Primordial Galactic Magnetic Fields from Domain Walls at the QCD Phase Transition
- 18 December 2000
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 85 (25) , 5268-5271
- https://doi.org/10.1103/physrevlett.85.5268
Abstract
We propose a mechanism to generate large-scale magnetic fields with correlation lengths of 100 kpc. Domain walls with QCD-scale internal structure form and coalesce, obtaining Hubble-scale correlations while aligning nucleon spins. Because of strong violation, the walls are ferromagnetic, which induces electromagnetic fields with Hubble-size correlations. The violation also induces a maximal helicity (Chern-Simons) which supports an “inverse cascade,” allowing the initial correlations to grow to 100 kpc today. We estimate the generated electromagnetic fields in terms of the QCD parameters and discuss the effects of the resulting fields.
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This publication has 33 references indexed in Scilit:
- Primordial Magnetic Fields, Right Electrons, and the Abelian AnomalyPhysical Review Letters, 1997
- Inverse cascades and primordial magnetic fieldsPhysics Letters B, 1997
- Primordial magnetic fields from cosmological first order phase transitionsPhysical Review D, 1997
- GALACTIC MAGNETISM: Recent Developments and PerspectivesAnnual Review of Astronomy and Astrophysics, 1996
- Magnetic fields produced by phase transition bubbles in the electroweak phase transitionPhysical Review D, 1996
- Primordial Magnetic Fields from String CosmologyPhysical Review Letters, 1995
- Extragalactic magnetic fieldsReports on Progress in Physics, 1994
- Electric charge asymmetry of the Universe and magnetic field generationPhysical Review D, 1993
- Large-scale structure from wiggly cosmic stringsPhysical Review Letters, 1991
- Inflation-produced, large-scale magnetic fieldsPhysical Review D, 1988