Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission

  • Daniele Gaggero

Part of the Springer Theses book series (Springer Theses)

Table of contents

  1. Front Matter
    Pages i-xi
  2. Daniele Gaggero
    Pages 1-5
  3. Daniele Gaggero
    Pages 7-28
  4. Daniele Gaggero
    Pages 35-57
  5. Daniele Gaggero
    Pages 59-109
  6. Daniele Gaggero
    Pages 111-126
  7. Daniele Gaggero
    Pages 127-130
  8. Back Matter
    Pages 131-146

About this book


The original work presented in this thesis constitutes an important contribution to modern Cosmic Ray (CR) physics, and comes during one of the most exciting periods of this field.
The first part introduces a new numerical code (DRAGON) to model the CR propagation in our Galaxy. The code is then used to perform a combined analysis of CR data, making it possible to determine their propagation properties with unprecedented accuracy.
The second part is dedicated to a theoretical interpretation of the recent crucial experimental results on cosmic electron and positron spectra (PAMELA, Fermi-LAT experiments).  Using the tools developed in the first part of the thesis, the author convincingly argues for the existence of a new spectral component, which could arise either from local astrophysical sources, such as pulsars, or from Dark Matter annihilation or decay.
This thesis is a highly advanced work; the methods, analysis and results are clearly and carefully presented.  This work is set to become an important reference document for any future work in this area.


Cosmic Ray Electrons Cosmic Ray Physics Cosmic Ray Positrons Cosmic Ray Propagation DRAGON Code Diffuse Gamma Ray Emission Fermi-LAT Numerical Solution of Cosmic Ray Diffusion Equation Positron Anomaly Positron Excess

Authors and affiliations

  • Daniele Gaggero
    • 1
  1. 1.INFN - Sezione di PisaPisaItaly

Bibliographic information

  • DOI
  • Copyright Information Springer-Verlag Berlin Heidelberg 2012
  • Publisher Name Springer, Berlin, Heidelberg
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-3-642-29948-3
  • Online ISBN 978-3-642-29949-0
  • Series Print ISSN 2190-5053
  • Series Online ISSN 2190-5061
  • Buy this book on publisher's site