Mechanism for the Suppression of Intermediate-Mass Black Holes
arXiv:1010.5325 · doi:10.1134/S1063773710110022
Abstract
A model for the formation of supermassive primordial black holes in galactic nuclei with the simultaneous suppression of the formation of intermediate-mass black holes is presented. A bimodal mass function for black holes formed through phase transitions in a model with a "Mexican hat" potential has been found. The classical motion of the phase of a complex scalar field during inflation has been taken into account. Possible observational manifestations of primordial black holes in galaxies and constraints on their number are discussed.
arXiv comment12 pages, 2 figures
References in corpus (21)
- Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research
- Intermediate-Mass Black Holes
- Gemini and Hubble Space Telescope Evidence for an Intermediate Mass Black Hole in omega Centauri
- New Limits on an Intermediate Mass Black Hole in Omega Centauri: II. Dynamical Models
- A 20 Thousand Solar Mass Black Hole in the Stellar Cluster G1
- Primordial Structure of Massive Black Hole Clusters
- Growth of structure seeded by primordial black holes
- X-ray observations of ultraluminous X-ray sources
- A Dynamical Model for the Globular Cluster G1
- Inhomogeneous baryogenesis, cosmic antimatter, and dark matter
- Multiple black holes in galactic bulges
- Massive black hole remnants of the first stars in galactic haloes
- The surface density profile of NGC 6388: a good candidate for harboring an intermediate-mass black hole
- Calculation of Particle Production by Nambu Goldstone Bosons with Application to Inflation Reheating and Baryogenesis
- Accretion Rates and Beaming in Ultraluminous X-ray Sources
- Constraints on Galactic Intermediate Mass Black Holes
- Ultra-Luminous X-ray Sources: Evidence for Very Efficient Formation of Population III Stars Contributing to the Cosmic Near-Infrared Background Excess?
- Early formation of galaxies initiated by clusters of primordial black holes
- Origin of Correlations between Central Black Holes Masses and Galactic Bulge Velocity Dispersions
- Growth of Intermediate Massive Black Holes in the Hierarchical Formation of Small Spiral Galaxies in the High-z Universe
- Gravitational Wave Bursts from Collisions of Primordial Black Holes in Clusters
Cited by in corpus (6)
- Clusters of primordial black holes
- Classical transitions with the topological number changing in the early Universe
- Clusters of Black Holes as Point-Like Gamma-ray Sources
- Transitions between topologically non-trivial configurations
- On mass spectra of primordial black holes
- A trial to understand the supersymmetry relations through extension of the second quantized fermion and boson fields, either to strings or to odd dimensional spaces