Cosmic ray diffusion in the galaxy and diffuse gamma emission
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 use...
محفوظ في:
| المؤلف الرئيسي: | |
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| التنسيق: | Thèse numérique |
| اللغة: | Anglais |
| منشور في: |
Berlin, Heidelberg :
Springer Berlin Heidelberg
[20..].
Cham : Springer Nature |
| الطبعة: | 1st ed. 2012. |
| سلاسل: | Springer Theses, Recognizing Outstanding Ph.D. Research
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| الموضوعات: | |
| الوصول للمادة أونلاين: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| ملاحظة: |
L'impression du document génère 140 p. Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission, Texte imprimé, 9783642299506 • Cosmic ray diffusion in the galaxy and diffuse gamma emission, Daniele Gaggero, Heidelberg, Springer, 2012, 1 vol. (XI-146 p.), Springer Theses, 978-3-642-29948-3 • Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission, Texte imprimé, 9783662510018 |
| الملخص: | 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 |
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| وصف المادة: | L'impression du document génère 140 p. Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| ردمك: | 3642299490 (en ligne) 9783642299490 (en ligne) |
| تدمد: | 2190-5061 |
| وصول: | Accès en ligne pour les établissements français bénéficiaires des licences nationales Accès soumis à abonnement pour tout autre établissement Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 |