2002/12/31 by Leonard S. Kisslinger
Physics and Astronomy · #Cosmology and Gravitation Theories #Pulsars and Gravitational Waves Research #Quantum Chromodynamics and Particle Interactions #hep-ph
paper · pdf · doi:10.1103/physrevd.68.043516
published as Phys.Rev. D68 (2003) 043516 · Eight pages, one figure, revtex. In revised version details of the derivation of the magnetic wall is given, and a comparison with inflationary models is given in the figure
arxiv created 2003/03/24 · openalex publication_date 2003/08/28 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Possible cosmic microwave background radiation (CMBR) correlations are estimated for a model in which a Hubble-size magnetic wall is formed during the QCD chiral phase transition. Measurable polarization correlations are found for l values greater than about 1000. It is also found that metric perturbations from the wall could give rise to observable CMBR correlations for large l.