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In first-order cosmological phase transitions, the asymptotic velocity of expanding bubbles is of crucial relevance for predicting observables like the spectrum of stochastic gravitational waves, or for establishing the viability of mechanisms explaining fundamental properties of the universe such as the observed baryon asymmetry.
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N. Seto, S. Kawamura, and T. Nakamura, “Possibility of direct measurement of the acceleration of the universe using 0.1-Hz band laser interferometer gravitational wave antenna in space”, Phys. Rev. Lett
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2007
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S. J. Huber and M. Sopena, “An efficient approach to electroweak bubble velocities”, arXiv:1302.1044
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T. Konstandin, G. Nardini, and I. Rues, “From Boltzmann equations to steady wall velocities”, JCAP
2014
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J. Kozaczuk, “Bubble Expansion and the Viability of Singlet-Driven Electroweak Baryogenesis”, JHEP
2015
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D. Bodeker and G. D. Moore, “Electroweak Bubble Wall Speed Limit”, JCAP
2017
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C. Caprini and D. G. Figueroa, “Cosmological Backgrounds of Gravitational Waves”, Class. Quant. Grav
2018
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