Bubble Wall Velocity at the Electroweak Phase Transition
arXiv:hep-ph/9503296 · doi:10.1103/PhysRevLett.75.777
Abstract
We calculate the velocity and thickness of a bubble wall at the electroweak phase transition in the Minimal Standard Model. We model the wall with semiclassical equations of motion and show that friction arises from the deviation of massive particle populations from thermal equilibrium. We treat these with Boltzmann equations in a fluid approximation in the background of the wall. Our analysis improves on the previous work by using the two loop effective potential, accounting for particle transport, and determining the wall thickness dynamically. We find that the wall is significantly thicker than at phase equilibrium, and that the velocity is fairly high, , and quite weakly dependent on the Higgs mass.
8 pages, plain LaTex
References in corpus (4)
- Evidence for Top Quark Production in Collisions at TeV
- The Growth of Bubbles in Cosmological Phase Transitions
- Finite Temperature Effective Potential to Order $g^4,\la^2$ and the Electroweak Phase Transition
- The Effects of Electro-weak Phase Transition Dynamics on Baryogenesis and Primordial Nucleosynthesis
Cited by in corpus (127)
- Cosmological Backgrounds of Gravitational Waves
- Detecting gravitational waves from cosmological phase transitions with LISA: an update
- Electroweak Baryogenesis
- Electroweak Baryon Number Non-Conservation in the Early Universe and in High Energy Collisions
- Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources
- How fast can the wall move? A study of the electroweak phase transition dynamics
- Cosmological phase transitions: from perturbative particle physics to gravitational waves
- Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
- Some Cosmological Implications of Hidden Sectors
- Non-local Electroweak Baryogenesis Part II : The Classical Regime
- Non-local Electroweak Baryogenesis Part I : Thin Wall Regime
- Transport equations for chiral fermions to order \hbar and electroweak baryogenesis: Part I
- Transport equations for chiral fermions to order \hbar and electroweak baryogenesis: Part II
- Quantum Transport and Electroweak Baryogenesis
- Towards an all-orders calculation of the electroweak bubble wall velocity
- Turning Around the Sphaleron Bound: Electroweak Baryogenesis in an Alternative Post-inflationary Cosmology
- Electroweak Phase Transition and Baryogenesis in the nMSSM
- Electroweak Baryogenesis and New TeV Fermions
- Updated predictions for gravitational waves produced in a strongly supercooled phase transition
- Model-independent energy budget of cosmological first-order phase transitions
- Bubble Expansion and the Viability of Singlet-Driven Electroweak Baryogenesis
- Filtered Dark Matter at a First Order Phase Transition
- Electroweak baryogenesis at high wall velocities
- Do Stops Slow Down Electroweak Bubble Walls?
- The Gravitational-Wave Physics II: Progress
- First principles determination of bubble wall velocity
- Relic gravitational waves from colliding bubbles and cosmic turbulence
- From Boltzmann equations to steady wall velocities
- Magnetic field generation in first order phase transition bubble collisions
- Electroweak bubble wall expansion: gravitational waves and baryogenesis in Standard Model-like thermal plasma
- The Science of the Einstein Telescope
- Bubble wall velocities in local equilibrium
- Baryogenesis and gravity waves from a UV-completed electroweak phase transition
- Field-theoretic derivation of bubble-wall force
- Bubble wall velocities in the Standard Model and beyond
- Gravitational waves from the electroweak phase transition
- Hearing without seeing: gravitational waves from hot and cold hidden sectors
- Velocity of electroweak bubble walls
- Model-independent bubble wall velocities in local thermal equilibrium
- Fluid equations for fast-moving electroweak bubble walls
- Bubble wall dynamics at the electroweak phase transition
- On Bubble Growth and Droplet Decay in Cosmological Phase Transitions
- Hydrodynamic obstruction to bubble expansion
- The Scalar Singlet Extension of the Standard Model: Gravitational Waves versus Baryogenesis
- Bubble Wall Velocity at Strong Coupling
- Classical Field Dynamics of the Electroweak Phase Transition
- Bubble nucleation and growth in very strong cosmological phase transitions
- Cosmological bubble friction in local equilibrium
- Bubble Wall Velocity from Holography
- Hydrodynamics of phase transition fronts and the speed of sound in the plasma
- Real-Time History of the Cosmological Electroweak Phase Transition
- Bubble Wall Profiles With More Than One Scalar Field: A Numerical Approach
- Gravitational waves from a very strong electroweak phase transition
- Detonations and deflagrations in cosmological phase transitions
- Effective picture of bubble expansion
