Gravitational wave cosmology
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arXiv
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| Format: | Preprint |
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2025
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| author | Bian, Ligong Cai, Rong-Gen Dong, Yu-Qi Gao, Qing Gong, Yungui Guo, Zong-Kuan Huang, Qing-Guo Kang, Zhaofeng Li, Li Liu, Jing Liu, Lang Liu, Yu-Xiao Lu, Xuchen Peng, Zhi-Zhang Qiao, Jin Wu, Puxun Wu, Yue-Liang Yu, Jiang-Hao Yuan, Chen Zhang, Chao Zhu, Tao |
| author_facet | Bian, Ligong Cai, Rong-Gen Dong, Yu-Qi Gao, Qing Gong, Yungui Guo, Zong-Kuan Huang, Qing-Guo Kang, Zhaofeng Li, Li Liu, Jing Liu, Lang Liu, Yu-Xiao Lu, Xuchen Peng, Zhi-Zhang Qiao, Jin Wu, Puxun Wu, Yue-Liang Yu, Jiang-Hao Yuan, Chen Zhang, Chao Zhu, Tao |
| contents | Gravitational waves (GWs) originating from cosmological sources offer direct insights into the physics of the primordial Universe, the fundamental nature of gravity, and the cosmic expansion of the Universe. In this review paper, we present a comprehensive overview of our recent advances in GW cosmology, supported by the national key research and development program of China, focusing on cosmological GW sources and their implications for fundamental physics and cosmology. We first discuss the generation mechanisms and characteristics of stochastic gravitational wave backgrounds generated by physical processes occurred in the early Universe, including those from inflation, phase transitions, and topological defects, and summarize current and possible future constraints from pulsar timing array and space-based detectors. Next, we explore the formation and observational prospects of primordial black holes as GW sources and their potential connection to dark matter. We then analyze how GWs are affected by large-scale structure, cosmological perturbations, and possible modifications of gravity on GW propagation, and how these effects can be used to test fundamental symmetry of gravity. Finally, we discuss the application of GW standard sirens in measuring the Hubble constant, the expansion history, and dark energy parameters, including their combination with electromagnetic observations. These topics together show how GW observations, especially with upcoming space-based detectors, such as LISA, Taiji, and Tianqin, can provide new information about the physics of the early Universe, cosmological evolution, and the nature of gravity. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_19747 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Gravitational wave cosmology Bian, Ligong Cai, Rong-Gen Dong, Yu-Qi Gao, Qing Gong, Yungui Guo, Zong-Kuan Huang, Qing-Guo Kang, Zhaofeng Li, Li Liu, Jing Liu, Lang Liu, Yu-Xiao Lu, Xuchen Peng, Zhi-Zhang Qiao, Jin Wu, Puxun Wu, Yue-Liang Yu, Jiang-Hao Yuan, Chen Zhang, Chao Zhu, Tao General Relativity and Quantum Cosmology High Energy Physics - Theory Gravitational waves (GWs) originating from cosmological sources offer direct insights into the physics of the primordial Universe, the fundamental nature of gravity, and the cosmic expansion of the Universe. In this review paper, we present a comprehensive overview of our recent advances in GW cosmology, supported by the national key research and development program of China, focusing on cosmological GW sources and their implications for fundamental physics and cosmology. We first discuss the generation mechanisms and characteristics of stochastic gravitational wave backgrounds generated by physical processes occurred in the early Universe, including those from inflation, phase transitions, and topological defects, and summarize current and possible future constraints from pulsar timing array and space-based detectors. Next, we explore the formation and observational prospects of primordial black holes as GW sources and their potential connection to dark matter. We then analyze how GWs are affected by large-scale structure, cosmological perturbations, and possible modifications of gravity on GW propagation, and how these effects can be used to test fundamental symmetry of gravity. Finally, we discuss the application of GW standard sirens in measuring the Hubble constant, the expansion history, and dark energy parameters, including their combination with electromagnetic observations. These topics together show how GW observations, especially with upcoming space-based detectors, such as LISA, Taiji, and Tianqin, can provide new information about the physics of the early Universe, cosmological evolution, and the nature of gravity. |
| title | Gravitational wave cosmology |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2505.19747 |