Primordial black holes and secondary gravitational waves from generalized power-law non-canonical inflation with quartic potential
Soma Heydari, Kayoomars Karami

TL;DR
This paper explores how a generalized power-law non-canonical inflation model with a quartic potential can produce primordial black holes and secondary gravitational waves consistent with observations, satisfying swampland criteria.
Contribution
It introduces a novel non-canonical inflation framework with a peaked mass scale parameter that enhances small-scale perturbations and generates PBHs and GWs matching observational data.
Findings
PBHs can explain LIGO-VIRGO events, microlensing, and dark matter.
The model satisfies latest observational and swampland constraints.
The gravitational wave spectrum exhibits a specific power-law behavior in the infrared.
Abstract
Here, generation of PBHs and secondary GWs from non-canonical inflation with quartic potential have been probed. It is illustrated that, quartic potential in non-canonical setup with a generalized power-law Lagrangian density can source a consistent inflationary era with the latest observational data. Besides, we show that our model satisfies the swampland criteria. At the same time, defining a peaked function of inflaton field as non-canonical mass scale parameter of the Lagrangian, gives rise to slow down the inflaton in a while. In this span, namely Ultra-Slow-Roll (USR) stage, the amplitude of the curvature perturbations on small scales enlarges versus CMB scales. It has been illustrated that, further to the peaked aspect of the chosen non-canonical mass scale parameter, the amount of parameter of the Lagrangian has enlarging impact on the amplitude of the scalar…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Black Holes and Theoretical Physics
