On Primordial Magnetic Fields
| dc.creator | Enqvist, Kari | |
| dc.date | 1994-05-18 | |
| dc.date.accessioned | 2026-07-07T03:56:51Z | |
| dc.date.available | 2026-07-07T03:56:51Z | |
| dc.description | A primordial magnetic field could be responsible for the observed magnetic fields of the galaxies. One possibility is that such a primordial field is generated at the electroweak phase transition because of the fluctuations in the Higgs field gradients. I describe a statistical averaging procedure which gives rise to a field of a correct magnitude. Another possibility, where the Yang-Mills vacuum itself is ferrromagnetic, is also discussed. | |
| dc.description | 12 pages, LaTeX. No figures. NORDITA-94/24 P. (Talk given at the NATO workshop "Electroweak Physics and the Early Universe", Sintra, Portugal, March 1994.) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9405315 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9405315 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45156 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | On Primordial Magnetic Fields | |
| dc.type | text |