國立虎尾科技大學 |

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

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators/ by Silvia Celli.
作者:	Celli, Silvia.
面頁冊數:	XXI, 252 p. 91 illus., 83 illus. in color.online resource. :
Contained By:	Springer Nature eBook
標題:	Astrophysics. -
電子資源:	https://doi.org/10.1007/978-3-030-33124-5
ISBN:	9783030331245

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. - 1st ed. 2019. - XXI, 252 p. 91 illus., 83 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.

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

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

646223
Astrophysics.

LC Class. No.: QB460-466

Dewey Class. No.: 523.01

Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators
LDR:02674nam a22004095i 4500 001 1008197
003 DE-He213
005 20200701083234.0
007 cr nn 008mamaa
008 210106s2019 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
035 $a 978-3-030-33124-5
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 $3 1301997
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. $3 646223
650 1 4 $a Astrophysics and Astroparticles. $3 782546
710 2 $a SpringerLink (Online service) $3 593884
773 0 $t Springer Nature eBook
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 $3 1253569
856 4 0 $u https://doi.org/10.1007/978-3-030-33124-5
912 $a ZDB-2-PHA
912 $a ZDB-2-SXP
950 $a Physics and Astronomy (SpringerNature-11651)
950 $a Physics and Astronomy (R0) (SpringerNature-43715)