|
|
|
|
| LEADER |
02974nam a2200457 4500 |
| 001 |
978-3-030-33124-5 |
| 003 |
DE-He213 |
| 005 |
20191218161139.0 |
| 007 |
cr nn 008mamaa |
| 008 |
191217s2019 gw | s |||| 0|eng d |
| 020 |
|
|
|a 9783030331245
|9 978-3-030-33124-5
|
| 024 |
7 |
|
|a 10.1007/978-3-030-33124-5
|2 doi
|
| 040 |
|
|
|d GrThAP
|
| 050 |
|
4 |
|a QB460-466
|
| 072 |
|
7 |
|a PHVB
|2 bicssc
|
| 072 |
|
7 |
|a SCI005000
|2 bisacsh
|
| 072 |
|
7 |
|a PHVB
|2 thema
|
| 082 |
0 |
4 |
|a 523.01
|2 23
|
| 100 |
1 |
|
|a Celli, Silvia.
|e author.
|4 aut
|4 http://id.loc.gov/vocabulary/relators/aut
|
| 245 |
1 |
0 |
|a Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators
|h [electronic resource] /
|c by Silvia Celli.
|
| 250 |
|
|
|a 1st ed. 2019.
|
| 264 |
|
1 |
|a Cham :
|b Springer International Publishing :
|b Imprint: Springer,
|c 2019.
|
| 300 |
|
|
|a XXI, 252 p. 91 illus., 83 illus. in color.
|b online resource.
|
| 336 |
|
|
|a text
|b txt
|2 rdacontent
|
| 337 |
|
|
|a computer
|b c
|2 rdamedia
|
| 338 |
|
|
|a online resource
|b cr
|2 rdacarrier
|
| 347 |
|
|
|a text file
|b PDF
|2 rda
|
| 490 |
1 |
|
|a Springer Theses, Recognizing Outstanding Ph.D. Research,
|x 2190-5053
|
| 505 |
0 |
|
|a 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.
|
| 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.
|
| 650 |
|
0 |
|a Astrophysics.
|
| 650 |
1 |
4 |
|a Astrophysics and Astroparticles.
|0 http://scigraph.springernature.com/things/product-market-codes/P22022
|
| 710 |
2 |
|
|a SpringerLink (Online service)
|
| 773 |
0 |
|
|t Springer eBooks
|
| 776 |
0 |
8 |
|i Printed edition:
|z 9783030331238
|
| 776 |
0 |
8 |
|i Printed edition:
|z 9783030331252
|
| 776 |
0 |
8 |
|i Printed edition:
|z 9783030331269
|
| 830 |
|
0 |
|a Springer Theses, Recognizing Outstanding Ph.D. Research,
|x 2190-5053
|
| 856 |
4 |
0 |
|u https://doi.org/10.1007/978-3-030-33124-5
|z Full Text via HEAL-Link
|
| 912 |
|
|
|a ZDB-2-PHA
|
| 950 |
|
|
|a Physics and Astronomy (Springer-11651)
|
