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- W1980487825 abstract "In a recent paper, we have shown that the evolution of a misaligned disc around a spinning black hole can result in tearing the disc into many distinct planes. Tearing discs with random orientations produce direct dynamical accretion on to the hole in ≈70 per cent of all cases. Here, we examine the evolution of a misaligned disc around a binary system. We show that these discs are susceptible to tearing for almost all inclinations. We also show that tearing of the disc can result in a significant acceleration of the disc evolution and subsequent accretion on to the binary – by factors up to 104 times that of a coplanar prograde disc with otherwise identical parameters. This provides a promising mechanism for driving mergers of supermassive black hole (SMBH) binaries on time-scales much shorter than a Hubble time. Disc tearing also suggests new observational signatures of accreting SMBH binaries and other systems such as protostellar binaries." @default.
- W1980487825 created "2016-06-24" @default.
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- W1980487825 date "2013-07-30" @default.
- W1980487825 modified "2023-10-12" @default.
- W1980487825 title "Tearing up the disc: misaligned accretion on to a binary" @default.
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- W1980487825 doi "https://doi.org/10.1093/mnras/stt1136" @default.
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