4.7 Article

Evolution of the N=82 shell gap below 132Sn inferred from core excited states in 131In

期刊

PHYSICS LETTERS B
卷 672, 期 4-5, 页码 313-316

出版社

ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2009.01.027

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资金

  1. EU
  2. Polish Ministry of Science and Higher Education [1-P03B-030-30, 620/E-77/SPB/GSI/P-03/DWM105/2004-2007]
  3. Spanish Ministerio de Educacion y Ciencia [FPA2005-00696, FPA2005-00732, FPA2007-66069]
  4. EPSRC/STFC (UK)
  5. Swedish Research Council
  6. Bulgarian Science Fund [VUF06/05]
  7. US Dept. of Energy [DEFG02-91ER-40609, DE-AC02-06CH11357]
  8. German Federal Ministry of Education and Research [06KY2051]
  9. Hungarian Science Foundation [OTKA K-68801]
  10. Italian INFN
  11. [506065]
  12. STFC [ST/F012012/1, EP/D072018/1] Funding Source: UKRI
  13. Science and Technology Facilities Council [EP/D072018/1, ST/F012012/1, ST/F012128/1] Funding Source: researchfish

向作者/读者索取更多资源

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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