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Li, Jun1; Guo, Guang-Hai | |
Measuring the scalar induced gravitational waves from observations | |
Source Publication | EUROPEAN PHYSICAL JOURNAL C
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Language | 英语 |
Abstract | We consider the scalar induced gravitational waves from the cosmic microwave background (CMB) observations and the gravitational wave observations. In the Lambda CDM+r model, we constrain the cosmological parameters within the evolution of the scalar induced gravitational waves by the additional scalar power spectrum. The two special cases called narrow power spectrum and wide power spectrum have influence on the cosmological parameters, especially the combinations of Planck18+BAO+BK15+LISA. We also compare these numerical results from four datasets within LIGO, LISA, IPTA and FAST projects, respectively. The constraints from FAST have a significant impact on tensor-to-scalar ratio. Besides, we only consider the relic density of induced gravitational waves with respect to different frequencies from CMB scale to high frequencies including the range of LIGO and LISA. |
2021 | |
ISSN | 1434-6044 |
Volume | 81Issue:7Pages:602 |
Cooperation Status | 国内 |
Subject Area | Physics |
MOST Discipline Catalogue | Physics, Particles & Fields |
DOI | 10.1140/epjc/s10052-021-09405-0 |
Indexed By | SCIE |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.itp.ac.cn/handle/311006/27395 |
Collection | SCI期刊论文 |
Affiliation | 1.Qingdao Univ Sci & Technol, Sch Math & Phys, Qingdao 266061, Peoples R China 2.Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China |
Recommended Citation GB/T 7714 | Li, Jun,Guo, Guang-Hai. Measuring the scalar induced gravitational waves from observations[J]. EUROPEAN PHYSICAL JOURNAL C,2021,81(7):602. |
APA | Li, Jun,&Guo, Guang-Hai.(2021).Measuring the scalar induced gravitational waves from observations.EUROPEAN PHYSICAL JOURNAL C,81(7),602. |
MLA | Li, Jun,et al."Measuring the scalar induced gravitational waves from observations".EUROPEAN PHYSICAL JOURNAL C 81.7(2021):602. |
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