Gravitational waves from bubble walls

DOI10.1088/1475-7516/2021/10/073zbMath1486.83025arXiv2108.05510OpenAlexW3209708161WikidataQ114824780 ScholiaQ114824780MaRDI QIDQ5061931

Ariel Mégevand, Federico Agustín Membiela

Publication date: 14 March 2022

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

Full work available at URL: https://arxiv.org/abs/2108.05510

zbMATH Keywords

physics of the early universecosmological phase transitionsgravitational waves/sources

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Liquid-gas two-phase flows, bubbly flows (76T10) Gravitational waves (83C35) Surgery obstructions, Wall groups (57R67) Collisions in celestial mechanics, regularization (70F16)

Related Items (2)

Detection of early-universe gravitational-wave signatures and fundamental physics ⋮ Thin and thick bubble walls. Part I. Vacuum phase transitions

Cites Work

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• Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
• Model-independent energy budget of cosmological first-order phase transitions—A sound argument to go beyond the bag model
• Gravitational waves from bubble dynamics: beyond the envelope

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