The first supermassive black holes
arXiv:1703.03083 · doi:10.1093/astrogeo/atx099
Abstract
We briefly review the historical development of the ideas regarding the first supermassive black hole seeds, the physics of their formation and radiative feedback, recent theoretical and observational progress, and our outlook for the future.
Invited review, Astronomy & Geophysics, 6 pages, 6 figures, updated to reflect the printed version
References in corpus (16)
- A luminous quasar at a redshift of z = 7.085
- Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
- An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
- Formation of z ~ 6 quasars from hierarchical galaxy mergers
- The Formation of the First Stars II. Radiative Feedback Processes and Implications for the Initial Mass Function
- Rapid growth of seed black holes in the early universe by supra-exponential accretion
- The aftermath of the first stars: massive black holes
- The Birth of a Galaxy. II. The Role of Radiation Pressure
- Identification of the brightest Lyα emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era
- How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes
- The Lyman-alpha signature of the first galaxies
- The suppression of direct collapse black hole formation by soft X-ray irradiation
- Lyman Alpha Driven Outflows Around Star Forming Galaxies
- Lyman-alpha radiation hydrodynamics of galactic winds before cosmic reionization
- The nature of the Lyman Alpha Emitter CR7: a persisting puzzle
- Metallicity evolution of direct collapse black hole hosts: CR7 as a case study
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- Radio jets from AGN in dwarf galaxies in the COSMOS survey: mechanical feedback out to redshift 3.4
- Signatures of primordial black holes as seeds of supermassive black holes
- Supermassive Black Holes in the Early Universe
- The first measurement of the quasar lifetime distribution
- Magnetorotational Collapse of Supermassive Stars: Black Hole Formation, Gravitational Waves and Jets
- Radiative effects during the assembly of direct collapse black holes
- The seeds of supermassive black holes and the role of local radiation and metal spreading
- Discrete diffusion Lyman-alpha radiative transfer
- Gravitational Waves from Disks Around Spinning Black Holes: Simulations in Full General Relativity
- Simulating the Magnetorotational Collapse of Supermassive Stars: Incorporating Gas Pressure Perturbations and Different Rotation Profiles
- Rapid formation of black holes in galaxies: a self-limiting growth mechanism
- On the effect of Lyman alpha trapping during the initial collapse of massive black hole seeds
- Extreme Primordial Star Formation Enabled by High Redshift Quasars
- Does our universe conform with the existence of a universal maximum energy-density ?
- High-redshift quasar selection from the CFHQSIR survey
- The GLEAMing of the first supermassive black holes: II. A new sample of high-redshift radio galaxy candidates
- Maximally Rotating Supermassive Stars at the Onset of Collapse: Effects of Gas Pressure
- Effect of magnetic fields on the dynamics and gravitational wave emission of PPI-saturated self-gravitating accretion disks: simulations in full GR
- AGN radiative feedback in the early growth of massive black holes
- Back to basics: Little Red Dots as galaxies and dust-obscured AGNs in a synthetic NIRCam sky simulated with L-GalaxiesBH
- Identification of Candidate Halos Hosting Massive Black Hole Seeds in the Simulations with Support Vector Machines
- A Simple Condition for Sustained Super-Eddington Black Hole Growth