Magnetic Fields from Bubble Collisions - A Progress Report

dc.creatorTornkvist, Ola
dc.date1999-02-22
dc.date1999-02-23
dc.date.accessioned2026-07-07T04:06:29Z
dc.date.available2026-07-07T04:06:29Z
dc.descriptionPrimordial magnetic fields may be created in collisions of expanding bubbles in a first-order cosmological phase transition and later serve as seed fields for galactic magnetic fields. Here I present results from numerical and analytical studies of U(1) bubble collisions done in collaboration with Ed Copeland and Paul Saffin. I also reveal preliminary results from analytical studies of SU(2)xU(1) bubble collisions, which provide first evidence that magnetic fields are created in electroweak two-bubble collisions.
dc.description6 pages, plain LaTeX. Figure 1 also available in COLOUR from http://www.damtp.cam.ac.uk/user/ot202/sewm98/ . Summary of presentations given at the International Conference on Strong and Electroweak Matter (SEWM-98), Copenhagen, Denmark, 2-5 Dec 1998, and at the 19th Texas Symposium on Relativistic Astrophysics, Paris, 14-18 Dec 1998, to appear in both proceedings. Typo corrected
dc.identifierhttps://arxiv.org/abs/hep-ph/9902432
dc.identifierhttp://arxiv.org/abs/hep-ph/9902432
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48787
dc.subjectHigh Energy Physics - Phenomenology
dc.titleMagnetic Fields from Bubble Collisions - A Progress Report
dc.typetext

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