The Physics of Accretion Discs, Winds And Jets in Tidal Disruption Events
arXiv:2101.05195 · doi:10.1007/s11214-020-00747-x
Abstract
Accretion onto black holes is an efficient mechanism in converting the gas mass-energy into energetic outputs as radiation, wind and jet. Tidal disruption events, in which stars are tidally torn apart and then accreted onto supermassive black holes, offer unique opportunities of studying the accretion physics as well as the wind and jet launching physics across different accretion regimes. In this review, we systematically describe and discuss the models that have been developed to study the accretion flows and jets in tidal disruption events. A good knowledge of these physics is not only needed for understanding the emissions of the observed events, but also crucial for probing the general relativistic space-time around black holes and the demographics of supermassive black holes via tidal disruption events.
Accepted for publication in Springer Space Science Reviews. Chapter in ISSI review, "The Tidal Disruption of Stars by Massive Black Holes," vol. 79
References in corpus (32)
- Super-critically accreting stellar-mass black holes as ultraluminous X-ray sources
- An ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core
- A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies
- A Global Three Dimensional Radiation Magneto-hydrodynamic Simulation of Super-Eddington Accretion Disks
- Global General Relativistic MHD Simulation of a Tilted Black-Hole Accretion Disk
- Stellar disruption by a supermassive black hole: is the light curve really proportional to ?
- Time Dependent Monte Carlo Radiative Transfer Calculations For 3-Dimensional Supernova Spectra, Lightcurves, and Polarization
- General Relativistic Hydrodynamic Simulation of Accretion Flow from a Stellar Tidal Disruption
- Alignment of Magnetized Accretion Disks and Relativistic Jets with Spinning Black Holes
- Semi-implicit scheme for treating radiation under M1 closure in general relativistic conservative fluid dynamics codes
- Accretion Discs with Strong Toroidal Magnetic Fields
- X-ray Brightening and UV Fading of Tidal Disruption Event ASASSN-15oi
- Warp diffusion in accretion discs: a numerical investigation
- A 200-s Quasi-Periodicity Following the Tidal Disruption of a Star by a Dormant Black Hole
- A likely decade-long sustained tidal disruption event
- Ultrafast Outflow in Tidal Disruption Event ASASSN-14li
- The spectral evolution of disc dominated tidal disruption events
- Tidal disruptions by rotating black holes: effects of spin and impact parameter
- Disk Winds as an Explanation for Slowly Evolving Temperatures in Tidal Disruption Events
- Discovery of Highly Blueshifted Broad Balmer and Metastable Helium Absorption Lines in a Tidal Disruption Event
- Disk origin of broad optical emission lines of the TDE candidate PTF09djl
- Tidal Disruption and Magnetic Flux Capture: Powering a Jet from a Quiescent Black Hole
- Frame-dragging, disk warping, jet precessing, and dipped X-ray lightcurve of Sw J1644+57
- Simulations of Magnetic Fields in Tidally-Disrupted Stars
- Local and global dynamics of eccentric astrophysical discs
- Papaloizou-Pringle instability suppression by the magnetorotational instability in relativistic accretion discs
- Hydrodynamic instability in eccentric astrophysical discs
- Scale-invariant radio jets and varying black hole spin
- Tidal Disruption Event Disks around Supermassive Black Holes: Disk Warp and Inclination Evolution
- Spin Evolution of Supermassive Black Holes and Galactic Nuclei
- On the Papaloizou-Pringle instability in tidal disruption events
- On the formation of a quasi-stationary twisted disc after a tidal disruption event