Astrophysical constraints on the proton-to-electron mass ratio with FAST
文献类型：期刊论文
| 作者 | Chen, Xi2,3; Ellingsen, Simon P.1; Mei, Ying2 |
| 刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2019-02-01 |
| 卷号 | 19期号:2页码:10 |
| 关键词 | ISM: molecules radio lines: ISM techniques: radial velocities elementary particles |
| ISSN号 | 1674-4527 |
| DOI | 10.1088/1674-4527/19/2/18 |
| 英文摘要 | That the laws of physics are the same at all times and places throughout the Universe is one of the basic assumptions of physics. Astronomical observations provide the only means to test this basic assumption on cosmological time and distance scales. The possibility of variations in the dimensionless physical constant mu - the proton-to-electron mass ratio, can be tested by comparing astronomical measurements of the rest frequency of certain spectral lines at radio wavelengths with laboratory determinations. Different types of molecular transitions have different dependencies on mu and so observations of two or more spectral lines towards the same astronomical source can be used to test whether there is any evidence for either temporal or spatial changes in the physical fundamental constants. mu will change if the relative strength of the strong nuclear force compared to the electromagnetic force varies. Theoretical studies have shown that the rotational transitions of some molecules which have transitions in the frequency range that will be covered by FAST (e.g., CH3OH, OH and CH) are sensitive to changes in mu. A number of studies looking for possible variations in mu have been undertaken with existing telescopes, however, the greater sensitivity of FAST means it will open new opportunities to significantly improve upon measurements made to date. In this paper, we discuss which molecular transitions and sources (both in the Galaxy and external galaxies) are likely targets for providing improved constraints on mu with FAST. |
| 资助项目 | National Natural Science Foundation of China[11590781] ; Strategic Priority Research Program of the Chinese Academy of Sciences (CAS)[XDA04060701] ; Key Laboratory for Radio Astronomy, CAS |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000458412900003 |
| 出版者 | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
| 源URL | [http://119.78.226.72/handle/331011/31961]  |
| 专题 | 中国科学院上海天文台 |
| 通讯作者 | Mei, Ying |
| 作者单位 | 1.Univ Tasmania, Sch Phys Sci, Private Bag 37, Hobart, Tas 7001, Australia 2.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China 3.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China |
| 推荐引用方式 GB/T 7714 | Chen, Xi,Ellingsen, Simon P.,Mei, Ying. Astrophysical constraints on the proton-to-electron mass ratio with FAST[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2019,19(2):10. |
| APA | Chen, Xi,Ellingsen, Simon P.,&Mei, Ying.(2019).Astrophysical constraints on the proton-to-electron mass ratio with FAST.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,19(2),10. |
| MLA | Chen, Xi,et al."Astrophysical constraints on the proton-to-electron mass ratio with FAST".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 19.2(2019):10. |
入库方式： OAI收割
来源：上海天文台
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