Bubble wall dynamics at the electroweak phase transition
arXiv:2201.08220 · doi:10.1007/JHEP03(2022)163
Abstract
First order phase transitions could play a major role in the early universe, providing important phenomenological consequences, such as the production of gravitational waves and the generation of baryon asymmetry. An important aspect that determines the properties of the phase transition is the dynamics of the true-vacuum bubbles, which is controlled by the density perturbations in the hot plasma. We study this aspect presenting, for the first time, the full solution of the linearized Boltzmann equation for the top quark species coupled to the Higgs field during a first-order electroweak phase transition. Our approach, differently from the traditional one based on the fluid approximation, does not rely on any ansatz and can fully capture the density perturbations in the plasma. We find that our results significantly differ from the ones obtained in the fluid approximation (including its extensions and modifications), both at the qualitative and quantitative level. In particular sizable differences are found for the friction acting on the bubble wall.
arXiv comment25 pages, 24 figures
References in corpus (40)
- TianQin: a space-borne gravitational wave detector
- Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions
- Detecting gravitational waves from cosmological phase transitions with LISA: an update
- Transport coefficients in high temperature gauge theories: (II) Beyond leading log
- Energy Budget of Cosmological First-order Phase Transitions
- Taiji Program: Gravitational-Wave Sources
- Electroweak Bubble Wall Speed Limit
- How fast can the wall move? A study of the electroweak phase transition dynamics
- The Growth of Bubbles in Cosmological Phase Transitions
- Supersymmetric Electroweak Baryogenesis
- Bubble Wall Velocity at the Electroweak Phase Transition
- Towards an all-orders calculation of the electroweak bubble wall velocity
- Friction pressure on relativistic bubble walls
- Bubble wall velocity: heavy physics effects
- Bubble Expansion and the Viability of Singlet-Driven Electroweak Baryogenesis
- Supersonic Deflagrations in Cosmological Phase Transitions
- Electroweak baryogenesis at high wall velocities
- Do Stops Slow Down Electroweak Bubble Walls?
- From Boltzmann equations to steady wall velocities
- Electroweak bubble wall expansion: gravitational waves and baryogenesis in Standard Model-like thermal plasma
- Bubble wall velocities in local equilibrium
- Bubble Growth as a Detonation
- Baryogenesis and gravity waves from a UV-completed electroweak phase transition
- Electroweak Bubble Wall Friction: Analytic Results
- Field-theoretic derivation of bubble-wall force
- Velocity of electroweak bubble walls
- Fluid equations for fast-moving electroweak bubble walls
- Bubble Wall Velocity at Strong Coupling
- Cosmological bubble friction in local equilibrium
- A sonic boom in bubble wall friction
- Hydrodynamics of phase transition fronts and the speed of sound in the plasma
- Effective picture of bubble expansion
- Wall speed and shape in singlet-assisted strong electroweak phase transitions
- An efficient approach to electroweak bubble velocities
- Spherical and non-spherical bubbles in cosmological phase transitions
- Friction forces on phase transition fronts
- Bubble wall velocity beyond leading-log approximation in electroweak phase transition
- Stability of cosmological deflagration fronts
- Stability of cosmological detonation fronts
- Lower bound on the electroweak wall velocity from hydrodynamic instability
Cited by in corpus (34)
- Cosmological phase transitions: from perturbative particle physics to gravitational waves
- First principles determination of bubble wall velocity
- Bubble wall velocities in local equilibrium
- Model-independent bubble wall velocities in local thermal equilibrium
- The Scalar Singlet Extension of the Standard Model: Gravitational Waves versus Baryogenesis
- Supercool subtleties of cosmological phase transitions
- Quantisation Across Bubble Walls and Friction
- Bubble wall velocity during electroweak phase transition in the inert doublet model
- Collision Integrals for Cosmological Phase Transitions
- Hydrodynamic backreaction force of cosmological bubble expansion
- A perfect fluid hydrodynamic picture of domain wall velocities at strong coupling
- Criterion for ultra-fast bubble walls: the impact of hydrodynamic obstruction
- Logarithmically divergent friction on ultrarelativistic bubble walls
- Multi-step phase transitions and gravitational waves in the inert doublet model
- The energy budget of cosmological first-order phase transitions beyond the bag equation of state
- Bounds on the bubble wall velocity
- Bubble expansion at strong coupling
- Droplet collapse during strongly supercooled transitions
- Gauged Q-ball dark matter through a cosmological first-order phase transition
- The hydrodynamics of inverse phase transitions
- Forbidden dark matter annihilation into leptons with full collision terms
- Bubble wall dynamics from nonequilibrium quantum field theory
- Bubble nucleation and gravitational wave from holography
- A-B transition in superfluid He and cosmological phase transitions
- Interpreting the 95 GeV resonance in the Two Higgs Doublet Model: Implications for the Electroweak Phase Transition
- General backreaction force of cosmological bubble expansion
- Bubble-wall speed with loop corrections
- Benchmarking a fading window: electroweak baryogenesis in the C2HDM, LHC constraints after Run 2 and prospects for LISA
- Dynamics of bubble walls at the electroweak phase transition
- PT2GWFinder: A Package for Cosmological First-Order Phase Transitions and Gravitational Waves
- Confinement Bubble Wall Velocity via Quasiparticle Determination
- Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
- A New Source of Phase Transition Gravitational Waves: Heavy Particle Braking Across Bubble Walls
- Investigating a strong first-order electroweak phase transition in the RxSM at future linear colliders and LISA