Dynamics and radiation from tidal disruption events

Leiden Repository

Dynamics and radiation from tidal disruption events

Type: Doctoral Thesis
Title: Dynamics and radiation from tidal disruption events
Author: Bonnerot, C.A.
Issue Date: 2017-10-05
Keywords: Tidal disruption events
Black hole physics
Accretion
Galactic nuclei
Magnetohydrodynamics
Abstract: When a star gets too close to a supermassive black hole, it is torn apart by strong tidal forces in a tidal disruption event (TDE). The stellar matter then fuels the compact object causing a bright flare that is a unique probe of the majority of galactic nuclei, otherwise quiescent. For example, the black hole properties can be estimated from this signal. In my thesis, I used analytical and numerical methods to shed light on the TDE dynamics and associated emission, a required step to optimally exploit this powerful predictive potential. I carried out a numerical study of the accretion disc formation from the stellar debris. The results strongly challenged previous assumptions, showing that this process can be slower and result in a more extended gas distribution than previously thought. In addition, I analytically demonstrated that disc formation can be accelerated if the stellar matter is significantly magnetized. I then highlighted the impact of hydrodynamical instabilities on the debris that can cause an efficient mixing with the surrounding gas, likely dimming the associated flare. Finally, I numerically studied the disruption of magnetized stars, proving that it can produce a thick debris distribution or result in a magnetically amplified remnant.
Promotor: Supervisor: Joop Schaye Co-Supervisors: Elena Maria Rossi; Giuseppe Lodato
Faculty: Science
University: Leiden
Uri: urn:isbn:9789462337312
Handle: http://hdl.handle.net/1887/56249
 

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