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Charge radii of exotic potassium isotopes challenge nuclear theory and the magic character of $N = 32$

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arxiv 2012.01864 v1 pith:52CEHL4Q submitted 2020-12-03 nucl-ex nucl-thphysics.atom-ph

classification nucl-exnucl-thphysics.atom-ph
keywords nuclearchargeradiitheoryisotopesmagicbeyondcalculations
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abstract

Nuclear charge radii are sensitive probes of different aspects of the nucleon-nucleon interaction and the bulk properties of nuclear matter; thus, they provide a stringent test and challenge for nuclear theory. The calcium region has been of particular interest, as experimental evidence has suggested a new magic number at $N = 32$ [1-3], while the unexpectedly large increases in the charge radii [4,5] open new questions about the evolution of nuclear size in neutron-rich systems. By combining the collinear resonance ionization spectroscopy method with $\beta$-decay detection, we were able to extend the charge radii measurement of potassium ($Z =19$) isotopes up to the exotic $^{52}$K ($t_{1/2}$ = 110 ms), produced in minute quantities. Our work provides the first charge radii measurement beyond $N = 32$ in the region, revealing no signature of the magic character at this neutron number. The results are interpreted with two state-of-the-art nuclear theories. For the first time, a long sequence of isotopes could be calculated with coupled-cluster calculations based on newly developed nuclear interactions. The strong increase in the charge radii beyond $N = 28$ is not well captured by these calculations, but is well reproduced by Fayans nuclear density functional theory, which, however, overestimates the odd-even staggering effect. These findings highlight our limited understanding on the nuclear size of neutron-rich systems, and expose pressing problems that are present in some of the best current models of nuclear theory.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Reduction in nuclear size and quadrupole deformation of high-spin isomers of 127,129In

    nucl-ex 2025-05 accept novelty 6.0 of 10

    High-spin isomers in neutron-rich indium isotopes have smaller charge radii than their ground states, with 129In showing a three times larger reduction than 127In, a pattern no current nuclear model reproduces.

  2. Radii of light nuclei from the Jacobi No-Core Shell Model

    nucl-th 2025-02 conditional novelty 6.0 of 10

    A density-tail repair method yields converged matter and charge radii for 4,6,8He and 6,7,8Li from Jacobi no-core shell model calculations with chiral forces.

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