现代天文学认为分子云核是恒星诞生的区域,对分子云核的检测和其性质的全方面研究有利于理解恒星的形成过程以及星系和宇宙的演化。随着银河画卷巡天项目(Milky Way Imaging Scroll Painting,MWISP)的开展和实测数据的快速积累,开发分...现代天文学认为分子云核是恒星诞生的区域,对分子云核的检测和其性质的全方面研究有利于理解恒星的形成过程以及星系和宇宙的演化。随着银河画卷巡天项目(Milky Way Imaging Scroll Painting,MWISP)的开展和实测数据的快速积累,开发分子云核智能仿真与检测系统成为必要。系统提供分子云核智能检测、仿真建模、参数还原、三维可视化、数据存储等功能。借助该系统,科研人员可以方便快捷地对银河画卷实测数据开展分子云核的检测和三维可视化,更好地研究其物理性质。展开更多
We study the nucleon form factors and the nucleon-△（1232） transitions in a framework of hypercentral constituent quark model. The pion meson cloud effect is taken into account explicitly. Our results show that the ...We study the nucleon form factors and the nucleon-△（1232） transitions in a framework of hypercentral constituent quark model. The pion meson cloud effect is taken into account explicitly. Our results show that the pion cloud contributes substantially to the nucleon form factors as well as to the helicity amplitudes of △（1232）, and it gives an improved agreement compared to the experimental.展开更多
文摘现代天文学认为分子云核是恒星诞生的区域,对分子云核的检测和其性质的全方面研究有利于理解恒星的形成过程以及星系和宇宙的演化。随着银河画卷巡天项目(Milky Way Imaging Scroll Painting,MWISP)的开展和实测数据的快速积累,开发分子云核智能仿真与检测系统成为必要。系统提供分子云核智能检测、仿真建模、参数还原、三维可视化、数据存储等功能。借助该系统,科研人员可以方便快捷地对银河画卷实测数据开展分子云核的检测和三维可视化,更好地研究其物理性质。
基金The project supported by National Natural Science Foundation of China under Grant Nos. 10475088 and 90103020, the CAS Knowledge Innovation Project under Grant No. KC2-SW-N02, and the Institute of Theoretical Physics The support from the Center of Theoretical Nuclear Physics, Lanzhou National Laboratory of Heavy Ion Accelerator is appreciated. 0ne of authors （Y.B. Dong） thanks the Department of Physics, Genova University for the hospitality. Authors are grateful to the discussions with M.M. Giannini and Santopinto.
文摘We study the nucleon form factors and the nucleon-△（1232） transitions in a framework of hypercentral constituent quark model. The pion meson cloud effect is taken into account explicitly. Our results show that the pion cloud contributes substantially to the nucleon form factors as well as to the helicity amplitudes of △（1232）, and it gives an improved agreement compared to the experimental.
