-675e9e23a346,
  abstract     = {{The gamma-ray decay of ail excited state in In-131, the one proton hole neighbor of the doubly magic (132)sn has been measured. A high-spin, core-excited isomer with T-1/2 = 630(60) us was identified following production by both relativistic fragmentation of a Xe-136 beam and fission Of a U-238 beam. This state deexcites by a single gamma-ray branch of 3782(2) keV from which direct evidence for the size of the N = 82 shell gal) is inferred. The results are discussed in comparison to a shell-model Calculation including configurations across the closed shells at N = 82 and Z = 50. (C) 2009 Elsevier B.V. All rights reserved.}},
  author       = {{Gorska, M. and Caceres, L. and Grawe, H. and Pfuetzner, M. and Jungclaus, A. and Pietri, S. and Werner-Malento, E. and Podolyak, Z. and Regan, P. H. and Rudolph, Dirk and Detistov, R. and Lalkovski, S. and Modamio, V. and Walker, J. and Beck, T. and Bednarczyk, P. and Doornenbal, P. and Geissel, H. and Gerl, J. and Grebosz, J. and Hoischen, Robert and Kojouharov, I. and Kurz, N. and Prokopowicz, W. and Schaffner, H. and Weick, H. and Wollersheim, H. -J. and Andgren, K. and Benlliure, J. and Benzoni, G. and Bruce, A. M. and Casarejos, E. and Cederwall, B. and Crespi, F. C. L. and Hadinia, B. and Hellström, Margareta and Ilie, G. and Khaplanov, A. and Kmiecik, M. and Kumar, R. and Maj, A. and Mandal, S. and Montes, F. and Myalski, S. and Simpson, G. S. and Steer, S. J. and Tashenov, S. and Wieland, O. and Dombradi, Zs. and Reiter, R. and Sohler, D.}},
  issn         = {{0370-2693}},
  language     = {{eng}},
  number       = {{4-5}},
  pages        = {{313--316}},
  publisher    = {{Elsevier}},
  series       = {{Physics Letters. Section B: Nuclear, Elementary Particle and High-Energy Physics}},
  title        = {{Evolution of the N=82 Shell Gap below 132Sn Inferred from Core Excited States in 131In}},
  url          = {{http://dx.doi.org/10.1016/j.physletb.2009.01.027}},
  doi          = {{10.1016/j.physletb.2009.01.027}},
  volume       = {{672}},
  year         = {{2009}},
}