Quasi-periodic eruptions: new transient probes of stars near supermassive black holes
…several in accretion discs created by tidal disruption even
Fri, Oct 23, 2026 · 21:00 UTC
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…several in accretion discs created by tidal disruption even
Fri, Oct 23, 2026 · 21:00 UTC
Shane Davis presents simulations of stellar disruption and the subsequent return of debris to a black hole. Observed light curves and spectra offer tests of accretion physics and black-hole spacetime, but interpreting them requires accounting for strong radiation forces during rapid fallback. Using Athena++ and AthenaK, the research models radiation transfer, including recent calculations in Kerr spacetime. Although the debris circularizes slowly, shocks involving the returning stream and an eccentric disk dominate early energy release and angular-momentum transport. Radiation drives unbound
Tue, Sep 22, 2026 · 15:00 UTC
…explains how observations of these tidal-disruption events reveal otherwise difficult-to-observe aspects of black-hole growth.
Mon, Jan 10, 2022 · 16:45 UTC