Supermassive black holes formed by direct collapse of inflationary perturbations
arXiv:1609.02245 · doi:10.1103/PhysRevD.94.103522
Abstract
We propose a mechanism of producing a new type of primordial perturbations that collapse to primordial black holes whose mass can be as large as necessary for them to grow to the supermassive black holes observed at high redshifts, without contradicting COBE/FIRAS upper limits on cosmic microwave background (CMB) spectral distortions. In our model, the observable Universe consists of two kinds of many small patches which experienced different expansion histories during inflation. Primordial perturbations large enough to form primordial black holes are realized on patches that experienced more Hubble expansion than the others. By making these patches the minor component, the rarity of supermassive black holes can be explained. On the other hand, most regions of the Universe experienced the standard history and, hence, only have standard almost-scale-invariant adiabatic perturbations confirmed by observations of CMB or large-scale structures of the Universe. Thus, our mechanism can evade the constraint from the nondetection of the CMB distortion set by the COBE/FIRAS measurement. Our model predicts the existence of supermassive black holes even at redshifts much higher than those observed. Hence, our model can be tested by future observations peeking into the higher-redshift Universe.
30 pages, 11 figures, accepted in PRD
References in corpus (19)
- A luminous quasar at a redshift of z = 7.085
- An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
- Four quasars above redshift 6 discovered by the Canada-France High-z Quasar Survey
- Gemini Near-infrared Spectroscopy of Luminous z~6 Quasars: Chemical Abundances, Black Hole Masses, and MgII Absorption
- Black hole masses and enrichment of z ~ 6 SDSS quasars
- A Survey of z~6 Quasars in the SDSS Deep Stripe: I. a Flux-Limited Sample at z_{AB}<21
- Primordial black hole formation from an axion-like curvaton model
- Primordial seeds of supermassive black holes
- Curvature profiles as initial conditions for primordial black hole formation
- Testing scenarios of primordial black holes being the seeds of supermassive black holes by ultracompact minihalos and CMB -distortions
- Discovery of eight z ~ 6 quasars from Pan-STARRS1
- Single-field inflation, anomalous enhancement of superhorizon fluctuations, and non-Gaussianity in primordial black hole formation
- Silk damping at a redshift of a billion: a new limit on small-scale adiabatic perturbations
- Formation of intermediate-mass black holes as primordial black holes in the inflationary cosmology with running spectral index
- Generating Primordial Black Holes Via Hilltop-Type Inflation Models
- Self-consistent initial conditions for primordial black hole formation
- The double formation of primordial black holes
- No quasi-stable scalaron lump forms after inflation
- Primordial black holes from temporally enhanced curvature perturbation
Cited by in corpus (10)
- Primordial Black Holes as Dark Matter: Recent Developments
- Gravitational Wave signatures of inflationary models from Primordial Black Hole Dark Matter
- Stochastic gravitational waves associated with the formation of primordial black holes
- Accelerating early massive galaxy formation with primordial black holes
- Primordial black holes from inflaton and spectator field perturbations in a matter-dominated era
- Primordial black hole formation by vacuum bubbles II
- Ultracompact minihalos associated with stellar-mass primordial black holes
- Strong clustering of primordial black holes from Affleck-Dine mechanism
- primordial black holes and string axion dark matter
- Primordial Black Holes from Spatially Varying Cosmological Constant Induced by Field Fluctuations in Extra Dimensions