Add to ORKGThe dynamical growth rate of bubbles nucleating in relativistic plasma in thermal first-order phase transitions is analyzed. The framework is a hydrodynamical model which consists of relativistic fluid and an order parameter field. The results of analytical approximations and numerical simulations coincide well
We investigate the scenario of homogeneous nucleation for a first order quark-hadron phase transitio...
This paper investigates the importance of radiative corrections for first-order phase transitions, w...
We estimate bubble-nucleation rates for cosmological phase transitions. We concentrate on the evalua...
By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles gener...
We study how bubbles grow after the initial nucleation event in generic first-order cosmological pha...
IGNATIUS J, KAJANTIE K, KURKISUONIO H, Laine M. THE GROWTH OF BUBBLES IN COSMOLOGICAL PHASE-TRANSITI...
This paper extends classical results by Langer and Kramers and combines them with modern methods fro...
8.69> ffiOE / e t : (2) Similar relations hold for perturbations of energy density and fluid ve...
By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles gener...
We study the dynamics of cosmological phase transitions in the case of small velocities of bubble wa...
Strongly first-order phase transitions, i.e., those with a large order parameter, are characterized ...
AbstractThe growth of bubbles in cosmological first-order phase transitions involves nontrivial hydr...
The growth of bubbles in cosmological first-order phase transitions involves nontrivial hydrodynamic...
We investigate the role played by subcritical bubbles at the onset of the electroweak phase transiti...
First order phase transitions could play a major role in the early universe, providing important phe...
We investigate the scenario of homogeneous nucleation for a first order quark-hadron phase transitio...
This paper investigates the importance of radiative corrections for first-order phase transitions, w...
We estimate bubble-nucleation rates for cosmological phase transitions. We concentrate on the evalua...
By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles gener...
We study how bubbles grow after the initial nucleation event in generic first-order cosmological pha...
IGNATIUS J, KAJANTIE K, KURKISUONIO H, Laine M. THE GROWTH OF BUBBLES IN COSMOLOGICAL PHASE-TRANSITI...
This paper extends classical results by Langer and Kramers and combines them with modern methods fro...
8.69> ffiOE / e t : (2) Similar relations hold for perturbations of energy density and fluid ve...
By means of a relativistic microscopic approach we calculate the expansion velocity of bubbles gener...
We study the dynamics of cosmological phase transitions in the case of small velocities of bubble wa...
Strongly first-order phase transitions, i.e., those with a large order parameter, are characterized ...
AbstractThe growth of bubbles in cosmological first-order phase transitions involves nontrivial hydr...
The growth of bubbles in cosmological first-order phase transitions involves nontrivial hydrodynamic...
We investigate the role played by subcritical bubbles at the onset of the electroweak phase transiti...
First order phase transitions could play a major role in the early universe, providing important phe...
We investigate the scenario of homogeneous nucleation for a first order quark-hadron phase transitio...
This paper investigates the importance of radiative corrections for first-order phase transitions, w...
We estimate bubble-nucleation rates for cosmological phase transitions. We concentrate on the evalua...