On the maximal strength of a first-order electroweak phase transition and its gravitational wave signal
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Publication:5862626
DOI10.1088/1475-7516/2019/04/003OpenAlexW2891839017MaRDI QIDQ5862626
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Publication date: 9 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1809.08242
cosmology of theories beyond the SMphysics of the early universecosmological phase transitionsprimordial gravitational waves (theory)
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Cites Work
- Bubble nucleation and growth in very strong cosmological phase transitions
- Strong electroweak phase transitions in the Standard Model with a singlet
- Gravitational waves from first order electroweak phase transition in models with the U\((1)_X\) gauge symmetry
- Gravitational wave and collider implications of electroweak baryogenesis aided by non-standard cosmology
- QCD-induced electroweak phase transition
- Cosmological phase transitions in warped space: gravitational waves and collider signatures
- Cosmological backgrounds of gravitational waves
- 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
- Gravitational waves from bubble dynamics: beyond the envelope
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