The bubble wall velocity in the minimal supersymmetric light stop scenario
arXiv:1112.1888 · doi:10.1103/PhysRevD.85.103507
Abstract
We build on existing calculations of the wall velocity of the expanding bubbles of the broken symmetry phase in a first-order electroweak phase transition within the light stop scenario (LSS) of the MSSM. We carry out the analysis using the 2-loop thermal potential for values of the Higgs mass consistent with present experimental bounds. Our approach relies on describing the interaction between the bubble and the hot plasma by a single friction parameter, which we fix by matching to an existing 1-loop computation and extrapolate it to our regime of interest. For a sufficiently strong phase transition (in which washout of the newly-created baryon asymmetry is prevented) we obtain values of the wall velocity, v_w~0.05, far below the speed of sound in the medium, and not very much deviating from the previous 1-loop calculation. We also find that the phase transition is about 10% stronger than suggested by simply evaluating the thermal potential at the critical temperature.
17pages, 3 figures
References in corpus (34)
- Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?
- Energy Budget of Cosmological First-order Phase Transitions
- Gravitational Wave Production by Collisions: More Bubbles
- Gravitational Waves from Phase Transitions at the Electroweak Scale and Beyond
- Strong Electroweak Phase Transitions in the Standard Model with a Singlet
- First-Order Electroweak Phase Transition in the Standard Model with a Low Cutoff
- Opening the Window for Electroweak Baryogenesis
- Can electroweak bubble walls run away?
- How fast can the wall move? A study of the electroweak phase transition dynamics
- Baryogenesis in the Two-Higgs Doublet Model
- Electroweak Baryogenesis and Dark Matter in the nMSSM
- The Growth of Bubbles in Cosmological Phase Transitions
- Electroweak Baryogenesis in Supersymmetric Models
- Electroweak Baryogenesis in Two Higgs Doublet Models and B meson anomalies
- Improved Results in Supersymmetric Electroweak Baryogenesis
- The Baryogenesis Window in the MSSM
- The Electroweak Phase Transition in a Nonminimal Supersymmetric Model
- The MSSM Electroweak Phase Transition on the Lattice
- Electroweak Baryogenesis: Concrete in a SUSY Model with a Gauge Singlet
- Dominant Two-Loop Corrections to the MSSM Finite Temperature Effective Potential
- Measuring the Broken Phase Sphaleron Rate Nonperturbatively
- The Baryon asymmetry in the Standard Model with a low cut-off
- Production of Gravitational Waves in the nMSSM
- Electroweak Baryogenesis in Non-minimal Composite Higgs Models
- MSSM Electroweak Baryogenesis and Flavour Mixing in Transport Equations
- The 2-loop MSSM finite temperature effective potential with stop condensation
- Do Stops Slow Down Electroweak Bubble Walls?
- Bubble Growth as a Detonation
- Velocity of electroweak bubble walls
- Real-Time History of the Cosmological Electroweak Phase Transition
- Yukawa Interactions and Supersymmetric Electroweak Baryogenesis
- Baryogenesis in the MSSM, nMSSM and NMSSM
- Supersonic Electroweak Baryogenesis: Achieving Baryogenesis for Fast Bubble Walls
- Electroweak Phase Transition and Baryogenesis
Cited by in corpus (34)
- Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
- A Second Higgs Doublet in the Early Universe: Baryogenesis and Gravitational Waves
- Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
- Quantum Transport and Electroweak Baryogenesis
- Gravitional radiation from first-order phase transitions in the presence of a fluid
- The Gravitational-Wave Physics II: Progress
- From Boltzmann equations to steady wall velocities
- Cosmological Phase Transitions and their Properties in the NMSSM
- Bubble wall velocities in local equilibrium
- Gravitational waves from the electroweak phase transition
- Model-independent bubble wall velocities in local thermal equilibrium
- Fluid equations for fast-moving electroweak bubble walls
- Lattice study of an electroweak phase transition at m_h ~ 126 GeV
- Gravitational waves from the asymmetric-dark-matter generating phase transition
- Cosmological bubble friction in local equilibrium
- Thermal Squeezeout of Dark Matter
- Gravitational waves from phase transition in split NMSSM
- Perturbative Non-Equilibrium Thermal Field Theory
- Effective picture of bubble expansion
- Wall speed and shape in singlet-assisted strong electroweak phase transitions
- An efficient approach to electroweak bubble velocities
- Friction forces on phase transition fronts
- Gravitational Waves at Strong Coupling from an Effective Action
- Bubble wall velocity beyond leading-log approximation in electroweak phase transition
- Gravitational wave and electroweak baryogenesis with two Higgs doublet models
- Logarithmically divergent friction on ultrarelativistic bubble walls
- Bounds on the bubble wall velocity
- Does zero temperature decide on the nature of the electroweak phase transition?
- Lower bound on the electroweak wall velocity from hydrodynamic instability
- Bubble wall dynamics from nonequilibrium quantum field theory
- Model-dependent analysis method for energy budget of the cosmological first-order phase transition
- Model-independent features of gravitational waves from bubble collisions
- Bubble wall velocity and gravitational wave in the minimal left-right symmetric model
- -ino-driven Electroweak Baryogenesis in the UMSSM