Angular correlation as a novel probe of supermassive primordial black holes
arXiv:2103.13692 · doi:10.1103/PhysRevD.104.023526
Abstract
We investigate the clustering property of primordial black holes (PBHs) in a scenario where PBHs can explain the existence of supermassive black holes (SMBHs) at high redshifts. We analyze the angular correlation function of PBHs originating from fluctuations of a spectator field which can be regarded as a representative model to explain SMBHs without conflicting with the constraint from the spectral distortion of cosmic microwave background. We argue that the clustering property of PBHs can give a critical test for models with PBHs as the origin of SMBHs and indeed show that the spatial distribution of PBHs in such a scenario is highly clustered, which suggests that those models may be disfavored from observations of SMBHs although a careful comparison with observational data would be necessary.
27 pages, 8 figures, References updated and some comments are added
References in corpus (18)
- Laser Interferometer Space Antenna
- Constraints on Primordial Black Holes
- A Luminous Quasar at Redshift 7.642
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- The aftermath of the first stars: massive black holes
- Off the Beaten Path: A New Approach to Realistically Model The Orbital Decay of Supermassive Black Holes in Galaxy Formation Simulations
- Primordial seeds of supermassive black holes
- Testing scenarios of primordial black holes being the seeds of supermassive black holes by ultracompact minihalos and CMB -distortions
- Very high redshift quasars and the rapid emergence of super-massive black holes
- Primordial black holes as biased tracers
- Signatures of non-gaussianity in the isocurvature modes of primordial black hole dark matter
- Supermassive black holes from primordial black hole seeds
- Supermassive black holes formed by direct collapse of inflationary perturbations
- Formation of the first stars and black holes
- Primordial black hole formation by vacuum bubbles II
- Primordial Black Holes from QCD Axion Bubbles
- NANOGrav signal as mergers of Stupendously Large Primordial Black Holes
- Spiky CMB distortions from primordial bubbles
Cited by in corpus (7)
- Primordial Black Holes Arise When The Inflaton Falls
- Gravitational Wave Astronomy With TianQin
- Primordial black holes generated by fast-roll mechanism in non-canonical natural inflation
- Constraints on the abundance of supermassive primordial black holes from lensing of compact radio sources
- Strong clustering of primordial black holes from Affleck-Dine mechanism
- Primordial Black Holes without fine-tuning from a light stochastic spectator field
- Primordial black holes from a curvaton: the role of bimodal distributions