High Energy Cosmic Rays (eBook, PDF) - Stanev, Todor
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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,…mehr

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Produktbeschreibung
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.

Autorenporträt
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.

Rezensionen
From the reviews of the first edition:

"... carefully crafted and well-written." (Stefan Westerhoff, Columbia University, Physics Today, September 2004)

"This publication ... is aimed at serious students of the subject. ... Arranged in two parts, Stanev first describes the standard model of cosmic rays and the interactions that are important ... . The second part describes the challenges of current cosmic ray research ... . It is a 'must read' for those with a passion to find out more about the high energy universe." (Roger Feasey, Journal of the Auckland Astronomical Society AAS, August, 2005)

"Todor Stanev ... has distilled the essence of cosmic ray physics. It is a magnificent achievement and will be invaluable for workers in the field. It should also be available for consultation by researchers in related disciplines ... there will also be a need to make use of excellent list of referenced material." (Roger Clay, The Physicist, Vol. 41 (5), September/October, 2004)