LEADER 01056nam a22002771i 4500 001 991002196849707536 005 20030922151837.0 008 030925s1997 it |||||||||||||||||ita 035 $ab12255476-39ule_inst 035 $aARCHE-030308$9ExL 040 $aBiblioteca Interfacoltà$bita$cA.t.i. Arché s.c.r.l. Pandora Sicilia s.r.l. 082 04$a272 100 1 $aWurmbrand, Richard$0452650 245 10$aTorturato per Cristo :$bl'intramontabile testimonianza della Chiesa clandestina nei paesi dietro la cortina di ferro /$cRichard Wurmbrand 250 $a7. ed. 260 $aMarchirolo :$bEUN,$c1997 300 $a1 v. ;$c24 cm 440 0$aTascabili Eun 650 4$aWurmbrand, Richard$xPrigionia 765 0 $tTortured for Christ 907 $a.b12255476$b02-04-14$c08-10-03 912 $a991002196849707536 945 $aLE002 Busta 186/1$g1$i2002000033307$lle002$o-$pE0.00$q-$rl$s- $t0$u0$v0$w0$x0$y.i12644584$z08-10-03 996 $aTorturato per Cristo$9151635 997 $aUNISALENTO 998 $ale002$b08-10-03$cm$da $e-$fita$git $h0$i1 LEADER 02901nam 22004935 450 001 9910373930003321 005 20250609110107.0 010 $a3-030-33124-5 024 7 $a10.1007/978-3-030-33124-5 035 $a(CKB)4100000010011886 035 $a(MiAaPQ)EBC5997263 035 $a(DE-He213)978-3-030-33124-5 035 $a(PPN)242819214 035 $a(MiAaPQ)EBC5997219 035 $a(EXLCZ)994100000010011886 100 $a20191217d2019 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aGamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators /$fby Silvia Celli 205 $a1st ed. 2019. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2019. 215 $a1 online resource (264 pages) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 08$a3-030-33123-7 327 $aIntroduction -- 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. 330 $aThis book addresses three ?hot? topics concerning the general problem of the origin of Galactic cosmic rays, namely (1) the acceleration, propagation, and radiation of particles in supernova remnants; (2) very high energy neutrinos from the Galactic Center; and (3) the potential held by the next-generation gamma-ray and neutrino detectors CTA and KM3NeT for studying extended non-thermal sources in the Galaxy. The topics are intrinsically connected to determining the nature (?hadronic or leptonic??) of gamma-ray emissions from young and middle-aged supernova remnants and the search for cosmic-ray PeVatrons. The results and conclusions provided here are based on extensive analytical and numerical simulations, which are formulated and presented in a straightforward format that can be readily used in the interpretations of gamma-ray and neutrino observations, as well as for confident predictions for future measurements. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstrophysics 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 615 0$aAstrophysics. 615 14$aAstrophysics and Astroparticles. 676 $a523.01 676 $a539.7223 700 $aCelli$b Silvia$4aut$4http://id.loc.gov/vocabulary/relators/aut$0837267 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910373930003321 996 $aGamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators$91870719 997 $aUNINA