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

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Springer Theses

ISBN: 3030331261
ISBN 13: 9783030331269
Autor: Celli, Silvia
Verlag: Springer Verlag GmbH
Umfang: xxi, 252 S., 8 s/w Illustr., 83 farbige Illustr., 252 p. 91 illus., 83 illus. in color.
Erscheinungsdatum: 02.01.2021
Auflage: 1/2019
Produktform: Kartoniert
Einband: KT

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.

Artikelnummer: 369172 Kategorie:

Beschreibung

Autorenporträt

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.

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