Rates of Stellar Tidal Disruption

N. C. Stone; E. Vasiliev; M. Kesden; E. M. Rossi; H. B. Perets; P. Amaro-Seoane

doi:10.1007/s11214-020-00651-4

Rates of Stellar Tidal Disruption

N. C. Stone^*, E. Vasiliev, M. Kesden, E. M. Rossi, H. B. Perets, P. Amaro-Seoane

^*Corresponding author for this work

Racah Institute of Physics

Research output: Contribution to journal › Review article › peer-review

74 Scopus citations

Abstract

Tidal disruption events occur rarely in any individual galaxy. Over the last decade, however, time-domain surveys have begun to accumulate statistical samples of these flares. What dynamical processes are responsible for feeding stars to supermassive black holes? At what rate are stars tidally disrupted in realistic galactic nuclei? What may we learn about supermassive black holes and broader astrophysical questions by estimating tidal disruption event rates from observational samples of flares? These are the questions we aim to address in this Chapter, which summarizes current theoretical knowledge about rates of stellar tidal disruption, and compares theoretical predictions to the current state of observations.

Original language	English
Article number	35
Journal	Space Science Reviews
Volume	216
Issue number	3
DOIs	https://doi.org/10.1007/s11214-020-00651-4
State	Published - 1 Apr 2020

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© 2020, Springer Nature B.V.

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Rates of Stellar Tidal Disruption

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