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High Energy Cosmic Rays
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High Energy Cosmic Rays

High Energy Cosmic Rays

Todor Stanev

342 pages, parution le 01/06/2021

Résumé

Offers an accessible text and reference (a cosmic-ray manual) for graduate students entering the field and high-energy astrophysicists will find this an accessible cosmic-ray manual

Easy to read for the general astronomer, the first part describes the standard model of cosmic rays based on our understanding of modern particle physics.

Offers an accessible text and reference (a cosmic-ray manual) for graduate students entering the field and high-energy astrophysicists will find this an accessible cosmic-ray manual

Easy to read for the general astronomer, the first part describes the standard model of cosmic rays based on our understanding of modern particle physics.

Presents the acceleration scenario in some detail in supernovae explosions as well as in the passage of cosmic rays through the Galaxy.

Compares experimental data in the atmosphere as well as underground are compared with theoretical models

  • Overview
  • Part I:The Standard Model of Cosmic Rays.- Cosmic ray interactions.- The birth of cosmic rays.- Cosmic rays in the Galaxy.- Cosmic rays at the top of the atmosphere.- Cosmic rays in the atmosphere.- Cosmic rays underground.-
  • Part II Contemporary Challenges.- Cosmic ray showers.- The end of the cosmic ray spectrum.- High energy neutrino and gamma-ray astronomy.
  • Appendix
  • References
  • Index

Todor Stanev is professor for astrophysics in the Department of Physics and Astronomy at the University of Delaware. He is a member of the IceCube neutrino observatory collaboration.

Caractéristiques techniques

  PAPIER
Éditeur(s) Springer
Auteur(s) Todor Stanev
Parution 01/06/2021
Nb. de pages 342
EAN13 9783030715663

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