Primordial black holes and Scalar-Induced Gravitational Waves formed by inflation potential with non-trivial characteristics

Fuente: arXiv
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Main Authors: Zheng, Ruifeng, Xu, Yanqing
Format: Preprint
Published: 2026
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author Zheng, Ruifeng
Xu, Yanqing
author_facet Zheng, Ruifeng
Xu, Yanqing
contents The formation of primordial black holes (PBHs) generally requires large density perturbations, which is widely supported by researchers. This paper studies the local coupling properties of the Starobinsky and Kachru-Kallosh-Linde-Trivedi (KKLT) potentials by introducing a linear Lorentzian-type coupling, which locally breaks the slow-roll conditions. We find that both positive and negative couplings can generate a considerable abundance of PBH. Additionally, we study the scalar-induced gravitational waves (SIGWs) generated by this model.
format Preprint
id arxiv_https___arxiv_org_abs_2601_21538
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Primordial black holes and Scalar-Induced Gravitational Waves formed by inflation potential with non-trivial characteristics
Zheng, Ruifeng
Xu, Yanqing
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
The formation of primordial black holes (PBHs) generally requires large density perturbations, which is widely supported by researchers. This paper studies the local coupling properties of the Starobinsky and Kachru-Kallosh-Linde-Trivedi (KKLT) potentials by introducing a linear Lorentzian-type coupling, which locally breaks the slow-roll conditions. We find that both positive and negative couplings can generate a considerable abundance of PBH. Additionally, we study the scalar-induced gravitational waves (SIGWs) generated by this model.
title Primordial black holes and Scalar-Induced Gravitational Waves formed by inflation potential with non-trivial characteristics
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2601.21538