Anomalous non-conservation of fermion/chiral number in Abelian gauge theories at finite temperature
arXiv:1707.09967 · doi:10.1007/JHEP04(2018)026
Abstract
We discuss the non-conservation of fermion number (or chirality breaking, depending on the fermionic charge assignment) in Abelian gauge theories at finite temperature. We study different mechanisms of fermionic charge disappearance in the high temperature plasma, using both analytical estimates and real-time classical lattice numerical simulations. We investigate the random walk of the Chern-Simons number , and show that it has a diffusive behaviour in the presence of an external magnetic field . This indicates that the mechanism for fermionic number non-conservation for , is due to fluctuations of the gauge fields, similarly as in the case of non-Abelian gauge theories. We determine numerically, with lattice simulations, the rate of chirality non-conservation associated with this diffusion. We find the rate to be a factor larger compared to previous theoretical estimates, what calls for a revision of the implications of Abelian fermion number and chirality non-conservation for baryogenesis, magnetogenesis and chiral symmetry evolution. An erratum can be found at the end of the manuscript, following the results obtained in JHEP 10 (2019) 142 (1904.11892 [hep-th]), which reduce our original claim in the discrepancy between theory and numerics by a factor .
Version matching publication, former Section V on 'Dynamics of chiral charge' removed, and erratum appended at the end in light of the results obtained in 1904.11892 [hep-th]
References in corpus (7)
- The Sphaleron Rate in the Minimal Standard Model
- A stochastic background of gravitational waves from hybrid preheating
- CMB power spectrum contribution from cosmic strings using field-evolution simulations of the Abelian Higgs model
- Exact Scale-Invariant Background of Gravitational Waves from Cosmic Defects
- Gravitational wave production from preheating: parameter dependence
- Parametric Resonance in the Early Universe - A Fitting Analysis
- Lattice implementation of Abelian gauge theories with Chern-Simons number and an axion field
Cited by in corpus (16)
- Gauge Field and Fermion Production during Axion Inflation
- The art of simulating the early Universe -- Part I
- Lattice formulation of axion inflation. Application to preheating
- Baryogenesis from axion inflation
- Chiral instabilities & the onset of chiral turbulence in QED plasmas
- Evolution of the Primordial Axial Charge across Cosmic Times
- Chiral charge dynamics in Abelian gauge theories at finite temperature
- Equilibration of the chiral asymmetry due to finite electron mass in electron-positron plasma
- Higher-form symmetries, anomalous magnetohydrodynamics, and holography
- Electroweak Sphaleron in a Magnetic field
- Baryogenesis via gauge field production from a relaxing Higgs
- Freeze-in and freeze-out generation of lepton asymmetries after baryogenesis in the MSM
- Higher-form symmetry and chiral transport in real-time Abelian lattice gauge theory
- Cosmological chirality and magnetic fields from parity violating particle decays
- Hydrodynamic fluctuations and topological susceptibility in chiral magnetohydrodynamics
- Electrical conductivity of hot Abelian plasma with scalar charge carriers