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Laser spectroscopy illuminates the $N=32$ shell closure

Authors: Tim E. Lellinger, Liss V. Rodriguez, Patrick Muller, Osama Ahmad, Mark L. Bissell, Klaus Blaum, Emily Burbach, Bradley Cheal, Till Fabritz, Ronald F. Garcia Ruiz, Matthias Heinz, Jack Hughes, Phillip Imgram, Kristian Konig, Yinshen Liu, Bernhard Maass, Edward N. Matthews, Takayuki Miyagi, Witold Nazarewicz, Rainer Neugart, Gerda Neyens, Lukas Nies, Wilfried Nortershauser, Julian Palmes, Peter Plattner, Paul-Gerhard Reinhard, Laura Renth, Rodolfo Sanchez, Achim Schwenk, Julien Spahn, Xiaofei Yang, Deyan T. YordanovPublished: 2026-08-11Paper ID: 2608.10943Category: nucl-thLicense: CC BY 4.0

Abstract

Atomic nuclei are strongly correlated quantum many-body systems, and how their shell structure evolves with increasing neutron excess remains a central open question in nuclear physics. Calcium isotopes are an ideal testing ground: alongside the traditional magic numbers $N=20,28$, new shell closures have been proposed at $N=32,34$ ($^{52,54}\mathrm{Ca}$). While the charge radius rises rapidly towards $N=32$, further moments and radii in the isotopic chain have remained inaccessible due to the low production yield of a few ions per second. Here we apply a highly sensitive collinear laser spectroscopy technique, which reveals a strikingly simple behaviour: adding one neutron to $^{52}\mathrm{Ca}$ yields a pure single-particle magnetic dipole moment in $^{53}\mathrm{Ca}$, while the charge-radius slope towards $^{54}\mathrm{Ca}$ exceeds that towards $^{52}\mathrm{Ca}$. This provides strong evidence for a robust $N=32$ shell closure and stringently constrains nuclear structure models.

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