Collision Integrals for Cosmological Phase Transitions
arXiv:2303.05846 · doi:10.1007/JHEP05(2023)194
Abstract
The dynamics of the true-vacuum bubbles nucleated during a first-order phase transition is affected by the distribution functions of the particle species in the plasma, driven out-of-equilibrium by the travelling domain wall. An accurate modelling of this phenomenon is relevant for a quantitative description of phase transitions in the early universe and for the determination of the corresponding cosmic relics, such as, among the others, the stochastic background of gravitational waves. We address this problem by developing a new spectral method devised for a fast and reliable computation of the collision integral in the Boltzmann equations. In a scalar singlet extension of the Standard Model chosen as a benchmark scenario, we test our algorithm, determining the bubble speed and profile, and we asses the impact of the out-of-equilibrium dynamics.
18 pages, 3 figures
References in corpus (7)
- Bubble wall dynamics at the electroweak phase transition
- Hydrodynamic obstruction to bubble expansion
- A sonic boom in bubble wall friction
- Hydrodynamics of phase transition fronts and the speed of sound in the plasma
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Cited by in corpus (11)
- Cosmological phase transitions: from perturbative particle physics to gravitational waves
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- Quantisation Across Bubble Walls and Friction
- Criterion for ultra-fast bubble walls: the impact of hydrodynamic obstruction
- Bounds on the bubble wall velocity
- The hydrodynamics of inverse phase transitions
- Bubble wall dynamics from nonequilibrium quantum field theory
- Bubbletrons: Ultrahigh-Energy Particle Collisions and Heavy Dark Matter at Phase Transitions
- Interpreting the 95 GeV resonance in the Two Higgs Doublet Model: Implications for the Electroweak Phase Transition
- Benchmarking a fading window: electroweak baryogenesis in the C2HDM, LHC constraints after Run 2 and prospects for LISA
- Investigating a strong first-order electroweak phase transition in the RxSM at future linear colliders and LISA