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Large fluctuations and primordial black holes
In this paper, we review in detail different mechanisms of generation of large primordial
fluctuations and their implications for the production of primordial black holes (PBHs) and …
fluctuations and their implications for the production of primordial black holes (PBHs) and …
[HTML][HTML] PBH formation in EFT of single field inflation with sharp transition
Abstract Using the Effective Field Theory (EFT) framework of single field inflation, we
investigate the possibility of the formation of Primordial Black Holes (PBHs) in the Slow Roll …
investigate the possibility of the formation of Primordial Black Holes (PBHs) in the Slow Roll …
Primordial Black Holes and loops in single-field inflation
Using the δN formalism we calculate the one-loop correction to the large-scale power
spectrum of the curvature perturbation in the standard scenario where primordial black holes …
spectrum of the curvature perturbation in the standard scenario where primordial black holes …
Quantum loop effects on the power spectrum and constraints on primordial black holes
We present a detailed exposition on the prospects of the formation of Primordial Black Holes
(PBHs) during Slow Roll (SR) to Ultra Slow Roll (USR) sharp transitions in the framework of …
(PBHs) during Slow Roll (SR) to Ultra Slow Roll (USR) sharp transitions in the framework of …
No-go for the formation of heavy mass Primordial Black Holes in Single Field Inflation
We examine the possibility of Primordial Black Holes (PBHs) formation in single field models
of inflation. Using the adiabatic or wave function renormalization scheme in the short range …
of inflation. Using the adiabatic or wave function renormalization scheme in the short range …
Galileon inflation evades the no-go for PBH formation in the single-field framework
We consider Galileon inflation in the Effective Field Theory (EFT) framework and examine
the possibility for PBH formation during slow roll (SR) to ultra slow roll (USR) transitions. We …
the possibility for PBH formation during slow roll (SR) to ultra slow roll (USR) transitions. We …
Non-Gaussianities in primordial black hole formation and induced gravitational waves
S Pi - arxiv preprint arxiv:2404.06151, 2024 - arxiv.org
The most promising mechanism of generating PBHs is by the enhancement of power
spectrum of the primordial curvature perturbation, which is usually accompanied by the the …
spectrum of the primordial curvature perturbation, which is usually accompanied by the the …
Numerical 1-loop correction from a potential yielding ultra-slow-roll dynamics
Single-field models of inflation might lead to amplified scalar fluctuations on small scales
due, for example, to a transient ultra-slow-roll phase. It was argued by Kristiano & Yokoyama …
due, for example, to a transient ultra-slow-roll phase. It was argued by Kristiano & Yokoyama …
Large approach to single field inflation
G Tasinato - Physical Review D, 2023 - APS
Single field models of inflation capable of producing primordial black holes usually require a
significant departure from the standard, perturbative slow-roll regime. In fact, in many of …
significant departure from the standard, perturbative slow-roll regime. In fact, in many of …
[HTML][HTML] Primordial non-Gaussianity as a saviour for PBH overproduction in SIGWs generated by Pulsar Timing Arrays for Galileon inflation
We investigate the explicit role of negative local non-Gaussianity, f NL, in suppressing the
abundance of primordial black holes (PBHs) in the single-field model of Galileon inflation …
abundance of primordial black holes (PBHs) in the single-field model of Galileon inflation …