Why We Do Not See the Radiative Decays of the $$D_{{s1}}^{ + }$$(2536) Meson?

The radiative decays of $${{D}_{{s1}}}{{(2536)}^{ + }}$$ charmed-strange meson have not been observed. We employ the available Babar measurements to derive an upper bound for the $${{D}_{{s1}}}{{(2536)}^{ + }} \to D_{s}^{ + }\gamma $$ decay width and discuss its implications for the quark structure of $${{D}_{{s1}}}{{(2460)}^{ + }}$$ .

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Publication Details

Journal
Journal of Experimental and Theoretical Physics Letters
Published
2025-02-01
DOI
https://doi.org/10.1134/s0021364024605037
Citations
1
Primary Topic
Quantum Chromodynamics and Particle Interactions
Type
article
Field-Weighted Citation Impact
1.87

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article

Why We Do Not See the Radiative Decays of the $$D_{{s1}}^{ + }$$(2536) Meson?

A. Bondar
1 citations
Journal of Experimental and Theoretical Physics Letters
Quantum Chromodynamics and Particle Interactions
1.87
article

Why We Do Not See the Radiative Decays of the $$D_{{s1}}^{ + }$$(2536) Meson?

A. Bondar
article en
1 citations

Abstract

The radiative decays of $${{D}_{{s1}}}{{(2536)}^{ + }}$$ charmed-strange meson have not been observed. We employ the available Babar measurements to derive an upper bound for the $${{D}_{{s1}}}{{(2536)}^{ + }} \to D_{s}^{ + }\gamma $$ decay width and discuss its implications for the quark structure of $${{D}_{{s1}}}{{(2460)}^{ + }}$$ .

Journal of Experimental and Theoretical Physics LettersVol. 121(4)
Novosibirsk State University (RU), Budker Institute of Nuclear Physics (RU)
Siberian Branch, Russian Academy of Sciences, Russian Academy of Sciences, Nuclear Physics
Openalex Percentile: Top 16%
Quantum Chromodynamics and Particle Interactions
1.87
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