Model-dependent analysis method for energy budget of the cosmological first-order phase transition

DOI10.1088/1475-7516/2023/07/006zbMath1528.83172arXiv2301.12328OpenAlexW4383067266MaRDI QIDQ6116497

Xiao Wang, Fa Peng Huang, Chi Tian

Publication date: 18 July 2023

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

Full work available at URL: https://arxiv.org/abs/2301.12328

zbMATH Keywords

cosmology of theories beyond the SMphysics of the early universecosmological phase transitionsgravitational waves/theory

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Signal detection and filtering (aspects of stochastic processes) (60G35) Geometrodynamics and the holographic principle (83E05) Hydro- and aero-acoustics (76Q05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Gravitational waves (83C35)

Cites Work

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• Model-independent energy budget for LISA
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• The timestep constraint in solving the gravitational wave equations sourced by hydromagnetic turbulence
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• On the wall velocity dependence of electroweak baryogenesis
• Model-independent energy budget of cosmological first-order phase transitions—A sound argument to go beyond the bag model
• Bubble wall velocities in local equilibrium
• A sonic boom in bubble wall friction
• Detecting the cosmic gravitational wave background with the Big Bang Observer
• On the maximal strength of a first-order electroweak phase transition and its gravitational wave signal

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