Composite Hybrid Inflation : Primordial Black Holes and Stochastic Gravitational Waves

TL;DR

This paper explores how composite hybrid inflation models can produce primordial black holes and stochastic gravitational waves, with their properties influenced by the theory's anomalous dimensions, potentially detectable by future observatories.

Contribution

It introduces a novel inflationary scenario based on effective chiral Lagrangians with walking dynamics, linking black hole and gravitational wave signatures to anomalous dimensions.

Findings

Primordial black hole mass is inversely related to anomalous dimensions.

Gravitational wave frequency increases with larger anomalous dimensions.

Predicted signals are within reach of upcoming gravitational wave detectors.

Abstract

We investigate the production of primordial black holes and gravitational waves in composite hybrid inflation. Starting from an effective chiral Lagrangian with a dilaton and pions, we identify inflation occurring due to the walking dynamics of the theory. A $\mathbb{Z}_2$ symmetry-breaking term in the pion sector induces a shift in the inflaton's trajectory, which leads to a tachyonic instability phase. Curvature perturbations grow exponentially, producing copious primordial black holes and a stochastic gravitational wave background. We show that the primordial black hole mass and the gravitational wave frequency are strongly restricted by the anomalous dimensions of the pion operators, with larger anomalous dimensions giving lighter primordial black holes and higher frequency gravitational waves. In both cases, the associated signatures lie within reach of future gravitational wave observatories.