Speaker
Description
The assumption of universal magic numbers, i.e. closed nuclear shells, all across the nuclear chart has been a fundamental paradigm of the nuclear shell model. However, when exploring nuclides far away from stability, a disappearance of well-established shell closures can be encountered, which, for instance, manifests itself in the island of inversion around $N = 20$ [1]. Describing this shell evolution from first principles is a formidable task for nuclear theory. Recently, nuclear ab-initio methods have been able to expand their reach also into open shell nuclei. This advance now allows for ab-initio calculations of nuclear observables within the $N = 20$ island of inversion [2]. In order to deepen our understanding of this region of nuclides and challenge the predictive power of modern nuclear theory, experimental knowledge about the nuclear charge radii of neutron-rich magnesium (Z = 12) isotopes is crucial.
A powerful tool to access nuclear charge radii is collinear laser spectroscopy (CLS) [3]. However, to extend previous measurements up to $^{32}$Mg [4] and explore the more exotic isotopes $^{33,34}$Mg with very low production yields at radioactive ion beam facilities, more sensitive methods have to be envisioned. The novel Multi-Ion-Reflection Apparatus for Collinear Laser Spectroscopy (MIRACLS) at ISOLDE/CERN [5] combines the high spectral resolution of conventional fluorescence-based CLS with high experimental sensitivity. This is achieved by trapping ion bunches in a Multi-Reflection Time of Flight (MR-ToF) device, in which the ions bounce back and forth between two electrostatic mirrors. Hence, the laser-ion interaction time is increased with each revolution in the MR-ToF apparatus, while retaining the high resolution of CLS.
Very recently in November 2024, we had a successful experimental campaign were we measured hyperfine spectra of $^{33,34}$Mg. This oral contribution will introduce the MIRACLS concept and present the first preliminary data of Mg charge radii from the aforementioned measurement.
[1] T. Otsuka et al., Rev. Mod. Phys. 92, 015002 (2020)
[2] T. Miyagi et al., Phys. Rev. C 102, 034320 (2020)
S. J. Novario et al., Phys. Rev. C 102, 051303 (2020)
G. Hagen et al., arXiv:2201.07298 (2022)
[3] K. Blaum, et al., Phys. Scr. T152, 014017 (2013)
P. Campbell et al., Prog. Part. and Nucl. Phys. 86, 127-180 (2016)
X. Yang et al., Prog. Part. and Nucl. Phys. 129, 104005 (2023)
[4] D. T. Yordanov et al., Phys. Rev. Lett. 108, 042504 (2012)
[5] S. Sels et al., Nucl. Inst. Meth. Phys. Res. Sec. B, 463, 310–314 (2020)
V. Lagaki et al., Nucl. Inst. Meth. Phys. Res. Sec. A, 165663 (2021)
F. Maier et al., Nucl. Inst. Meth. Phys. Res. Sec. A, 167927 (2023)