Primordial Black Holes in Induced Gravity Inflationary Models with Two Scalar Fields
arXiv:2407.00999 · doi:10.1134/S1063779624701934
Abstract
We propose a two-field inflationary model with the induced gravity term. Using conformal transformation of the metric, we get the chiral cosmological model with two scalar fields. We demonstrate that the constructed inflationary model does not contradict to the recent observation data and is suitable for primordial black hole (PBH) formation. The estimation of PBH masses allows to consider PBHs as dark matter candidates.
arXiv comment11 pages, 2 figures, v2: a table and references added, to appear in Physics of Particles and Nuclei
References in corpus (39)
- The Standard Model Higgs boson as the inflaton
- Primordial Black Holes as Dark Matter: Recent Developments
- Density Perturbations and Black Hole Formation in Hybrid Inflation
- Primordial Black Holes as a dark matter candidate
- Primordial Black Holes
- Higgs inflation: consistency and generalisations
- Running Inflation in the Standard Model
- Inflation scenario via the Standard Model Higgs boson and LHC
- Scalaron from -gravity as a Heavy Field
- Induced gravity inflation in the standard model of particle physics
- Jordan Frame Supergravity and Inflation in NMSSM
- Generating PBHs and small-scale GWs in two-field models of inflation
- The Higgs field as an inflaton
- Higgs boson, renormalization group, and naturalness in cosmology
- Inflation and Primordial Black Holes
- Quantum scale of inflation and particle physics of the early universe
- Renormalization-Group Improved Effective Lagrangian for Interacting Theories in Curved Spacetime
- Multifield Dynamics of Higgs Inflation
- Non-Canonical Inflation and Primordial Black Holes Production
- Updated constraints on amplitude and tilt of the tensor primordial spectrum
- Primordial Black Holes from Multifield Inflation with Nonminimal Couplings
- Hybrid -attractors, primordial black holes and gravitational wave backgrounds
- On the geometrical interpretation of scale-invariant models of inflation
- Primordial black hole dark matter in dilaton-extended two-field Starobinsky inflation
- Renormalization-group inflationary scalar electrodynamics and SU(5) scenarios confronted with Planck2013 and BICEP2 results
- Massive and supermassive black holes in the contemporary and early universe and the new problems of cosmology and astrophysics
- Primordial black holes and gravitational waves from nonminimally coupled supergravity inflation
- Cosmological attractor inflation from the RG-improved Higgs sector of finite gauge theory
- The Inflaton that Could : Primordial Black Holes and Second Order Gravitational Waves from Tachyonic Instability induced in Higgs- Inflation
- Superpotential method for chiral cosmological models connected with modified gravity
- Natural Inflation in SUSY and Gauge-Mediated Curvature of the Flat Directions
- Exact and slow-roll solutions for exponential power-law inflation connected with f(R) gravity and observational constraints
- Asymptotically Safe Non-Minimal Inflation
- Improved model of primordial black hole formation after Starobinsky inflation
- MSSM-inspired multifield inflation
- Superpotential method and the amplification of inflationary perturbations
- Reconstruction methods and the amplification of the inflationary spectrum
- Induced Gravity and Quantum Cosmology
- Renormalization-group improved inflationary scenarios