Gravitational waves from first-order phase transitions: ultra-supercooled transitions and the fate of relativistic shocks
From MaRDI portal
Publication:5067130
DOI10.1088/1475-7516/2019/10/033OpenAlexW2942734881MaRDI QIDQ5067130
Masahiro Takimoto, Hyeonseok Seong, Choong Min Um, Ryusuke Jinno
Publication date: 1 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://bib-pubdb1.desy.de/record/426497
Related Items (9)
Gravitational waves from first order cosmological phase transitions in the Sound Shell Model ⋮ Phase transition dynamics and gravitational wave spectra of strong first-order phase transition in supercooled universe ⋮ Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source ⋮ Model-independent energy budget of cosmological first-order phase transitions—A sound argument to go beyond the bag model ⋮ Reflections on bubble walls ⋮ Detection of early-universe gravitational-wave signatures and fundamental physics ⋮ Friction pressure on relativistic bubble walls ⋮ A hybrid simulation of gravitational wave production in first-order phase transitions ⋮ Universal gravitational-wave signatures from heavy new physics in the electroweak sector
Cites Work
- On gauge dependence of gravitational waves from a first-order phase transition in classical scale-invariant \(U(1)^\prime\) models
- QCD-induced electroweak phase transition
- New high-resolution central schemes for nonlinear conservation laws and convection-diffusion equations
- Hearing without seeing: gravitational waves from hot and cold hidden sectors
- The supercooled universe
- Relic gravitational waves from colliding bubbles and cosmic turbulence
- Gravitational waves from first-order phase transitions: towards model separation by bubble nucleation rate
- Electroweak bubble wall speed limit
- Laser interferometry for the Big Bang Observer
- Gravitational waves from conformal symmetry breaking
- Gravitational waves from bubble dynamics: beyond the envelope
- On the maximal strength of a first-order electroweak phase transition and its gravitational wave signal
- Where does the hot electroweak phase transition end?
This page was built for publication: Gravitational waves from first-order phase transitions: ultra-supercooled transitions and the fate of relativistic shocks
