双黑洞并合事件中发现第三致密天体存在迹象

Core Insights - The research team led by Han Wenbiao from the Shanghai Astronomical Observatory has discovered that binary black holes may not be "lonely wanderers," but could be influenced by a third dense celestial body during merger events, providing new clues to the formation of binary black holes [1][2] - The findings were published on August 1 in the Astrophysical Journal Letters, marking a significant advancement in understanding the mechanisms behind binary black hole formation and evolution [1] Group 1 - The international gravitational wave detection collaboration has observed over 100 gravitational wave events since the first detection in 2015, with most originating from binary black hole mergers, which are crucial for understanding the physical processes involved [1] - The research team previously proposed a bold scientific hypothesis in 2018, suggesting that a supermassive black hole and a stellar-mass binary black hole could form a "trio," where the binary black holes are influenced by the supermassive black hole's gravity, leading to gravitational wave emissions [1][2] - The LISA gravitational wave detection plan has included this "trio" system in its white paper, and it has been recognized as a unique wave source by China's space gravitational wave detection program [1] Group 2 - The research focused on the gravitational wave event GW190814, which features two black holes with a mass difference of nearly ten times, suggesting they may have formed as part of a "trio" with a supermassive black hole [2] - The team identified that if binary black holes merge near a third dense body, their orbital motion would produce a line-of-sight acceleration, altering the gravitational wave frequency through the Doppler effect, leaving a unique "signature" in the signal [2] - This discovery marks the first clear indication of a third dense body in a binary black hole merger event, implying that the binary black holes may not have formed in isolation but within a more complex gravitational system, which is significant for revealing the channels of binary black hole formation [2]