The post-inflationary cosmology of the VISH$\nu$ axion-majoron model

TL;DR

This paper explores the cosmological implications of the VISH axion-majoron model, detailing reheating, leptogenesis, gravitational waves, and phenomenological distinctions, to address fundamental issues in the Standard Model.

Contribution

It provides a detailed, lattice-informed analysis of the reheating era in the VISH model, refining inflationary and leptogenesis predictions and ensuring consistency with dark radiation constraints.

Findings

Reheating scenarios compatible with naturalness and dark radiation bounds.

Precise estimates of reheating temperature and expansion history.

Characterization of the high-frequency gravitational wave spectrum.

Abstract

It was previously shown how several explanatory deficiencies of the Standard Model (including the origin of dark matter, matter-antimatter asymmetry, small active neutrino mass, strong CP-conservation and the seeds for large-scale structure formation) may be economically resolved when an experimentally-accessible QCD axion also plays the role of the majoron, and the scalar partner of the axion is dynamical during inflation. In this paper, we complete this general study of the cosmological history for a unit domain-wall number option of the DFSZ-type, dubbed VISH$\nu$, by performing a detailed lattice-informed analysis of the reheating era. In doing so, we make inflationary and leptogenesis predictions more precise through estimates of the reheating temperature and the expansion history. The viable reheating scenarios, which at the same time satisfy strict conditions for naturalness (radiative stability), are also shown to respect dark radiation bounds. We also characterise the high-frequency spectrum of gravitational waves, and mention other phenomenological implications that distinguish VISH$\nu$ from alternative proposals.