Bödeker D, Moore GD. Can electroweak bubble walls run away? JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. 2009;2009(05): 009.In extensions of the Standard Model with SU(2) singlet scalar fields, there can be regions of parameter space for which the electroweak phase transition is first order already at the mean-field level of analysis. We show that in this case the phase interface ( bubble wall) can become ultra-relativistic, with the relativistic gamma factor gamma = (1 - v(wall)(2))(-1/2) growing linearly with the wall's propagation distance. We provide a simple criterion for determining whether the bubble wall "runs away" in this way or if gamma approaches a terminal value
In cosmological first-order phase transitions, gravitational waves are generated by the collisions o...
AbstractIn cosmological first-order phase transitions, gravitational waves are generated by the coll...
Kurki-Suonio H, Laine M. Real-time history of the cosmological electroweak phase transition. Physica...
Bödeker D, Moore GD. Electroweak bubble wall speed limit. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHY...
We consider the dynamics of bubble growth in the Minimal Standard Model at the electroweak phase tra...
Despite electroweak baryogenesis being a promising and testable explanation of the matter-antimatter...
We present results for the bubble wall velocity and bubble wall thickness during a cosmological firs...
We derive a general quantum field theoretic formula for the force acting on expanding bubbles of a f...
We perform large-scale real-time simulations of a bubble wall sweeping through an out-of-equilibrium...
By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles gener...
First order phase transitions could play a major role in the early universe, providing important phe...
Bubbles in a first-order electroweak phase transition are nucleated with radii R0 and expand with ve...
During a cosmological first-order phase transition, particles of the plasma crossing the bubble wall...
The first order phase transition proceeds via nucleation and growth of true vacuum bubbles. When cha...
We study scalar bubble collisions in first-order phase transitions focusing on the relativistic limi...
In cosmological first-order phase transitions, gravitational waves are generated by the collisions o...
AbstractIn cosmological first-order phase transitions, gravitational waves are generated by the coll...
Kurki-Suonio H, Laine M. Real-time history of the cosmological electroweak phase transition. Physica...
Bödeker D, Moore GD. Electroweak bubble wall speed limit. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHY...
We consider the dynamics of bubble growth in the Minimal Standard Model at the electroweak phase tra...
Despite electroweak baryogenesis being a promising and testable explanation of the matter-antimatter...
We present results for the bubble wall velocity and bubble wall thickness during a cosmological firs...
We derive a general quantum field theoretic formula for the force acting on expanding bubbles of a f...
We perform large-scale real-time simulations of a bubble wall sweeping through an out-of-equilibrium...
By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles gener...
First order phase transitions could play a major role in the early universe, providing important phe...
Bubbles in a first-order electroweak phase transition are nucleated with radii R0 and expand with ve...
During a cosmological first-order phase transition, particles of the plasma crossing the bubble wall...
The first order phase transition proceeds via nucleation and growth of true vacuum bubbles. When cha...
We study scalar bubble collisions in first-order phase transitions focusing on the relativistic limi...
In cosmological first-order phase transitions, gravitational waves are generated by the collisions o...
AbstractIn cosmological first-order phase transitions, gravitational waves are generated by the coll...
Kurki-Suonio H, Laine M. Real-time history of the cosmological electroweak phase transition. Physica...