skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: From Boltzmann equations to steady wall velocities

Journal Article · · Journal of Cosmology and Astroparticle Physics

By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles generated during a first-order electroweak phase transition. In particular, we use the gradient expansion of the Kadanoff-Baym equations to set up the fluid system. This turns out to be equivalent to the one found in the semi-classical approach in the non-relativistic limit. Finally, by including hydrodynamic deflagration effects and solving the Higgs equations of motion in the fluid, we determine velocity and thickness of the bubble walls. Our findings are compared with phenomenological models of wall velocities. As illustrative examples, we apply these results to three theories providing first-order phase transitions with a particle content in the thermal plasma that resembles the Standard Model.

OSTI ID:
22375881
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2014, Issue 09; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Lower bound on the electroweak wall velocity from hydrodynamic instability
Journal Article · Sun Mar 01 00:00:00 EST 2015 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22375881

Lower bound on the electroweak wall velocity from hydrodynamic instability
Journal Article · Fri Mar 27 00:00:00 EDT 2015 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22375881

Towards an all-orders calculation of the electroweak bubble wall velocity
Journal Article · Mon Jul 20 00:00:00 EDT 2020 · TBD · OSTI ID:22375881