Primordial Galactic Magnetic Fields: An Application of QCD Domain Walls

dc.creatorForbes, Michael McNeil
dc.creatorZhitnitsky, Ariel R.
dc.date2001-02-13
dc.date.accessioned2026-07-07T03:43:53Z
dc.date.available2026-07-07T03:43:53Z
dc.descriptionWe present a mechanism for generating primordial magnetic fields with large correlation lengths on the order of 100 kpc today. The mechanism is based on recently conjectured QCD domain walls or similar CP violating domain walls with QCD scale structure. Such domain walls align the electric and magnetic dipole moments of the nucleons shortly after the QCD phase transition, producing electromagnetic fields correlated along the domain walls. Through the Kibble mechanism, the domain walls attain Hubble-scale correlations which they transfer to the aligned electromagnetic fields. Due to the CP violation, the Hubble-scale walls produce helical (non-zero Chern-Simons) magnetohydrodynamic turbulence which then undergoes an inverse cascade, allowing the correlation lengths to grow to 100 kpc today. We present an estimate the magnitude of the generated electromagnetic fields in terms of the QCD parameters. We also discuss some other unexplained astrophysical phenomena which may be related to this mechanism. In particular, we discuss the relation between primordial magnetic fields and the Greisen-Zatsepin-Kuzmin (GZK) cutoff violations. We also outline how, by creating inhomogeneities in the nucleon density, QCD domain walls may lead to inhomogeneous big bang nucleosynthesis (IBBN) explaining the Omega_B excess recently measured through cosmic microwave background (CMB) distortions.
dc.description17 pages, 1 figure. (REVTeX 4)
dc.identifierhttps://arxiv.org/abs/hep-ph/0102158
dc.identifierhttp://arxiv.org/abs/hep-ph/0102158
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40397
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titlePrimordial Galactic Magnetic Fields: An Application of QCD Domain Walls
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