A hybrid simulation of gravitational wave production in first-order phase transitions

DOI10.1088/1475-7516/2021/04/014zbMath1485.83146arXiv2010.00971OpenAlexW3091064703MaRDI QIDQ5026096

Thomas Konstandin, Henrique Rubira, Ryusuke Jinno

Publication date: 7 February 2022

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

Full work available at URL: https://arxiv.org/abs/2010.00971

zbMATH Keywords

physics of the early universecosmological phase transitionsprimordial gravitational waves (theory)gravitational waves/sources

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Electromagnetic interaction; quantum electrodynamics (81V10) Hydro- and aero-acoustics (76Q05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Weak interaction in quantum theory (81V15) Statistical mechanics of plasmas (82D10) Liquid-gas two-phase flows, bubbly flows (76T10) Kinetic theory of gases in equilibrium statistical mechanics (82B40) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (6)

Higgsless simulations of cosmological phase transitions and gravitational waves ⋮ Effect of density fluctuations on gravitational wave production in first-order phase transitions ⋮ Detection of early-universe gravitational-wave signatures and fundamental physics ⋮ Model-independent bubble wall velocities in local thermal equilibrium ⋮ Electroweak bubble wall expansion: gravitational waves and baryogenesis in standard model-like thermal plasma ⋮ Gravitational waves from bubble collisions in FLRW spacetime

Uses Software

• FFTW

Cites Work

• New high-resolution central schemes for nonlinear conservation laws and convection-diffusion equations
• Electroweak bubble wall speed limit
• Phase transitions in an expanding universe: stochastic gravitational waves in standard and non-standard histories
• Model-independent energy budget for LISA
• Towards an all-orders calculation of the electroweak bubble wall velocity
• Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
• Gravitational waves from first-order phase transitions: ultra-supercooled transitions and the fate of relativistic shocks
• Model-independent energy budget of cosmological first-order phase transitions—A sound argument to go beyond the bag model
• Weak solutions of nonlinear hyperbolic equations and their numerical computation
• Symmetric hyperbolic linear differential equations
• Gravitational waves from bubble dynamics: beyond the envelope
• Where does the hot electroweak phase transition end?

This page was built for publication: A hybrid simulation of gravitational wave production in first-order phase transitions