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Gamma-ray and neutrino signatures of...

Celli, Silvia.

Gamma-ray and neutrino signatures of galactic cosmic-ray accelerators

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Gamma-ray and neutrino signatures of galactic cosmic-ray acceleratorsby Silvia Celli.
作者:	Celli, Silvia.
出版者:	Cham :Springer International Publishing :2019.
面頁冊數:	xxi, 252 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Galactic cosmic rays.
電子資源:	https://doi.org/10.1007/978-3-030-33124-5
ISBN:	9783030331245$q(electronic bk.)

Gamma-ray and neutrino signatures of galactic cosmic-ray accelerators
Celli, Silvia.

Gamma-ray and neutrino signatures of galactic cosmic-ray accelerators[electronic resource] /by Silvia Celli. - Cham :Springer International Publishing :2019. - xxi, 252 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

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.

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.

ISBN: 9783030331245$q(electronic bk.)

Standard No.: 10.1007/978-3-030-33124-5doiSubjects--Topical Terms:

857007
Galactic cosmic rays.

LC Class. No.: QC485.9.G34 / C45 2019

Dewey Class. No.: 539.7223

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245 1 0 $a Gamma-ray and neutrino signatures of galactic cosmic-ray accelerators $h [electronic resource] / $c by Silvia Celli.
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520 $a 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.
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