Bubble nucleation and growth in very strong cosmological phase transitions
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Publication:529287
DOI10.1016/j.nuclphysb.2017.03.009zbMath1361.83031arXiv1611.05853OpenAlexW2556158121MaRDI QIDQ529287
Ariel Mégevand, Santiago Ramírez
Publication date: 18 May 2017
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1611.05853
Relativistic cosmology (83F05) Nuclear physics (81V35) Gravitational waves (83C35) Dynamic and nonequilibrium phase transitions (general) in statistical mechanics (82C26)
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Cites Work
- Unnamed Item
- Hydrodynamics of ultra-relativistic bubble walls
- Spherical and non-spherical bubbles in cosmological phase transitions
- Hydrodynamics of phase transition fronts and the speed of sound in the plasma
- Detonations and deflagrations in cosmological phase transitions
- Velocity of electroweak bubble walls
- Topology of cosmic domains and strings
- Precise determination of the critical threshold and exponents in a three-dimensional continuum percolation model
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