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

M. Górska; L. Cáceres; H. Grawe; M. Pfützner; A. Jungclaus; S. Pietri; E. Werner-Malento; Z. Podolyák; P.H. Regan; D. Rudolph; P. Detistov; S. Lalkovski; V. Modamio; J. Walker; T. Beck; P. Bednarczyk; P. Doornenbal; H. Geissel; J. Gerl; J. Grëbosz; R. Hoischen; I. Kojouharov; N. Kurz; W. Prokopowicz; H. Schaffner; H. Weick; H.J. Wollersheim; K. Andgren; J. Benlliure; G. Benzoni; Alison Bruce; E. Casarejos; B. Cederwall; F.C.L. Crespi; B. Hadinia; M. Hellström; G. Ilie; A. Khaplanov; M. Kmiecik; R. Kumar; A. Maj; S. Mandal; F. Montes; S. Myalski; G.S. Simpson; S.J. Steer; S. Tashenov; O. Wieland; Zs. Dombrádi; P. Reiter

doi:10.1016/j.physletb.2009.01.027

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

M. Górska, L. Cáceres, H. Grawe, M. Pfützner, A. Jungclaus, S. Pietri, E. Werner-Malento, Z. Podolyák, P.H. Regan, D. Rudolph, P. Detistov, S. Lalkovski, V. Modamio, J. Walker, T. Beck, P. Bednarczyk, P. Doornenbal, H. Geissel, J. Gerl, J. GrëboszR. Hoischen, I. Kojouharov, N. Kurz, W. Prokopowicz, H. Schaffner, H. Weick, H.J. Wollersheim, K. Andgren, J. Benlliure, G. Benzoni, Alison Bruce, E. Casarejos, B. Cederwall, F.C.L. Crespi, B. Hadinia, M. Hellström, G. Ilie, A. Khaplanov, M. Kmiecik, R. Kumar, A. Maj, S. Mandal, F. Montes, S. Myalski, G.S. Simpson, S.J. Steer, S. Tashenov, O. Wieland, Zs. Dombrádi, P. Reiter

University of Brighton

Research output: Contribution to journal › Article › peer-review

Abstract

The γ-ray decay of an excited state in 131In, the one proton hole neighbor of the doubly magic 132Sn has been measured. A high-spin, core-excited isomer with T1/2=630(60) ns was identified following production by both relativistic fragmentation of a 136Xe beam and fission of a 238U beam. This state deexcites by a single γ-ray branch of 3782(2) keV from which direct evidence for the size of the N=82 shell gap 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.

Original language	English
Pages (from-to)	313-316
Number of pages	4
Journal	Physics Letters B
Volume	672
Issue number	4-5
DOIs	https://doi.org/10.1016/j.physletb.2009.01.027
Publication status	Published - Mar 2009

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Górska, M., Cáceres, L., Grawe, H., Pfützner, M., Jungclaus, A., Pietri, S., Werner-Malento, E., Podolyák, Z., Regan, P. H., Rudolph, D., Detistov, P., Lalkovski, S., Modamio, V., Walker, J., Beck, T., Bednarczyk, P., Doornenbal, P., Geissel, H., Gerl, J., ... Reiter, P. (2009). Evolution of the N=82 shell gap below ¹³²Sn inferred from core excited states in ¹³¹In. Physics Letters B, 672(4-5), 313-316. https://doi.org/10.1016/j.physletb.2009.01.027

@article{a43c6779429d4d3c9588cc4a51a37e9f,

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

abstract = "The γ-ray decay of an excited state in 131In, the one proton hole neighbor of the doubly magic 132Sn has been measured. A high-spin, core-excited isomer with T1/2=630(60) ns was identified following production by both relativistic fragmentation of a 136Xe beam and fission of a 238U beam. This state deexcites by a single γ-ray branch of 3782(2) keV from which direct evidence for the size of the N=82 shell gap 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.",

author = "M. G{\'o}rska and L. C{\'a}ceres and H. Grawe and M. Pf{\"u}tzner and A. Jungclaus and S. Pietri and E. Werner-Malento and Z. Podoly{\'a}k and P.H. Regan and D. Rudolph and P. Detistov and S. Lalkovski and V. Modamio and J. Walker and T. Beck and P. Bednarczyk and P. Doornenbal and H. Geissel and J. Gerl and J. Gr{\"e}bosz and R. Hoischen and I. Kojouharov and N. Kurz and W. Prokopowicz and H. Schaffner and H. Weick and H.J. Wollersheim and K. Andgren and J. Benlliure and G. Benzoni and Alison Bruce and E. Casarejos and B. Cederwall and F.C.L. Crespi and B. Hadinia and M. Hellstr{\"o}m and G. Ilie and A. Khaplanov and M. Kmiecik and R. Kumar and A. Maj and S. Mandal and F. Montes and S. Myalski and G.S. Simpson and S.J. Steer and S. Tashenov and O. Wieland and Zs. Dombr{\'a}di and P. Reiter",

