2–5 Feb 2026
INFN - Laboratori Nazionali di Legnaro
Europe/Rome timezone
Organized by INTRANS, the Instrumentation and Training task of EURO-LABS for Nuclear Spectroscopy and Reaction Dynamics

Study of shape coexistence in Sn isotopes around A=110

Not scheduled
15m
Oral Contribution Monday 2

Speaker

Giacomo Corbari (Università degli Studi di Milano and INFN)

Description

The shape coexistence phenomenon was investigated in the Sn isotopes region around A=110, by means of $\gamma$-ray spectroscopy and lifetime measurements of low-spin states. Recent observations of prolate axially deformed $0^+$ states in $^{64,66}$Ni isotopes, with a strongly hindered decay to the first $2^+$ excited state of spherical nature (shape-isomer-like excitations), were reported [1,2,3]. Similar excitations were suggested in the stable Sn isotopes, across the $Z=50$ shell gap, due to analogies in the orbital configuration. Such hypothesis is corroborated by Monte Carlo Shell Model (MCSM) calculations, performed with the interaction of Ref. [4], whose potential energy surfaces of $^{110-118}$Sn exhibit a well-separated prolate secondary minimum, as in the Ni case.\
Experimentally, several excited $0^+$ states have been observed in even-even $^{110-120}$Sn, mainly via particle spectroscopy (e.g. [5,6]), however limited information on their lifetimes is available. To address this issue, a series of complementary experiments was carried out by our collaboration between LNL and IFIN-HH, employing the ROSPHERE-SORCERER and the AGATA-PRISMA setup, respectively. In particular, even-even $^{110-120}$Sn isotopes were studied via low-energy multi-nucleon transfer reactions and several lifetimes of excited 0$^+_2$, 0$^+_3$ and 0$^+_4$ states were measured for the first time with the RDDS and the DSAM methods. Results will be compared with MCSM calculations, giving an insight into the microscopic mechanism leading to the onset of deformation in this region.\par
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\textbf{References}
%\newline [1] R.~Reference1 \textit{et al.}, Journal \textbf{volume} (year) pages.
\newline [1] N.~Marginean \textit{et al.}, Phys. Rev. Lett. \textbf{125}, (2020) 102502.
\newline [2] S.~Leoni \textit{et al.}, Phys. Rev. Lett. \textbf{118}, (2017) 162502.
\newline [3] S. Leoni \textit{et al.}, Prog. Part. Nucl. Phys. \textbf{139}, (2024) 104119.
%\newline [4] P.~Guazzoni \textit{et al.}, Phys. Rev. C \textbf{74}, (2006) 054605.
%\newline [5] H.~W.~Fielding \textit{et al.}, Nuc. Phys. \textbf{A382}, (1977) 389.
\newline [4] T.~Togashi \textit{et al.}, Phys. Rev. Lett. \textbf{121}, (2018) 062501.
\newline [5] P.~Guazzoni \textit{et al.}, Phys. Rev. C \textbf{85},(2012) 054609.
\newline [6] A.~Backlin \textit{et al.}, Nuc. Phys. \textbf{A351}, (1981) 490.

Author

Giacomo Corbari (Università degli Studi di Milano and INFN)

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