Author
Listed:
- J. Ha
(Institute for Basic Science, Center for Exotic Nuclear Studies
Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova
KU Leuven, Instituut voor Kern- en Stralingsfysica)
- F. Recchia
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova)
- S. M. Lenzi
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova)
- H. Iwasaki
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- D. D. Dao
(CNRS, IPHC UMR7178, Université de Strasbourg)
- F. Nowacki
(CNRS, IPHC UMR7178, Université de Strasbourg)
- A. Revel
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- P. Aguilera
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova)
- G. de Angelis
(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro)
- J. Ash
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- D. Bazin
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- M. A. Bentley
(University of York, School of Physics, Engineering and Technology)
- S. Biswas
(Michigan State University, Facility for Rare Isotope Beams)
- S. Carollo
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova)
- M. L. Cortes
(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro)
- R. Elder
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- R. Escudeiro
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova
Universidade de São Paulo, Instituto de Fisica)
- P. Farris
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- A. Gade
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- T. Ginter
(Michigan State University, Facility for Rare Isotope Beams)
- M. Grinder
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- J. Li
(Michigan State University, Facility for Rare Isotope Beams)
- D. R. Napoli
(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro)
- S. Noji
(Michigan State University, Facility for Rare Isotope Beams)
- J. Pereira
(Michigan State University, Facility for Rare Isotope Beams)
- S. Pigliapoco
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova)
- A. Pompermaier
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia)
- A. Poves
(Universidad Autónoma de Madrid, Departamento de Física Teórica and IFT UAM-CSIC)
- K. Rezynkina
(Università Degli Studi di Padova, Dipartimento di Fisica e Astronomia
Istituto Nazionale di Fisica Nucleare, Sezione di Padova)
- A. Sanchez
(Michigan State University, Facility for Rare Isotope Beams
Michigan State University, Department of Physics and Astronomy)
- R. Wadsworth
(University of York, School of Physics, Engineering and Technology)
- D. Weisshaar
(Michigan State University, Facility for Rare Isotope Beams)
Abstract
Like electrons in atoms, protons and neutrons in nuclei occupy orbitals in a shell structure with energy gaps at magic numbers. Radioactive-beam experiments revealed the disappearance of magic numbers in some neutron-rich isotopes. In these nuclei, configurations involving particles excited across the shell gap gain correlation energy, becoming the ground state. Neutron-rich regions of the nuclear chart that exhibit this property are known as “Islands of Inversion”. Here we present the lifetime measurement of the first 2+ states in 84Mo (N = Z) and 86Mo (N = Z + 2) revealing an unexpected sharp structural change between them defining the edge of the region of deformation around 80Zr. Similarly to the neutron-rich N = 40 Island of Inversion near 64Cr where cross-shell excitations dominate, we identify this region as an Island of Inversion with symmetrical proton and neutron excitations that we term “Isospin-Symmetric Island of Inversion”. Three-nucleon forces are suggested to drive Mo isotope structural changes.
Suggested Citation
J. Ha & F. Recchia & S. M. Lenzi & H. Iwasaki & D. D. Dao & F. Nowacki & A. Revel & P. Aguilera & G. de Angelis & J. Ash & D. Bazin & M. A. Bentley & S. Biswas & S. Carollo & M. L. Cortes & R. Elder &, 2025.
"Abrupt structural transition in exotic molybdenum isotopes unveils an isospin-symmetric island of inversion,"
Nature Communications, Nature, vol. 16(1), pages 1-8, December.
Handle:
RePEc:nat:natcom:v:16:y:2025:i:1:d:10.1038_s41467-025-65621-2
DOI: 10.1038/s41467-025-65621-2
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