Abstract
A supermassive binary black-hole candidate SDSS J1430+2303 reported recently motivates us to investigate an imminent binary of supermassive black holes as potential gravitational wave source, and the radiated gravitational waves at the end of the merger are shown to be in the band of space-borne detectors. We provide a general analysis on the required detecting sensitivity needed for probing such type gravitational wave sources and make a full discussion by considering two typically designed configurations of space-borne antennas. If a source is so close, it is possible to be detected with Taiji pathfinder-plus which is proposed to be an extension for the planned Taiji pathfinder by just adding an additional satellite to the initial two satellites. The gravitational wave detection on such kind of source enables us to explore the properties of supermassive black holes and the nature of gravity.
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This work was supported by the National Key R&D Program of China (Grant Nos. 2021YFC2203002, and 2020YFC2201501), the National Natural Science Foundation of China (Grant Nos. 11773059, 12173071, 12147103, and 11821505), and the Strategic Priority Research Program of the CAS (Grant No. XDA15021102). Wen-Biao Han was supported by the CAS Project for Young Scientists in Basic Research (Grant No. YSBR-006).
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Zhong, X., Han, WB., Luo, Z. et al. Exploring the nature of black hole and gravity with an imminent merging binary of supermassive black holes. Sci. China Phys. Mech. Astron. 66, 230411 (2023). https://doi.org/10.1007/s11433-022-2028-7
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DOI: https://doi.org/10.1007/s11433-022-2028-7