Gas-phase thorium clusters from laser ablation suggest magicity of Th$$_{13}^+$$

Abstract Laser ablation of a metallic thorium foil produces cationic thorium clusters Th $$_n^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> composed of up to $$n=15$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>=</mml:mo> <mml:mn>15</mml:mn> </mml:mrow> </mml:math> atoms as well as oxide clusters Th $$_n$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mrow/> </mml:mmultiscripts> </mml:math> O $$_m^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>m</mml:mi> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> . Mass spectra are recorded using a multi-reflection time-of-flight analyzer. Up to $$n\lesssim 8$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>≲</mml:mo> <mml:mn>8</mml:mn> </mml:mrow> </mml:math> , the most abundant species for a given cluster size is the Th $$_n$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mrow/> </mml:mmultiscripts> </mml:math> O $$_{2n-1}^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow> <mml:mn>2</mml:mn> <mml:mi>n</mml:mi> <mml:mo>-</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> configuration. Notably, pure thorium clusters Th $$_n^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> become dominant for $$n &gt; rsim 9$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>≳</mml:mo> <mml:mn>9</mml:mn> </mml:mrow> </mml:math> . Production drops sharply after Th $$_{13}^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow> <mml:mn>13</mml:mn> </mml:mrow> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> indicating increased relative stability associated with a “magic number” cluster size. Graphical abstract

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Journal
The European Physical Journal D
Published
2025-04-01
DOI
https://doi.org/10.1140/epjd/s10053-025-00983-2
Citations
1
Primary Topic
Cold Atom Physics and Bose-Einstein Condensates
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article
Field-Weighted Citation Impact
1.25

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article

Gas-phase thorium clusters from laser ablation suggest magicity of Th$$_{13}^+$$

Jonas Stricker, Ch. E. Düllmann, Dennis Renisch, Paul Fischer et al.
1 citations
The European Physical Journal D
Cold Atom Physics and Bose-Einstein Condensates
1.25
article

Gas-phase thorium clusters from laser ablation suggest magicity of Th$$_{13}^+$$

Jonas Stricker, Ch. E. Düllmann, Dennis Renisch, Paul Fischer, L. Schweikhard
article en
1 citations

Abstract

Abstract Laser ablation of a metallic thorium foil produces cationic thorium clusters Th $$_n^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> composed of up to $$n=15$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>=</mml:mo> <mml:mn>15</mml:mn> </mml:mrow> </mml:math> atoms as well as oxide clusters Th $$_n$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mrow/> </mml:mmultiscripts> </mml:math> O $$_m^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>m</mml:mi> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> . Mass spectra are recorded using a multi-reflection time-of-flight analyzer. Up to $$n\lesssim 8$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>≲</mml:mo> <mml:mn>8</mml:mn> </mml:mrow> </mml:math> , the most abundant species for a given cluster size is the Th $$_n$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mrow/> </mml:mmultiscripts> </mml:math> O $$_{2n-1}^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow> <mml:mn>2</mml:mn> <mml:mi>n</mml:mi> <mml:mo>-</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> configuration. Notably, pure thorium clusters Th $$_n^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mi>n</mml:mi> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> become dominant for $$n &gt; rsim 9$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>≳</mml:mo> <mml:mn>9</mml:mn> </mml:mrow> </mml:math> . Production drops sharply after Th $$_{13}^+$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow> <mml:mn>13</mml:mn> </mml:mrow> <mml:mo>+</mml:mo> </mml:mmultiscripts> </mml:math> indicating increased relative stability associated with a “magic number” cluster size. Graphical abstract

The European Physical Journal DVol. 79(4)
GSI Helmholtz Centre for Heavy Ion Research (DE), Johannes Gutenberg University Mainz (DE), Universität Greifswald (DE), Helmholtz Institute Mainz (DE)
Deutsche Forschungsgemeinschaft
Openalex Percentile: Top 22%
Cold Atom Physics and Bose-Einstein Condensates
1.25
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