Results 61 to 70 of about 23,762 (159)
Non-linearities in cosmological bubble wall dynamics
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 relics, including the stochastic background of gravitational waves.
Stefania De Curtis +4 more
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Bubble friction in symmetry-restoring transitions
In standard (symmetry-breaking) first-order phase transitions, the frictional pressure on expanding bubble walls can be dominated by transition radiation — the emission of a gauge boson with phase-dependent masses as particles present in the thermal ...
Andrew J. Long +2 more
doaj +1 more source
From friction scaling to an efficient method for estimating bubble wall velocity
We present a unified description of first-order cosmological phase transition dynamics that links the phenomenological friction model employed in hydrodynamic simulations to the microscopic treatment based on Boltzmann equations. We derive an approximate
Tomasz Krajewski +4 more
doaj +1 more source
Bounds on the bubble wall velocity
Determining the bubble wall velocity in first-order phase transitions is a challenging task, requiring the solution of (coupled) equations of motion for the scalar field and Boltzmann equations for the particles in the plasma.
Wen-Yuan Ai +2 more
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Super-slow phase transition catalyzed by BHs and the birth of baby BHs
We discuss the unique phenomenology of first-order phase transitions catalyzed by primordial black holes (BHs). If the number of BHs within one Hubble volume is smaller than unity at the time of bubble nucleation, each bubble catalyzed around them can ...
Ryusuke Jinno +2 more
doaj +1 more source
Particle shells from relativistic bubble walls
Relativistic bubble walls from cosmological phase transitions (PT) necessarily accumulate expanding shells of particles. We systematically characterize shell properties, and identify and calculate the processes that prevent them from free streaming ...
Iason Baldes +3 more
doaj +1 more source
We numerically construct a series of axisymmetric rotating magnetic wind solutions, aiming at exploring the observation properties of massive white dwarf (WD) merger remnants with a strong magnetic field, a fast spin, and an intense mass loss, as ...
Yici Zhong +4 more
doaj +1 more source
How fast does the WallGo? A package for computing wall velocities in first-order phase transitions
WallGo is an open-source software designed to compute the bubble wall velocity in first-order cosmological phase transitions. Additionally, it evaluates the energy budget available for generating gravitational waves.
Andreas Ekstedt +6 more
doaj +1 more source
Steady-state bubbles beyond local thermal equilibrium
We investigate the hydrodynamic solutions for expanding bubbles in cosmological first-order phase transitions going beyond local thermal equilibrium approximation.
Tomasz Krajewski +3 more
doaj +1 more source
WallGo investigates: Theoretical uncertainties in the bubble wall velocity
We examine theoretical uncertainties in state-of-the-art calculations of the bubble wall velocity during first-order cosmological phase transitions.
Jorinde van de Vis +5 more
doaj +1 more source

