中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Dirac spinor scattering states with positive-energy in rotating spheroid models

文献类型:期刊论文

作者Gao, Zhi-Fu3,4; Chen, Ci-Xing2; Wang, Na4; Zhao, Xin-Jun3,6; Wang, Zhao-Jun1,5
刊名ASTRONOMISCHE NACHRICHTEN
出版日期2024-02-17
卷号345期号:2-3页码:e240012
关键词dirac spinors quantum field theory scattering state rotating spheroids
ISSN号0004-6337
DOI10.1002/asna.20240012
产权排序1
英文摘要There are many rotating spheroids in the universe, and many astronomers and physicists have used theoretical methods to study the characteristics of stellar gravity since Newton's time. This paper derives the solutions of eight scattering states (phi((0)), chi((0)), phi((1)), chi((1)), phi((2)), chi((2)), phi((3)), and chi((3))) for the Dirac equation with positive-energy E = im, and establishes the relationship between the differential scattering cross section sigma(i)(p, theta, phi) and the stellar density mu. It is found that: (1) For the eight scattering states, their average scattering cross-sections (sigma(i)) over bar are proportional to mu(2), and depend on the star's radius, and the higher the stellar density mu, the greater the sensitivity of (sigma(i)) over bar to the change of mu; (2) For the four scattering states chi((i)), i = 0, 1, 2, 3, their average scattering amplitudes f (p, theta) and (sigma(i)) over bar (p, theta) depend on themass m of the particles; while for the other four scattering states phi((i)), i = 0, 1, 2, 3, then (f) over bar and (sigma) over bar are independent of m. This study links the gravitational characteristics of stars with the scattering cross section, creating a new method for studying the gravitational characteristics, which helps to reveal the mystery of the gravity of rotating ellipsoidal stars.
WOS关键词INTERSTELLAR SCINTILLATION OBSERVATIONS ; EQUATION ; SYSTEMS ; TORSION
资助项目Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Key Research and Development Program of China[2022YFC2205202] ; Chinese National Science Foundation[12041304] ; [2022A03013-1]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001163561800001
出版者WILEY-V C H VERLAG GMBH
资助机构Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Key Research and Development Program of China ; Chinese National Science Foundation
源URL[http://ir.xao.ac.cn/handle/45760611-7/5850]  
专题研究单元未命名
通讯作者Zhao, Xin-Jun; Wang, Zhao-Jun
作者单位1.Xinjiang Univ Sci & Technol, Korla, Xinjiang, Peoples R China
2.Univ Sci & Technol China, Dept Astron, Hefei, Anhui, Peoples R China
3.Yili Normal Univ, Coll Phys Sci & Technol, Xinjiang Lab Phase Transit & Microstruct Condensed, Yining, Xinjiang, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Xinjiang, Peoples R China
5.Xinjiang Univ Sci & Technol, Korla 841000, Xinjiang, Peoples R China
6.Yili Normal Univ, Coll Phys Sci & Technol, Xinjiang Lab Phase Transit & Microstruct Condensed, Yining 83500, Xinjiang, Peoples R China
推荐引用方式
GB/T 7714
Gao, Zhi-Fu,Chen, Ci-Xing,Wang, Na,et al. Dirac spinor scattering states with positive-energy in rotating spheroid models[J]. ASTRONOMISCHE NACHRICHTEN,2024,345(2-3):e240012.
APA Gao, Zhi-Fu,Chen, Ci-Xing,Wang, Na,Zhao, Xin-Jun,&Wang, Zhao-Jun.(2024).Dirac spinor scattering states with positive-energy in rotating spheroid models.ASTRONOMISCHE NACHRICHTEN,345(2-3),e240012.
MLA Gao, Zhi-Fu,et al."Dirac spinor scattering states with positive-energy in rotating spheroid models".ASTRONOMISCHE NACHRICHTEN 345.2-3(2024):e240012.

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