Primordial black holes and gravitational waves from nonminimally coupled supergravity inflation

TL;DR

This paper investigates how nonminimally coupled supergravity inflation models can produce primordial black holes and gravitational waves, potentially explaining dark matter and offering detectable signals for future observatories.

Contribution

It introduces a supersymmetric model with multiple scalar fields analyzing primordial black hole formation and gravitational wave spectra, linking inflationary parameters to observable phenomena.

Findings

Primordial black holes could account for a significant fraction of dark matter.

Gravitational wave spectra are within reach of future detection.

Parameter regions identified for copious black hole production.

Abstract

We study the formation of primordial black holes and the generation of gravitational waves in a class of cosmological models that are direct supersymmetric analogs of the observationally favored nonminimally coupled Higgs inflation model. It is known that this type of model naturally includes multiple scalar fields which may be regarded as the inflaton. For the sake of simplicity we focus on the case where the inflaton field space is two dimensional. We analyze the multifield dynamics and find the region of parameters that gives copious production of primordial black holes that may comprise a significant part of the present dark matter abundance. We also compute the spectrum of the gravitational waves and discuss their detectability by means of future ground-based and space-borne gravitational wave observatories.