Yrast 6
seniority isomers of
Sn
Snにおけるイラスト
状態のセニョリティ核異性体
Simpson, G. S.*; Gey, G.*; Jungclaus, A.*; Taprogge, J.*; 西村 俊二*; Sieja, K.*; Doornenbal, P.*; Lorusso, G.*; S
derstr
m, P.-A.*; 炭竃 聡之*; Xu, Z. Y.*; 馬場 秀忠*; Browne, F.*; 福田 直樹*; 稲辺 尚人*; Isobe, T.*; Jung, H. S.*; 亀田 大輔*; Kim, G. D.*; Kim, Y.-K.*; Kojouharov, I.*; 久保 敏幸*; Kurz, N.*; Kwon, Y. K.*; Li, Z.*; 櫻井 博儀*; Schaffner, H.*; Shimizu, Y.*; Suzuki, H.*; Takeda, H.*; Vajta, Zs.*; Watanabe, H.*; Wu, J.*; Yagi, A.*; 吉永 健太*; B
nig, S.*; Daugas, J.-M.*; Drouet, F.*; Gernh
user, R.*; Ilieva, S.*; Kr
ll, T.*; Montaner-Piz
, A.*; Moschner, K.*; M
cher, D.*; Na
dja, H.*; 西畑 洸希*; Nowacki, F.*; 小田原 厚子*; Orlandi, R.
; Steiger, K.*; Wendt, A.*
Simpson, G. S.*; Gey, G.*; Jungclaus, A.*; Taprogge, J.*; Nishimura, Shunji*; Sieja, K.*; Doornenbal, P.*; Lorusso, G.*; S
derstr
m, P.-A.*; Sumikama, Toshiyuki*; Xu, Z. Y.*; Baba, Hidetada*; Browne, F.*; Fukuda, Naoki*; Inabe, Naoto*; Isobe, T.*; Jung, H. S.*; Kameda, Daisuke*; Kim, G. D.*; Kim, Y.-K.*; Kojouharov, I.*; Kubo, Toshiyuki*; Kurz, N.*; Kwon, Y. K.*; Li, Z.*; Sakurai, Hiroyoshi*; Schaffner, H.*; Shimizu, Y.*; Suzuki, H.*; Takeda, H.*; Vajta, Zs.*; Watanabe, H.*; Wu, J.*; Yagi, A.*; Yoshinaga, Kenta*; B
nig, S.*; Daugas, J.-M.*; Drouet, F.*; Gernh
user, R.*; Ilieva, S.*; Kr
ll, T.*; Montaner-Piz
, A.*; Moschner, K.*; M
cher, D.*; Na
dja, H.*; Nishibata, Hiroki*; Nowacki, F.*; Odahara, Atsuko*; Orlandi, R.; Steiger, K.*; Wendt, A.*
Delayed
-ray cascades, originating from the decay of 6
isomeric states, in the very neutron-rich, semimagic isotopes
Sn were observed following the projectile fission of a
U beam at RIBF, RIKEN. The wave functions of these isomeric states are proposed to be predominantly a fully aligned pair of f
neutrons. Shell-model calculations, performed using a realistic effective interaction, reproduce well the energies of the excited states of these nuclei and the measured transition rates, with the exception of the
2;6
) rate of
Sn, which deviates from a simple seniority scheme. Empirically reducing the 
orbit matrix elements produces a 4+1 state with almost equal seniority 2 and 4 components, correctly reproducing the experimental
2;6
) rate of
Sn. These data provide a key benchmark for shell-model interactions far from stability.