00970nam a2200253 i 4500991002201589707536 0521842980b13491106-39ule_instDip.to Studi Storiciita872.01Karakasis, Evangelos476955Terence and the language of Roman comedy /Evangelos KarakasisCambridge [etc.] :Cambridge University Press,2005XIV, 309 p. ;23 cmCambridge classical studiesCon bibliografiaTerentius Afro, Publius,sec. II a.C.Lingua.b1349110628-01-1406-03-07991002201589707536LE023 872.01 KAR 1 1 12023000092187le023-E77.81-l- 00000.i1438540506-03-07Terence and the language of roman comedy988703UNISALENTOle02306-03-07ma -engxxk0002901nam 22004935 450 991037393000332120250609110107.03-030-33124-510.1007/978-3-030-33124-5(CKB)4100000010011886(MiAaPQ)EBC5997263(DE-He213)978-3-030-33124-5(PPN)242819214(MiAaPQ)EBC5997219(EXLCZ)99410000001001188620191217d2019 u| 0engurcnu||||||||txtrdacontentcrdamediacrrdacarrierGamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators /by Silvia Celli1st ed. 2019.Cham :Springer International Publishing :Imprint: Springer,2019.1 online resource (264 pages)Springer Theses, Recognizing Outstanding Ph.D. Research,2190-50533-030-33123-7 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.Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053AstrophysicsAstrophysics and Astroparticleshttps://scigraph.springernature.com/ontologies/product-market-codes/P22022Astrophysics.Astrophysics and Astroparticles.523.01539.7223Celli Silviaauthttp://id.loc.gov/vocabulary/relators/aut837267MiAaPQMiAaPQMiAaPQBOOK9910373930003321Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators1870719UNINA