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![]() ![]() |
刊名 | ASTRONOMISCHE NACHRICHTEN
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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 |
DOI | 10.1002/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. |
入库方式: OAI收割
来源:新疆天文台
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