Study of entropy production due to electroweak phase transition in symmetric extension of the Standard Model
arXiv:2206.08699 · doi:10.1103/PhysRevD.106.095016
Abstract
In this work we consider the simple symmetric extension to the Standard Model (SM) and proceed to study the nature of electroweak phase transition (EWPT) in the early universe. We show that the nature of the phase transition changes from a smooth crossover in the SM to a strong first order with this addition of the real scalar. Furthermore, we show the entropy release in this scenario is higher than that of the SM. This can lead to a strong dilution of frozen out dark matter particles and baryon asymmetry, if something existed before the onset of the phase transition.
arXiv comment12 pages, 3 figures
References in corpus (35)
- Planck 2015 results. XIII. Cosmological parameters
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm
- Gravitational Radiation from First-Order Phase Transitions
- Electroweak baryogenesis
- Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?
- Gravitational Wave Production by Collisions: More Bubbles
- Gravitational waves from the sound of a first order phase transition
- Numerical simulations of acoustically generated gravitational waves at a first order phase transition
- Gravitational Radiation from Colliding Vacuum Bubbles: Envelope Approximation to Many-Bubble Collisions
- The stochastic gravitational wave background from turbulence and magnetic fields generated by a first-order phase transition
- Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources
- Gravitational wave generation from bubble collisions in first-order phase transitions: an analytic approach
- Gravitational waves from stochastic relativistic sources: primordial turbulence and magnetic fields
- Dynamics of Non-renormalizable Electroweak Symmetry Breaking
- Electroweak Baryogenesis in Supersymmetric Models
- Phase Transitions in an Expanding Universe: Stochastic Gravitational Waves in Standard and Non-Standard Histories
- Vacuum Stability of a General Scalar Potential of a Few Fields
- Consistent Use of the Standard Model Effective Potential
- Taming Infrared Divergences in the Effective Potential
- Detectability of Gravitational Waves from Phase Transitions
- Gravitational Radiation Generated by Cosmological Phase Transition Magnetic Fields
- Consistent Use of Effective Potentials
- Gravitational Radiation from Primordial Helical Inverse Cascade MHD Turbulence
- Synergy between measurements of the gravitational wave and the triple Higgs coupling in probing first order phase transition
- Electroweak phase transition with spontaneous -breaking
- Strong First Order EWPT and Strong Gravitational Waves in -symmetric Singlet Scalar Extension
- Probing the seesaw scale with gravitational waves
- Gravitational Wave Signals of Pseudo-Goldstone Dark Matter in the Complex Singlet Model
- PBH evaporation, baryon asymmetry,and dark matter
- First-order electroweak phase transition in a complex singlet model with symmetry
- The Cosmological QCD Phase Transition Revisited
- Gravitational Waves from first-order phase transition and domain wall
- Electroweak phase transition and entropy release in the early universe
- Particle dark matter density and entropy production in the early universe