Propagation of CR Nuclei: Our Results

  • Daniele Gaggero
Part of the Springer Theses book series (Springer Theses)


Hadrons are the most abundant particles of the CR flux and it is natural to start with this dominant component. In this chapter I will describe how to build a CR propagation model, which assumptions are necessary on the source term, the gas distribution and other astrophysical inputs.


Convective Velocity Particle Dark Matter Diffusion Halo Injection Spectrum Local Interstellar Spectrum 
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© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  • Daniele Gaggero
    • 1
  1. 1.Instituto Nazionale di Fisica Nucleare (INFN)—Sezione di PisaPisaItaly

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