Observational constraints on Rastall gravity from rotation curves of low surface brightness galaxies | |
Tang, Meirong1,3,4,5; Xu, Zhaoyi2; Wang JC(王建成)1,3,4,5 | |
发表期刊 | CHINESE PHYSICS C |
2020-08-01 | |
卷号 | 44期号:8页码:8 |
DOI | 10.1088/1674-1137/44/8/085104 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Rastall gravity energy condition LSB galaxies |
摘要 | Rastall gravity is a modification of Einstein's general relativity in which the energy-momentum conservation is not satisfied and depends on the gradient of the Ricci curvature. It is currently in dispute whether Rastall gravity is equivalent to general relativity (GR). In this work, we constrain the theory using the rotation curves of low surface brightness (LSB) spiral galaxies. By fitting the rotation curves of LSB galaxies, we obtain parameter beta of the Rastall gravity. The beta values of LSB galaxies satisfy the weak energy condition (WEC) and strong energy condition (SEC). Combining the beta values of type Ia supernovae and the gravitational lensing of elliptical galaxies on Rastall gravity, we conclude that Rastall gravity may be equivalent to general relativity. |
资助项目 | National Natural Science Foundation of China[11503078] ; National Natural Science Foundation of China[11573060] ; National Natural Science Foundation of China[11847310] ; National Natural Science Foundation of China[11661161010] |
项目资助者 | National Natural Science Foundation of China[11503078, 11573060, 11847310, 11661161010] |
语种 | 英语 |
学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学 |
文章类型 | Article |
出版者 | IOP PUBLISHING LTD |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
ISSN | 1674-1137 |
URL | 查看原文 |
WOS记录号 | WOS:000557439000001 |
WOS研究方向 | Physics |
WOS类目 | Physics, Nuclear ; Physics, Particles & Fields |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/23633 |
专题 | 高能天体物理研究组 中国科学院天体结构与演化重点实验室 |
通讯作者 | Tang, Meirong |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, China 2.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, China 4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China 5.University of Chinese Academy of Sciences, Beijing 100049, China |
第一作者单位 | 中国科学院云南天文台 |
通讯作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Tang, Meirong,Xu, Zhaoyi,Wang JC. Observational constraints on Rastall gravity from rotation curves of low surface brightness galaxies[J]. CHINESE PHYSICS C,2020,44(8):8. |
APA | Tang, Meirong,Xu, Zhaoyi,&Wang JC.(2020).Observational constraints on Rastall gravity from rotation curves of low surface brightness galaxies.CHINESE PHYSICS C,44(8),8. |
MLA | Tang, Meirong,et al."Observational constraints on Rastall gravity from rotation curves of low surface brightness galaxies".CHINESE PHYSICS C 44.8(2020):8. |
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