Primordial black holes within Higgs hybrid metric-Palatini approach

TL;DR

This paper explores how primordial black holes could form during the early universe within a Higgs hybrid metric-Palatini framework, showing they might explain dark matter depending on model parameters.

Contribution

It introduces a novel analysis of PBH formation in the Higgs hybrid metric-Palatini model, linking inflationary fluctuations to PBH abundance and dark matter.

Findings

Primordial curvature power spectrum shows significant enhancement at small scales.

PBH abundance can match current dark matter levels depending on model parameters.

Results are consistent with observational constraints.

Abstract

In this paper, we investigate the production of primordial black holes (PBHs) during the radiation-dominated era. The collapse of significant density perturbations originating from large primordial scalar fluctuations generated during inflation can lead to the formation of primordial black holes. In our study, we adopt the Higgs hybrid metric-Palatini model as our framework, in which the inflaton field and the Palatini curvature are non-minimally coupled. To achieve our objective, we analyze the behavior of the primordial curvature power spectrum, which exhibits a large enhancement at small scales corresponding to large wavenumbers $k$. Furthermore, we examine the probability of PBHs formation by studying the mass variance, $\sigma(M_{PBH})$, and the mass fraction of the total energy density collapsing into PBHs, $\beta(M_{PBH})$. The evolution of both functions is consistent with current observational constraints. Finally, we investigate the abundance of primordial black holes as a dark matter candidate. We found that they can account for the totality or a fraction of the current dark matter content, depending primarily on the values of the coupling constant and the e-folds number.