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- W765991331 abstract "In this chapter, we review the literature on ways in which general relativity (GR) can strongly modify aspects of stellar tidal disruption. It is natural to expect that GR should play an important role in TDEs, as these events occur deep in the potential wells of supermassive black holes (SMBHs): for a (10^6 M_{odot}) SMBH, the gravitational radius (R_{rm g}=GM_{rm BH}/c^2) is roughly (1/47) the value of the tidal radius (R_{rm t})." @default.
- W765991331 created "2016-06-24" @default.
- W765991331 creator A5019013125 @default.
- W765991331 date "2014-12-14" @default.
- W765991331 modified "2023-09-26" @default.
- W765991331 title "General Relativistic Effects in Tidal Disruption Flares" @default.
- W765991331 doi "https://doi.org/10.1007/978-3-319-12676-0_6" @default.
- W765991331 hasPublicationYear "2014" @default.
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