Cosmologial magnetic field amplification around z~100

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dc.creatorCalzetta, Esteban A.
dc.creatorKandus, Alejandra
dc.date1999-01-03
dc.date1999-04-26
dc.date.accessioned2026-07-07T02:29:52Z
dc.date.available2026-07-07T02:29:52Z
dc.descriptionWe study the corrections to the conformal evolution of primordial magnetic fields after recombination, produced by the fall of the ionized fraction of matter into the dark matter gravitational wells. This effect enhances the field around the protostructures being formed, and might help to understand the fields observed in galaxy clusters and hydrogen clouds.
dc.description35 pages, essential addings,uses AASLaTex macros, submitted to ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/9901009
dc.identifierhttp://arxiv.org/abs/astro-ph/9901009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13639
dc.subjectAstrophysics
dc.titleCosmologial magnetic field amplification around z~100
dc.typetext

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