検索対象:     
報告書番号:
※ 半角英数字
 年 ~ 
 年

Are there signatures of harmonic oscillator shells far from stability?; First spectroscopy of $$^{110}$$Zr

不安定原子核領域における調和振動子型の殻構造の存在について; $$^{110}$$Zrの最初の核分光

Paul, N.*; Corsi, A.*; Obertelli, A.*; Doornenbal, P.*; Authelet, G.*; Baba, H.*; Bally, B.*; Bender, M.*; Calvet, D.*; Ch$^a$teau, F.*; Chen, S.*; Delaroche, J.-P.*; Delbart, A.*; Gheller, J.-M.*; Giganon, A.*; Gillibert, A.*; Girod, M.*; Heenen, P.-H.*; Lapoux, V.*; Libert, J.*; 本林 透*; 新倉 潤*; Otsuka, T.*; Rodr$'i$guez, T. R.*; Rouss$'e$, J.-Y.*; 櫻井 博儀*; Santamaria, C.*; 清水 則孝*; Steppenbeck, D.*; Taniuchi, R.*; 富樫 智章*; 角田 佑介*; Uesaka, T.*; Ando, T.*; Arici, T.*; Blazhev, A.*; Browne, F.*; Bruce, A.*; Carroll, R.*; Chung, L. X.*; Cort$'e$s, M. L.*; Dewald, M.*; Ding, B.*; Flavigny, F.*; Franchoo, S.*; G$'o$rska, M.*; Gottardo, A.*; Jungclaus, A.*; Lee, J.*; Lettmann, M.*; Linh, B. D.*; Liu, J.*; Liu, Z.*; Lizarazo, C.*; Momiyama, S.*; Moschner, K.*; Nagamine, S.*; Nakatsuka, N.*; Nita, C.*; Nobs, C.*; Olivier, L.*; Patel, Z.*; Podoly$'a$k, Zs.*; Rudigier, M.*; Saito, T.*; Shand, C.*; S$"o$derstr$"o$m, P. A.*; Stefan, I.*; Orlandi, R.; Vaquero, V.*; Werner, V.*; Wimmer, K.*; Xu, Z.*

Paul, N.*; Corsi, A.*; Obertelli, A.*; Doornenbal, P.*; Authelet, G.*; Baba, H.*; Bally, B.*; Bender, M.*; Calvet, D.*; Ch$^a$teau, F.*; Chen, S.*; Delaroche, J.-P.*; Delbart, A.*; Gheller, J.-M.*; Giganon, A.*; Gillibert, A.*; Girod, M.*; Heenen, P.-H.*; Lapoux, V.*; Libert, J.*; Motobayashi, Toru*; Niikura, Megumi*; Otsuka, T.*; Rodr$'i$guez, T. R.*; Rouss$'e$, J.-Y.*; Sakurai, Hiroyoshi*; Santamaria, C.*; Shimizu, Noritaka*; Steppenbeck, D.*; Taniuchi, R.*; Togashi, Tomoaki*; Tsunoda, Yusuke*; Uesaka, T.*; Ando, T.*; Arici, T.*; Blazhev, A.*; Browne, F.*; Bruce, A.*; Carroll, R.*; Chung, L. X.*; Cort$'e$s, M. L.*; Dewald, M.*; Ding, B.*; Flavigny, F.*; Franchoo, S.*; G$'o$rska, M.*; Gottardo, A.*; Jungclaus, A.*; Lee, J.*; Lettmann, M.*; Linh, B. D.*; Liu, J.*; Liu, Z.*; Lizarazo, C.*; Momiyama, S.*; Moschner, K.*; Nagamine, S.*; Nakatsuka, N.*; Nita, C.*; Nobs, C.*; Olivier, L.*; Patel, Z.*; Podoly$'a$k, Zs.*; Rudigier, M.*; Saito, T.*; Shand, C.*; S$"o$derstr$"o$m, P. A.*; Stefan, I.*; Orlandi, R.; Vaquero, V.*; Werner, V.*; Wimmer, K.*; Xu, Z.*

The first measurement of $$gamma$$ rays emitted by the very neutron rich nuclei $$^{112}$$Mo (Z=42) and $$^{110}$$Zr (Z=40) was carried out at the RIBF facility at RIKEN. These data shine light on the postulated N=70 harmonic oscillator shell. If the spin-orbit splitting which gives rise to the N=82 shell gap is reduced in very neutron-rich nuclei, the harmonic oscillator gap at N=70 should open instead. However, both the measured energy of the first excited state $$^{112}$$Mo and $$^{110}$$Zr, respectively 235(7) keV and 185(11) keV, and their E(4$$^+$$)/E(2$$^+$$) ratio, indicate that these nuclei are good rotors, and exclude the shell stabilization scenario at Z=40 and N=70. These results were compared to state-of-the-art density functional theoretical calculations using Gogny and Skyrme effective interactions.

Access

:

- Accesses

InCites™

:

パーセンタイル:9.07

分野:Physics, Multidisciplinary

Altmetrics

:

[CLARIVATE ANALYTICS], [WEB OF SCIENCE], [HIGHLY CITED PAPER & CUP LOGO] and [HOT PAPER & FIRE LOGO] are trademarks of Clarivate Analytics, and/or its affiliated company or companies, and used herein by permission and/or license.