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dc.date.accessioned 2019-08-22T14:19:45Z
dc.date.available 2019-08-22T14:19:45Z
dc.date.issued 1997-02
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/79534
dc.description.abstract In this work we re-examine the influence of the microwave background radiation on the propagation of extremely high energy cosmic rays. We present a recalculation of the rate of fractional energy loss in the continuous energy loss approximation including the effects of resonances other than the Δ. We also discuss the distortion of the cosmic ray spectrum due to interactions with the relic photons. en
dc.format.extent 249-252 es
dc.language en es
dc.subject Radiación cósmica es
dc.subject Efectos de la Radiación es
dc.title Opacity of the microwave background radiation to ultrahigh energy cosmic rays en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.1016/S0920-5632(96)00898-5
sedici.identifier.issn 0550-3213 es
sedici.creator.person Anchordoqui, Luis Alfredo es
sedici.creator.person Dova, María Teresa es
sedici.creator.person Epele, Luis Nicolás es
sedici.creator.person Swain, John D. 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 es
sedici.relation.journalVolumeAndIssue vol. 52, no. 3 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)