- Local and Nonlocal Defect-Mediated Electroweak Baryogenesis
- Quantisation Across Bubble Walls and Friction
- Wall speed and shape in singlet-assisted strong electroweak phase transitions
- Baryogenesis from an Earlier Phase Transition
- Cosmological Signatures of a UV-Conformal Standard Model
- Gravitational traces of broken gauge symmetries
- Bubble wall velocity during electroweak phase transition in the inert doublet model
- Spherical and non-spherical bubbles in cosmological phase transitions
- Holographic Bubbles with Jecco: Expanding, Collapsing and Critical
- CP-violation for Electroweak Baryogenesis from Dynamical CKM Matrix
- Collision Integrals for Cosmological Phase Transitions
- Friction forces on phase transition fronts
- Hydrodynamic backreaction force of cosmological bubble expansion
- Gravitational Waves at Strong Coupling from an Effective Action
- New benchmark scenarios of electroweak baryogenesis in aligned two Higgs double models
- A perfect fluid hydrodynamic picture of domain wall velocities at strong coupling
- First-order cosmological phase transitions in the radiation dominated era
- Criterion for ultra-fast bubble walls: the impact of hydrodynamic obstruction
- Bubble-wall velocity in local thermal equilibrium: hydrodynamical simulations vs analytical treatment
- Prospects of gravitational waves in the minimal left-right symmetric model
- Bubble wall velocity beyond leading-log approximation in electroweak phase transition
- Generation of baryon inhomogeneities in the electroweak phase transition
- Gravitational wave and electroweak baryogenesis with two Higgs doublet models
- Gravitational waves triggered by charged hidden scalar and leptogenesis
- Logarithmically divergent friction on ultrarelativistic bubble walls
- Stability of cosmological deflagration fronts
- Stability of cosmological detonation fronts
- Constraints on holographic QCD phase transitions from PTA observations
- Is electroweak baryogenesis dead?
- Bounds on the bubble wall velocity
- Bubble expansion at strong coupling
- Effect of reheating on electroweak baryogenesis
- Baryogenesis via leptonic CP-violating phase transition
- Bubble dynamics in fluids with N-body simulations
- Detailed Calculation of Primordial Black Hole Formation During First-Order Cosmological Phase Transitions
- Sound velocity effects on the phase transition gravitational wave spectrum in the sound shell model
- Lower bound on the electroweak wall velocity from hydrodynamic instability
- Electroweak Phase Transition in a Right-Handed Neutrino Superfield Extended NMSSM
- Analytic approach to the motion of cosmological phase transition fronts
- Gravitational waves from burdened primordial black holes dark matter
- Electroweak Phase Transition with a Double Well Done Doubly Well
- Energy budget of cosmological first-order phase transition in FLRW background
- The hydrodynamics of inverse phase transitions
- Electroweak Baryogenesis Using Baryon Number Carrying Scalars
- Hydrodynamics of ultra-relativistic bubble walls
- Cosmological Consequences of Slow-Moving Bubbles in First-Order Phase Transitions
- Bubble Collisions and Defect Formation in a Damping Environment
- Bubble wall dynamics from nonequilibrium quantum field theory
- Model-dependent analysis method for energy budget of the cosmological first-order phase transition
- Impact of SM parameters and of the vacua of the Higgs potential in gravitational waves detection
- Bubble velocities and oscillon precursors in first-order phase transitions
- Fluctuations and Bubble Dynamics in First-Order Phase Transitions
- Hydrodynamic effects on the filtered dark matter produced by a first-order phase transition
- Bubble wall velocity and gravitational wave in the minimal left-right symmetric model
- Model-independent features of gravitational waves from bubble collisions
- An exact solution of the Dirac equation with CP violation
- Bubble nucleation and gravitational wave from holography
- Towards TeV-Scale Supersymmetric Electroweak Baryogenesis
- Instability of bubble expansion at zero temperature
- Defect Formation in First Order Phase Transitions with Damping
- Bubble Trouble: a Review on Electroweak Baryogenesis
- Non-thermal production of heavy vector dark matter from relativistic bubble walls
- Upper limit on first-order electroweak phase transition strength
- General backreaction force of cosmological bubble expansion
- Dynamics of bubble walls at the electroweak phase transition
- Defect Formation Rates in Cosmological First-Order Phase Transitions
- PT2GWFinder: A Package for Cosmological First-Order Phase Transitions and Gravitational Waves
- Electroweak-like Baryogenesis with New Chiral Matter
- 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
- Electroweak Baryogenesis in Supersymmetric Variants
- Gravitational waves from bubble walls