We compute the terminal bubble wall velocity during a cosmological phase transition by
modelling non-equilibrium effects in the plasma with the so-called" extended fluid Ansatz". A …

The Bödeker-Moore thermal friction [1] is usually used to determine whether or not a bubble
wall can run away. However, the friction on the wall is not necessarily a monotonous …

A bstract A precise modelling of the dynamics of bubbles nucleated during first-order phase
transitions in the early Universe is pivotal for a quantitative determination of various cosmic …

The gravitational-wave energy-density spectra from cosmological first-order phase
transitions crucially depend on the terminal wall velocity of asymptotic bubble expansion …

Dark matter, if represented by a Bbb Z 2-symmetric scalar field, can manifest as both
particles and condensates. In this paper, we study the evolution of an oscillating …

Cosmological first-order phase transitions (FOPTs) serve as comprehensive probes into our
early Universe with associated generations of stochastic gravitational waves and …

We propose a new mechanism of primordial black hole formation via an aborted phase
transition during the early matter-dominated stage of reheating after inflation. In reheating …

Heavy vector boson dark matter at the TeV scale or higher may be produced non-thermally
in a first-order phase transition taking place at a lower energy scale. While the production of …

Our understanding of the Universe, particularly its earliest moments, is grounded in two
fundamental pillars of theoretical physics: General Relativity (GR) and the Standard Model …