| Campo DC | Valor | Idioma |
|---|
| dc.contributor.author | Pepe, Iuri Muniz | - |
| dc.contributor.author | Abraham, J. | - |
| dc.contributor.author | Abreu, P. | - |
| dc.contributor.author | Aglietta, M. | - |
| dc.contributor.author | Aguirre, C. | - |
| dc.creator | Pepe, Iuri Muniz | - |
| dc.creator | Abraham, J. | - |
| dc.creator | Abreu, P. | - |
| dc.creator | Aglietta, M. | - |
| dc.creator | Aguirre, C. | - |
| dc.date.accessioned | 2013-11-29T19:12:52Z | - |
| dc.date.available | 2013-11-29T19:12:52Z | - |
| dc.date.issued | 2008 | - |
| dc.identifier.issn | 0031-9007 | - |
| dc.identifier.uri | http://repositorio.ufba.br/ri/handle/ri/14021 | - |
| dc.description | p. 1-7 | pt_BR |
| dc.description.abstract | The energy spectrum of cosmic rays above 2.5×1018 eV, derived from 20 000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J∝E-γ, at energies between 4×1018 eV and 4×1019 eV is 2.69±0.02(stat)±0.06(syst), steepening to 4.2±0.4(stat)±0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz’min. | pt_BR |
| dc.language.iso | en | pt_BR |
| dc.rights | Acesso Aberto | pt_BR |
| dc.source | http://dx.doi.org/10.1103/PhysRevLett.101.061101 | pt_BR |
| dc.subject | Física nuclear | pt_BR |
| dc.subject | Raios cosmicos | pt_BR |
| dc.title | Observation of the suppression of the flux of cosmic rays above 4×1019eV | pt_BR |
| dc.title.alternative | Physical Review Letters | pt_BR |
| dc.type | Artigo de Periódico | pt_BR |
| dc.identifier.number | v. 101, n. 6 | pt_BR |
| dc.publisher.country | Brasil | pt_BR |
| Aparece nas coleções: | Artigo Publicado em Periódico (FIS)
|
