2–3 Oct 2023
INFN-LNL
Europe/Rome timezone

Searching for the second proton 0+ in the bubble nucleus 46Ar

3 Oct 2023, 09:30
20m
INFN-LNL

INFN-LNL

Viale dell'Università, 2, 35020 Legnaro PD

Speaker

Andrea Gottardo (Istituto Nazionale di Fisica Nucleare)

Description

Physics aim

A recent measurement at the Spiral1 facility at GANIL has revealed that the $^{46}$Ar nucleus is a bubble nucleus with a filled $\pi d_{3/2}$ shell and an empty $\pi s_{1/2}$ [1]. This finding also explain the small B(E2) value for $^{46}$Ar 2$^+$ state.
This important discovery is in agreement with ab-initio calculations with the NNLOsat parametrization of the chiral effective Hamiltonian, but in disagreement with shell-model calculations with the well-established SDPF-U interaction. This latter Hamiltonian predicts the $^{46}$Ar 0$^+$ ground state to be an even mixture of the $\pi d_{3/2}$ and $\pi s_{1/2}$ shells. This also somehow what would be suggested by an heuristic reasoning, considering that in $^{47}$K the $\pi d_{3/2}$ and $\pi s_{1/2}$ shells appear to be separated by only 360 keV.
A key point then arises: if the $^{46}$Ar 0$^+$ ground state has the $\pi d_{3/2}^{4} s_{1/2}^0$ proton configuration, at which energy is the second $0^+$ with the $\pi d_{3/2}^{2} s_{1/2}^2$ wave function ? And why it does not mix with the ground state ? A measurement of its excitation energy would provide crucial information to understand if the lack of mixing is coming from a large energy difference between the two $0^+$ levels or from the small diagonal pairing between them.

Proposed measurement
We propose to populate the $\pi d_{3/2}^{2} s_{1/2}^2$ excited $0^+$ state $^{46}$Ar using a $^{48}$Ca($^6$Li,$^8$B)$^{46}$Ar reaction at about 10 MeV/u. Gamma rays will be detected by the AGATA array, while the $^8$B ejectile by a DSSD detector like TRACE or OSCAR. The reaction can be performed in direct kinematics, using a $^6$Li 56 MeV beam from the Tandem and a CaF target or in inverse kinematics with a Tandem-ALPI or PIAVE-ALPI $^{48}$Ca beam at around 500 MeV.
Considering that a cross section of about 1 $\mu$b can be intercepted by the DSSD detector, we predict that about seven days of beam time will be sufficient to detect the desired $\pi d_{3/2}^{2} s_{1/2}^2$ excited $0^+$ state. The use of PRISMA can be considered for ancillary detection of heavy recoils, at least in A/Q.

[1] D. Brugnara et al., to be submitted

Primary authors

Andrea Gottardo (Istituto Nazionale di Fisica Nucleare) Daniele Brugnara (Istituto Nazionale di Fisica Nucleare)

Co-authors

Alain Goasduff (Università di Padova - INFN Sezione di Padova) Daniele Mengoni (Istituto Nazionale di Fisica Nucleare) Franco Galtarossa (Istituto Nazionale di Fisica Nucleare) Ivano Lombardo (Istituto Nazionale di Fisica Nucleare) Jose' Javier Valiente Dobon (Istituto Nazionale di Fisica Nucleare) Marlène Assié (IPN Orsay)

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