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The B\"{o}deker-Moore thermal friction is usually used to determine whether or not a bubble wall can run away.
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A. Azatov and M. Vanvlasselaer, “Phase transitions in perturbative walking dynamics,” JHEP
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F. Bigazzi, A. Caddeo, A. L. Cotrone, and A. Paredes, “Dark Holograms and Gravitational Waves,” JHEP
2011
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T. Konstandin and J. M. No, “Hydrodynamic obstruction to bubble expansion,” JCAP
2011
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2011
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A. Kurkela and G. D. Moore, “Thermalization in Weakly Coupled Nonabelian Plasmas,” JHEP
2011
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D. E. Morrissey and M. J. Ramsey-Musolf, “Electroweak baryogenesis,” New J. Phys
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2022
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W.-Y. Ai, B. Garbrecht, and C. Tamarit, “Bubble wall velocities in local equilibrium,” JCAP
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2012
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2012
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2012
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2012
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2014
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2015
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P. Schwaller, “Gravitational Waves from a Dark Phase Transition,” Phys. Rev. Lett
2015
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2015
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2022
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Y. Gouttenoire, R. Jinno, and F. Sala, “Friction pressure on relativistic bubble walls,” JHEP
2022
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2022
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G. C. Dorsch, S. J. Huber, and T. Konstandin, “A sonic boom in bubble wall friction,” JCAP
2022
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2022
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2022
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2023
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2023
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2023
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2023
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L. Li, S.-J. Wang, and Z.-Y. Yuwen, “Bubble expansion at strong coupling,” Phys. Rev. D
2023
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2023
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2023
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2023
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2023
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W.-Y. Ai, “Logarithmically divergent friction on ultrarelativistic bubble walls,” JCAP
2023
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2023
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2023
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2023
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I. Garcia Garcia, G. Koszegi, and R. Petrossian-Byrne, “Reflections on bubble walls,” JHEP
2023
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2023
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2023
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M. O. Olea-Romacho, “Primordial magnetogenesis in the two-Higgs-doublet model,” Phys. Rev. D
2024
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