Gravitational wave background from non-Abelian reheating after axion-like inflation

DOI10.1088/1475-7516/2022/05/021zbMath1505.83005arXiv2201.02317OpenAlexW4221150304WikidataQ114824724 ScholiaQ114824724MaRDI QIDQ5099300

S. Procacci, P. Klose, Mikko Laine

Publication date: 31 August 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2201.02317

zbMATH Keywords

inflationaxionsparticle physics-cosmology connectionprimordial gravitational waves (theory)

Mathematics Subject Classification ID

Other elementary particle theory in quantum theory (81V25) Geometrodynamics and the holographic principle (83E05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Gravitational waves (83C35) Collision of rigid or pseudo-rigid bodies (70F35) Bosonic systems in quantum theory (81V73)

Related Items (4)

Shapes of non-Gaussianity in warm inflation ⋮ Maximal temperature of strongly-coupled dark sectors ⋮ Shape of the hot topological charge density spectral function ⋮ Gravitational wave background from vacuum and thermal fluctuations during axion-like inflation

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