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. Gorska; S. Pietri; Dirk Rudolph; C. Domingo-Pardo; S. J. Steer; A. Atac; L. Bettermann; L. Caceres; K. Eppinger; T. Engert; T. Faestermann; F. Farinon; F. Finke; K. Geibel; J. Gerl; R. Gernhaeuser; N. Goel; A. Gottardo; J. Grebosz; C. Hinke; Robert Hoischen; G. Ilie; H. Iwasaki; J. Jolie; A. Kaskas; I. Kojouharov; R. Kruecken; N. Kurz; E. Merchan; C. Nociforo; J. Nyberg; M. Pfuetzner; A. Prochazka; Zs. Podolyak; P. H. Regan; P. Reiter; S. Rinta-Antila; C. Scholl; H. Schaffner; P. -A. Soderstrom; 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. Gorska, S. Pietri, Dirk Rudolph, C. Domingo-Pardo, S. J. Steer, A. Atac, L. Bettermann, L. Caceres, K. Eppinger, T. Engert, T. Faestermann, F. FarinonF. Finke, K. Geibel, J. Gerl, R. Gernhaeuser, N. Goel, A. Gottardo, J. Grebosz, C. Hinke, Robert Hoischen, G. Ilie, H. Iwasaki, J. Jolie, A. Kaskas, I. Kojouharov, R. Kruecken, N. Kurz, E. Merchan, C. Nociforo, J. Nyberg, M. Pfuetzner, A. Prochazka, Zs. Podolyak, P. H. Regan, P. Reiter, S. Rinta-Antila, C. Scholl, H. Schaffner, P. -A. Soderstrom, N. Warr, H. Weick, H. -J. Wollersheim, P. J. Woods, F. Nowacki, K. Sieja

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A beta-decaying high-spin isomer in Cd-96, 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 Xe-124 on a Be-9 target. From the half-life and the observed gamma decays in the daughter nucleus, Ag-96, we conclude that the beta-decaying state is the long predicted 16(+) "spin-gap'' isomer. Shell-model calculations, using the Gross-Frenkel interaction and the pi nu(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, Bd(GT) distributions have been studied via large-scale shell-model calculations using the pi nu(g, d, s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.

Originalspråk	engelska
Artikelnummer	172502
Tidskrift	Physical Review Letters
Volym	107
Nummer	17
DOI	https://doi.org/10.1103/PhysRevLett.107.172502
Status	Published - 2011

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Singh, B. S. N., Liu, Z., Wadsworth, R., Grawe, H., Brock, T. S., Boutachkov, P., Braun, N., Blazhev, A., Gorska, M., Pietri, S., Rudolph, D., Domingo-Pardo, C., Steer, S. J., Atac, A., Bettermann, L., Caceres, 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{dfa6faa8657d40689a010ac2bd7bf36c,

title = "16+ Spin-Gap Isomer in 96Cd",

abstract = "A beta-decaying high-spin isomer in Cd-96, 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 Xe-124 on a Be-9 target. From the half-life and the observed gamma decays in the daughter nucleus, Ag-96, we conclude that the beta-decaying state is the long predicted 16(+) {"}spin-gap'' isomer. Shell-model calculations, using the Gross-Frenkel interaction and the pi nu(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, Bd(GT) distributions have been studied via large-scale shell-model calculations using the pi nu(g, d, s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.",

author = "Singh, {B. S. Nara} and Z. Liu and R. Wadsworth and H. Grawe and Brock, {T. S.} and P. Boutachkov and N. Braun and A. Blazhev and M. Gorska and S. Pietri and Dirk Rudolph and C. Domingo-Pardo and Steer, {S. J.} and A. Atac and L. Bettermann and L. Caceres and K. Eppinger and T. Engert and T. Faestermann and F. Farinon and F. Finke and K. Geibel and J. Gerl and R. Gernhaeuser and N. Goel and A. Gottardo and J. Grebosz and C. Hinke and Robert Hoischen and G. Ilie and H. Iwasaki and J. Jolie and A. Kaskas and I. Kojouharov and R. Kruecken and N. Kurz and E. Merchan and C. Nociforo and J. Nyberg and M. Pfuetzner and A. Prochazka and Zs. Podolyak and Regan, {P. H.} and P. Reiter and S. Rinta-Antila and C. Scholl and H. Schaffner and Soderstrom, {P. -A.} and N. Warr and H. Weick and Wollersheim, {H. -J.} and Woods, {P. J.} and F. Nowacki and K. Sieja",

