Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators
(Sprache: Englisch)
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;...
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Klappentext zu „Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators “
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.
Inhaltsverzeichnis zu „Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators “
Introduction.- Propagation and Radiation of Accelerated Particles In Super-Nova Remnants With Clumpy Structures.- Particle Escape From Supernova Remnants.- The Galactic Center Region.- Sensitivity studies for Gamma-Ray and Neutrino Telescopes.- Summary and Conclusions.- Appendix.
Autoren-Porträt von Silvia Celli
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.
Bibliographische Angaben
- Autor: Silvia Celli
- 2021, 1st ed. 2019, XXI, 252 Seiten, 83 farbige Abbildungen, Maße: 15,5 x 23,5 cm, Kartoniert (TB), Englisch
- Verlag: Springer, Berlin
- ISBN-10: 3030331261
- ISBN-13: 9783030331269
Sprache:
Englisch
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