Abstract

In this paper we revisit Dsf0(980) form factors from the light-cone sum rules based on the q¯q picture of f0(980). The main motivation of this study is the decay width of Ds+ππSI=0e+νe measured recently by BESIII collaboration and the Dsf0(980) form factor extracted under the resonant model, here the subscript S and superscript I=0 indicate the S-wave isoscalar dipion system. Our result of the differential width of Ds+f0(980)(ππSI=0)e+νe decay obtained under the narrow width approximation is lower than the data, the result obtained under the resonant Flatté model is consistent with the data, indicating a sizable mixing 20 between s¯s and u¯u+d¯d of f0. In order to get a model independent prediction, we suggest to calculate DsππI=0 form factors with the isoscalar dipion light-cone distribution amplitudes. Our calculation of DsππI=0 form factors is carried out at leading twist level due to the finite knowledge of dipion system, the differential width shows a moderate evolution in contrast to that obtained from the narrow width approximation and the Flatté model. Since the Dsf0(980) form factors is dominated by the twist three contribution, further measurements on four-body semileptonic charm decays would help us to study the dimeson light-cone distribution amplitudes, especially for the subleading twist one.

Details

Title
Ds→f0(980) form factors and the Ds+→(f0(980)→)ππSI=0e+νe decay from light-cone sum rules
Author
Cheng, Shan 1   VIAFID ORCID Logo  ; Zhang, Shu-Lei 1 

 Hunan University, School of Physics and Electronics, Changsha, People’s Republic of China (GRID:grid.67293.39); Hunan University, School for Theoretical Physics, Changsha, People’s Republic of China (GRID:grid.67293.39); Hunan Provincial Key Laboratory of High-Energy Scale Physics and Applications, Changsha, People’s Republic of China (GRID:grid.67293.39) 
Pages
379
Publication year
2024
Publication date
Apr 2024
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3034896627
Copyright
© The Author(s) 2024. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.