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Original
2011
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Leonardo Leitao and Ariel Megevand, “Spherical and non-spherical bubbles in cosmological phase transitions,” Nucl. Phys. B 844
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Thomas Konstandin, Germano Nardini, and Ingo Rues, “From Boltzmann equations to steady wall velocities,” JCAP 1409
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Then

Jing Liu, Ligong Bian, Rong-Gen Cai, Zong-Kuan Guo, and Shao-Jiang Wang, “Primordial black hole production during first-order phase transitions,” Phys. Rev. D 105
Original
2022
Later among the works it cites.
Wen-Yuan Ai, Bjorn Garbrecht, and Carlos Tamarit, “Bubble wall velocities in local equilibrium,” JCAP 03
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2022
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Stefania De Curtis, Luigi Delle Rose, Andrea Guiggiani, Ángel Gil Muyor, and Giuliano Panico, “Bubble wall dynamics at the electroweak phase transition,” JHEP 03
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2022
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Original
2022
Later among the works it cites.
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2023

Bubble expansion at strong coupling

Li, Li, Wang, Shao-Jiang, Yuwen, Zi-Yan

Understand

The cosmological first-order phase transition (FOPT) can be of strong dynamics but with its bubble wall velocity difficult to be determined due to lack of detailed collision terms.

Recent holographic numerical simulations of strongly coupled theories with a FOPT prefer a relatively small wall velocity linearly correlated with the phase pressure difference between false and true vacua for a planar wall.
In this Letter, we have analytically revealed the non-relativistic limit of a planar/cylindrical/spherical wall expansion of a bubble strongly interacting with the thermal plasma.
The planar-wall result reproduces the linear relation found previously in the holographic numerical simulations.