Effect of density fluctuations on gravitational wave production in first-order phase transitions

DOI10.1088/1475-7516/2021/12/019zbMath1487.83020arXiv2108.11947OpenAlexW3193484523WikidataQ114824756 ScholiaQ114824756MaRDI QIDQ5064656

Henrique Rubira, Jorinde van de Vis, Ryusuke Jinno, Thomas Konstandin

Publication date: 16 March 2022

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

Full work available at URL: https://arxiv.org/abs/2108.11947

zbMATH Keywords

cosmological phase transitionsgravitational waves/sources

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Signal detection and filtering (aspects of stochastic processes) (60G35) Phase transitions (general) in equilibrium statistical mechanics (82B26) Gravitational waves (83C35)

Related Items (2)

Higgsless simulations of cosmological phase transitions and gravitational waves ⋮ Maximal temperature of strongly-coupled dark sectors

Cites Work

• Primordial black holes—perspectives in gravitational wave astronomy
• Gravitational waves from first-order phase transitions: towards model separation by bubble nucleation rate
• Model-independent energy budget for LISA
• A hybrid simulation of gravitational wave production in first-order phase transitions
• Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
• Deformation of the gravitational wave spectrum by density perturbations
• 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
• Relativistic bubble collisions—a closer look

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