Author
Listed:
- R. Taniuchi
(The University of Tokyo
RIKEN Nishina Center)
- C. Santamaria
(RIKEN Nishina Center
IRFU, CEA, Université Paris-Saclay)
- P. Doornenbal
(RIKEN Nishina Center)
- A. Obertelli
(RIKEN Nishina Center
IRFU, CEA, Université Paris-Saclay
Institut für Kernphysik, Technische Universität Darmstadt)
- K. Yoneda
(RIKEN Nishina Center)
- G. Authelet
(IRFU, CEA, Université Paris-Saclay)
- H. Baba
(RIKEN Nishina Center)
- D. Calvet
(IRFU, CEA, Université Paris-Saclay)
- F. Château
(IRFU, CEA, Université Paris-Saclay)
- A. Corsi
(IRFU, CEA, Université Paris-Saclay)
- A. Delbart
(IRFU, CEA, Université Paris-Saclay)
- J.-M. Gheller
(IRFU, CEA, Université Paris-Saclay)
- A. Gillibert
(IRFU, CEA, Université Paris-Saclay)
- J. D. Holt
(TRIUMF)
- T. Isobe
(RIKEN Nishina Center)
- V. Lapoux
(IRFU, CEA, Université Paris-Saclay)
- M. Matsushita
(The University of Tokyo)
- J. Menéndez
(The University of Tokyo)
- S. Momiyama
(The University of Tokyo
RIKEN Nishina Center)
- T. Motobayashi
(RIKEN Nishina Center)
- M. Niikura
(The University of Tokyo)
- F. Nowacki
(IPHC, CNRS/IN2P3, Université de Strasbourg)
- K. Ogata
(Osaka University
Osaka City University)
- H. Otsu
(RIKEN Nishina Center)
- T. Otsuka
(The University of Tokyo
RIKEN Nishina Center
The University of Tokyo)
- C. Péron
(IRFU, CEA, Université Paris-Saclay)
- S. Péru
(CEA, DAM, DIF)
- A. Peyaud
(IRFU, CEA, Université Paris-Saclay)
- E. C. Pollacco
(IRFU, CEA, Université Paris-Saclay)
- A. Poves
(Universidad Autónoma de Madrid)
- J.-Y. Roussé
(IRFU, CEA, Université Paris-Saclay)
- H. Sakurai
(The University of Tokyo
RIKEN Nishina Center)
- A. Schwenk
(Institut für Kernphysik, Technische Universität Darmstadt
ExtreMe Matter Institute (EMMI), GSI Helmholtzzentrum für Schwerionenforschung
Max-Planck-Institut für Kernphysik)
- Y. Shiga
(RIKEN Nishina Center
Rikkyo University)
- J. Simonis
(Institut für Kernphysik, Technische Universität Darmstadt
ExtreMe Matter Institute (EMMI), GSI Helmholtzzentrum für Schwerionenforschung
Johannes Gutenberg-Universität Mainz)
- S. R. Stroberg
(TRIUMF
Physics Department, Reed College)
- S. Takeuchi
(RIKEN Nishina Center)
- Y. Tsunoda
(The University of Tokyo)
- T. Uesaka
(RIKEN Nishina Center)
- H. Wang
(RIKEN Nishina Center)
- F. Browne
(University of Brighton)
- L. X. Chung
(Institute for Nuclear Science & Technology, VINATOM)
- Z. Dombradi
(MTA Atomki)
- S. Franchoo
(Université Paris-Saclay)
- F. Giacoppo
(University of Oslo)
- A. Gottardo
(Université Paris-Saclay)
- K. Hadyńska-Klęk
(University of Oslo)
- Z. Korkulu
(MTA Atomki)
- S. Koyama
(The University of Tokyo
RIKEN Nishina Center)
- Y. Kubota
(RIKEN Nishina Center
The University of Tokyo)
- J. Lee
(The University of Hong Kong)
- M. Lettmann
(Institut für Kernphysik, Technische Universität Darmstadt)
- C. Louchart
(Institut für Kernphysik, Technische Universität Darmstadt)
- R. Lozeva
(IPHC, CNRS/IN2P3, Université de Strasbourg
CSNSM, CNRS/IN2P3, Université Paris-Saclay)
- K. Matsui
(The University of Tokyo
RIKEN Nishina Center)
- T. Miyazaki
(The University of Tokyo
RIKEN Nishina Center)
- S. Nishimura
(RIKEN Nishina Center)
- L. Olivier
(Université Paris-Saclay)
- S. Ota
(The University of Tokyo)
- Z. Patel
(University of Surrey)
- E. Şahin
(University of Oslo)
- C. Shand
(University of Surrey)
- P.-A. Söderström
(RIKEN Nishina Center)
- I. Stefan
(Université Paris-Saclay)
- D. Steppenbeck
(The University of Tokyo)
- T. Sumikama
(Tohoku University)
- D. Suzuki
(Université Paris-Saclay)
- Z. Vajta
(MTA Atomki)
- V. Werner
(Institut für Kernphysik, Technische Universität Darmstadt)
- J. Wu
(RIKEN Nishina Center
Peking University)
- Z. Y. Xu
(The University of Hong Kong)
Abstract
Nuclear magic numbers correspond to fully occupied energy shells of protons or neutrons inside atomic nuclei. Doubly magic nuclei, with magic numbers for both protons and neutrons, are spherical and extremely rare across the nuclear landscape. Although the sequence of magic numbers is well established for stable nuclei, experimental evidence has revealed modifications for nuclei with a large asymmetry between proton and neutron numbers. Here we provide a spectroscopic study of the doubly magic nucleus 78Ni, which contains fourteen neutrons more than the heaviest stable nickel isotope. We provide direct evidence of its doubly magic nature, which is also predicted by ab initio calculations based on chiral effective-field theory interactions and the quasi-particle random-phase approximation. Our results also indicate the breakdown of the neutron magic number 50 and proton magic number 28 beyond this stronghold, caused by a competing deformed structure. State-of-the-art phenomenological shell-model calculations reproduce this shape coexistence, predicting a rapid transition from spherical to deformed ground states, with 78Ni as the turning point.
Suggested Citation
R. Taniuchi & C. Santamaria & P. Doornenbal & A. Obertelli & K. Yoneda & G. Authelet & H. Baba & D. Calvet & F. Château & A. Corsi & A. Delbart & J.-M. Gheller & A. Gillibert & J. D. Holt & T. Isobe &, 2019.
"78Ni revealed as a doubly magic stronghold against nuclear deformation,"
Nature, Nature, vol. 569(7754), pages 53-58, May.
Handle:
RePEc:nat:nature:v:569:y:2019:i:7754:d:10.1038_s41586-019-1155-x
DOI: 10.1038/s41586-019-1155-x
Download full text from publisher
As the access to this document is restricted, you may want to search for a different version of it.
Corrections
All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:nat:nature:v:569:y:2019:i:7754:d:10.1038_s41586-019-1155-x. See general information about how to correct material in RePEc.
If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.
We have no bibliographic references for this item. You can help adding them by using this form .
If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.
For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: Sonal Shukla or Springer Nature Abstracting and Indexing (email available below). General contact details of provider: http://www.nature.com .
Please note that corrections may take a couple of weeks to filter through
the various RePEc services.