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High Energy Cosmic Rays

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  • © 2021

Overview

  • Third updated edition of a successful book used for study and reference of cosmic ray astrophysics
  • Covers the very latest topics in cosmic ray research, including high energy neutrino and gamma-ray astronomy
  • Allows the understanding of theoretical models and experimental results without working through the mathematics

Part of the book series: Astrophysics and Space Science Library (ASSL, volume 462)

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Table of contents (10 chapters)

  1. The Standard Model of Cosmic Rays

  2. Contemporary Challenges

Keywords

About this book

This book on high-energy cosmic rays deals in its first part with the standard model of cosmic rays, describing how they are born in a wide range of cosmic processes, how they are accelerated and how they interact with matter, magnetic fields and radiation during their journey across the Galaxy. In its second part the book presents contemporary challenges in very high energy cosmic rays, with focus on their detection in the Earth’s atmosphere and underground, as well as new developments in gamma-ray and neutrino astronomy.

A decade after the publication of the second edition of this book, there are many new experimental results in the fields of high energy neutrino astronomy and in the whole energy range of detection of gamma-rays. There have also been many attempts for studies for multi-messenger events in these and all other fields. These new experimental efforts and their results are covered in this third edition. This is accompanied by a general analysis of these new results and the additional knowledge that they bring to our understanding of cosmic rays and their propagation in our Galaxy and extragalactic space.
A large part of the interpretation of these new findings is related to the development of the hadronic interaction models that we use to understand and describe the experimental results. The author describes the relation between the new high energy physics experiments and such models.

In addition to the discussion of new research, descriptions and graphs of the previous edition have been updated where appropriate. The third edition ends with a discussion of some possible and already planned experiments for future observations and an explanation of their importance for the better understanding of all processes that lead to the increase of our knowledge of high energy cosmic rays.
Students and lecturers of advanced undergraduate courses on cosmic rays and astroparticle physics as well as post-graduates and researchers will continue tofind this book a valuable source of learning and reference.

  

Authors and Affiliations

  • University of Delaware Bartol Research Institute, Newark, USA

    Todor Stanev

About the author

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.

  

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