Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2021-08-24T14:01:25Z
dc.date.available 2021-08-24T14:01:25Z
dc.date.issued 1998-10-08
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/123263
dc.description.abstract We study the propagation of ultra-high energy cosmic ray nuclei through the background of cosmic microwave and intergalactic infrared photons, using recent re-estimates for the density of the last ones. We perform a detailed Monte Carlo simulation to follow the disintegration histories of nuclei starting as Fe and reaching the Earth from extragalactic sources. We obtain the maximum energies of the arriving nuclear fragments as well as the mass composition as a function of the distance traveled. Cosmic rays with energies in excess of 2 × 1020 eV cannot originate from Fe nuclei produced in sources beyond 10 Mpc. en
dc.language en es
dc.subject High Energy Cosmic Rays es
dc.subject Electromagnetic Processes and Properties es
dc.title On the propagation of the highest energy cosmic ray nuclei en
dc.type Articulo es
sedici.identifier.other arXiv:astro-ph/9808104 es
sedici.identifier.other doi:10.1088/1126-6708/1998/10/009 es
sedici.identifier.issn 1029-8479 es
sedici.creator.person Epele, Luis Nicolás es
sedici.creator.person Roulet, Esteban 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 Journal of High Energy Physics es
sedici.relation.journalVolumeAndIssue vol. 1998, no. 10 es


Descargar archivos

Thumbnail
Documento completo
Descargar archivo (297.8Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

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)