01046nam0-2200313 --450 991031214720332120190314110623.0978-88-7000-628-5IT2016-274420190314d2015----kmuy0itay5050 baitaproIT 001yy<<Il >>canzoniere Occitano LBiblioteca Apostolica Vaticana Vat. lat. 3206Beatrice SollaModenaMucchi2015478 p., [6] c. di tav.24 cmStudi, testi e manualiNuova serie19Subsidia al Corpus des troubadoursNuova serie14Con la trascrizione del manoscrittoCanzonieriManoscrittiVat. lat. 3206 <manoscritto ; Biblioteca apostolica vaticana>849.1322Solla,Beatrice762633ITUNINAREICATUNIMARCBK9910312147203321849.13 SOL 1Bibl.2019FLFBCFLFBCCanzoniere Occitano L1546283UNINA02723nam 2200481 450 99641843620331620210213172657.03-030-56810-510.1007/978-3-030-56810-8(CKB)4100000011457874(DE-He213)978-3-030-56810-8(MiAaPQ)EBC6350845(PPN)250221659(EXLCZ)99410000001145787420210213d2020 uy 0engurnn|008mamaatxtrdacontentcrdamediacrrdacarrierReheating after inflation /Kaloian Lozanov1st ed. 2020.Cham, Switzerland :Springer,[2020]©20201 online resource (IX, 92 p. 15 illus., 13 illus. in color.) SpringerBriefs in Physics,2191-54233-030-56809-1 Inflation and initial conditions for reheating -- Preheating: the decay of the infliaton condensate -- Non-linear reheating -- Reheating and High-Energy Physics models -- Observational implications and signatures of reheating.This book provides a pedagogical introduction to the rapidly growing field of reheating after inflation. It begins with a brief review of the inflationary paradigm and a motivation for why the reheating of the universe is an integral part of inflationary cosmology. It then goes on to survey different aspects of reheating in a chronological manner, starting from the young, empty and cold universe at the end of inflation, and going all the way to the hot and thermal universe at the beginning of the Big Bang nucleosynthesis epoch. Different particle production mechanisms are considered with a focus on the non-perturbative excitation of scalar fields at the beginning of reheating (fermionic and vector fields are also discussed). This is followed by a review of the subsequent non-linear dynamical processes, such as soliton formation and relativistic turbulence. Various thermalization processes are also discussed. High energy physics embeddings of phenomenological models as well as observational implications of reheating such as gravitational waves generation and imprints on the cosmic microwave background are also covered.SpringerBriefs in Physics,2191-5423AstrophysicsResearchBig bang theoryAstrophysicsResearch.Big bang theory.523.01Lozanov Kaloian843810MiAaPQMiAaPQMiAaPQBOOK996418436203316Reheating After Inflation1882676UNISA