We consider the scenario in which the knee in the cosmic ray spectrum is due to a change in the escape mechanism of cosmic rays from the Galaxy from one dominated by transverse diffusion to one dominated by drifts. We show that this scenario explains not only the changes in spectral slope at the knee and at the second knee, but can also account for the main characteristics of the observed energy-dependent anisotropy amplitude and phase of first harmonic in the energy range between 10¹⁵ and 10¹⁸ eV. This provides a useful handle to distinguish this diffusion/drift model from other scenarios proposed to explain the knee in the spectrum.
Información general
Fecha de publicación:8 de mayo de 2003
Idioma del documento:Inglés
Revista:Journal of Cosmology and Astroparticle Physics; vol. 2003, no. 5
Institución de origen:Facultad de Ciencias Exactas
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)