Turn up the volume: listening to phase transitions in hot dark sectors

DOI10.1088/1475-7516/2022/02/014zbMath1487.83019arXiv2109.06208OpenAlexW3199173885MaRDI QIDQ5063485

Felix Kahlhoefer, Carlo Tasillo, Fatih Ertas

Publication date: 21 March 2022

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

Full work available at URL: https://arxiv.org/abs/2109.06208

zbMATH Keywords

cosmology of theories beyond the SMcosmological phase transitionsparticle physics-cosmology connectionprimordial gravitational waves (theory)

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Computational methods for stochastic equations (aspects of stochastic analysis) (60H35) Gravitational waves (83C35) Dark matter and dark energy (83C56)

Related Items (6)

Gravitational wave imprints of left-right symmetric model with minimal Higgs sector ⋮ Decaying warm dark matter revisited ⋮ Reflections on bubble walls ⋮ The domain of a cannibal dark matter ⋮ Maximal temperature of strongly-coupled dark sectors ⋮ Barrow entropy and stochastic gravitational wave background generated from cosmological QCD phase transition

Cites Work

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• Gravitational waves from first order phase transitions as a probe of an early matter domination era and its inverse problem
• Causal gravitational waves as a probe of free streaming particles and the expansion of the universe
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• Hearing without seeing: gravitational waves from hot and cold hidden sectors
• Electroweak bubble wall speed limit
• Bubble wall velocity: heavy physics effects
• Towards an all-orders calculation of the electroweak bubble wall velocity
• Fate of electroweak symmetry in the early Universe: non-restoration and trapped vacua in the N2HDM
• Phase transition dynamics and gravitational wave spectra of strong first-order phase transition in supercooled universe

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