Subir material

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

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2019-09-26T13:09:33Z
dc.date.available 2019-09-26T13:09:33Z
dc.date.issued 2001-06-30
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82052
dc.description.abstract The observation of cosmic ray particles with unexpected high energies is pushing astroparticle physics into a period of rapid progress both theoretically and experimentally. Different proposed models for the generation of these particles are constrained by the absence of the predicted GZK cutoff in the cosmic ray spectrum and by the composition and the distribution of arrival directions observed. The database increase due to the Pierre Auger Observatory will provide a clearer picture of the spectral anisotropy and properties of such high energy particles, enabling tests of their origin and nature. en
dc.language en es
dc.subject Radiación cósmica es
dc.subject Altas energías es
dc.subject astroparticle physics es
dc.title Future directions in astroparticle physics and the Auger experiment en
dc.type Objeto de conferencia es
sedici.identifier.uri http://inspirehep.net/record/539986 es
sedici.creator.person Dova, María Teresa 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 Objeto de conferencia 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.date.exposure 2000-10
sedici.relation.event 30th International Symposium on Multiparticle Dynamics (ISMD 2000) (Tihany, Hungary, October 9-15, 2000) es
sedici.description.peerReview peer-review es


Descargar archivos

Thumbnail
Documento completo
Descargar archivo (232.3Kb) - PDF
Icon
Enlace externo

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)