Large scale structure in the intergalactic magnetic field and ultra-high energy cosmic ray propagation

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dc.creatorTanco, Gustavo Medina
dc.date1998-07-31
dc.date.accessioned2026-07-07T02:27:31Z
dc.date.available2026-07-07T02:27:31Z
dc.descriptionThe possibility that the magnetic field is strongly correlated with the large-scale structure of the universe has been recently proposed in the literature. In this scenario the intergalactic magnetic field has a strong (m Gauss) regular component spanning tens of Mpc. This could have severe consequences on the propagation of ultra-high energy cosmic rays, and the observed spectra, isotropy and composition. A quantitative discussion of these effects is given in the present work.
dc.description4 pages, talk at 16th ECRS, University of Alcala, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9807344
dc.identifierhttp://arxiv.org/abs/astro-ph/9807344
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12727
dc.subjectAstrophysics
dc.titleLarge scale structure in the intergalactic magnetic field and ultra-high energy cosmic ray propagation
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