Magnetic field generation in first order phase transition bubble collisions
arXiv:hep-ph/9704334 · doi:10.1103/PhysRevD.57.664
Abstract
We consider the formation of a ring-like magnetic field in collisions of bubbles of broken phase in an abelian Higgs model. Particular attention is paid on multiple collisions. The small collision velocity limit, appropriate to the electroweak phase transition, is discussed. We argue that after the completion of the electroweak phase transition, when averaged over nucleation center distances, there exists a mean magnetic field G with a coherence length (for m_H=68 GeV). Because of the ring-like nature of B, the volume average behaves as . Taking into account the turbulent enhancement of the field by inverse cascade, we estimate that colliding electroweak bubbles would give rise to a mean field G at 10 Mpc comoving scale today.
Latex, 18 pages, 8 figures
References in corpus (2)
Cited by in corpus (77)
- Magnetic Fields in the Early Universe
- Cosmological Magnetic Fields: Their Generation, Evolution and Observation
- The stochastic gravitational wave background from turbulence and magnetic fields generated by a first-order phase transition
- Cosmology with the Laser Interferometer Space Antenna
- Primordial magnetogenesis
- Gravitational waves from stochastic relativistic sources: primordial turbulence and magnetic fields
- Primordial Magnetic Fields and Causality
- Gravitational wave production: A strong constraint on primordial magnetic fields
- Tensor Microwave Anisotropies from a Stochastic Magnetic Field
- Evolution of Primordial Magnetic Fields from Phase Transitions
- Primordial Magnetic Fields
- Magnetic field production during preheating at the electroweak scale
- Gravitational Radiation Generated by Cosmological Phase Transition Magnetic Fields
- Natural Magnetogenesis from Inflation
- Effects of a Primordial Magnetic Field on Low and High Multipoles of the CMB
- New Constraints on the Primordial Magnetic Field
- The Search for a Primordial Magnetic Field
- Backreaction of electromagnetic fields and the Schwinger effect in pseudoscalar inflation magnetogenesis
- Constraining primordial magnetic fields with distortions of the black-body spectrum of the cosmic microwave background: pre- and post-decoupling contributions
- Magnetic Fields from Phase Transitions
- Neutrino Propagation in a Strongly Magnetized Medium
- Gauge Invariant Wave Equations in Curved Space-Times and Primordial Magnetic Fields
- CMB anisotropies due to cosmological magnetosonic waves
- Polarized Gravitational Waves from Cosmological Phase Transitions
- Influence of backreaction of electric fields and Schwinger effect on inflationary magnetogenesis
- Ward-Takahashi Identity with External Field in Ladder QED
- Supercooling and phase coexistence in cosmological phase transitions
- Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments
- Anomalous Global Strings and Primordial Magnetic Fields
- Implications of a Primordial Magnetic Field for Magnetic Monopoles, Axions, and Dirac Neutrinos
- Magnetic field generation from non-equilibrium phase transitions
- CMB anisotropies in the presence of a stochastic magnetic field
- Effects of helical magnetic fields on the cosmic microwave background
- Lepton asymmetries and primordial hypermagnetic helicity evolution
- Large scale magnetogenesis from a non-equilibrium phase transition in the radiation dominated era
- Magnetic Fields at First Order Phase Transition: A Threat to Electroweak Baryogenesis
- Simulations and observational tests of primordial magnetic fields from Cosmic Microwave Background constraints
- Resonant amplification of magnetic seed fields by gravitational waves in the early universe
- First-order cosmological phase transitions in the radiation dominated era
- The evolution of primordial magnetic field since its generation
- Magnetogenesis during inflation and preheating in the Starobinsky model
- Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018
- Magnetic Wall From Chiral Phase Transition and CMBR Correlations
- Symmetry restoration at finite temperature with weak magnetic fields
- Transport coefficients in the early universe
- Magnetic field generation from bubble collisions during first-order phase transition
- Magnetogenesis in Higgs-Starobinsky inflation
- Statistical Properties of Scale-Invariant Helical Magnetic Fields and Applications to Cosmology
- Role of Charged Gauge Fields in Generating Magnetic Seed Fields in Bubble Collisions during the Cosmological Electroweak Phase Transition
- Phase Equilibration and Magnetic Field Generation in U(1) Bubble Collisions
- Primordial Magnetic Field Effects on the CMB and Large Scale Structure
- Morphology of blazar-induced gamma ray halos due to a helical intergalactic magnetic field
- Evolution of primordial magnetic fields in mean-field approximation
- Electroweak Origin of Cosmological Magnetic Fields
- Kinetic approach to the Schwinger effect during inflation
- Development of the electroweak phase transition and baryogenesis
- Discovery of Yttrium, Zirconium, Niobium, Technetium, and Ruthenium Isotopes
- Non-equilibrium quantum plasmas in scalar QED: photon production, magnetic and Debye masses, and conductivity
- Gravitational waves from first order phase transitions during inflation
- Magnetic Seed Field Generation from Electroweak Bubble Collisions, with Bubble Walls of Finite Thickness
- CMB with the background primordial magnetic field
- Bubbletrons: Ultrahigh-Energy Particle Collisions and Heavy Dark Matter at Phase Transitions
- Bubble wall dynamics from nonequilibrium quantum field theory
- EWPT Nucleation With MSSM and Electromagnetic Field Creation
- LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
- 21cm fluctuations from primordial magnetic fields
- Basic Treatment of QCD Phase Transition Bubble Nucleation
- Bubble collisions in a SU(2) model of QCD
- Inflationary and phase-transitional primordial magnetic fields in galaxy clusters
- Primordial Magnetic Fields in Light of Dark Ages Global 21-cm Signal
- Constraints on the multi-lognormal magnetic fields from the observations of the cosmic microwave background and the matter power spectrum
- Random Primordial Magnetic Fields and the Gas Content of Dark Matter Halos
- Non-abelian dynamics in first-order cosmological phase transitions
- Effects on the CMB from magnetic field dissipation before recombination
- Magnetic Fields from the Electroweak Phase Transition
- Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating
- Instanton-inspired Model of QCD Phase Transition and Bubble Dynamics