2014/05/09 by Martin Cleven, Harald W. Grießhammer, Feng-Kun Guo +3 · 74 citations
Physics and Astronomy · #Hadron #High-Energy Particle Collisions Research #Nuclear physics #Observable #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum Chromodynamics and Particle Interactions #Quantum mechanics #Radiative transfer #hep-ex #hep-ph
paper · pdf · doi:10.1140/epja/i2014-14149-y
published in The European Physical Journal A 50(9) (Springer Science+Business Media)
arxiv created 2014/05/09 · openalex publication_date 2014/09/01 · arxiv updated 2014/09/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Since their discovery in 2003, the open charm states Ds0^*(2317) and Ds1(2460) provide a challenge to the conventional quark model. In recent years, theoretical evidence has been accumulated for both states in favor of a predominantly DK and D^*K molecular nature, respectively. However, a direct experimental proof of this hypothesis still needs to be found. Since radiative decays are generally believed to be sensitive to the inner structure of the decaying particles, we study in this work the radiative and strong decays of both the Ds0^*(2317) and Ds1(2460), as well as of their counterparts in the bottom sector. While the strong decays are indeed strongly enhanced for molecular states, the radiative decays are of similar order of magnitude in different pictures. Thus, the experimental observable that allows one to conclusively quantify the molecular components of the Ds0^*(2317) and Ds1(2460) is the hadronic width, and not the radiative one, in contradistinction to common belief. We also find that radiative decays of the sibling states in the bottom sector are significantly more frequent than the hadronic ones. Based on this, we identify their most promising discovery channels.