Advertisement

© 2019

Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators

Book
  • 513 Downloads

Part of the Springer Theses book series (Springer Theses)

Table of contents

  1. Front Matter
    Pages i-xxi
  2. Silvia Celli
    Pages 1-47
  3. Silvia Celli
    Pages 85-142
  4. Silvia Celli
    Pages 143-168
  5. Silvia Celli
    Pages 189-193
  6. Back Matter
    Pages 195-252

About this book

Introduction

This book addresses three “hot” topics concerning the general problem of the origin of Galactic cosmic rays, namely (1) the acceleration, propagation, and radiation of particles in supernova remnants; (2) very high energy neutrinos from the Galactic Center; and (3) the potential held by the next-generation gamma-ray and neutrino detectors CTA and KM3NeT for studying extended non-thermal sources in the Galaxy. The topics are intrinsically connected to determining the nature (“hadronic or leptonic?”) of gamma-ray emissions from young and middle-aged supernova remnants and the search for cosmic-ray PeVatrons. The results and conclusions provided here are based on extensive analytical and numerical simulations, which are formulated and presented in a straightforward format that can be readily used in the interpretations of gamma-ray and neutrino observations, as well as for confident predictions for future measurements.

Keywords

The Origin of Cosmic Rays Galactic Cosmic-Ray Pevatrons Supernova Remnants The Galactic Center region Particle Acceleration in Supernova Shocks Particle Escape From Supernova Shocks Radiation From Supernova Remnants Neutrinos and Gamma Rays From Hadronic Processes Clumpy Interstellar Medium The Magneto-Hydrodinamics of Shock-Clump Interaction

Authors and affiliations

  1. 1.Department of PhysicsGran Sasso Science InstituteL’AquilaItaly

About the authors

Silvia Celli received her Ph.D. in Astroparticle Physics from Gran Sasso Science Institute in 2019. Later, she has been working as a researcher at the Max-Planck-Institut für Kernphysik in Heidelberg (Germany). Her main research interests are related to the high-energy emissions of astrophysical sources in the multi-messenger framework, in particular to the gamma-ray and neutrino signatures of Galactic cosmic-ray accelerators. She is a member of three large international scientific collaborations, namely ANTARES, CTA, and KM3NeT. 

Bibliographic information

  • Book Title Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators
  • Authors Silvia Celli
  • Series Title Springer Theses
  • Series Abbreviated Title Springer Theses
  • DOI https://doi.org/10.1007/978-3-030-33124-5
  • Copyright Information Springer Nature Switzerland AG 2019
  • Publisher Name Springer, Cham
  • eBook Packages Physics and Astronomy Physics and Astronomy (R0)
  • Hardcover ISBN 978-3-030-33123-8
  • Softcover ISBN 978-3-030-33126-9
  • eBook ISBN 978-3-030-33124-5
  • Series ISSN 2190-5053
  • Series E-ISSN 2190-5061
  • Edition Number 1
  • Number of Pages XXI, 252
  • Number of Illustrations 8 b/w illustrations, 83 illustrations in colour
  • Topics Astrophysics and Astroparticles
  • Buy this book on publisher's site