Literature DB >> 24745408

1p3/2 proton-hole state in 132Sn and the shell structure along N = 82.

J Taprogge1, A Jungclaus2, H Grawe3, S Nishimura4, P Doornenbal4, G Lorusso4, G S Simpson5, P-A Söderström4, T Sumikama6, Z Y Xu7, H Baba4, F Browne8, N Fukuda4, R Gernhäuser9, G Gey10, N Inabe4, T Isobe4, H S Jung11, D Kameda4, G D Kim12, Y-K Kim13, I Kojouharov3, T Kubo4, N Kurz3, Y K Kwon12, Z Li14, H Sakurai15, H Schaffner3, K Steiger9, H Suzuki4, H Takeda4, Zs Vajta16, H Watanabe4, J Wu17, A Yagi18, K Yoshinaga19, G Benzoni20, S Bönig21, K Y Chae22, L Coraggio23, A Covello24, J-M Daugas25, F Drouet5, A Gadea26, A Gargano23, S Ilieva21, F G Kondev27, T Kröll21, G J Lane28, A Montaner-Pizá26, K Moschner29, D Mücher9, F Naqvi30, M Niikura7, H Nishibata18, A Odahara18, R Orlandi31, Z Patel32, Zs Podolyák32, A Wendt29.   

Abstract

A low-lying state in 131In82, the one-proton hole nucleus with respect to double magic 132Sn, was observed by its γ decay to the Iπ=1/2- β-emitting isomer. We identify the new state at an excitation energy of Ex=1353  keV, which was populated both in the β decay of 131Cd83 and after β-delayed neutron emission from 132Cd84, as the previously unknown πp3/2 single-hole state with respect to the 132Sn core. Exploiting this crucial new experimental information, shell-model calculations were performed to study the structure of experimentally inaccessible N=82 isotones below 132Sn. The results evidence a surprising absence of proton subshell closures along the chain of N=82 isotones. The consequences of this finding for the evolution of the N=82 shell gap along the r-process path are discussed.

Entities:  

Year:  2014        PMID: 24745408     DOI: 10.1103/PhysRevLett.112.132501

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  1 in total

1.  Nuclear moments of indium isotopes reveal abrupt change at magic number 82.

Authors:  A R Vernon; R F Garcia Ruiz; T Miyagi; C L Binnersley; J Billowes; M L Bissell; J Bonnard; T E Cocolios; J Dobaczewski; G J Farooq-Smith; K T Flanagan; G Georgiev; W Gins; R P de Groote; R Heinke; J D Holt; J Hustings; Á Koszorús; D Leimbach; K M Lynch; G Neyens; S R Stroberg; S G Wilkins; X F Yang; D T Yordanov
Journal:  Nature       Date:  2022-07-13       Impact factor: 69.504

  1 in total

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