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dc.date.accessioned 2019-09-12T14:57:09Z
dc.date.available 2019-09-12T14:57:09Z
dc.date.issued 2001-04
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/81068
dc.description.abstract We critically review the common belief that ultrahigh energy cosmic rays are protons or atomic nuclei with masses not exceeding that of iron. We find that heavier nuclei are indeed possible, and discuss possible sources and acceleration mechanisms for such primaries. We also show detailed simulations of extensive air showers produced by “superheavy” nuclei, and discuss prospects for their detection in future experiments. en
dc.format.extent 203-206 es
dc.language en es
dc.subject Radiación cósmica es
dc.subject Cascada atmosférica extensa es
dc.title A pot of gold at the end of the cosmic “raynbow”? en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.1016/S0920-5632(01)01264-6 es
sedici.identifier.issn 0920-5632 es
sedici.creator.person Anchordoqui, Luis Alfredo es
sedici.creator.person Dova, María Teresa es
sedici.creator.person McCauley, Thomas es
sedici.creator.person Paul, Thomas es
sedici.creator.person Reucroft, Stephen es
sedici.creator.person Swain, John es
sedici.subject.materias Ciencias Exactas es
sedici.subject.materias Física 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 Nuclear Physics B - Proceedings Supplements es
sedici.relation.journalVolumeAndIssue vol. 97, no. 1-3 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)