Super-Eddington accreting massive black holes explore high-z cosmology: Monte-Carlo simulations
文献类型：期刊论文
| 作者 | Cai, RG ; Guo, ZK; Huang, QG; Yang, T3
|
| 刊名 | PHYSICAL REVIEW D
 |
| 出版日期 | 2018 |
| 卷号 | 97期号:12页码:123502 |
| ISSN号 | 2470-0010 |
| 关键词 | ACTIVE GALACTIC NUCLEI BROAD-LINE REGION REVERBERATION MAPPING CAMPAIGN BARYON ACOUSTIC-OSCILLATIONS GALAXIES RATES DISKS II. CONSTRAINTS CONSTANT |
| DOI | 10.1103/PhysRevD.97.123502 |
| 英文摘要 | In this paper, we simulate Super-Eddington accreting massive black holes (SEAMBHs) as the candles to probe cosmology for the first time. SEAMBHs have been demonstrated to be able to provide a new tool for estimating cosmological distance. Thus, we create a series of mock data sets of SEAMBHs, especially in the high rcdshift region, to check their abilities to probe the cosmology. To fulfill the potential of the SEAMBHs on the cosmology, we apply the simulated data to three projects. The first is the exploration of their abilities to constrain the cosmological parameters, in which we combine different data sets of current observations such as the cosmic microwave background from Planck and type Ia supernovae from Joint Light-curve Analysis (JLA). We find that the high redshift SEAMBHs can help to break the degeneracies of the background cosmological parameters constrained by Planck and JLA, thus giving much tighter constraints of the cosmological parameters. The second uses the high redshift SEAMBHs as the complements of the low redshift JLA to constrain the early expansion rate and the dark energy density evolution in the cold dark matter frame. Our results show that these high redshift SEAMBHs arc very powerful on constraining the early Hubble rate and the evolution of the dark energy density; thus they can give us more information about the expansion history of our Universe, which is also crucial for testing the ACDM model in the high redshift region. Finally, we check the SEAMBH candles' abilities to reconstruct the equation of state for dark energy at high redshift. In summary, our results show that the SEAMBHs, as the rare candles in the high rcdshift region, can provide us a new and independent observation to probe cosmology in the future. |
| 学科主题 | Astronomy & Astrophysics ; Physics |
| 语种 | 英语 |
| 源URL | [http://ir.itp.ac.cn/handle/311006/22887]  |
| 专题 | 理论物理研究所_理论物理所1978-2010年知识产出 |
| 作者单位 | 1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 2.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China 3.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China |
| 推荐引用方式 GB/T 7714 | Cai, RG,Guo, ZK,Huang, QG,et al. Super-Eddington accreting massive black holes explore high-z cosmology: Monte-Carlo simulations[J]. PHYSICAL REVIEW D,2018,97(12):123502. |
| APA | Cai, RG,Guo, ZK,Huang, QG,&Yang, T.(2018).Super-Eddington accreting massive black holes explore high-z cosmology: Monte-Carlo simulations.PHYSICAL REVIEW D,97(12),123502. |
| MLA | Cai, RG,et al."Super-Eddington accreting massive black holes explore high-z cosmology: Monte-Carlo simulations".PHYSICAL REVIEW D 97.12(2018):123502. |
入库方式： OAI收割
来源：理论物理研究所
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