KMS National Astronomical Observatories, CAS
| Strong-field effects in massive scalar-tensor gravity for slowly spinning neutron stars and application to x-ray pulsar pulse profiles | |
| Xu, Rui1; Gao, Yong1,2; Shao, Lijing1,3 | |
| 2020-09-22 | |
| Source Publication | PHYSICAL REVIEW D
 |
| ISSN | 1550-7998 |
| Volume | 102Issue:6Pages:15 |
| Abstract | Neutron stars (NSs) in scalar-tensor (ST) theories of gravitation can acquire scalar charges and generate distinct spacetimes from those in general relativity (GR) through the celebrated phenomenon of spontaneous scalarization. Taking on an ST theory with the mass term of the scalar field, we determine the theory parameter space for spontaneous scalarization by investigating the linearized scalar field equation. Then the full numerical solutions for slowly rotating NSs are obtained and studied in great detail. The resulted spacetime is used to calculate test-particle geodesics. The lightlike geodesics are used to construct the profile of x-ray radiation from a pair of hot spots on the surface of scalarized NSs, which potentially can be compared with the data from the Neutron star Interior Composition Explorer (NICER) mission for testing the ST theory. |
| Funding Organization | National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University |
| DOI | 10.1103/PhysRevD.102.064057 |
| WOS Keyword | SPECTRA ; MODELS |
| Language | 英语 |
| Funding Project | National Natural Science Foundation of China[11975027] ; National Natural Science Foundation of China[11991053] ; National Natural Science Foundation of China[11721303] ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology[2018QNRC001] ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB23010200] ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University |
| Funding Organization | National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Boya Postdoctoral Fellowship at Peking University ; Boya Postdoctoral Fellowship at Peking University ; High-performance Computing Platform of Peking University ; High-performance Computing Platform of Peking University |
| WOS Research Area | Astronomy & Astrophysics ; Physics |
| WOS Subject | Astronomy & Astrophysics ; Physics, Particles & Fields |
| WOS ID | WOS:000571654000003 |
| Publisher | AMER PHYSICAL SOC |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.bao.ac.cn/handle/114a11/81529 |
| Collection | 中国科学院国家天文台 |
| Corresponding Author | Xu, Rui; Shao, Lijing |
| Affiliation | 1.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 2.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| Recommended Citation GB/T 7714 | Xu, Rui,Gao, Yong,Shao, Lijing. Strong-field effects in massive scalar-tensor gravity for slowly spinning neutron stars and application to x-ray pulsar pulse profiles[J]. PHYSICAL REVIEW D,2020,102(6):15. |
| APA | Xu, Rui,Gao, Yong,&Shao, Lijing.(2020).Strong-field effects in massive scalar-tensor gravity for slowly spinning neutron stars and application to x-ray pulsar pulse profiles.PHYSICAL REVIEW D,102(6),15. |
| MLA | Xu, Rui,et al."Strong-field effects in massive scalar-tensor gravity for slowly spinning neutron stars and application to x-ray pulsar pulse profiles".PHYSICAL REVIEW D 102.6(2020):15. |
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