year = "2009",

month = mar,

doi = "10.1016/j.physletb.2009.01.027",

language = "English",

volume = "672",

pages = "313--316",

journal = "Physics Letters B",

issn = "0370-2693",

number = "4-5",

}

Górska, M, Cáceres, L, Grawe, H, Pfützner, M, Jungclaus, A, Pietri, S, Werner-Malento, E, Podolyák, Z, Regan, PH, Rudolph, D, Detistov, P, Lalkovski, S, Modamio, V, Walker, J, Beck, T, Bednarczyk, P, Doornenbal, P, Geissel, H, Gerl, J, Grëbosz, J, Hoischen, R, Kojouharov, I, Kurz, N, Prokopowicz, W, Schaffner, H, Weick, H, Wollersheim, HJ, Andgren, K, Benlliure, J, Benzoni, G, Bruce, A, Casarejos, E, Cederwall, B, Crespi, FCL, Hadinia, B, Hellström, M, Ilie, G, Khaplanov, A, Kmiecik, M, Kumar, R, Maj, A, Mandal, S, Montes, F, Myalski, S, Simpson, GS, Steer, SJ, Tashenov, S, Wieland, O, Dombrádi, Z & Reiter, P 2009, 'Evolution of the N=82 shell gap below ¹³²Sn inferred from core excited states in ¹³¹In', Physics Letters B, vol. 672, no. 4-5, pp. 313-316. https://doi.org/10.1016/j.physletb.2009.01.027

TY - JOUR

T1 - Evolution of the N=82 shell gap below 132Sn inferred from core excited states in 131In

AU - Górska, M.

AU - Cáceres, L.

AU - Grawe, H.

AU - Pfützner, M.

AU - Jungclaus, A.

AU - Pietri, S.

AU - Werner-Malento, E.

AU - Podolyák, Z.

AU - Regan, P.H.

AU - Rudolph, D.

AU - Detistov, P.

AU - Lalkovski, S.

AU - Modamio, V.

AU - Walker, J.

AU - Beck, T.

AU - Bednarczyk, P.

AU - Doornenbal, P.

AU - Geissel, H.

AU - Gerl, J.

AU - Grëbosz, J.

AU - Hoischen, R.

AU - Kojouharov, I.

AU - Kurz, N.

AU - Prokopowicz, W.

AU - Schaffner, H.

AU - Weick, H.

AU - Wollersheim, H.J.

AU - Andgren, K.

AU - Benlliure, J.

AU - Benzoni, G.

AU - Bruce, Alison

AU - Casarejos, E.

AU - Cederwall, B.

AU - Crespi, F.C.L.

AU - Hadinia, B.

AU - Hellström, M.

AU - Ilie, G.

AU - Khaplanov, A.

AU - Kmiecik, M.

AU - Kumar, R.

AU - Maj, A.

AU - Mandal, S.

AU - Montes, F.

AU - Myalski, S.

AU - Simpson, G.S.

AU - Steer, S.J.

AU - Tashenov, S.

AU - Wieland, O.

AU - Dombrádi, Zs.

AU - Reiter, P.

PY - 2009/3

Y1 - 2009/3

N2 - The γ-ray decay of an excited state in 131In, the one proton hole neighbor of the doubly magic 132Sn has been measured. A high-spin, core-excited isomer with T1/2=630(60) ns was identified following production by both relativistic fragmentation of a 136Xe beam and fission of a 238U beam. This state deexcites by a single γ-ray branch of 3782(2) keV from which direct evidence for the size of the N=82 shell gap 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.

AB - The γ-ray decay of an excited state in 131In, the one proton hole neighbor of the doubly magic 132Sn has been measured. A high-spin, core-excited isomer with T1/2=630(60) ns was identified following production by both relativistic fragmentation of a 136Xe beam and fission of a 238U beam. This state deexcites by a single γ-ray branch of 3782(2) keV from which direct evidence for the size of the N=82 shell gap 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.

U2 - 10.1016/j.physletb.2009.01.027

DO - 10.1016/j.physletb.2009.01.027

M3 - Article

SN - 0370-2693

VL - 672

SP - 313

EP - 316

JO - Physics Letters B

JF - Physics Letters B

IS - 4-5

ER -

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

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