16+ spin-gap isomer in 96Cd

B.S. Nara Singh; Z. Liu; R. Wadsworth; H. Grawe; T. S. Brock; P. Boutachkov; N. Braun; A. Blazhev; M. Górska; S. Pietri; D. Rudolph; C. Domingo-Pardo; S. J. Steer; A. Ataç; L. Bettermann; L. Cáceres; K. Eppinger; T. Engert; T. Faestermann; F. Farinon; F. Finke; K. Geibel; J. Gerl; R. Gernhäuser; N. Goel; A. Gottardo; J. Grębosz; C. Hinke; R. Hoischen; G. Ilie; H. Iwasaki; J. Jolie; A. Kaşkaş; I. Kojouharov; R. Krücken; N. Kurz; E. Merchán; C. Nociforo; J. Nyberg; M. Pfützner; A. Prochazka; Zs. Podolyák; P. H. Regan; P. Reiter; S. Rinta-Antila; C. Scholl; H. Schaffner; P-A. Söderström; N. Warr; H. Weick; H. J. Wollersheim; P.J. Woods; F. Nowacki; K. Sieja

doi:10.1103/PhysRevLett.107.172502

16+ spin-gap isomer in 96Cd

B.S. Nara Singh, Z. Liu, R. Wadsworth, H. Grawe, T. S. Brock, P. Boutachkov, N. Braun, A. Blazhev, M. Górska, S. Pietri, D. Rudolph, C. Domingo-Pardo, S. J. Steer, A. Ataç, L. Bettermann, L. Cáceres, K. Eppinger, T. Engert, T. Faestermann, F. FarinonF. Finke, K. Geibel, J. Gerl, R. Gernhäuser, N. Goel, A. Gottardo, J. Grębosz, C. Hinke, R. Hoischen, G. Ilie, H. Iwasaki, J. Jolie, A. Kaşkaş, I. Kojouharov, R. Krücken, N. Kurz, E. Merchán, C. Nociforo, J. Nyberg, M. Pfützner, A. Prochazka, Zs. Podolyák, P. H. Regan, P. Reiter, S. Rinta-Antila, C. Scholl, H. Schaffner, P-A. Söderström, N. Warr, H. Weick, H. J. Wollersheim, P.J. Woods, F. Nowacki, K. Sieja

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Abstract

A β-decaying high-spin isomer in (96)Cd, with a half-life T(1/2)=0.29(-0.10)(+0.11) s, has been established in a stopped beam rare isotope spectroscopic investigations at GSI (RISING) experiment. The nuclei were produced using the fragmentation of a primary beam of (124)Xe on a (9)Be target. From the half-life and the observed γ decays in the daughter nucleus, (96)Ag, we conclude that the β-decaying state is the long predicted 16(+) "spin-gap" isomer. Shell-model calculations, using the Gross-Frenkel interaction and the πν(p(1/2),g(9/2)) model space, show that the isoscalar component of the neutron-proton interaction is essential to explain the origin of the isomer. Core excitations across the N=Z=50 gaps and the Gamow-Teller strength, B(GT) distributions have been studied via large-scale shell-model calculations using the πν(g,d,s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.

Original language	English
Article number	172502
Journal	Physical Review Letters
Volume	107
Issue number	17
DOIs	https://doi.org/10.1103/PhysRevLett.107.172502
Publication status	Published - 21 Oct 2011
Externally published	Yes

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Nara Singh, B. S., Liu, Z., Wadsworth, R., Grawe, H., Brock, T. S., Boutachkov, P., Braun, N., Blazhev, A., Górska, M., Pietri, S., Rudolph, D., Domingo-Pardo, C., Steer, S. J., Ataç, A., Bettermann, L., Cáceres, L., Eppinger, K., Engert, T., Faestermann, T., ... Sieja, K. (2011). 16+ spin-gap isomer in 96Cd. Physical Review Letters, 107(17), [172502]. https://doi.org/10.1103/PhysRevLett.107.172502

@article{4180b90ab91c478aa1a772cd37dcd20a,

title = "16+ spin-gap isomer in 96Cd",

abstract = "A β-decaying high-spin isomer in (96)Cd, with a half-life T(1/2)=0.29(-0.10)(+0.11) s, has been established in a stopped beam rare isotope spectroscopic investigations at GSI (RISING) experiment. The nuclei were produced using the fragmentation of a primary beam of (124)Xe on a (9)Be target. From the half-life and the observed γ decays in the daughter nucleus, (96)Ag, we conclude that the β-decaying state is the long predicted 16(+) {"}spin-gap{"} isomer. Shell-model calculations, using the Gross-Frenkel interaction and the πν(p(1/2),g(9/2)) model space, show that the isoscalar component of the neutron-proton interaction is essential to explain the origin of the isomer. Core excitations across the N=Z=50 gaps and the Gamow-Teller strength, B(GT) distributions have been studied via large-scale shell-model calculations using the πν(g,d,s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.",

author = "{Nara Singh}, B.S. and Z. Liu and R. Wadsworth and H. Grawe and Brock, {T. S.} and P. Boutachkov and N. Braun and A. Blazhev and M. G{\'o}rska and S. Pietri and D. Rudolph and C. Domingo-Pardo and Steer, {S. J.} and A. Ata{\c c} and L. Bettermann and L. C{\'a}ceres and K. Eppinger and T. Engert and T. Faestermann and F. Farinon and F. Finke and K. Geibel and J. Gerl and R. Gernh{\"a}user and N. Goel and A. Gottardo and J. Gr{\c e}bosz and C. Hinke and R. Hoischen and G. Ilie and H. Iwasaki and J. Jolie and A. Ka{\c s}ka{\c s} and I. Kojouharov and R. Kr{\"u}cken and N. Kurz and E. Merch{\'a}n and C. Nociforo and J. Nyberg and M. Pf{\"u}tzner and A. Prochazka and Zs. Podoly{\'a}k and Regan, {P. H.} and P. Reiter and S. Rinta-Antila and C. Scholl and H. Schaffner and P-A. S{\"o}derstr{\"o}m and N. Warr and H. Weick and Wollersheim, {H. J.} and P.J. Woods and F. Nowacki and K. Sieja",