year = "2011",

doi = "10.1103/PhysRevLett.107.172502",

language = "English",

volume = "107",

journal = "Physical Review Letters",

issn = "1079-7114",

publisher = "American Physical Society",

number = "17",

}

Singh, BSN, Liu, Z, Wadsworth, R, Grawe, H, Brock, TS, Boutachkov, P, Braun, N, Blazhev, A, Gorska, M, Pietri, S, Rudolph, D, Domingo-Pardo, C, Steer, SJ, Atac, A, Bettermann, L, Caceres, L, Eppinger, K, Engert, T, Faestermann, T, Farinon, F, Finke, F, Geibel, K, Gerl, J, Gernhaeuser, R, Goel, N, Gottardo, A, Grebosz, J, Hinke, C, Hoischen, R, Ilie, G, Iwasaki, H, Jolie, J, Kaskas, A, Kojouharov, I, Kruecken, R, Kurz, N, Merchan, E, Nociforo, C, Nyberg, J, Pfuetzner, M, Prochazka, A, Podolyak, Z, Regan, PH, Reiter, P, Rinta-Antila, S, Scholl, C, Schaffner, H, Soderstrom, P-A, Warr, N, Weick, H, Wollersheim, H-J, Woods, PJ, Nowacki, F & Sieja, K 2011, '16+ Spin-Gap Isomer in 96Cd', Physical Review Letters, vol. 107, nr. 17, 172502. https://doi.org/10.1103/PhysRevLett.107.172502

TY - JOUR

T1 - 16+ Spin-Gap Isomer in 96Cd

AU - Singh, B. S. Nara

AU - Liu, Z.

AU - Wadsworth, R.

AU - Grawe, H.

AU - Brock, T. S.

AU - Boutachkov, P.

AU - Braun, N.

AU - Blazhev, A.

AU - Gorska, M.

AU - Pietri, S.

AU - Rudolph, Dirk

AU - Domingo-Pardo, C.

AU - Steer, S. J.

AU - Atac, A.

AU - Bettermann, L.

AU - Caceres, L.

AU - Eppinger, K.

AU - Engert, T.

AU - Faestermann, T.

AU - Farinon, F.

AU - Finke, F.

AU - Geibel, K.

AU - Gerl, J.

AU - Gernhaeuser, R.

AU - Goel, N.

AU - Gottardo, A.

AU - Grebosz, J.

AU - Hinke, C.

AU - Hoischen, Robert

AU - Ilie, G.

AU - Iwasaki, H.

AU - Jolie, J.

AU - Kaskas, A.

AU - Kojouharov, I.

AU - Kruecken, R.

AU - Kurz, N.

AU - Merchan, E.

AU - Nociforo, C.

AU - Nyberg, J.

AU - Pfuetzner, M.

AU - Prochazka, A.

AU - Podolyak, Zs.

AU - Regan, P. H.

AU - Reiter, P.

AU - Rinta-Antila, S.

AU - Scholl, C.

AU - Schaffner, H.

AU - Soderstrom, P. -A.

AU - Warr, N.

AU - Weick, H.

AU - Wollersheim, H. -J.

AU - Woods, P. J.

AU - Nowacki, F.

AU - Sieja, K.

PY - 2011

Y1 - 2011

N2 - A beta-decaying high-spin isomer in Cd-96, 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 Xe-124 on a Be-9 target. From the half-life and the observed gamma decays in the daughter nucleus, Ag-96, we conclude that the beta-decaying state is the long predicted 16(+) "spin-gap'' isomer. Shell-model calculations, using the Gross-Frenkel interaction and the pi nu(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, Bd(GT) distributions have been studied via large-scale shell-model calculations using the pi nu(g, d, s) model space to compare with the experimental B(GT) value obtained from the half-life of the isomer.

AB - A beta-decaying high-spin isomer in Cd-96, 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 Xe-124 on a Be-9 target. From the half-life and the observed gamma decays in the daughter nucleus, Ag-96, we conclude that the beta-decaying state is the long predicted 16(+) "spin-gap'' isomer. Shell-model calculations, using the Gross-Frenkel interaction and the pi nu(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, Bd(GT) distributions have been studied via large-scale shell-model calculations using the pi nu(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 - Letter

C2 - 22107511

SN - 1079-7114

VL - 107

JO - Physical Review Letters

JF - Physical Review Letters

IS - 17

M1 - 172502

ER -

16+ Spin-Gap Isomer in 96Cd

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