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dc.contributor.authorBorges, Ernesto Pinheiro-
dc.contributor.authorTsallis, Constantino-
dc.contributor.authorAnjos, João C.-
dc.creatorBorges, Ernesto Pinheiro-
dc.creatorTsallis, Constantino-
dc.creatorAnjos, João C.-
dc.date.accessioned2014-02-13T17:29:01Z-
dc.date.issued2003-
dc.identifier.issn0375-9601-
dc.identifier.urihttp://repositorio.ufba.br/ri/handle/ri/14594-
dc.descriptionTexto completo: acesso restrito. p. 372–376pt_BR
dc.description.abstractThe analysis of cosmic rays fluxes as a function of energy reveals a knee slightly below 1016 eV and an ankle close to 1019 eV. Their physical origins remain up to now quite enigmatic; in particular, no elementary process is known which occurs at energies close to 1016 eV. We propose a phenomenological approach along the lines of nonextensive statistical mechanics, a formalism which contains Boltzmann–Gibbs statistical mechanics as a particular case. The knee then appears as a crossover between two fractal-like thermal regimes, the crossover being caused by process occurring at energies ten million times lower than that of the knee, in the region of the quark hadron transition (≃109 eV). This opens the door to an unexpected standpoint for further clarifying the phenomenon.pt_BR
dc.language.isoenpt_BR
dc.rightsAcesso Abertopt_BR
dc.sourcehttp://dx.doi.org.ez10.periodicos.capes.gov.br/10.1016/S0375-9601(03)00377-3pt_BR
dc.subjectRaios cósmicospt_BR
dc.subjectFísica nuclearpt_BR
dc.titleFluxes of cosmic rays: a delicately balanced stationary statept_BR
dc.title.alternativePhysics Letters Apt_BR
dc.typeArtigo de Periódicopt_BR
dc.identifier.numberv. 310, n. 5-6pt_BR
dc.embargo.liftdate10000-01-01-
Aparece nas coleções:Artigo Publicado em Periódico (FIS)

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