Charge distribution of d* (2380) | |
Dong, Yubing1,2,3; Huang, Fei3; Shen, Pengnian1,2,4; Zhang, Zongye1,2,3 | |
刊名 | Physical review d |
2017-11-08 | |
卷号 | 96期号:9页码:11 |
ISSN号 | 2470-0010 |
DOI | 10.1103/physrevd.96.094001 |
通讯作者 | Dong, yubing() |
英文摘要 | Based on a chiral constituent quark model, we calculate the charge distributions of d*(2380). we consider the existence of two different interpretations of the d* : a compact structure in the two-coupled-channel (delta delta + cc) approximation, and a resonant structure of d-12 pi. we calculate the charge distribution of the d* with a compact structure, and we also roughly estimate the charge distribution for a d-12 pi structure on the same base. the result shows that there is a remarkable difference in the charge distributions of the two structural pictures. therefore, we expect that future experiments may provide a clear signal for the d* structure. |
WOS关键词 | ELECTROMAGNETIC FORM-FACTORS ; NUCLEON-NUCLEON-INTERACTION ; CONSTITUENT QUARK-MODEL ; DIBARYON RESONANCES ; REPULSIVE CORE ; CLUSTER MODEL ; BRANCHING RATIOS ; MESON PRODUCTION ; STATES ; D-ASTERISK(2380) |
WOS研究方向 | Astronomy & Astrophysics ; Physics |
WOS类目 | Astronomy & Astrophysics ; Physics, Particles & Fields |
语种 | 英语 |
出版者 | AMER PHYSICAL SOC |
WOS记录号 | WOS:000414667600001 |
内容类型 | 期刊论文 |
URI标识 | http://www.corc.org.cn/handle/1471x/2176895 |
专题 | 高能物理研究所 |
通讯作者 | Dong, Yubing |
作者单位 | 1.Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China 2.Chinese Acad Sci, TPCSF, Beijing 100049, Peoples R China 3.Univ Chinese Acad Sci, Sch Phys Sci, Beijing 101408, Peoples R China 4.Guangxi Normal Univ, Coll Phys & Technol, Guilin 541004, Peoples R China |
推荐引用方式 GB/T 7714 | Dong, Yubing,Huang, Fei,Shen, Pengnian,et al. Charge distribution of d* (2380)[J]. Physical review d,2017,96(9):11. |
APA | Dong, Yubing,Huang, Fei,Shen, Pengnian,&Zhang, Zongye.(2017).Charge distribution of d* (2380).Physical review d,96(9),11. |
MLA | Dong, Yubing,et al."Charge distribution of d* (2380)".Physical review d 96.9(2017):11. |
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