Massive black hole demographics with tidal disruption events
APA
Mummery, A. (2026). Massive black hole demographics with tidal disruption events. Perimeter Institute. https://pirsa.org/26030092
MLA
Mummery, Andrew. Massive black hole demographics with tidal disruption events. Perimeter Institute, Apr. 02, 2026, https://pirsa.org/26030092
BibTex
@misc{ pirsa_PIRSA:26030092,
doi = {10.48660/26030092},
url = {https://pirsa.org/26030092},
author = {Mummery, Andrew},
keywords = {Strong Gravity},
language = {en},
title = {Massive black hole demographics with tidal disruption events},
publisher = {Perimeter Institute},
year = {2026},
month = {apr},
note = {PIRSA:26030092 see, \url{https://pirsa.org}}
}
Andrew Mummery Institute for Advanced Study (IAS)
Abstract
Tidal disruption events — where an unfortunate star is destroyed by a previously quiescent supermassive black hole — offer a unique probe of the low mass end of the supermassive black hole population. Recent observational advances have lead to the discovery of ~100 such events, many of which are comprehensively followed up across the entire electromagnetic spectrum. I will discuss how time-dependent relativistic accretion theory can be used to understand this multi wavelength emission from optical through X-ray energies, and how this theory allows tidal disruption events to act as probes of the massive black hole population. I will present current constraints on the occupation fraction of intermediate mass black holes, and look forward to what can be expected in the LSST era.