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dc.date.accessioned 2019-04-17T16:45:19Z
dc.date.available 2019-04-17T16:45:19Z
dc.date.issued 2001-06-04
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/74307
dc.description.abstract Ultrahigh energy cosmic rays present a major unsolved puzzle. Not only do we not know their origin, but we also have no really solid evidence that they are protons or iron nuclei—the two most popular candidates. We examine briefly a couple of “nonstandard” possibilities: light magnetic monopoles, which are rather exotic, and nuclei heavier than iron, which are perhaps less exotic, but have many attractive features. en
dc.format.extent 295-300 es
dc.language en es
dc.subject Física es
dc.subject ultrahigh energy cosmic rays en
dc.subject protons en
dc.subject iron nuclei en
dc.title Exotic and not-so-exotic candidates for ultrahigh energy cosmic rays en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.1063/1.1378639
sedici.identifier.issn 0094-243X es
sedici.creator.person Swain, John es
sedici.creator.person Anchordoqui, Luis Alfredo es
sedici.creator.person Dova, María Teresa es
sedici.creator.person McCauley, T. es
sedici.creator.person Paul, T. es
sedici.creator.person Reucroft, S. es
sedici.subject.materias Ciencias Exactas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo 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 AIP Conference Proceedings es
sedici.relation.journalVolumeAndIssue vol. 566, no. 295 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)