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How fast can the wall move? A study of the electroweak phase transition dynamics
Open accessAbstract
We consider the dynamics of bubble growth in the minimal standard model at the electroweak phase transition and determine the shape and the velocity of the phase boundary, or bubble wall. We show that in the semiclassical approximation the friction on the wall arises from the deviation of massive particle populations from thermal equilibrium. We treat these with Boltzmann equations in a fluid approximation. This approximation is reasonable for the top quarks and the light species while it underestimates the friction from the infrared W bosons and Higgs particles. We use the two-loop finite temperature effective potential and find a subsonic bubble wall for the whole range of Higgs boson masses 0${\mathit{m}}_{\mathit{H}}$90 GeV. This result is weakly dependent on ${\mathit{m}}_{\mathit{H}}$: the wall velocity ${\mathit{v}}_{\mathit{w}}$ falls in the range 0.36${\mathit{v}}_{\mathit{w}}$0.44, while the wall thickness is in the range 29>LT>23. The wall is thicker than the phase equilibrium value because out of equilibrium particles exert more friction on the back than on the base of a moving wall. We also consider the effect of an infrared gauge condensate which may exist in the symmetric phase; modeling it simple mindedly, we find that the wall may become supersonic, but not ultrarelativistic. \textcopyright{} 1995 The American Physical Society.
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Cited by
Hindmarsh, M., Huber, S. J., Rummukainen, K., & Weir, D. J. (2015) · Physical Review D · doi:10.1103/physrevd.92.123009 · Cited by 554
Trodden, M. (1999) · Reviews of Modern Physics · doi:10.1103/revmodphys.71.1463 · Cited by 521
Shape of the acoustic gravitational wave power spectrum from a first order phase transition
Hindmarsh, M., Huber, S. J., Rummukainen, K., & Weir, D. J. (2017) · Physical Review D · doi:10.1103/physrevd.96.103520 · Cited by 451
Is cosmological tuning fine or coarse?
Díaz-Pachón, D. A., Hössjer, O., & Marks II, R. J. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/07/020 · Cited by 10
Metadata
- Authors
- Moore, G. D., & Prokopec, T.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1995-12-15
- Volume
- 52
- Issue
- 12
- Pages
- 7182-7204
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2133915860
- Cited by
- 266
- References
- 3
- FWCI
- 3.64
- Type
- journal article
- Language
- en
- Open access
- green
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