note = "{\textcopyright} 2011 American Physical Society",

year = "2011",

month = oct,

day = "21",

doi = "10.1103/PhysRevLett.107.172502",

language = "English",

volume = "107",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "17",

}

Nara Singh, BS, Liu, Z, Wadsworth, R, Grawe, H, Brock, TS, Boutachkov, P, Braun, N, Blazhev, A, Górska, M, Pietri, S, Rudolph, D, Domingo-Pardo, C, Steer, SJ, Ataç, A, Bettermann, L, Cáceres, L, Eppinger, K, Engert, T, Faestermann, T, Farinon, F, Finke, F, Geibel, K, Gerl, J, Gernhäuser, R, Goel, N, Gottardo, A, Grębosz, J, Hinke, C, Hoischen, R, Ilie, G, Iwasaki, H, Jolie, J, Kaşkaş, A, Kojouharov, I, Krücken, R, Kurz, N, Merchán, E, Nociforo, C, Nyberg, J, Pfützner, M, Prochazka, A, Podolyák, Z, Regan, PH, Reiter, P, Rinta-Antila, S, Scholl, C, Schaffner, H, Söderström, P-A, Warr, N, Weick, H, Wollersheim, HJ, Woods, PJ, Nowacki, F & Sieja, K 2011, '16+ spin-gap isomer in 96Cd', Physical Review Letters, vol. 107, no. 17, 172502. https://doi.org/10.1103/PhysRevLett.107.172502

TY - JOUR

T1 - 16+ spin-gap isomer in 96Cd

AU - Nara Singh, B.S.

AU - Liu, Z.

AU - Wadsworth, R.

AU - Grawe, H.

AU - Brock, T. S.

AU - Boutachkov, P.

AU - Braun, N.

AU - Blazhev, A.

AU - Górska, M.

AU - Pietri, S.

AU - Rudolph, D.

AU - Domingo-Pardo, C.

AU - Steer, S. J.

AU - Ataç, A.

AU - Bettermann, L.

AU - Cáceres, L.

AU - Eppinger, K.

AU - Engert, T.

AU - Faestermann, T.

AU - Farinon, F.

AU - Finke, F.

AU - Geibel, K.

AU - Gerl, J.

AU - Gernhäuser, R.

AU - Goel, N.

AU - Gottardo, A.

AU - Grębosz, J.

AU - Hinke, C.

AU - Hoischen, R.

AU - Ilie, G.

AU - Iwasaki, H.

AU - Jolie, J.

AU - Kaşkaş, A.

AU - Kojouharov, I.

AU - Krücken, R.

AU - Kurz, N.

AU - Merchán, E.

AU - Nociforo, C.

AU - Nyberg, J.

AU - Pfützner, M.

AU - Prochazka, A.

AU - Podolyák, Zs.

AU - Regan, P. H.

AU - Reiter, P.

AU - Rinta-Antila, S.

AU - Scholl, C.

AU - Schaffner, H.

AU - Söderström, P-A.

AU - Warr, N.

AU - Weick, H.

AU - Wollersheim, H. J.

AU - Woods, P.J.

AU - Nowacki, F.

AU - Sieja, K.

PY - 2011/10/21

Y1 - 2011/10/21

N2 - A β-decaying high-spin isomer in (96)Cd, with a half-life T(1/2)=0.29(-0.10)(+0.11) s, has been established in a stopped beam rare isotope spectroscopic investigations at GSI (RISING) experiment. The nuclei were produced using the fragmentation of a primary beam of (124)Xe on a (9)Be target. From the half-life and the observed γ decays in the daughter nucleus, (96)Ag, we conclude that the β-decaying state is the long predicted 16(+) "spin-gap" isomer. Shell-model calculations, using the Gross-Frenkel interaction and the πν(p(1/2),g(9/2)) model space, show that the isoscalar component of the neutron-proton interaction is essential to explain the origin of the isomer. Core excitations across the N=Z=50 gaps and the Gamow-Teller strength, B(GT) distributions have been studied via large-scale shell-model calculations using the πν(g,d,s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.

AB - A β-decaying high-spin isomer in (96)Cd, with a half-life T(1/2)=0.29(-0.10)(+0.11) s, has been established in a stopped beam rare isotope spectroscopic investigations at GSI (RISING) experiment. The nuclei were produced using the fragmentation of a primary beam of (124)Xe on a (9)Be target. From the half-life and the observed γ decays in the daughter nucleus, (96)Ag, we conclude that the β-decaying state is the long predicted 16(+) "spin-gap" isomer. Shell-model calculations, using the Gross-Frenkel interaction and the πν(p(1/2),g(9/2)) model space, show that the isoscalar component of the neutron-proton interaction is essential to explain the origin of the isomer. Core excitations across the N=Z=50 gaps and the Gamow-Teller strength, B(GT) distributions have been studied via large-scale shell-model calculations using the πν(g,d,s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.

U2 - 10.1103/PhysRevLett.107.172502

DO - 10.1103/PhysRevLett.107.172502

M3 - Article

C2 - 22107511

SN - 0031-9007

VL - 107

JO - Physical Review Letters

JF - Physical Review Letters

IS - 17

M1 - 172502

ER -

16+ spin-gap isomer in 96Cd

Abstract

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