LEADER 02723nam 2200481 450 001 996418436203316 005 20210213172657.0 010 $a3-030-56810-5 024 7 $a10.1007/978-3-030-56810-8 035 $a(CKB)4100000011457874 035 $a(DE-He213)978-3-030-56810-8 035 $a(MiAaPQ)EBC6350845 035 $a(PPN)250221659 035 $a(EXLCZ)994100000011457874 100 $a20210213d2020 uy 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aReheating after inflation /$fKaloian Lozanov 205 $a1st ed. 2020. 210 1$aCham, Switzerland :$cSpringer,$d[2020] 210 4$dİ2020 215 $a1 online resource (IX, 92 p. 15 illus., 13 illus. in color.) 225 1 $aSpringerBriefs in Physics,$x2191-5423 311 $a3-030-56809-1 327 $aInflation 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. 330 $aThis book provides a pedagogical introduction to the rapidly growing field of reheating after inflation. It begins with a brief review of the inflationary paradigm and a motivation for why the reheating of the universe is an integral part of inflationary cosmology. It then goes on to survey different aspects of reheating in a chronological manner, starting from the young, empty and cold universe at the end of inflation, and going all the way to the hot and thermal universe at the beginning of the Big Bang nucleosynthesis epoch. Different particle production mechanisms are considered with a focus on the non-perturbative excitation of scalar fields at the beginning of reheating (fermionic and vector fields are also discussed). This is followed by a review of the subsequent non-linear dynamical processes, such as soliton formation and relativistic turbulence. Various thermalization processes are also discussed. High energy physics embeddings of phenomenological models as well as observational implications of reheating such as gravitational waves generation and imprints on the cosmic microwave background are also covered. 410 0$aSpringerBriefs in Physics,$x2191-5423 606 $aAstrophysics$xResearch 606 $aBig bang theory 615 0$aAstrophysics$xResearch. 615 0$aBig bang theory. 676 $a523.01 700 $aLozanov$b Kaloian$0843810 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a996418436203316 996 $aReheating After Inflation$91882676 997 $aUNISA LEADER 01534oam 2200421 a 450 001 9910694509403321 005 20160204111308.0 035 $a(CKB)5470000002363600 035 $a(OCoLC)61762850 035 $a(EXLCZ)995470000002363600 100 $a20051003d2005 ua 0 101 0 $aeng 135 $aurmn| ||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aSchool meal programs$b[electronic resource] $ecompetitive foods are widely available and generate substantial revenues for schools : report to congressional requesters 210 1$a[Washington, D.C.] :$cU.S. Government Accountability Office,$d[2005] 215 $aiii pages, 59 unnumbered pages $cdigital, PDF file 300 $aTitle from title screen (viewed on Sept. 26, 2005). 300 $a"August 2005." 300 $aPaper version available from: U.S. Government Accountability Office, 441 G St., NW, Rm. LM, Washington, D.C. 20548. 300 $a"GAO-05-563." 320 $aIncludes bibliographical references. 517 $aSchool meal programs 606 $aSchool children$xNutrition$zUnited States 606 $aNutrition policy$zUnited States 606 $aNational school lunch program 615 0$aSchool children$xNutrition 615 0$aNutrition policy 615 0$aNational school lunch program. 801 0$bGPO 801 1$bGPO 801 2$bGPO 906 $aBOOK 912 $a9910694509403321 996 $aSchool meal programs$93426859 997 $aUNINA