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Multi-messenger astronomy with black holes: tidal disruption events
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This chapter provides an overview of tidal disruption events, aiming to provide an overview of both the theoretical and the observational state of the field, with the overarching goal of introducing them as tools to indirectly observe massive black holes in the Universe. We start by introducing the relevant theoretical concepts, physical scales and timescales with an emphasis on the classical framework and how this has been (and continues to be) improved since the inception of the field. We then cover the current and future prospects of observing TDEs through a variety of messengers, including photons across the electromagnetic spectrum, as well as gravitational waves and neutrino particles. More recent advancements in the field, including repeating TDEs as well as TDEs by stellar-mass black holes, are also highlighted.
Forward citations
Cited by 2 Pith papers
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Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
High-velocity collisions between main-sequence stars near supermassive black holes should produce bright, fast-fading ultraviolet flares whose light curves and spectra correlate with the collision parameters.
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On the Double: Two Luminous Flares from the Nearby Tidal Disruption Event ASASSN-22ci (AT2022dbl) and Connections to Repeating TDE Candidates
ASASSN-22ci shows two similar TDE flares separated by 720 days, likely from repeated partial disruptions of the same star, with the next flare predicted for early February 2026.
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