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Axion isocurvature perturbations in low-scale models of hybrid inflation

2018/06/30 by Kai Schmitz, Tsutomu T. Yanagida · 1 citation
Physics and Astronomy · #Anisotropy #Axion #Cosmic microwave background #Cosmic string #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Grand Unified Theory #Gravitino #Hidden sector #Inflation (cosmology) #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum chromodynamics #Quantum mechanics #String (physics) #Strong CP problem #Supergravity #Supersymmetry #Supersymmetry breaking #Theoretical physics #astro-ph.CO #hep-ph #hep-th

paper · pdf · doi:10.1103/physrevd.98.075003

published as Phys. Rev. D 98, 075003 (2018) · 40 pages + references, 5 figures, 1 table. v2: typos removed, updated references. v3: matches version published in PRD

openalex publication_date 2018/10/02 · arxiv created 2018/10/10 · arxiv updated 2018/10/11 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The quantum chromodynamics (QCD) axion solves the strong CP problem and represents an attractive particle candidate for cold dark matter (CDM). However, quantum fluctuations of the axion field during inflation easily result in large CDM isocurvature perturbations that are in conflict with observations of the cosmic microwave background. In this paper, we demonstrate how this problem can be solved in low-scale models of hybrid inflation that may emerge from supersymmetric grand unified theories. We consider both F-term hybrid inflation and D-term hybrid inflation in supergravity, explicitly taking into account the effect of hidden-sector supersymmetry breaking. We discuss the production of cosmic strings and show how the soft terms in the scalar potential readily allow us to achieve the correct scalar spectral index. In both cases, we are able to identify large regions in parameter space that are consistent with all constraints. In particular, we find that evading the CDM isocurvature constraint always requires a small Yukawa or gauge coupling of O(10^\ensuremath-3) or smaller. This translates into upper bounds on the gravitino mass of O(105) GeV in F-term hybrid inflation and O(109) GeV in D-term hybrid inflation. Our results point to interesting scenarios in well-motivated parameter regions that will be tested in future axion and cosmic microwave background experiments.

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