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dc.date.accessioned 2021-08-23T17:02:17Z
dc.date.available 2021-08-23T17:02:17Z
dc.date.issued 1998
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/123164
dc.description.abstract We re-examine the interaction of ultra high energy nuclei with the microwave background radiation. We find that the giant dipole resonance leaves a new signature in the differential energy spectrum of iron sources located around 3 Mpc: A depression before the bump which is followed by the expected cutof en
dc.format.extent 7103-7107 es
dc.language en es
dc.subject Cosmic ray es
dc.subject Physics es
dc.subject Resonance (particle physics) es
dc.subject Dipole es
dc.subject Energy (signal processing) es
dc.subject Cosmic microwave background es
dc.subject Cutoff es
dc.subject Astrophysics es
dc.subject Cosmic background radiation es
dc.subject Ultra-high-energy cosmic ray es
dc.title A depression before a bump in the highest energy cosmic ray spectrum en
dc.type Articulo es
sedici.identifier.other arXiv:astro-ph/9708082 es
sedici.identifier.other doi:10.1103/physrevd.57.7103 es
sedici.identifier.issn 0556-2821 es
sedici.identifier.issn 1089-4918 es
sedici.creator.person Anchordoqui, Luis Alfredo es
sedici.creator.person Dova, María Teresa es
sedici.creator.person Epele, Luis Beltrán es
sedici.creator.person Swain, John es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physical Review D es
sedici.relation.journalVolumeAndIssue vol. 57, no. 12 es


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