Hubble-induced phase transitions: Walls are not forever

DOI10.1088/1475-7516/2020/01/002zbMath1489.83072arXiv1911.03484OpenAlexW3103315090MaRDI QIDQ5067787

Javier Rubio, Dario Bettoni

Publication date: 4 April 2022

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

Full work available at URL: https://arxiv.org/abs/1911.03484

zbMATH Keywords

inflationmonopolesdomain wallscosmic stringsphysics of the early universecosmological phase transitions

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Geometrodynamics and the holographic principle (83E05) Symmetry breaking in quantum theory (81R40) Classical and relativistic thermodynamics (80A10) Dynamic and nonequilibrium phase transitions (general) in statistical mechanics (82C26) Surgery obstructions, Wall groups (57R67) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)

Related Items (7)

Palatini R ² quintessential inflation ⋮ Boosting ultraviolet freeze-in in NO models ⋮ Primordial dark matter from curvature induced symmetry breaking ⋮ Gravitational shine of dark domain walls ⋮ From Hubble to bubble ⋮ Hubble-induced phase transitions on the lattice with applications to Ricci reheating ⋮ Phase transitions in an expanding universe: stochastic gravitational waves in standard and non-standard histories

Cites Work

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• Quantum-to-classical transition of cosmological perturbations for non-vacuum initial states
• Warm Little Inflaton becomes dark energy
• Warm quintessential inflation
• Emergence of classicality for primordial fluctuations: Concepts and analogies
• Semiclassicality and decoherence of cosmological perturbations
• Non-minimal gravitational reheating during kination
• Ricci reheating
• Ability of LIGO and LISA to probe the equation of state of the early Universe
• Gravitational waves from global cosmic strings in quintessential inflation
• False vacuum decay after inflation

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